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  • richardmitnick 12:35 pm on December 4, 2018 Permalink | Reply
    Tags: 176-meter-long 800-million-electronvolt superconducting linear accelerator at FNAL, , FNAL LBNF/ DUNE at SURF, , INFN-Istituto Nazionale di Fisica Nucleare Laboratory for Accelerators and Applied Superconductivity   

    From Fermi National Accelerator Lab: “U.S. Department of Energy and Italy’s Ministry of Education, Universities and Research to collaborate on particle accelerator construction at Fermilab” 

    FNAL II photo

    FNAL Art Image
    FNAL Art Image by Angela Gonzales

    From Fermi National Accelerator Lab , an enduring source of strength for the US contribution to scientific research world wide.

    December 4, 2018

    1
    Jim Siegrist, associate director of the DOE Office of High-Energy Physics, and Maurizio Greganti, deputy chief of mission for the Embassy of Italy to the United States, sign an agreement to collaborate on Fermilab’s PIP-II project.

    Today the U.S. Department of Energy (DOE) and Italy’s Ministry of Education, Universities and Research (MIUR) signed an agreement to collaborate on the development and production of technical components for PIP-II, a major U.S. particle accelerator project to be located at DOE’s Fermi National Accelerator Laboratory in Batavia, Illinois. The signing took place at the Embassy of Italy in Washington.

    Italy and its National Institute of Nuclear Physics (INFN) will provide major contributions to the construction of the 176-meter-long superconducting particle accelerator that is the centerpiece of the PIP-II (Proton Improvement Plan-II) project. The new accelerator will become the heart of the Fermilab accelerator complex and provide the proton beam to power a broad program of accelerator-based particle physics research for many decades to come. In particular, PIP-II will enable the world’s most powerful high-energy neutrino beam to power the international Fermilab-hosted Deep Underground Neutrino Experiment (DUNE).

    FNAL Particle Accelerator

    FNAL LBNF/DUNE from FNAL to SURF, Lead, South Dakota, USA

    “It is with great appreciation that the Department of Energy enters into this agreement with our partners at MIUR and INFN,” said DOE Undersecretary for Science Paul Dabbar. “We’re proud that Fermilab’s PIP-II accelerator project, designed to create one of the most advanced machines for enabling discovery in the United States, is attracting major contributions from international partners for its construction.”

    The INFN Laboratory for Accelerators and Applied Superconductivity is expected to build components for the PIP-II accelerator. Based in Segrate, Italy, the laboratory is a center of excellence on an international scale for the development of advanced particle accelerators technologies.

    “The Agreement signed today by the Italian Ministry of Education, Universities and Research and DOE is the latest example of the scope and breadth of the scientific and technological cooperation between our two countries and of the importance of international cooperation,” said Armando Varricchio, ambassador of Italy to the United States. “This new step in our cooperation comes at a very significant time as we celebrate the 30th anniversary of the U.S.-Italy Agreement on Scientific and Technological Cooperation and renew our bilateral projects portfolio for the next three years.”

    At the signing, representatives from both countries recognized the long tradition of collaboration between Italian scientists and Fermilab, named after Italy’s own Enrico Fermi.

    “Following a long tradition of collaboration, the engagement of INFN on the construction of the PIP-II accelerator constitutes an important step in the context of unraveling neutrino properties through the ambitious DUNE project,” said INFN President Fernando Ferroni.

    The centerpiece of the PIP-II project will be an 800-million-electronvolt superconducting linear accelerator, which will modernize the front end of the existing Fermilab accelerator chain and provide a platform for future enhancements. The new accelerator will feature acceleration cavities made of niobium and double the beam energy of its predecessor. Such a boost will enable the Fermilab accelerator complex to achieve megawatt-scale proton beam power.

    “Our Italian partners are critical to the successful completion of Fermilab’s PIP-II superconducting accelerator,” said PIP-II Project Director Lia Merminga of Fermilab. “It takes a global community to build advanced, state-of-the-art accelerators like the one we’re developing for PIP-II.”

    In addition to Italy, other international partners are making significant contributions to PIP-II. They include India, the United Kingdom, and France. DOE’s Argonne and Lawrence Berkeley National Laboratories are also contributing key components to the project.

    “At the INFN Laboratory for Accelerators and Applied Superconductivity, we have a great experience of fruitful collaboration with Fermilab on advanced technologies for superconducting particle accelerators,” said Carlo Pagani of the University of Milan, Italian PIP-II project manager. “We are colleagues and friends, and I am excited for the opportunity that PIP-II is giving both for further growing together.”

    The partnership is one example of the increasingly global character of particle physics-related projects. The PIP-II accelerator complex will be made available to the international particle physics community and will extend the scientific discovery potential beyond that which currently can be reached.

    “It’s exciting to think that, in just a few years, the new PIP-II accelerator will produce some of the world’s most intense neutrino beams, which could give us a clearer picture of our universe’s evolution,” said Fermilab Director Nigel Lockyer. “This bright future is thanks in large part to our Italian partners. And since these partnerships strengthen over time, we could very well build on the relationship for future exciting projects in fundamental science.”


    This 40-second animation provides an overview of the PIP-II project. To learn more, visit pip2.fnal.gov.

    The DOE Office of Science is the single largest supporter of basic research in the physical sciences in the United States and is working to address some of the most pressing challenges of our time. For more information, please visit science.energy.gov.

    INFN, Istituto Nazionale di Fisica Nucleare, is the public Italian research institute dedicated to the study of the fundamental constituents of matter and their interactions. INFN conducts theoretical and experimental research in the fields of subnuclear, nuclear and astroparticle physics. Fundamental research in these areas requires the use of cutting-edge technology and instruments, developed by the INFN at its own laboratories and in collaboration with industries. All of the INFN’s research activities are conducted in close collaboration with Italian universities and undertaken within an international framework.

    See the full article here .


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    Fermi National Accelerator Laboratory (Fermilab), located just outside Batavia, Illinois, near Chicago, is a US Department of Energy national laboratory specializing in high-energy particle physics. Fermilab is America’s premier laboratory for particle physics and accelerator research, funded by the U.S. Department of Energy. Thousands of scientists from universities and laboratories around the world
    collaborate at Fermilab on experiments at the frontiers of discovery.


    FNAL/MINERvA

    FNAL DAMIC

    FNAL Muon g-2 studio

    FNAL Short-Baseline Near Detector under construction

    FNAL Mu2e solenoid

    Dark Energy Camera [DECam], built at FNAL

    FNAL DUNE Argon tank at SURF

    FNAL/MicrobooNE

    FNAL Don Lincoln

    FNAL/MINOS

    FNAL Cryomodule Testing Facility

    FNAL Minos Far Detector

    FNAL LBNF/DUNE from FNAL to SURF, Lead, South Dakota, USA

    FNAL/NOvA experiment map

    FNAL NOvA Near Detector

    FNAL ICARUS

    FNAL Holometer

     
  • richardmitnick 2:49 pm on October 26, 2018 Permalink | Reply
    Tags: , , FNAL LBNF/ DUNE at SURF, , J-PARC accelerator, , , Super Kamiokande experiment, T2K (Tokai to Kamiokande) experiment   

    From Live Science: “Could Misbehaving Neutrinos Explain Why the Universe Exists?” 

    Livescience
    From Live Science

    October 24, 2018

    FNAL’s Don Lincoln

    1
    Credit: Shutterstock

    Scientists revel in exploring mysteries, and the bigger the mystery, the greater the enthusiasm. There are many huge unanswered questions in science, but when you’re going big, it’s hard to beat “Why is there something, instead of nothing?”

    That might seem like a philosophical question, but it’s one that is very amenable to scientific inquiry. Stated a little more concretely, “Why is the universe made of the kinds of matter that makes human life possible so that we can even ask this question?” Scientists conducting research in Japan have announced a measurement last month that directly addresses that most fascinating of inquiries. It appears that their measurement disagrees with the simplest expectations of current theory and could well point toward an answer of this timeless question.

    Their measurement seems to say that for a particular set of subatomic particles, matter and antimatter act differently.

    Matter v. Antimatter

    Using the J-PARC accelerator, located in Tokai, Japan, scientists fired a beam of ghostly subatomic particles called neutrinos and their antimatter counterparts (antineutrinos) through the Earth to the Super Kamiokande experiment, located in Kamioka, also in Japan.

    J-PARC Facility Japan Proton Accelerator Research Complex , located in Tokai village, Ibaraki prefecture, on the east coast of Japan

    Super-Kamiokande experiment. located under Mount Ikeno near the city of Hida, Gifu Prefecture, Japan

    This experiment, called T2K (Tokai to Kamiokande), is designed to determine why our universe is made of matter. A peculiar behavior exhibited by neutrinos, called neutrino oscillation, might shed some light on this very vexing problem.

    T2K map, T2K Experiment, Tokai to Kamioka, Japan

    Asking why the universe is made of matter might sound like a peculiar question, but there is a very good reason that scientists are surprised by this. It’s because, in addition to knowing of the existence of matter, scientists also know of antimatter.

