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  • richardmitnick 1:00 pm on November 10, 2017 Permalink | Reply
    Tags: Hyper-Kamiokande project, Interactions.org, , , MEXT, NNSO-Next-generation Neutrino Science Organization   

    From Interactions.org: “Inauguration of Next-generation Neutrino Science Organization for the Hyper-Kamiokande Nucleon Decay and Neutrino Experiment” 

    Interactions.org

    10 November 2017
    Kavli Institute for the Physics and Mathematics of the Universe

    Date Issued:
    November 10th, 2017
    Source:
    Kavli Institute for the Physics and Mathematics of the Universe
    Content:
    Press Release
    Contact:

    John Amari
    Public Relations Office
    The University of Tokyo International Institute for Advanced Studies
    Kavli Institute for the Physics and Mathematics of the Universe
    E-mail: press@ipmu.jp
    Tel: 04-7136-5977

    The Hyper-Kamiokande project aims to address the mysteries of the origin and evolution of the Universe’s matter as well as to confront theories of elementary particle unification.

    Hyper-Kamiokande, a neutrino physics laboratory located underground in the Mozumi Mine of the Kamioka Mining and Smelting Co. near the Kamioka section of the city of Hida in Gifu Prefecture, Japan.

    To realize these goals it will combine a high intensity neutrino beam from J-PARC with a new detector based upon precision neutrino experimental techniques developed in Japan and built to be approximately 10 times larger than the running Super-Kamiokande.

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

    On October 1st, 2017, The University of Tokyo launched its “Next-generation Neutrino Science Organization (NNSO),” in cooperation with the Institute for Cosmic Ray Research (ICRR), the Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU), and the University of Tokyo’s School of Science. The NNSO is a means of pioneering the future of neutrino physics through the development of neutrino research techniques and detector technologies. In particular, it aims to advance what will become its flagship facility, the Hyper-Kamiokande project. To mark the occasion, an inaugural ceremony was held on November 8th, 2017, at the Kamioka Observatory in Japan.

    Professor Takaaki Kajita, director of NNSO and a Nobel laureate for the discovery of neutrino oscillations demonstrating that neutrinos have mass, started the ceremony with opening remarks: “Understanding the neutrino, whose mass is extremely small, is not only important to particle physics, but is also thought to have deep connections to the origins of matter. Indeed, by observing neutrinos created with the high intensity proton accelerator J-PARC at Hyper-Kamiokande and testing whether or not neutrino and antineutrino oscillations are the same, we expect to close in on the mysteries of our matter-dominated universe. Further, we would like to discover the decay of the proton and thereby verify the unification of the three forces that act between elementary particles. Through the research represented by these goals, I would like to greatly expand our knowledge of elementary particles and the universe.”

    Professor Masashi Haneda, Executive Vice President of The University of Tokyo and Director of The University of Tokyo Institutes for Advanced Study, greeted attendees with these words: “Through the cooperation of these three important institutions, I’m sure that a world-class center for neutrino research will be established. Further, it will contribute much to cultivate talented young researchers. Succeeding Kamiokande and Super-Kamiokande, the Hyper-Kamiokande project will lead the world’s neutrino research. I would like to underline that the University of Tokyo will do our best to support this newly established organization.”

    Professor Hiroyuki Takeda, Dean of the School of Science, also gave an address: “The School of Science has a long and intimate relationship to the research in Kamioka, because Professor Koshiba started the original Kamiokande experiment when he was a faculty member of the School of Science. It is our great pleasure that we can further deepen the relationship with ICRR and Kavli IPMU through this organization to promote neutrino physics and the Hyper-Kamiokande project.”

    Professor Hitoshi Murayama, director of the Kavli Institute for the Physics and Mathematics of the Universe, delivered this message: “I firmly believe that the Hyper-Kamiokande experiment will be one of the most important experiments in the foreseeable future to study the Universe. Kavli IPMU would like to contribute to the Hyper-Kamiokande experiment with experimental expertise, theoretical support, and international networking. I’m very excited. Let’s make the Hyper-Kamiokande experiment happen!”

