From DOE’s Brookhaven National Laboratory (US) via Interactions.org : “Start-up of 22nd Run at the Relativistic Heavy Ion Collider (RHIC)”

From DOE’s Brookhaven National Laboratory (US)

via

Interactions.org

13 December 2021

Karen McNulty Walsh
+1 (631) 344-8350
kmcnulty@bnl.gov

Peter Genzer
+1 (631) 344-3174
genzer@bnl.gov

Physicists will try out innovative accelerator techniques and deliver high-energy polarized protons for explorations of protons’ inner structure using new detector components at the STAR detector.

Particle smashups have begun for Run 22 at the Relativistic Heavy Ion Collider (RHIC)[below]. RHIC, a 2.4-mile-circumference particle collider at the U.S. Department of Energy’s Brookhaven National Laboratory, operates as a Department of Energy (US) Office of Science user facility, serving up data from particle collisions to nuclear physicists all around the world. On the menu this run: collisions between beams of polarized protons interspersed with tests of innovative accelerator techniques. During the run, RHIC’s recently upgraded STAR detector [original image below, no upgrade images made available by BNL] will track particles emerging from collisions at a wider range of angles than ever before.

The new data will add to earlier RHIC datasets exploring the fundamental building blocks of visible matter. In addition, the physics findings, accelerator tests, and detector technologies will play important roles in the Electron-Ion Collider (EIC) [below]—DOE’s next planned nuclear physics facility, which will reuse key components of RHIC.

Discovering the universal properties of protons and how they emerge from the interactions of quarks and gluons, the building blocks within protons, is a central goal of both facilities. RHIC’s proton-proton collisions could reveal unprecedented details and a preview of how certain characteristics depend on the dynamic motions of the quarks and gluons.

“Our goal this run is basically doing EIC physics with proton-proton collisions,” said Brookhaven Lab physicist Elke-Caroline Aschenauer, a member of the STAR collaboration who is also involved in planning the experiments and scientific program at the EIC. “It’s important to do both [using RHIC and the EIC] because you have to verify that what you measure in electron-proton collisions at the EIC and in proton-proton events at RHIC is universal—meaning it doesn’t depend on which probe you use to measure it,” she explained.

The measurements rely on RHIC’s ability to align the “spins” of protons in an upward pointing direction. This alignment, or polarization—a capability unique among colliders like RHIC—gives scientists a directional frame of reference for tracking how particles generated in the collisions move.

“We are using polarization as a vehicle to study proton structure, and particularly the 3D structure, including how the internal particles (quarks and gluons) are moving inside the proton,” Aschenauer said.

Delivering proton beams

The physicists in Brookhaven Lab’s Collider-Accelerator Department (C-AD), who steer the beams around RHIC, are determined to give STAR what it needs.

“For Run 22 we are going to focus on being as efficient as possible and racking up the collisions at the highest possible polarization,” said C-AD physicist Vincent Schoefer, this year’s run coordinator.

When we spoke with Schoefer, he was busy “waking up” equipment that hasn’t been used since Run 17—the last time polarized protons were collided at RHIC. This equipment includes “helical dipole” magnets that help preserve the polarization of the protons as they make millions of turns around RHIC’s twin accelerator rings. This year’s run will take place at the highest collision energy: 500 billion electron volts (GeV) per colliding proton.

The C-AD team was also preparing “polarimeters” to measure just how aligned those proton spins are.

“It doesn’t matter how highly polarized your beam is if you can’t measure that. So, the polarimetry is really crucial,” Schoefer said.

Accelerator physicists in C-AD and experimental physicists involved in making measurements that rely on polarized beams collaborated on the design of RHICs polarimeters.

“This work is an example of the type of collaboration between groups that has been going on since the start of RHIC,” said C-AD physicist Haixin Huang.

Pumping up polarization

Keeping proton beams tightly packed helps preserve polarization. It also maximizes the likelihood that you get collisions when the beams cross. But keeping protons close together is a challenge.

“They’re all positively charged particles, so they want to repel one another,” Schoefer explained. “The more tightly you pack them, the more they resist that packing.”

The repulsion is particularly strong in the early stages of acceleration—before protons have been ramped up to full collision energy. So, this run, the C-AD team will try a technique that’s worked when RHIC accelerates larger particles but has never been used with protons before.