    In 1928, British physicist Paul Dirac proposed the existence of antimatter — an antagonistic sibling of matter. Combine equal amounts of matter and antimatter and the two annihilate each other, resulting in the release of an enormous amount of energy. And, because physics principles usually work equally well in reverse, if you have a prodigious quantity of energy, it can convert into exactly equal amounts of matter and antimatter. Antimatter was discovered in 1932 by American Carl Anderson and researchers have had nearly a century to study its properties.

    However, that “into exactly equal amounts” phrase is the crux of the conundrum. In the brief moments immediately after the Big Bang, the universe was full of energy. As it expanded and cooled, that energy should have converted into equal parts matter and antimatter subatomic particles, which should be observable today. And yet our universe consists essentially entirely of matter. How can that be?

    By counting the number of atoms in the universe and comparing that with the amount of energy we see, scientists determined that “exactly equal” isn’t quite right. Somehow, when the universe was about a tenth of a trillionth of a second old, the laws of nature skewed ever-so-slightly in the direction of matter. For every 3,000,000,000 antimatter particles, there were 3,000,000,001 matter particles. The 3 billion matter particles and 3 billion antimatter particles combined — and annihilated back into energy, leaving the slight matter excess to make up the universe we see today.

    Since this puzzle was understood nearly a century ago, researchers have been studying matter and antimatter to see if they could find behavior in subatomic particles that would explain the excess of matter. They are confident that matter and antimatter are made in equal quantities, but they have also observed that a class of subatomic particles called quarks exhibit behaviors that slightly favor matter over antimatter. That particular measurement was subtle, involving a class of particles called K mesons which can convert from matter to antimatter and back again. But there is a slight difference in matter converting to antimatter as compared to the reverse. This phenomenon was unexpected and its discovery led to the 1980 Nobel prize, but the magnitude of the effect was not enough to explain why matter dominates in our universe.

    Ghostly beams

    Thus, scientists have turned their attention to neutrinos, to see if their behavior can explain the excess matter. Neutrinos are the ghosts of the subatomic world. Interacting via only the weak nuclear force, they can pass through matter without interacting nearly at all. To give a sense of scale, neutrinos are most commonly created in nuclear reactions and the biggest nuclear reactor around is the Sun. To shield one’s self from half of the solar neutrinos would take a mass of solid lead about 5 light-years in depth. Neutrinos really don’t interact very much.

    Between 1998 and 2001, a series of experiments — one using the Super Kamiokande detector, and another using the SNO detector in Sudbury, Ontario ­­— proved definitively that neutrinos also exhibit another surprising behavior. They change their identity.

    SNOLAB, a Canadian underground physics laboratory at a depth of 2 km in Vale’s Creighton nickel mine in Sudbury, Ontario


    SNOLAB, Sudbury, Ontario, Canada.

    Physicists know of three distinct kinds of neutrinos, each associated with a unique subatomic sibling, called electrons, muons and taus. Electrons are what causes electricity and the muon and tau particle are very much like electrons, but heavier and unstable.

    The three kinds of neutrinos, called the electron neutrino, muon neutrino and tau neutrino, can “morph” into other types of neutrinos and back again. This behavior is called neutrino oscillation.

    Neutrino oscillation is a uniquely quantum phenomenon, but it is roughly analogous to starting out with a bowl of vanilla ice cream and, after you go and find a spoon, you come back to find that the bowl is half vanilla and half chocolate. Neutrinos change their identity from being entirely one type, to a mix of types, to an entirely different type, and then back to the original type.

    Antineutrino oscillations

    Neutrinos are matter particles, but antimatter neutrinos, called antineutrinos, also exist. And that leads to a very important question. Neutrinos oscillate, but do antineutrinos also oscillate and do they oscillate in exactly the same way as neutrinos? The answer to the first question is yes, while the answer to the second is not known.

    Let’s consider this a little more fully, but in a simplified way: Suppose that there were only two neutrino types — muon and electron. Suppose further that you had a beam of purely muon type neutrinos. Neutrinos oscillate at a specific speed and, since they move near the speed of light, they oscillate as a function of distance from where they were created. Thus, a beam of pure muon neutrinos will look like a mix of muon and electron types at some distance, then purely electron types at another distance and then back to muon-only. Antimatter neutrinos do the same thing.

    However, if matter and antimatter neutrinos oscillate at slightly different rates, you’d expect that if you were a fixed distance from the point at which a beam of pure muon neutrinos or muon antineutrinos were created, then in the neutrino case you’d see one blend of muon and electron neutrinos, but in the antimatter neutrino case, you’d see a different blend of antimatter muon and electron neutrinos. The actual situation is complicated by the fact that there are three kinds of neutrinos and the oscillation depends on beam energy, but these are the big ideas.

    The observation of different oscillation frequencies by neutrinos and antineutrinos would be an important step towards understanding the fact that the universe is made of matter. It’s not the entire story, because additional new phenomena must also hold, but the difference between matter and antimatter neutrinos is necessary to explain why there is more matter in the universe.

    In the current prevailing theory describing neutrino interactions, there is a variable that is sensitive to the possibility that neutrinos and antineutrinos oscillate differently. If that variable is zero, the two types of particles oscillate at identical rates; if that variable differs from zero, the two particle types oscillate differently.

    When T2K measured this variable, they found it was inconsistent with the hypothesis that neutrinos and antineutrinos oscillate identically. A little more technically, they determined a range of possible values for this variable. There is a 95 percent chance that the true value for that variable is within that range and only a 5 percent chance that the true variable is outside that range. The “no difference” hypothesis is outside the 95 percent range.

    In simpler terms, the current measurement suggests that neutrinos and antimatter neutrinos oscillate differently, although the certainty does not rise to the level to make a definitive claim. In fact, critics point out that measurements with this level of statistical significance should be viewed very, very skeptically. But it is certainly an enormously provocative initial result, and the world’s scientific community is extremely interested in seeing improved and more precise studies.

    The T2K experiment will continue to record additional data in hopes of making a definitive measurement, but it’s not the only game in town. At Fermilab, located outside Chicago, a similar experiment called NOvA is shooting both neutrinos and antimatter neutrinos to northern Minnesota, hoping to beat T2K to the punch.

    FNAL NOvA Near Detector


    FNAL/NOvA experiment map


    FNAL NOvA far detector in northern Minnesota


    NOvA Far Detector Block

    And, looking more to the future, Fermilab is working hard on what will be its flagship experiment, called DUNE (Deep Underground Neutrino Experiment), which will have far superior capabilities to study this important phenomenon.


    FNAL LBNF/DUNE from FNAL to SURF, Lead, South Dakota, USA


    SURF DUNE LBNF Caverns at Sanford Lab

    While the T2K result is not definitive and caution is warranted, it is certainly tantalizing. Given the enormity of the question of why our universe seems to have no appreciable antimatter, the world’s scientific community will avidly await further updates.

    See the full article here .

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  • richardmitnick 12:41 pm on October 23, 2018 Permalink | Reply
    Tags: , FNAL LBNF/ DUNE at SURF, , , High-Luminosity LHC (HL-LHC) at CERN, , LBNL/DESI Dark Energy Spectroscopic Instrument for the Nicholas U. Mayall 4-meter telescope at Kitt Peak National Observatory near Tucson Ariz USA, SLAC Large Synoptic Survey Telescope at Cerro Pachon Chile, ,   

    From Symmetry: “The building boom” 

    Symmetry Mag
    From Symmetry

    10/23/18
    By Diana Kwon

    4
    Illustration by Sandbox Studio, Chicago with Ana Kova

    These international projects, selected during the process to plan the future of US particle physics, are all set to come online within the next 10 years.

    A mile below the surface at Sanford Underground Research Facility in South Dakota, crews are preparing to excavate more than 800,000 tons of rock. Once the massive caverns they’re creating are complete, they will install four modules that make up a giant particle detector for the Deep Underground Neutrino Experiment. DUNE, hosted by the US Department of Energy’s Fermi National Accelerator Laboratory, is an ambitious, international effort to study neutrinos—the tiny, elusive and yet most abundant matter particles in the universe.

    DUNE is one of several particle physics and astrophysics projects with US participation currently under some stage of construction. These include large-scale projects, such as the construction of Mu2e, the muon-to-electron conversion experiment at Fermilab, and upgrades to the Large Hadron Collider at CERN. And they include smaller ones, such as the assembly of the LZ and SuperCDMS dark matter experiments. Together, these scientific endeavors will investigate a wide range of important concepts, including neutrino mass, the nature of dark matter and cosmic acceleration.

    “In the last 10 years, there have been many facilities in the US that wound down,” says Saul Gonzalez, a program director at the National Science Foundation. “But right now we’re definitely going through a boom—it’s a very exciting time.”

    A community effort

    Members of the US particle physics community identified these projects through a regularly occurring study of the field called the Snowmass planning process, named after the Colorado village where some of the first such dialogs took place in the early 1980s.