    Tomonori Nishii, Director of Scientific Research Institutes Division, Ministry of Education, Culture, Science and Technology (MEXT), Japan, presented congratulations: “In July of this year, the MEXT Roadmap 2017, which outlines the basic plan for pursuing large-scale projects, has been compiled by the Council for Science and Technology. It made the implementation priority of such projects clear. “Nucleon Decay and Neutrino Oscillation Experiment with a Large Advanced Detector”, that is Hyper-Kamiokande, is highly evaluated and listed in the roadmap with six other projects. MEXT, together with you, looks forward to seeing this new organization thrive as an international collaborative research hub and produce excellent scientific research achievements.”

    The ceremony was attended by about 100 people from MEXT, the University of Tokyo, KEK, local government and community, the Kamioka Mining and Smelting Company, and collaborating scientists. At the end, all attendees got together to take a group photo and celebrated the start of the new organization for promotion of neutrino physics and the Hyper-Kamiokande project.

    ABOUT THE HYPER-KAMIOKANDE

    Hyper-Kamiokande, or Hyper-K, is a straightforward extension of the successful water Cherenkov detector experiment Super-Kamiokande.

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

    It employs well-proven and high-performance water Cherenkov detector technology with established capabilities of neutrino oscillation studies by accelerator and atmospheric neutrinos, proton decay searches, and precision measurements of solar and supernova neutrinos. Hyper-Kamiokande will provide major new capabilities to make new discoveries in particle and astroparticle physics thanks to an order of magnitude increase in detector mass and improvements in photon detection, along with the envisioned J-PARC Megawatt-class neutrino beam.

    An international Hyper-Kamiokande proto-collaboration has been formed to carry out the experiment; it consists of about 300 researchers from 15 countries as of April 2017. The Hyper-Kamiokande member states are Armenia, Brazil, Canada, Ecuador, France, Italy, Japan, Korea, Poland, Russia, Spain, Switzerland, UK, Ukraine, and USA. The Institute for Cosmic Ray Research of the University of Tokyo and the Institute of Particle and Nuclear Studies of the High Energy Accelerator Research Organization KEK have signed a MoU affirming cooperation in the Hyper-K project to review and develop the program.

    Hyper-K is to be built as a tank with a 187 kiloton fiducial volume containing about 40,000 50-cm photo-multiplier tubes (PMTs), providing 40% photo cathode coverage. The proto-collaboration has succeeded in developing new PMTs with double the single-photon-sensitivity of those in Super-K.

    The Hyper-K and J-PARC neutrino beam measurement of neutrino oscillation is more likely to provide a 5-sigma discovery of CP violation than any other existing or proposed experiment. Hyper-K will also be the world leader for nucleon decays. The sensitivity to the partial lifetime of protons for the decay modes of p→e+π0 is expected to exceed 1035 years. This is the only known, realistic detector option capable of reaching such a sensitivity for the p→e+π0 mode. Finally, the astrophysical neutrino program involves precision measurement of solar neutrinos and their matter effects, as well as high-statistics supernova burst and supernova relic neutrinos.

    See the full article here .

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  • richardmitnick 8:26 pm on May 21, 2017 Permalink | Reply
    Tags: , , Interactions.org, , , ,   

    From interactions.org: “XENON1T, the most sensitive detector on Earth searching for WIMP dark matter, releases its first result” 

    Interactions.org

    Laboratori Nazionali del Gran Sasso – INFN

    18 May 2017
    Contact:

    XENON spokesperson
    Prof. Elena Aprile, Columbia University, New York, US.
    Tel. +39 3494703313
    Tel. +1 212 854 3258
    age@astro.columbia.edu

    INFN spokesperson
    Roberta Antolini
    + 39 0862 437216
    Roberta.antolini@lngs.infn.it

    Gran Sasso LABORATORI NAZIONALI del GRAN SASSO, located in the Abruzzo region of central Italy

    INFN Gran Sasso ICARUS, since moved to FNAL

    “The best result on dark matter so far! … and we have just started!”