“We are going to split each proton bunch into two when they’re still at low energy in the Booster, and accelerate those as two separate bunches,” Schoefer said. “That splitting will alleviate some of the stress during low energy, and then we can merge the bunches back together to put very dense bunches into RHIC.”

This merging maneuver is challenging, Schoefer said, because it takes “a really long time—where a really long time is one second! For the protons, that’s 300,000 turns around the Alternating Gradient Synchrotron (AGS).” (The AGS is the link in the accelerator chain after the Booster that feeds particle beams into RHIC.) “During those 300,000 turns, we have to handle the protons very gently, so we don’t ruin the nice beams we have prepared.”

The CA-D team will also calculate very careful trajectories for the particles’ paths through the collider. This step should help counteract the tendency of the accelerator’s magnetic fields (which physicists use to steer and focus the beams) to rotate the spins of protons away from ideal alignment.

“We’re going to try different trajectories and see if we can learn something about what is making this misalignment happen,” Schoefer said.

The combination of techniques is now delivering highly polarized proton beams to collide inside STAR.

STAR upgrades

When they analyze results from these collisions, STAR physicists will be looking for differences in the numbers of certain particles emerging to the left and right of the polarized protons’ upward pointing direction.

For example, they want to test whether there’s a repulsive interaction between particles with like “color” charges that’s opposite to the attractive interaction observed between unlike color-charged particles. (Color charge is they type of charge through which quarks interact.) The opposite force should produce the opposite directional preference for certain particle decay products.

STAR first saw hints of this effect in data collected in 2011, published in 2016 [Physical Review Letters]. A preliminary analysis of additional data collected in Run 17 indicates a small effect but with large uncertainties. Run 22 will help STAR reduce those uncertainties with larger data sets.

In addition, the recently installed STAR upgrades will give physicists the ability to track particles at previously inaccessible angles toward the front and rear of the detector.

“This is the region where we expect the left-right directional preference to be larger,” Aschenauer said.

The upgrades include an inner Time Projection Chamber (iTPC), installed in 2019, which placed many more sensors in the inner sectors of the cylindrical STAR detector, close to the colliding particles. Then, earlier this year, the STAR team installed “forward” particle-tracking components outside one end of the detector.

To picture how these upgrades increase STAR’s particle tracking range, think of STAR as a barrel lying on its side with colliding particles entering at each end. Ever since RHIC’s first collisions in 2000, STAR has tracked particles emerging perpendicular to the colliding particles’ path all around the barrel. The classic end-on views of STAR particle tracks showcase this 360-degree detection capability. But looking from the side, the original STAR detector could only track particles emerging at angles up to 45 degrees off vertical in either the forward or rearward direction.

The upgrades “open wider the cone where the particles can go and be detected,” said Zhenyu Ye, a STAR collaborator from The University of Illinois-Chicago(US). Ye led the design and construction of the new silicon-based particle-tracking components installed at the forward end of STAR, working with scientists from The National Cheng Kung University [國立成功大學](TW) and Shandong University [山東大學](CN).

These components give scientists the ability to detect particles emerging almost in line with the colliding beams, including jets of particles that reveal information about the colliding quarks’ energy, direction, and spin.

“This information is essential for mapping the 3D arrangement of the proton’s inner building blocks,” said Chi Yang from Shandong University. Yang worked with colleagues from the The University of Electronic Science and Technology of China[电子科技大学](CN) and Brookhaven Lab to build additional subdetector systems for the forward tracking detector.

“These upgrades cover exactly the angles where jets would go in the EIC,” said Brookhaven Lab physicist Prashanth Shanmuganathan. So, in addition to increasing the data set for exploring the color charge interactions, “Run 22 will help us learn about the detector technology and the behavior of nucleon structure so we can apply that knowledge to the EIC.”

Cooling protons

Interspersed with delivering proton-proton collisions for STAR’s Run 22 measurements, the C-AD team will also spend the equivalent of two weeks’ time testing a technique for keeping high-energy protons tightly packed.

You’ll recall that keeping particles packed is important for maximizing collision rates and maintaining polarization. But particle spreading, or heating up, is a problem for all accelerated ion beams—from protons to uranium nuclei (the heaviest ions that have been collided at RHIC).