    After the most recent Snowmass meeting in Minneapolis in 2013, the 25-member Particle Physics Project Prioritization Panel, or P5, gathered to pinpoint the most important scientific problems in particle physics and propose a 10-year plan to take them on. “Snowmass enabled us to get the questions out there as a field,” says Steven Ritz, the University of California, Santa Cruz physicist who led the P5 panel. “But we’re also aware that budgets are constrained—so P5’s job was to prioritize them.”

    P5’s report, which was published in May 2014 [PDF], outlined five key areas of study: the Higgs boson; neutrinos; dark matter; dark energy and cosmic inflation; and undiscovered particles, interactions and physical principles.

    Shorter-term efforts to address questions in these areas, such as the Mu2e experiment and the Large Synoptic Survey Telescope in Chile, both already under construction, have projected start-up dates around 2020. Longer-term plans, such as DUNE and the high-luminosity upgrade to the LHC, are expected be ready for physics in the mid to latter part of the 2020s.

    “If you look at the timeline, we don’t build everything at once, because of budget and resource constraints,” says Young-Kee Kim, a physicist at the University of Chicago and a former member of the High Energy Physics Advisory Panel, the advisory group that P5 reports to.

    Another consideration was the importance of maintaining a continual stream of data, Ritz says. “We didn’t want to have a building boom where there was no new data for 5 or 10 years.”

    Having multiple experiments at various stages of completion is important for junior scientists. “If you’re a grad student or a postdoc and you’re working on something that’s not going to have physics data until 2024, that’s kind of a problem,” says Kate Scholberg, a physicist at Duke University who was on the P5 panel.

    A staggered timeline gives junior scientists the option of working on a project like DUNE, where they can contribute to research and development, then switch to another experiment where data is available for analysis.

    “Being in a construction phase does have some short-term challenges, but it’s really important as an investment for the future,” Scholberg says. “Because if you stop constructing, then eventually you’re not going to have any more data.”

    Global contributions

    The United States is not undertaking these experiments alone. “Every experiment is really an international collaboration,” Gonzalez says.

    The DUNE collaboration, for example, already includes more than 1100 scientists from 32 countries and counting. And although the Long-Baseline Neutrino Facility, the future home of DUNE, will be in the US, researchers are currently building prototype detectors for the project at the CERN research center in Europe.

    More than 1700 US scientists participate in research at the LHC at CERN; many of them are currently working on future upgrades to the accelerator and its experiments. Although LSST will operate on a mountaintop in Chile, its gigantic digital camera is being assembled at SLAC National Accelerator Laboratory using parts from institutions elsewhere in the United States and in France, Germany and the UK.

    Smaller experiments also have a global presence. Dark matter experiment SuperCDMS, a 23-institution collaboration led by SLAC, will be located at SNOLAB underground laboratory in Ontario and has members in Canada, France and India.

    People with specialized expertise are needed to build the apparatus for these experiments. For example, Fermilab’s Proton Improvement Plan-II, a project to upgrade the lab’s particle accelerator complex to provide protons beams for DUNE, requires individuals with expertise in superconducting radio-frequency technology. “We’re tapping into the SRF expertise around the world to build this,” says Michael Procario, the Director of the Facilities Division in the Office of High Energy Physics within DOE’s Office of Science.

    These DOE-supported endeavors—and the theory and data analysis that go along with them—will likely keep scientists busy until 2035 and beyond. “All the experiments are going to give us definitive answers. Even a null result will give us important information,” Ritz says. “I think it’s a great time for physics.”

    The experiments:

    Muon g-2

    FNAL Muon g-2 studio

    This experiment will measure the magnetic moment of a muon, a subatomic particle 200 times more massive than an electron, in an attempt to identify physics beyond the Standard Model.

    Location: Fermilab, Illinois, United States
    Lead institution: Fermilab
    Currently running

    Axion Dark Matter Experiment (ADMX-Gen 2)

    Inside the ADMX experiment hall at the University of Washington Credit Mark Stone U. of Washington

    U Washington ADMX

    Physicists are probing for signs of axions, hypothetical low-mass dark matter particles at the University of Washington-based ADMX detector.

    Location: University of Washington, United States
    Lead institution: University of Washington
    Currently running

    Physicists will use Mu2e to search for the never-observed direct conversion of a muon into an electron, a process predicted by theories beyond the Standard Model.

    FNAL Mu2e facility under construction


    FNAL Mu2e solenoid

    Location: Fermilab, Illinois, United States
    Lead institution: Fermilab
    Scheduled start-up: 2020

    LUX-ZEPLIN (LZ)

    LBNL LZ project at SURF, Lead, SD, USA


    LZ Dark Matter Experiment at SURF lab

    A liquified xenon detector surrounded by 70,000 gallons of water will be located more than 4000 feet underground at the Sanford Underground Research Facility, where researchers will hunt for interactions between matter and dark matter.

    Location: Sanford Lab, South Dakota, United States
    Lead institution: Berkeley Lab
    Scheduled start-up: 2020

    Dark Energy Spectroscopic Instrument (DESI)

    LBNL/DESI Dark Energy Spectroscopic Instrument for the Nicholas U. Mayall 4-meter telescope at Kitt Peak National Observatory near Tucson, Ariz, USA


    NOAO/Mayall 4 m telescope at Kitt Peak, Arizona, USA, Altitude 2,120 m (6,960 ft)

    Scientists will measure the effect of dark energy on cosmic expansion at the 4-meter Mayall Telescope at Kitt Peak National Observatory in Arizona.

    Location: Kitt Peak National Observatory, Arizona, United States
    Lead institution: Berkeley Lab
    Scheduled start-up: 2021

    Super Cyogenic Dark Matter Search (SuperCDMS)

    SNOLAB, a Canadian underground physics laboratory at a depth of 2 km in Vale’s Creighton nickel mine in Sudbury, Ontario

    SNOLAB, a Canadian underground physics laboratory at a depth of 2 km in Vale’s Creighton nickel mine in Sudbury, Ontario

    SLAC SuperCDMS, at SNOLAB (Vale Inco Mine, Sudbury, Canada)

    SLAC SuperCDMS, at SNOLAB (Vale Inco Mine, Sudbury, Canada)

    Physicists will hunt for dark matter particles with a cryogenic germanium detector located deep underground at SNOLAB in Canada.

    Location: SNOLAB, Ontario, Canada
    Lead institution: SLAC
    Scheduled start-up: Early 2020s

    Large Synoptic Survey Telescope (LSST)

    LSST


    LSST Camera, built at SLAC



    LSST telescope, currently under construction on the El Peñón peak at Cerro Pachón Chile, a 2,682-meter-high mountain in Coquimbo Region, in northern Chile, alongside the existing Gemini South and Southern Astrophysical Research Telescopes.

    The 8-meter Large Synoptic Survey Telescope, situated in northern Chile, will observe the whole accessible sky hundreds of times over 10 years to produce the deepest, widest image of the universe to date. This will allow physicists to probe questions about dark energy, dark matter, galaxy formation and more.

    Location: Cerro Pachon, Chile
    Lead institution: SLAC
    Scheduled start-up: Early 2020s

    Proton Improvement Pla-II (PIP-II)

    Upgrades to the Fermilab accelerator complex, including the construction of a 175-meter-long superconducting linear particle accelerator, will create the high-intensity proton beam that will produce beams of neutrinos for DUNE.

    Location: Fermilab, Illinois, United States
    Lead institution: Fermilab
    Scheduled start-up: mid-2020s

    Deep Underground Neutrino Experiment (DUNE)

    CERN Proto DUNE Maximillian Brice

    FNAL LBNF/DUNE from FNAL to SURF, Lead, South Dakota, USA

    SURF DUNE LBNF Caverns at Sanford Lab

    Scientists will send the world’s most powerful beam of neutrinos through two sets of detectors separated by 800 miles—one at the source of the beam at Fermilab in Illinois and the other at Sanford Underground Research Facility in South Dakota—to help scientists address fundamental concepts in particle physics, such as neutrino mass, matter-antimatter asymmetry, proton decay and black hole formation.

    Location: Fermilab, Illinois and Sanford Lab, South Dakota, United States
    Lead institution: Fermilab
    Scheduled partial start-up (with two detector modules): 2026

    High-Luminosity LHC (HL-LHC)

    LHC

    CERN map


    CERN LHC Tunnel

    CERN LHC particles

    An upgrade to CERN’s Large Hadron Collider will increase its luminosity—the number of collisions it can achieve—by a factor of 10. More collisions means more data and a higher probability of spotting rare events. The LHC experiments will receive upgrades to manage the higher collision frequency.

    Location: CERN, near Geneva, Switzerland
    Lead institution: CERN
    Scheduled start-up: 2026

    See the full article here .


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    Symmetry is a joint Fermilab/SLAC publication.


     
  • richardmitnick 1:00 pm on September 6, 2018 Permalink | Reply
    Tags: , , FNAL LBNF/ DUNE at SURF, , , ,   

    From Symmetry: “ProtoDUNE in pictures” 

    Symmetry Mag
    From Symmetry

    09/06/18
    Lauren Biron

    4
    Photo by CERN

    Twenty photos, two detectors, one goal.