    This is how scientists behind XENON1T, now the most sensitive dark matter experiment world-wide, hosted in the INFN Laboratori Nazionali del Gran Sasso, Italy, commented on their first result from a short 30-day run presented today to the scientific community.

    XENON1T at Gran Sasso

    Dark matter is one of the basic constituents of the Universe, five times more abundant than ordinary matter. Several astronomical measurements have corroborated the existence of dark matter, leading to a world-wide effort to observe directly dark matter particle interactions with ordinary matter in extremely sensitive detectors, which would confirm its existence and shed light on its properties. However, these interactions are so feeble that they have escaped direct detection up to this point, forcing scientists to build detectors that are more and more sensitive. The XENON Collaboration, that with XENON100 led the field for years in the past, is now back on the frontline with XENON1T. The result from a first short 30-day run shows that this detector has a new record low radioactivity level, many orders of magnitude below surrounding materials on Earth. With a total mass of about 3200 kg, XENON1T is at the same time the largest detector of this type ever built. The combination of significantly increased size with much lower background implies an excellent discovery potential in the years to come.

    The XENON Collaboration consists of 135 researchers from the US, Germany, Italy, Switzerland, Portugal, France, the Netherlands, Israel, Sweden and the United Arab Emirates. The latest detector of the XENON family has been in science operation at the LNGS underground laboratory since autumn 2016. The only things you see when visiting the underground experimental site now are a gigantic cylindrical metal tank, filled with ultra-pure water to shield the detector at his center, and a three-story-tall, transparent building crowded with equipment to keep the detector running, with physicists from all over the world. The XENON1T central detector, a so-called Liquid Xenon Time Projection Chamber (LXeTPC), is not visible. It sits within a cryostat in the middle of the water tank, fully submersed, in order to shield it as much as possible from natural radioactivity in the cavern. The cryostat allows keeping the xenon at a temperature of -95°C without freezing the surrounding water.

    The mountain above the laboratory further shields the detector, preventing it to be perturbed by cosmic rays. But shielding from the outer world is not enough since all materials on Earth contain tiny traces of natural radioactivity. Thus extreme care was taken to find, select and process the materials making up the detector to achieve the lowest possible radioactive content. Laura Baudis, professor at the University of Zürich and professor Manfred Lindner from the Max-Planck-Institute for Nuclear Physics in Heidelberg emphasize that this allowed XENON1T to achieve record “silence”, which is necessary to listen with a larger detector much better for the very weak voice of dark matter.

    A particle interaction in liquid xenon leads to tiny flashes of light. This is what the XENON scientists are recording and studying to infer the position and the energy of the interacting particle and whether it might be dark matter or not. The spatial information allows to select interactions occurring in the central 1 ton core of the detector. The surrounding xenon further shields the core xenon target from all materials which already have tiny surviving radioactive contaminants. Despite the shortness of the 30-day science run the sensitivity of XENON1T has already overcome that of any other experiment in the field, probing un-explored dark matter territory.

    “WIMPs did not show up in this first search with XENON1T, but we also did not expect them so soon!” says Elena Aprile, Professor at Columbia University and spokesperson of the project. “The best news is that the experiment continues to accumulate excellent data which will allow us to test quite soon the WIMP hypothesis in a region of mass and cross-section with normal atoms as never before. A new phase in the race to detect dark matter with ultra-low background massive detectors on Earth has just began with XENON1T. We are proud to be at the forefront of the race with this amazing detector, the first of its kind.”

    Further information:
    http://www.xenon1t.org
    http://www.lngs.infn.it

    See the full article here .

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