“There’s no natural shrinking of these ion beams; they never get denser by accident,” Schoefer said.

So RHIC accelerator physicists have developed a variety of successful techniques to keep ion beams “cool.” Some of these cooling methods involve delivering “kicks” to push particles closer together, while others literally use cool beams of other particles (electrons) to extract heat from circulating ions.

Realizing that different cooling techniques work best for different types of particles at different energies, physicists are exploring several strategies for possible use at the EIC. In Run 22 they’ll test something called “coherent electron cooling” (CeC) on high energy polarized protons.

Instead of just being cool in temperature, as described above, the negatively charged electrons in CeC play a more active role: They clump around each positively charged proton to create a “mold” of the proton beam.

“It’s a little bit like getting braces when the orthodontist takes a mold of your teeth,” Schoefer said. “We take a mold of the proton beam and then we adjust the electron beam slightly to attract the protons closer to a central position. As the electrons move, their electrical attraction drags the protons with them.”

In 36-hour stints, the C-AD physicists will test and try to fine-tune the technique.

Measuring ion polarization

In addition, every two weeks during Run 22, the C-AD team will stop proton acceleration for 12- to 16-hour stretches of accelerator R&D experiments. For one of these projects, they’ll ramp up beams of Helium-3 ions to work on methods for measuring the polarization of particles other than protons.

“In RHIC, the only polarized species we’ve ever had is polarized protons. But EIC will do experiments with polarized ions such as Helium-3. That’s an entirely different beast,” Schoefer said.

The C-AD team worked in collaboration with members of the “Cold-QCD” group in the Physics Department to design ways to measure the polarization of these more complicated ions.

To measure polarization, physicists spray a gas through the beam to act as a target, and measure how the particles in the beam scatter.

“For a proton, that’s already a challenge, but at least the proton stays a proton. When Helium-3 scatters off a target, it may break up into two protons and a neutron, or a proton and a deuteron. To accurately measure the polarization, we have to identify when breakup occurs,” said William Schmidke, a scientist in the physics department who’s been developing polarimetry detectors to make the measurements.

During Run 22, physicists will test the components’ ability to accurately characterize scattering products using unpolarized beams of Helium-3.

“We can do these tests, without measuring polarization, to develop the methods so we’ll be able to measure polarization when we eventually have polarized beams at the EIC,” said Brookhaven physicist Oleg Eyser, another member of the Cold-QCD team.

“Many people made important contributions to the detector and accelerator components needed for Run 22 at RHIC. We are looking forward to the exciting opportunities for physics discoveries and for advancing the technologies and physics analysis methods we will need for the EIC,” said Haiyan Gao, Brookhaven’s Associate Laboratory Director for Nuclear and Particle Physics.

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One of ten national laboratories overseen and primarily funded by the DOE(US) Office of Science, DOE’s Brookhaven National Laboratory (US) conducts research in the physical, biomedical, and environmental sciences, as well as in energy technologies and national security. Brookhaven Lab also builds and operates major scientific facilities available to university, industry and government researchers. The Laboratory’s almost 3,000 scientists, engineers, and support staff are joined each year by more than 5,000 visiting researchers from around the world. Brookhaven is operated and managed for DOE’s Office of Science by Brookhaven Science Associates, a limited-liability company founded by Stony Brook University(US), the largest academic user of Laboratory facilities, and Battelle(US), a nonprofit, applied science and technology organization.

Research at BNL specializes in nuclear and high energy physics, energy science and technology, environmental and bioscience, nanoscience and national security. The 5,300 acre campus contains several large research facilities, including the Relativistic Heavy Ion Collider [below] and National Synchrotron Light Source II [below]. Seven Nobel prizes have been awarded for work conducted at Brookhaven lab.

BNL is staffed by approximately 2,750 scientists, engineers, technicians, and support personnel, and hosts 4,000 guest investigators every year. The laboratory has its own police station, fire department, and ZIP code (11973). In total, the lab spans a 5,265-acre (21 km^2) area that is mostly coterminous with the hamlet of Upton, New York. BNL is served by a rail spur operated as-needed by the New York and Atlantic Railway. Co-located with the laboratory is the Upton, New York, forecast office of the National Weather Service.