    To investigate some of the biggest mysteries in the universe, particle physicists design and build high-tech detectors. On top of the incredible science they make possible, these experiments are often staggeringly beautiful. Views of the process of putting them together look like they could come straight out of a sci-fi film or from an alien planet.

    This is true of the ProtoDUNE detectors, which often appear in photographs as giant gold-colored cubes. These test beds are how scientists assess the technologies that will go into the Deep Underground Neutrino Experiment, the biggest international science project in the United States.

    Hosted by the US Department of Energy’s Fermi National Accelerator Laboratory, DUNE will send particles called neutrinos 800 miles (1300 kilometers) through the earth from Illinois to South Dakota.

    FNAL LBNF/DUNE from FNAL to SURF, Lead, South Dakota, USA

    There, about a mile (1.5 kilometers) underground, the largest liquid-argon neutrino detector ever built will analyze how those neutrinos behave. Researchers will use the data to investigate some of the biggest unsolved mysteries in particle physics, including why matter exists and what role neutrinos played in the universe’s evolution.

    DUNE is an international endeavor with 1100 scientists and engineers from more than 30 countries. DUNE is supported by international funding agencies, including the DOE Office of Science. The prototype detectors for DUNE are under construction at the neutrino platform at CERN, the European Center for Nuclear Physics and home of another amazing science machine, the Large Hadron Collider.

    The two ProtoDUNE detectors will help finalize the two different technologies that will be used for the four modules that will comprise DUNE’s far detector and will be filled with 70,000 tons of liquid argon.

    Take a look at the construction and evolution of the two prototypes in these 20 photographs—and keep in mind that each of the final DUNE detector modules in South Dakota will be 20 times bigger.

    2
    The first step in constructing the mammoth, cube-shaped ProtoDUNE detectors was to weld together portions of the steel cages, the red objects in this photo.
    Photo by CERN

    3
    Welders assemble parts of the steel cages for ProtoDUNE. This outer structure provides the necessary support for the interior membrane (or cryostat) that holds the liquid argon.
    Photo by CERN

    Please see the full article for all 20 photos.

    See the full article here .


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    Symmetry is a joint Fermilab/SLAC publication.


     
  • richardmitnick 1:25 pm on July 30, 2018 Permalink | Reply
    Tags: , FNAL LBNF/ DUNE at SURF, ,   

    From Fermilab: “DUNE collaboration completes Interim Design Report for gigantic particle detectors” 

    FNAL II photo

    FNAL Art Image
    FNAL Art Image by Angela Gonzales

    From Fermilab , an enduring source of strength for the US contribution to scientific research world wide.

    July 30, 2018
    Kurt Riesselmann

    1

    The more than 1,000 scientists and engineers from 32 countries working on the international Deep Underground Neutrino Experiment (DUNE), hosted by the Department of Energy’s Fermilab, achieved a milestone on July 29 when the collaboration released its 687-page Interim Design Report for the construction of gigantic particle detector modules a mile underground in South Dakota.

    The three-volume interim report, which was posted on the scientific online repository arXiv (Volume One, Volume Two, Volume Three), summarizes the DUNE physics goals and the design of the detector to meet these goals. It is based on the experience that DUNE scientists have gained during the design and construction of three-story-tall prototype detectors at CERN in Europe. The final detector modules, to be sited in the United States, will be about 20 times the size of the prototypes.

    “It is amazing how much work this collaboration has accomplished in the last couple of years,” said DUNE co-spokesperson Stefan Soldner-Rembold, professor at the University of Manchester in the UK. “The Interim Design Report is a major step toward the preparation of the final, more detailed Technical Design Report, which we will write next.”

    The DUNE Technical Design Report for the first two detector modules will be finalized roughly a year from now and will be the blueprint for the construction of those modules.

    “The Interim Design Report presents an enormous body of work,” said Sam Zeller, Fermilab, who served as the co-editor of the document together with Tim Bolton, Kansas State University. “The document doesn’t just contain drawings. It also includes detailed technical specifications and photos of the prototype equipment that was built during the last 12 months.”

    DUNE is an experiment to unlock the mysteries of neutrinos, the particles that could be the key to explaining why matter and the universe exist. The experiment will send a neutrino beam generated by Fermilab’s particle accelerator complex in Illinois 800 miles straight through Earth to the DUNE far detector modules to be built at the Sanford Underground Research Facility in South Dakota. DUNE scientists also will use the large detector modules to search for rare subatomic processes such as proton decay and watch for neutrinos stemming from the explosion of stars in our galaxy.

    2
    The giant DUNE detector will record images of particle tracks created by neutrinos colliding with argon atoms. No image credit.

    “The DUNE physics program addresses key questions that will give us further insight in the understanding of the universe,” said DUNE collaborator Albert de Roeck, leader of the CERN experimental neutrino group. “Neutrinos are still very enigmatic particles and no doubt will surprise us in future.”

    Groundbreaking for the construction of the caverns that will host the DUNE modules took place in July 2017, and the experiment is expected to be operational with two far detector modules online by 2026. Ultimately, DUNE will comprise four far detector modules filled with a total of 70,000 tons of liquid argon, as well as a smaller near detector at Fermilab.

    The Interim Design Report specifies the two technologies that DUNE scientists will use for the far detector: single- and dual-phase time projection chambers filled with cold, crystal clear liquid argon, the same technologies used to build the two prototype detectors at CERN, known as the ProtoDUNE detectors.

    “Designing liquid-argon time projection chambers of this size is an unprecedented effort requiring state-of-the-art technologies,” said CNRS Research Director Dario Autiero of the French National Institute of Nuclear and Particle Physics, Institut de Physique Nucleaire, Lyon, and DUNE collaborator. “DUNE pushes the technological limits in detector design, high-voltage systems, photon detection systems, low-noise electronics, and high-bandwidth data acquisition systems. DUNE collaborators have been developing these technologies for years, and they are being deployed in the two prototype detectors at CERN.”

    Both types of far detector modules will record images of particle tracks created by neutrinos colliding with argon atoms. In the single-phase technology, the entire volume of the detector is filled with liquid argon, and a horizontal high-voltage electric field “projects” the particle tracks towards the walls of the detector. Arrays of thin wires placed in front of the detector walls capture the signals created by the particle tracks and send them to a data acquisition system.

    “These giant detectors are being designed and developed by a great team of scientists and engineers, working together to unveil the secrets of the universe,” said Inés Gil-Botella, leader of the CIEMAT neutrino group, Madrid, Spain, and member of the DUNE collaboration. “Careful planning and coordination is the key to the success of DUNE.”

    The three volumes of the DUNE Far Detector Interim Design Report are available online: Volume One, Volume Two, Volume Three.

    The DUNE collaboration comprises 175 institutions from 32 countries: Armenia, Brazil, Bulgaria, Canada, Chile, China, Colombia, Czech Republic, Finland, France, Greece, India, Iran, Italy, Japan, Madagascar, Mexico, Netherlands, Paraguay, Peru, Poland, Portugal, Romania, Russia, South Korea, Spain, Sweden, Switzerland, Turkey, Ukraine, United Kingdom, and United States. More information is at dunescience.org.

    To learn more about the Deep Underground Neutrino Experiment, the Long-Baseline Neutrino Facility that will house the experiment, and the PIP-II particle accelerator project at Fermilab that will power the neutrino beam for the experiment, visit http://www.fnal.gov/dune.

    FNAL LBNF/DUNE from FNAL to SURF, Lead, South Dakota, USA


    FNAL DUNE Argon tank at SURF


    Surf-Dune/LBNF Caverns at Sanford



    SURF building in Lead SD USA

    See the full article here .


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    FNAL Icon

    Fermi National Accelerator Laboratory (Fermilab), located just outside Batavia, Illinois, near Chicago, is a US Department of Energy national laboratory specializing in high-energy particle physics. Fermilab is America’s premier laboratory for particle physics and accelerator research, funded by the U.S. Department of Energy. Thousands of scientists from universities and laboratories around the world
    collaborate at Fermilab on experiments at the frontiers of discovery.


    FNAL/MINERvA

    FNAL DAMIC

    FNAL Muon g-2 studio

    FNAL Short-Baseline Near Detector under construction

    FNAL Mu2e solenoid

    Dark Energy Camera [DECam], built at FNAL

    FNAL DUNE Argon tank at SURF

    FNAL/MicrobooNE

    FNAL Don Lincoln

    FNAL/MINOS

    FNAL Cryomodule Testing Facility

    FNAL Minos Far Detector

    FNAL LBNF/DUNE from FNAL to SURF, Lead, South Dakota, USA

    FNAL/NOvA experiment map

    FNAL NOvA Near Detector

    FNAL ICARUS

    FNAL Holometer

     
  • richardmitnick 4:30 pm on December 19, 2017 Permalink | Reply
    Tags: , , CERN Large Hadron Collider, FNAL LBNF/ DUNE at SURF, , , , Large Electron-Positron Collider, , , , , ,   

    From Symmetry: “Machine evolution” 

    Symmetry Mag
    Symmetry

    12/19/17
    Amanda Solliday

    1
    Courtesy of SLAC

    Planning the next big science machine requires consideration of both the current landscape and the distant future.

    Around the world, there’s an ecosystem of large particle accelerators where physicists gather to study the most intricate details of matter.

    These accelerators are engineering marvels. From planning to construction to operation to retirement, their lifespans stretch across decades.

    But to get the most out of their investments of talent and funding, laboratories planning such huge projects have to think even longer-term: What could these projects become in their next lives?

    The following examples show how some of the world’s big physics machines have evolved to stay at the forefront of science and technology.

    Same tunnel, new collisions

    Before CERN research center in Geneva, Switzerland, had its Large Hadron Collider, it had the Large Electron-Positron Collider. LEP was the largest electron-positron collider ever built, occupying a nearly 17-mile circular tunnel dug beneath the border of Switzerland and France. The tunnel took three years to completely excavate and build.

    The first particle beam traveled around the LEP circular collider in 1989. Long before then, the international group of CERN physicists and engineers were already thinking about what CERN’s next machine could be.

    “People were saying, ‘Well, if we do build LEP, then we should make it compatible with the [then-proposed] Large Hadron Collider,’” says James Gillies, a senior communications advisor and member of the strategic planning and evaluation unit at CERN. “If you want to have a future facility, you often have to engage the people who just finished designing one machine to start thinking about the next one.”

    LEP’s designers chose an energy for the collider that would mass-produce Z bosons, fundamental particles discovered by earlier experiments at CERN. The LHC would be a step up from LEP, reaching higher energies that scientists hoped could produce the Higgs boson. In the 1960s, theorists proposed the Higgs as a way to explain the origin of the mass of elementary particles. And the new machine to look for it could be built in the same 17-mile tunnel excavated for LEP.

    Engineers began working on the LHC while LEP was still running. The new machine required enlargements to underground areas—it needed bigger detectors and new experimental halls.

    “That was challenging because these caverns are huge. As they were being excavated, the pressure on the LEP tunnel was reduced and the LEP beamline needed realignment,” Gillies says. “So you constantly had to realign the collider for experiments as you were digging.”

    After LEP reached its highest energy in 2000, it was switched off. The tunnel remained the same, says Gillies, but there were many other changes. Only one of the LEP detectors, DELPHI, remains underground at CERN as a visitors’ point.

    In 2012, LHC scientists announced the discovery of the long-sought Higgs boson. The LHC is planned to continue running until at least 2035, gradually increasing the intensity of its particle collisions. The research and development into the accelerator’s successor is already happening. The possibilities include a higher energy LHC, a compact linear collider or an even larger circular collider.

    2

    Large Electron-Positron Collider
    Location: CERN—Geneva, Switzerland
    First beam: 1989
    Link to LEP Timeline: Timeline
    Courtesy of CERN

    LHC

    CERN/LHC Map

    CERN LHC Tunnel

    CERN LHC particles

    Large Hadron Collider
    Location: CERN—Geneva, Switzerland
    First beam: 2008
    Link to LHC Timeline: Timeline
    Courtesy of CERN

    High-powered science
    Decades before the LHC came into existence, a suburb of Chicago was home to the most powerful collider in the world: the Tevatron. A series of accelerators at Fermi National Accelerator Laboratory boosted protons and antiprotons to nearly the speed of light. In the final, 4-mile Tevatron ring, the particles reached record energy levels, and more than 1000 superconducting magnets steered them into collisions. Physicists used the Tevatron to make the first direct measurement of the tau neutrino and to discover the top quark, the last observed lepton and quark, respectively, in the Standard Model.

    The Tevatron shut down in 2011 after the LHC came up to speed, but the rest of Fermilab’s accelerator infrastructure was still hard at work powering research in particle physics—particularly on the abundant, mysterious and difficult-to-detect neutrino.

    Starting in 1999, a brand-new, 2-mile circular accelerator called the Main Injector was added to the Fermilab complex to increase the number of Tevatron particle collisions tenfold. It was joined in its tunnel by the Recycler, a permanent magnet ring that stored and cooled antiprotons.

    But before the Main Injector was even completed, scientists had identified a second purpose: producing powerful beams of neutrinos for experiments in Illinois and 500 miles away in Minnesota.

    FNAL/NOvA experiment map

    By 2005, the proton beam circulating in the Main Injector was doing double duty: sending ever-more-intense beams to the Tevatron collider and smashing into a target to produce neutrinos. Following the shutdown of the Tevatron, the Recycler itself was recycled to increase the proton beam power for neutrino research.

    “I’m still amazed at how we are able to use the Recycler. It can be difficult to transition if a machine wasn’t originally built for that purpose,” says Ioanis Kourbanis, the head of the Main Injector department at Fermilab.

    Fermilab’s high-energy neutrino beam is already the most intense in the world, but the laboratory plans to enhance it with future improvements to the Main Injector and the Recycler, and to build a brand-new neutrino beamline.

    Neutrinos almost never interact with matter, so they can pass straight through the Earth on their way to detectors onsite and others several hundred miles away. Scientists hope to learn more about neutrinos and their possible role in shaping our early universe.

    The new beamline will be part of the Long-Baseline Neutrino Facility, which will send neutrinos 800 miles underground to the massive, mile-deep detectors of the Deep Underground Neutrino Experiment.

    FNAL LBNF/DUNE from FNAL to SURF, Lead, South Dakota, USA


    FNAL DUNE Argon tank at SURF


    Surf-Dune/LBNF Caverns at Sanford



    SURF building in Lead SD USA

    Scientists from around the world will use the DUNE data to answer questions about neutrinos, thanks to the repurposed pieces of the Fermilab accelerator complex.

    5

    FNAL Tevatron

    FNAL/Tevatron map


    FNAL/Tevatron DZero detector


    FNAL/Tevatron CDF detector

    Tevatron
    Location: Fermilab—Batavia, Illinois
    First beam: 1983
    Link to Tevatron Timeline: Timeline
    Courtesy of Fermilab

    6

    Neutrinos at the Main Injector (NuMI) beam
    Location: Fermilab—Batavia, Illinois
    First beam: 2004
    Link to Fermilab Timeline: Timeline
    Courtesy of Fermilab

    A monster accelerator

    When physicists first came up with the idea to build a two-mile linear accelerator at what is now called SLAC National Accelerator Laboratory, managed by Stanford University, they called it “Project M” for “Monster.” Engineers began building it from hand-drawn designs. Once completed, the machine was able to accelerate electrons to near the speed of light, producing its first particle beam in May 1966.

    SLAC Campus

    The accelerator’s scientific purpose has gone through several iterations of particle physics experiments over the decades, from fixed-target experiments to the Stanford Linear Collider (the only electron-positron linear collider ever built) to an injector for a circular collider, the Positron-Electron Project.

    These experiments led to the discovery that protons are made of quarks, the first evidence that the charm quark existed (through observations of the J/psi particle, co-discovered with researchers at MIT) and the discovery of the tau lepton.

    In 2009, the lab used the accelerator as the backbone for a different type of science machine—an X-ray free-electron laser, the Linac Coherent Light Source.

    “Looking around, SLAC was the only place in the world with a linear accelerator capable of driving a free-electron laser,” says Claudio Pellegrini, a distinguished professor emeritus of physics at the University of California, Los Angeles and a visiting scientist and consulting professor at SLAC. Pellegrini first proposed the idea to transform SLAC’s linear accelerator.

    The new machine, a DOE Office of Science user facility, would be the world’s first laser of its kind that could produce extremely bright hard X-rays, the high-energy X-rays that let scientists take snapshots of atoms and molecules.

    “Much of the physics and many of the tools learned and developed during the operation of the Stanford Linear Collider were directly applicable to the free electron laser,” says Lia Merminga, head of the accelerator directorate at SLAC. “This was a big factor in the LCLS being commissioned in record time. Without the Stanford Linear Collider experience, this significant body of work would have to be reinvented and reproduced almost from scratch.”

    Little about the accelerator itself needed to change. But to create a free-electron laser, scientists needed to design a new part: an electron gun, a device that generates electrons to be injected into the accelerator. A collaboration of several national labs and UCLA created a new type of electron gun for LCLS, while other national labs helped build undulators, a series of magnets that would wiggle the electrons to create X-rays.

    LCLS used only the last third of SLAC’s original linear accelerator. In part of the remaining section, scientists are developing plasma wakefield and other new particle acceleration techniques.

    For the X-ray laser’s next iteration, LCLS-II, scientists are aiming for an even brighter laser that will fire 1 million pulses per second, allowing them to observe rare and exceptionally transient events.

    SLAC/LCLS II

    To do this, they will need to replace the original copper structures with superconducting technology. The technology is derived from designs for a large International Linear Collider [ILC] proposed to be built in Japan.

    ILC schematic

    “I’m in awe of the foresight of the original builders of SLAC’s linear accelerator,” Merminga adds. “We’ve been able to do so much with this machine, and the end is not yet in sight.”