Major programs

Although originally conceived as a nuclear research facility, Brookhaven Lab’s mission has greatly expanded. Its foci are now:

Nuclear and high-energy physics
Physics and chemistry of materials
Environmental and climate research
Nanomaterials
Energy research
Nonproliferation
Structural biology
Accelerator physics

Operation

Brookhaven National Lab was originally owned by the Atomic Energy Commission(US) and is now owned by that agency’s successor, the United States Department of Energy (DOE). DOE subcontracts the research and operation to universities and research organizations. It is currently operated by Brookhaven Science Associates LLC, which is an equal partnership of Stony Brook University(US) and Battelle Memorial Institute(US). From 1947 to 1998, it was operated by Associated Universities, Inc. (AUI) (US), but AUI lost its contract in the wake of two incidents: a 1994 fire at the facility’s high-beam flux reactor that exposed several workers to radiation and reports in 1997 of a tritium leak into the groundwater of the Long Island Central Pine Barrens on which the facility sits.

Foundations

Following World War II, the US Atomic Energy Commission was created to support government-sponsored peacetime research on atomic energy. The effort to build a nuclear reactor in the American northeast was fostered largely by physicists Isidor Isaac Rabi and Norman Foster Ramsey Jr., who during the war witnessed many of their colleagues at Columbia University leave for new remote research sites following the departure of the Manhattan Project from its campus. Their effort to house this reactor near New York City was rivalled by a similar effort at the Massachusetts Institute of Technology (US) to have a facility near Boston, Massachusettes(US). Involvement was quickly solicited from representatives of northeastern universities to the south and west of New York City such that this city would be at their geographic center. In March 1946 a nonprofit corporation was established that consisted of representatives from nine major research universities — Columbia University(US), Cornell University(US), Harvard University(US), Johns Hopkins University(US), Massachusetts Institute of Technology(US), Princeton University(US), University of Pennsylvania(US), University of Rochester(US), and Yale University(US).

Out of 17 considered sites in the Boston-Washington corridor, Camp Upton on Long Island was eventually chosen as the most suitable in consideration of space, transportation, and availability. The camp had been a training center from the US Army during both World War I and World War II. After the latter war, Camp Upton was deemed no longer necessary and became available for reuse. A plan was conceived to convert the military camp into a research facility.

On March 21, 1947, the Camp Upton site was officially transferred from the U.S. War Department to the new U.S. Atomic Energy Commission (AEC), predecessor to the U.S. Department of Energy (DOE).

Research and facilities

Reactor history

In 1947 construction began on the first nuclear reactor at Brookhaven, the Brookhaven Graphite Research Reactor. This reactor, which opened in 1950, was the first reactor to be constructed in the United States after World War II. The High Flux Beam Reactor operated from 1965 to 1999. In 1959 Brookhaven built the first US reactor specifically tailored to medical research, the Brookhaven Medical Research Reactor, which operated until 2000.

Accelerator history

In 1952 Brookhaven began using its first particle accelerator, the Cosmotron. At the time the Cosmotron was the world’s highest energy accelerator, being the first to impart more than 1 GeV of energy to a particle.

BNL Cosmotron 1952-1966

The Cosmotron was retired in 1966, after it was superseded in 1960 by the new Alternating Gradient Synchrotron (AGS).

BNL Alternating Gradient Synchrotron (AGS)

The AGS was used in research that resulted in 3 Nobel prizes, including the discovery of the muon neutrino, the charm quark, and CP violation.

In 1970 in BNL started the ISABELLE project to develop and build two proton intersecting storage rings.

The groundbreaking for the project was in October 1978. In 1981, with the tunnel for the accelerator already excavated, problems with the superconducting magnets needed for the ISABELLE accelerator brought the project to a halt, and the project was eventually cancelled in 1983.

The National Synchrotron Light Source (US) operated from 1982 to 2014 and was involved with two Nobel Prize-winning discoveries. It has since been replaced by the National Synchrotron Light Source II (US) [below].

BNL National Synchrotron Light Source (US).