    7

    Fixed target and collider experiments

    Location: SLAC—Menlo Park, California
    First beam: 1966
    Link to SLAC Timeline: Timeline
    Courtesy of SLAC

    8

    Linac Coherent Light Source
    Location: SLAC—Menlo Park, California
    First beam: 2009
    Link to SLAC Timeline: Timeline
    Courtesy of SLAC

    See the full article here .

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    Symmetry is a joint Fermilab/SLAC publication.


     
  • richardmitnick 1:05 pm on December 7, 2017 Permalink | Reply
    Tags: , , Dan Rederth, FNAL LBNF/ DUNE at SURF, South Dakota is already home to a growing suite of physics experiments located a mile beneath the surface in the Sanford Underground Research Facility, , Wenzhao Wei, Wenzhao Wei and Dan Rederth are the first to earn physics PhDs within the state of South Dakota,   

    From Symmetry: Women in STEM – “The PhD pioneers” Wenzhao Wei and also Dan Rederth, obviously not a Woman in STEM 

    Symmetry Mag
    Symmetry

    12/07/17
    Tom Barratt

    1
    Wenzhao Wei

    2
    Dan Rederth

    Wenzhao Wei and Dan Rederth are the first to earn physics PhDs within the state of South Dakota.

    Completing a PhD in physics is hard. It’s even harder when you’re one of the first to do it not just at your university, but at any university in your entire state.

    That’s exactly the situation Wenzhao Wei and Dan Rederth found themselves in earlier this year, when completing their doctorates at the University of South Dakota and the South Dakota School of Mines and Technology, respectively. Wei and Rederth are graduates of a joint program between the two institutions.

    Wei found out just a few weeks before going in front of a committee at USD to defend her thesis. A couple of students ahead of her had dropped out of the PhD program, leaving her suddenly at the head of the pack.

    “When I found out, I was very nervous,” Wei says. “When you’re the first, you don’t have any examples to follow, you don’t know how to prepare your defense, and you can’t get experience from other people who have already done it.”

    She recalls running between as many professors and committee members as she could for advice. “I did a lot of checking with them and asking questions. I had no idea what they would be expecting from the first PhD student.”

    Despite her wariness, and with some significant publications in the field as the first author, Dr. Wei’s defense was successful, and she is now working as a postdoc at the University of South Dakota.

    Rederth knew he was the first at SDSMT but wasn’t aware it was a first in South Dakota until after he had handed in his dissertation and completed his defense. “The president of the school told me I was the first in South Dakota after I finished,” he says. “But I wasn’t aware that Wenzhao had also completed her PhD at the same time.

    “Being the first, I was not prepared for the level of questioning I received during my defense – it went much deeper into physics than just my research. Together with Wenzhao, being the first in South Dakota really is a feather in the cap to something which took years of hard work to achieve.”

    Different paths to physics

    Rederth started on his path to physics research at a young age. “The most satisfying aspect of my PhD research dates back to my childhood,” he says. “I was always intrigued by magnetism and the mystery of how it works, so it was fascinating to do my research.”

    His work involved studying strange magnetic quantum effects that arise when certain particles are confined in special materials. A computer program he developed to model the effects could help bring new technologies into electronics.

    For Wei’s success, you might expect she had also always made a beeline to research, but physics was actually a late calling for her. At Central China Normal University, she had studied computer science and only switched to physics at master’s level.

    “In high school, I remember liking physics, but I ended up choosing computer science,” Wei says. “Then at college, I had some friends who did physics who were part of the same clubs as me, and they kept talking about really interesting things. I found I was becoming less interested in computer science and more interested in physics, so I switched.”

    Wei’s thesis, entitled “Advanced germanium detectors for rare event physics searches,” and her current research involve developing technologies for new kinds of particle physics detectors—ones that use germanium, a metal-like element similar to tin and silicon. Such detectors could be used for future neutrino and dark matter experiments.

    South Dakota is already home to a growing suite of physics experiments located a mile beneath the surface in the Sanford Underground Research Facility. It was in part a result of these experiments being located in the same state that Wei’s pioneering PhD program came about. USD has been involved with several experiments at SURF, among them the Deep Underground Neutrino Experiment, which will study neutrinos in a beam sent from Fermilab 1300 kilometers away.

    FNAL LBNF/DUNE from FNAL to SURF, Lead, South Dakota, USA


    FNAL DUNE Argon tank at SURF


    Surf-Dune/LBNF Caverns at Sanford



    SURF building in Lead SD USA

    “DUNE and SURF have been a vehicle to move the physics PhD program at USD forward,” says Dongming Mei, Wei’s doctoral advisor at USD. “With the progress of DUNE, future PhD students from USD will be exposed to thousands of world-class scientists and engineers.”

    Post-doctorate, Wei is now continuing the research she began during her thesis. But with a twist.

    “For my PhD, I did lots of computer simulations of dark matter interactions, so I spent a lot of time stuck at a computer,” Wei says. “Now I’m actually able to get hands-on with the germanium crystals we grow here at USD and test them for things like their electrical properties.”

    So where next for South Dakota’s first locally certified doctors of physics?

    “I want to stay in physics for the long-term,” Wei says. “I taught some physics to undergraduates during my PhD and really loved it, so I’m hoping to be a researcher and lecturer one day.”

    Rederth, too, wants to help inspire the next generation. “I want to stay in the Black Hills area to help raise science and math proficiency in the local schools. I’ve been a judge for the local science fair and would like to become more involved,” he says.

    Perhaps some of their future students will go on to join the list of South Dakota’s physics doctorates, started by their trailblazing teachers.

    See the full article here .

    Please help promote STEM in your local schools.

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    Symmetry is a joint Fermilab/SLAC publication.


     
  • richardmitnick 1:06 pm on November 17, 2017 Permalink | Reply
    Tags: FNAL LBNF/ DUNE at SURF, LBNC-Long-Baseline Neutrino Committee, ,   

    From SURF: “The LBNC encourages full momentum” 

    SURF logo
    Sanford Underground levels

    Sanford Underground Research facility

    First,

    LBNC meets at Sanford Lab
    October 30, 2017
    Constance Walter

    Last week, the Long-Baseline Neutrino Committee (LBNC) met at Sanford Lab. The committee consists of leading scientists from around the world who review the scientific, technical and managerial progress of the Long-Baseline Neutrino Facility and associated Deep Underground Neutrino Experiment (LBNF/DUNE).

    FNAL LBNF/DUNE from FNAL to SURF, Lead, South Dakota, USA


    FNAL DUNE Argon tank at SURF

    The committee meets three times each year in different locations; the previous meeting was held at CERN in Switzerland. In addition to attending meetings and writing reports, committee members toured Sanford Lab’s facilities, including the underground laboratories.

    “This is an independent group of scientists who were selected for their expertise,” said Nigel Lockyer, Fermilab director, who formed the committee. “Through this process, we ensure the project remains technically sound.”

    With more than 1,000 scientists from 176 institutions and 31 countries, LBNF/DUNE is the first international mega-science project to be hosted by a U.S. Department of Energy National Laboratory—Fermilab. The scientific collaboration hopes to revolutionize our understanding of the role neutrinos play in the creation of the universe. Using the Long-Baseline Neutrino Facility, they’ll shoot the world’s highest-intensity beam of neutrinos from Fermilab in Batavia, Illinois, 800 miles straight through the earth to huge detectors deep underground at Sanford Lab.

    The LBNC is analogous to the LHCC (Large Hadron Collider Committee) and has been in existence for two years. “That committee is a successful model that has been in place for more than 20 years,” Lockyer added.

    A sister committee, the Neutrino Cost Group, reviews the management schedule and costs of the project, Lockyer said.

    The LBNC writes a report that is delivered to the various funding agencies in countries that are supporting LBNF/DUNE, including the Department of Energy and National Science Foundation in the United States, CERN in Switzerland and the United Kingdom, which recently committed $88 million to the project.

    “We’re very pleased with the way the project is going,” Lockyer said.

    Now:

    The LBNC encourages full momentum

    November 16, 2017
    Anne Heavey
    Eric James

    The Long-Baseline Neutrino Committee (LBNC) — the experts responsible for advising the Fermilab Director on LBNF’s and DUNE’s scientific, technical, and managerial progress — had an opportunity to gain first-hand impressions of the DUNE Far Detector site during their recent review of the projects, held for the first time at SURF in late October.