After ISABELLE’S cancellation, physicist at BNL proposed that the excavated tunnel and parts of the magnet assembly be used in another accelerator. In 1984 the first proposal for the accelerator now known as the Relativistic Heavy Ion Collider (RHIC)[below] was put forward. The construction got funded in 1991 and RHIC has been operational since 2000. One of the world’s only two operating heavy-ion colliders, RHIC is as of 2010 the second-highest-energy collider after the Large Hadron Collider(CH). RHIC is housed in a tunnel 2.4 miles (3.9 km) long and is visible from space.

On January 9, 2020, It was announced by Paul Dabbar, undersecretary of the US Department of Energy Office of Science, that the BNL eRHIC design has been selected over the conceptual design put forward by DOE’s Thomas Jefferson National Accelerator Facility [Jlab] (US) as the future Electron–ion collider (EIC) in the United States.

Brookhaven Lab Electron-Ion Collider (EIC) (US) to be built inside the tunnel that currently houses the RHIC.

In addition to the site selection, it was announced that the BNL EIC had acquired CD-0 from the Department of Energy. BNL’s eRHIC design proposes upgrading the existing Relativistic Heavy Ion Collider, which collides beams light to heavy ions including polarized protons, with a polarized electron facility, to be housed in the same tunnel.

Other discoveries

In 1958, Brookhaven scientists created one of the world’s first video games, Tennis for Two. In 1968 Brookhaven scientists patented Maglev, a transportation technology that utilizes magnetic levitation.

Major facilities

Relativistic Heavy Ion Collider (RHIC), which was designed to research quark–gluon plasma and the sources of proton spin. Until 2009 it was the world’s most powerful heavy ion collider. It is the only collider of spin-polarized protons.

Center for Functional Nanomaterials (CFN), used for the study of nanoscale materials.

BNL National Synchrotron Light Source II(US), Brookhaven’s newest user facility, opened in 2015 to replace the National Synchrotron Light Source (NSLS), which had operated for 30 years. NSLS was involved in the work that won the 2003 and 2009 Nobel Prize in Chemistry.

Alternating Gradient Synchrotron, a particle accelerator that was used in three of the lab’s Nobel prizes.
Accelerator Test Facility, generates, accelerates and monitors particle beams.
Tandem Van de Graaff, once the world’s largest electrostatic accelerator.

Computational Science resources, including access to a massively parallel Blue Gene series supercomputer that is among the fastest in the world for scientific research, run jointly by Brookhaven National Laboratory and Stony Brook University-SUNY (US).

Interdisciplinary Science Building, with unique laboratories for studying high-temperature superconductors and other materials important for addressing energy challenges.
NASA Space Radiation Laboratory, where scientists use beams of ions to simulate cosmic rays and assess the risks of space radiation to human space travelers and equipment.

Off-site contributions

It is a contributing partner to the ATLAS experiment, one of the four detectors located at the Large Hadron Collider (LHC).

European Organization for Nuclear Research (Organisation européenne pour la recherche nucléaire)(EU) [CERN] map

Iconic view of the European Organization for Nuclear Research [Organisation européenne pour la recherche nucléaire](CH)CERN ATLAS detector.

It is currently operating at The European Organization for Nuclear Research [Organisation européenne pour la recherche nucléaire] [Europäische Organisation für Kernforschung](CH) [CERN] near Geneva, Switzerland.

Brookhaven was also responsible for the design of the SNS accumulator ring in partnership with Spallation Neutron Source at DOE’s Oak Ridge National Laboratory (US), Tennessee.

DOE’s Oak Ridge National Laboratory(US) Spallation Neutron Source annotated.

Brookhaven plays a role in a range of neutrino research projects around the world, including the Daya Bay Neutrino Experiment (CN) nuclear power plant, approximately 52 kilometers northeast of Hong Kong and 45 kilometers east of Shenzhen, China.

Daya Bay Neutrino Experiment (CN) nuclear power plant, approximately 52 kilometers northeast of Hong Kong and 45 kilometers east of Shenzhen, China

FNAL DUNE LBNF (US) from FNAL to Sanford Underground Research Facility, Lead, South Dakota, USA

BNL Center for Functional Nanomaterials.

BNL National Synchrotron Light Source II(US).

BNL NSLS II (US).

BNL Relative Heavy Ion Collider (US) Campus.

BNL/RHIC Star Detector.

BNL/RHIC Phenix detector.