    SURF-Sanford Underground Research Facility

    SURF An Empty Slate


    SURF Carving New Space


    SURF Shotcreting


    SURF Bolting and Wire Mesh


    SURF Outfitting Begins


    SURF circular wooden frame was built to form a concrete ring to hold the 72,000-gallon (272,549 liters) water tank that would house the LUX dark matter detector


    SURF LUX water tank was transported in pieces and welded together in the Davis Cavern


    SURF Ground Support


    SURF Dedicated to Science


    SURF Building a Ship in a Bottle


    SURF Tight Spaces


    SURF Ready for Science


    SURF Entrance Before Outfitting


    SURF Entrance After Outfitting


    SURF Common Corridior


    SURF Davis


    SURF Davis A World Class Site


    SURF Davis a Lab Site


    U Washington LUX Xenon experiment at SURF


    SURF Before Majorana


    U Washington Majorana Demonstrator Experiment at SURF

    1
    LBNC and LBNF members at the 4850 level at SURF. Photo: Josh Willhite

    Josh Willhite, the LBNF Far Site Conventional Facilities Manager, guided many of the attendees on an extensive tour of the 4850 level where pre-excavation activities will begin in the next few months followed by the start of actual rock excavation in 2019. The required clunky jumpsuits, helmets and boots in no way inhibited the group’s nonstop photos, questions and smiles.

    This review marked a transition in the LBNC’s focus. With the ProtoDUNE designs largely complete and construction underway, and the DUNE Far Detector Technical Proposal and Technical Design Report (TDR) now in the crosshairs, the LBNC is largely turning its attention towards plans for the Far Detector construction.

    CERN Proto DUNE Maximillian Brice

    The LBNC commended DUNE on establishing the consortium-based structure for the Far Detector in a timely manner, considering it “a demonstration of a major step in building up the collaborative spirit.”

    The committee applauded the steady growth in the DUNE Collaboration, which now includes 176 institutions in 31 nations and “a healthy fraction of PhD Students,” and on the “significant progress” in negotiations with new prospective partners in Europe, South America and Asia.

    “Overall, the Committee was very impressed by the significant progress achieved by both LBNF and DUNE since the last LBNC review (in June at CERN),” the committee wrote. In particular, on the LBNF side, the LBNC’s report highlighted the completion of the Ross shaft refurbishment, the award of the CM/GC contract, and the imminent start of the final design phase for the Far Site Conventional Facilities. On the DUNE side, they congratulated CERN Neutrino Platform and the Collaboration on the “tremendous progress” made on the ProtoDUNE cryostats.

    A special Wednesday evening session focused on plans for the Technical Proposal and the TDR. While acknowledging that the plans are “ambitious,” the LBNC agreed with the framework that the DUNE leadership presented, recognizing that such a plan “will allow the Collaboration to maintain full momentum for developing the project in a focused and timely fashion, including the detailed construction strategies and schedules for the various components.” The group discussed the review schedule in accordance with getting final approval in late 2019 to move forward with construction of the cryostats, cryogenic systems, and detector components.

    See the full article here .

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    About us.
    The Sanford Underground Research Facility in Lead, South Dakota, advances our understanding of the universe by providing laboratory space deep underground, where sensitive physics experiments can be shielded from cosmic radiation. Researchers at the Sanford Lab explore some of the most challenging questions facing 21st century physics, such as the origin of matter, the nature of dark matter and the properties of neutrinos. The facility also hosts experiments in other disciplines—including geology, biology and engineering.

    The Sanford Lab is located at the former Homestake gold mine, which was a physics landmark long before being converted into a dedicated science facility. Nuclear chemist Ray Davis earned a share of the Nobel Prize for Physics in 2002 for a solar neutrino experiment he installed 4,850 feet underground in the mine.

    Homestake closed in 2003, but the company donated the property to South Dakota in 2006 for use as an underground laboratory. That same year, philanthropist T. Denny Sanford donated $70 million to the project. The South Dakota Legislature also created the South Dakota Science and Technology Authority to operate the lab. The state Legislature has committed more than $40 million in state funds to the project, and South Dakota also obtained a $10 million Community Development Block Grant to help rehabilitate the facility.

    In 2007, after the National Science Foundation named Homestake as the preferred site for a proposed national Deep Underground Science and Engineering Laboratory (DUSEL), the South Dakota Science and Technology Authority (SDSTA) began reopening the former gold mine.

    In December 2010, the National Science Board decided not to fund further design of DUSEL. However, in 2011 the Department of Energy, through the Lawrence Berkeley National Laboratory, agreed to support ongoing science operations at Sanford Lab, while investigating how to use the underground research facility for other longer-term experiments. The SDSTA, which owns Sanford Lab, continues to operate the facility under that agreement with Berkeley Lab.

    The first two major physics experiments at the Sanford Lab are 4,850 feet underground in an area called the Davis Campus, named for the late Ray Davis. The Large Underground Xenon (LUX) experiment is housed in the same cavern excavated for Ray Davis’s experiment in the 1960s.
    LUX/Dark matter experiment at SURFLUX/Dark matter experiment at SURF

    In October 2013, after an initial run of 80 days, LUX was determined to be the most sensitive detector yet to search for dark matter—a mysterious, yet-to-be-detected substance thought to be the most prevalent matter in the universe. The Majorana Demonstrator experiment, also on the 4850 Level, is searching for a rare phenomenon called “neutrinoless double-beta decay” that could reveal whether subatomic particles called neutrinos can be their own antiparticle. Detection of neutrinoless double-beta decay could help determine why matter prevailed over antimatter. The Majorana Demonstrator experiment is adjacent to the original Davis cavern.

    Another major experiment, the Long Baseline Neutrino Experiment (LBNE)—a collaboration with Fermi National Accelerator Laboratory (Fermilab) and Sanford Lab, is in the preliminary design stages. The project got a major boost last year when Congress approved and the president signed an Omnibus Appropriations bill that will fund LBNE operations through FY 2014. Called the “next frontier of particle physics,” LBNE will follow neutrinos as they travel 800 miles through the earth, from FermiLab in Batavia, Ill., to Sanford Lab.

    Fermilab LBNE
    LBNE

     
  • richardmitnick 10:28 am on September 18, 2017 Permalink | Reply
    Tags: Alex Himmel of Fermilab, , , Chao Zhang of BNL, Congratulations to two award-winning DUNE collaborators, , FNAL LBNF/ DUNE at SURF, ,   

    From NUS TO SURF: “Congratulations to two award-winning DUNE collaborators” 

    NUS TO SURF

    1

    “It is great news that the US DOE has recognized the talents of two early career DUNE scientists — both Alex and Chao have made invaluable contributions to DUNE and are both deserving recipients of these prestigious funding awards.”
    — DUNE spokespersons Mark Thomson and Ed Blucher

    FNAL LBNF/DUNE from FNAL to SURF, Lead, South Dakota, USA


    FNAL DUNE Argon tank at SURF


    Surf-Dune/LBNF Caverns at Sanford



    SURF building in Lead SD USA

    2
    Chao Zhang of BNL. Credit: BNL

    Exerpted and adapted from Three Brookhaven Lab Scientists Selected to Receive Early Career Research Program Funding, BNL Newsroom, 15 Aug 2017.

    Brookhaven Lab physicist and DUNE collaborator Chao Zhang was selected by DOE’s Office of High Energy Physics to receive funding for a project titled Optimization of Liquid Argon TPCs for Nucleon Decay and Neutrino Physics. Liquid Argon TPCs form the heart of many large-scale particle detectors designed to explore fundamental mysteries in particle physics.

    Chao’s aim is to optimize the performance of the DUNE far detector LArTPCs to fully realize their potential to track and identify particles in three dimensions, with a particular focus on making them sensitive to rare proton decays.

    His team at Brookhaven Lab will establish a hardware calibration system to ensure the experiment’s ability to extract subtle signals using specially designed cold electronics that will sit within the detector. They will also develop software to reconstruct the three-dimensional details of complex events, and analyze data collected at a prototype experiment (ProtoDUNE, located at Europe’s CERN laboratory) to verify that these methods are working, before incorporating any needed adjustments into the design of the detectors for DUNE.

    “I am honored and thrilled to receive this distinguished award,” said Chao. “With this support, my colleagues and I will be able to develop many new techniques to enhance the performance of LArTPCs, and we are excited to be involved in the search for answers to one of the most intriguing mysteries in science, the matter-antimatter asymmetry in the universe.”

    Read full article.


    Alex Himmel of Fermilab. Credit: Fermilab

    This article is excerpted and adapted from a Fermilab news article, 14 September 2017.

    Fermilab’s Alex Himmel expects to spend a large chunk of his career working on the Deep Underground Neutrino Experiment (DUNE), the flagship experiment of the U.S. particle physics community. That is incentive, he says, to lay the groundwork now to ensure its success.

    The Department of Energy has selected Himmel, a Wilson fellow, for a 2017 DOE Early Career Research Award to do just that. He will receive $2.5 million over five years to build a team and optimize software that will measure the flashes of ultraviolet light generated in neutrino collisions in a way that will determine the energy of the neutrino more precisely than is currently possible.

    Photons released from neutrino collisions will arrive at their detectors deteriorated and distorted due to scattering and reflections; the light measured is not the same as what was given off.

    “What we want to know is, given an amount of energy deposited in the argon, how much light do we see, taking out all the other things we know about how the light moves inside the detector,” he explained.

    Researchers are already looking forward to the long-term, positive impact of Himmel’s research.

    “Alex has been a true leader in understanding the physics potential of scintillation light in liquid-argon detectors,” said Ed Blucher. “His plan to develop techniques to make the most effective use of photon detection will help to enable the best and broadest possible physics program for DUNE.”

    Himmel has deep ties with Fermilab and neutrinos, starting with his first job as a summer student at Fermilab when he was 16. In 2012, he won the Universities Research Association Thesis Award for his research on muon antineutrino oscillations at Fermilab’s MINOS experiment.

    Read full article.

    Please help promote STEM in your local schools.

    STEM Icon

    Stem Education Coalition

     
  • richardmitnick 9:55 pm on September 5, 2017 Permalink | Reply
    Tags: , , , , , , , FNAL LBNF/ DUNE at SURF, , , , , ,   

    From Symmetry: “What can particles tell us about the cosmos?” 

    Symmetry Mag
    Symmetry

    09/05/17
    Amanda Solliday

    The minuscule and the immense can reveal quite a bit about each other.

    In particle physics, scientists study the properties of the smallest bits of matter and how they interact. Another branch of physics—astrophysics—creates and tests theories about what’s happening across our vast universe.

    1
    The current theoretical framework that describes elementary particles and their forces, known as the Standard Model, is based on experiments that started in 1897 with the discovery of the electron. Today, we know that there are six leptons, six quarks, four force carriers and a Higgs boson. Scientists all over the world predicted the existence of these particles and then carried out the experiments that led to their discoveries. Learn all about the who, what, where and when of the discoveries that led to a better understanding of the foundations of our universe.

    While particle physics and astrophysics appear to focus on opposite ends of a spectrum, scientists in the two fields actually depend on one another. Several current lines of inquiry link the very large to the very small.

    The seeds of cosmic structure

    For one, particle physicists and astrophysicists both ask questions about the growth of the early universe.

    In her office at Stanford University, Eva Silverstein explains her work parsing the mathematical details of the fastest period of that growth, called cosmic inflation.

    Lambda-Cold Dark Matter, Accelerated Expansion of the Universe, Big Bang-Inflation (timeline of the universe) Date 2010 Credit: Alex MittelmannColdcreation

    “To me, the subject is particularly interesting because you can understand the origin of structure in the universe,” says Silverstein, a professor of physics at Stanford and the Kavli Institute for Particle Astrophysics and Cosmology. “This paradigm known as inflation accounts for the origin of structure in the most simple and beautiful way a physicist can imagine.”

    Scientists think that after the Big Bang, the universe cooled, and particles began to combine into hydrogen atoms. This process released previously trapped photons—elementary particles of light.

    The glow from that light, called the cosmic microwave background, lingers in the sky today.

    CMB per ESA/Planck

    Scientists measure different characteristics of the cosmic microwave background to learn more about what happened in those first moments after the Big Bang.

    According to scientists’ models, a pattern that first formed on the subatomic level eventually became the underpinning of the structure of the entire universe. Places that were dense with subatomic particles—or even just virtual fluctuations of subatomic particles—attracted more and more matter. As the universe grew, these areas of density became the locations where galaxies and galaxy clusters formed. The very small grew up to be the very large.

    Universe map Sloan Digital Sky Survey (SDSS) 2dF Galaxy Redshift Survey

    Scientists studying the cosmic microwave background hope to learn about more than just how the universe grew—it could also offer insight into dark matter, dark energy and the mass of the neutrino.

    Dark Matter

    Dark matter cosmic web and the large-scale structure it forms The Millenium Simulation, V. Springel et al

    Dark Matter Particle Explorer China

    DEAP Dark Matter detector, The DEAP-3600, suspended in the SNOLAB deep in Sudbury’s Creighton Mine

    LUX Dark matter Experiment at SURF, Lead, SD, USA

    ADMX Axion Dark Matter Experiment, U Uashington

    Dark Energy Survey


    Dark Energy Camera [DECam], built at FNAL


    NOAO/CTIO Victor M Blanco 4m Telescope which houses the DECam at Cerro Tololo, Chile, housing DECam at an altitude of 7200 feet

    FNAL LBNF/DUNE from FNAL to SURF, Lead, South Dakota, USA


    FNAL DUNE Argon tank at SURF


    Surf-Dune/LBNF Caverns at Sanford



    SURF building in Lead SD USA

    “It’s amazing that we can probe what was going on almost 14 billion years ago,” Silverstein says. “We can’t learn everything that was going on, but we can still learn an incredible amount about the contents and interactions.”

    For many scientists, “the urge to trace the history of the universe back to its beginnings is irresistible,” wrote theoretical physicist Stephen Weinberg in his 1977 book The First Three Minutes. The Nobel laureate added, “From the start of modern science in the sixteenth and seventeenth centuries, physicists and astronomers have returned again and again to the problem of the origin of the universe.”

    Searching in the dark

    Particle physicists and astrophysicists both think about dark matter and dark energy. Astrophysicists want to know what made up the early universe and what makes up our universe today. Particle physicists want to know whether there are undiscovered particles and forces out there for the finding.

    “Dark matter makes up most of the matter in the universe, yet no known particles in the Standard Model [of particle physics] have the properties that it should possess,” says Michael Peskin, a professor of theoretical physics at SLAC.

    The Standard Model of elementary particles (more schematic depiction), with the three generations of matter, gauge bosons in the fourth column, and the Higgs boson in the fifth.

    “Dark matter should be very weakly interacting, heavy or slow-moving, and stable over the lifetime of the universe.”

    There is strong evidence for dark matter through its gravitational effects on ordinary matter in galaxies and clusters. These observations indicate that the universe is made up of roughly 5 percent normal matter, 25 percent dark matter and 70 percent dark energy. But to date, scientists have not directly observed dark energy or dark matter.

    “This is really the biggest embarrassment for particle physics,” Peskin says. “However much atomic matter we see in the universe, there’s five times more dark matter, and we have no idea what it is.”

    But scientists have powerful tools to try to understand some of these unknowns. Over the past several years, the number of models of dark matter has been expanding, along with the number of ways to detect it, says Tom Rizzo, a senior scientist at SLAC and head of the theory group.

    Some experiments search for direct evidence of a dark matter particle colliding with a matter particle in a detector. Others look for indirect evidence of dark matter particles interfering in other processes or hiding in the cosmic microwave background. If dark matter has the right properties, scientists could potentially create it in a particle accelerator such as the Large Hadron Collider.

    LHC

    CERN/LHC Map

    CERN LHC Tunnel

    CERN LHC particles

    Physicists are also actively hunting for signs of dark energy. It is possible to measure the properties of dark energy by observing the motion of clusters of galaxies at the largest distances that we can see in the universe.

    “Every time that we learn a new technique to observe the universe, we typically get lots of surprises,” says Marcelle Soares-Santos, a Brandeis University professor and a researcher on the Dark Energy Survey. “And we can capitalize on these new ways of observing the universe to learn more about cosmology and other sides of physics.”

    Forces at play

    Particle physicists and astrophysicists find their interests also align in the study of gravity. For particle physicists, gravity is the one basic force of nature that the Standard Model does not quite explain. Astrophysicists want to understand the important role gravity played and continues to play in the formation of the universe.

    In the Standard Model, each force has what’s called a force-carrier particle or a boson. Electromagnetism has photons. The strong force has gluons. The weak force has W and Z bosons. When particles interact through a force, they exchange these force-carriers, transferring small amounts of information called quanta, which scientists describe through quantum mechanics.

    General relativity explains how the gravitational force works on large scales: Earth pulls on our own bodies, and planetary objects pull on each other. But it is not understood how gravity is transmitted by quantum particles.

    Discovering a subatomic force-carrier particle for gravity would help explain how gravity works on small scales and inform a quantum theory of gravity that would connect general relativity and quantum mechanics.

    Compared to the other fundamental forces, gravity interacts with matter very weakly, but the strength of the interaction quickly becomes larger with higher energies. Theorists predict that at high enough energies, such as those seen in the early universe, quantum gravity effects are as strong as the other forces. Gravity played an essential role in transferring the small-scale pattern of the cosmic microwave background into the large-scale pattern of our universe today.

    “Another way that these effects can become important for gravity is if there’s some process that lasts a long time,” Silverstein says. “Even if the energies aren’t as high as they would need to be sensitive to effects like quantum gravity instantaneously.”

    Physicists are modeling gravity over lengthy time scales in an effort to reveal these effects.

    Our understanding of gravity is also key in the search for dark matter. Some scientists think that dark matter does not actually exist; they say the evidence we’ve found so far is actually just a sign that we don’t fully understand the force of gravity.

    Big ideas, tiny details

    Learning more about gravity could tell us about the dark universe, which could also reveal new insight into how structure in the universe first formed.

    Scientists are trying to “close the loop” between particle physics and the early universe, Peskin says. As scientists probe space and go back further in time, they can learn more about the rules that govern physics at high energies, which also tells us something about the smallest components of our world.

    See the full article here .

    Please help promote STEM in your local schools.

    STEM Icon

    Stem Education Coalition

    Symmetry is a joint Fermilab/SLAC publication.


     
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