Rice University logo
 
Top blue bar image
Home of the Particle and Nuclear Physics groups at Rice University
 

Posts Tagged ‘STAR’


NPP Seminar by Isaac Upsal (BNL)

April 27th, 2021 by geurts

Date: Tuesday April  27, 2021 at 4pm
Location: online

Title: Exploring the Frontier of Vorticity in Heavy-ion Collisions
Speaker: Isaac Upsal (BNL)

Abstract

In accelerators like RHIC, heavy atomic nuclei are collided at high energies to study emergent properties of the strong-nuclear force. At high-enough energies with heavy-enough nuclei such collisions create a short-lived novel fluid of deconfined quarks and gluons called the “Quark Gluon Plasma”. Because the nuclei themselves are so large, the transverse size of the nuclear overlap is a variable of significance to the field. Collisions with large impact parameters (low degree of overlap) have large angular momentum (~1000 hbar). For a collision which takes a finite amount of time one would expect an excess of particles with spin along the direction of system angular momentum due to spin-orbit coupling.

In 2017 STAR reported the first non-trivial measurement of this alignment, called the global polarization, at the order of a few percent (https://doi.org/10.1038/nature23004). In a thermalized fluid this polarization would come about through a vorticity. Using such a framework it’s possible to extract a vorticity on the order of 10^22 s^-1, which is notably higher than any previously known fluid. This measurement renewed interest in this physics within the heavy-ion physics community and there have been a number of interesting new calculations as well as measurements from STAR, ALICE, and HADES. I plan on discussing this measurement, newer developments, and the future of similar measurements.

NPP Seminar by Shuai Yang (BNL)

January 8th, 2019 by geurts

Date: Thursday Jan. 17, 2019 at 3pm
Location: 223 Herman Brown Hall, Rice University

Title: Measurements of photon interactions in hadronic heavy-ion collisions at STAR
Speaker: Shuai Yang (BNL)

Abstract

Photon-photon and photonuclear interactions can be induced by the strong electromagnetic fields arising from relativistic heavy ions. These two types of interactions are conventionally studied in ultra-peripheral collisions (UPC). The ALICE collaboration has observed a significant excess of $J/\psi$ yields at low transverse momenta ($p_T$) in peripheral Pb+Pb collisions, which can be qualitatively explained by coherent photonuclear production mechanism. Such an explanation implies that photon-photon interactions would be also measurable and contribute to the $l^+l^-$ pair production in hadronic heavy-ion collisions. Since the nuclei break up in peripheral heavy-ion collisions unlike in the UPCs, it is non-trivial to incorporate the coherence condition for the aforementioned photon interactions in such collisions. Measurements of $J/\psi$ and $e^+e^-$ pair productions at very low $p_T$ for different collision systems and energies, discussed in this talk, are thus important to verify and further understand photon interactions and their possible impacts on emerging phenomena in hadronic heavy-ion collisions.

NPP Seminar by Zaochen Ye (UIC)

September 7th, 2018 by geurts

Date: Thursday Sept. 13, 2018  at 4pm
Location: 223 Herman Brown Hall, Rice University

Title: Quarkonium Measurements in p+p, p+Au and Au+Au Collisions at √sNN=200 GeV with the STAR Experiment
Speaker: Zaochen Ye (UIC)

Abstract

Measurements of quarkonium production are an important tool to study the properties of the Quark-Gluon Plasma (QGP) formed in relativistic heavy-ion collisions. Quarkonium suppression due to the color-screening effect was proposed as a direct evidence of the QGP formation. However, other effects, such as cold nuclear matter effects and regeneration, add additional complications to the interpretation of the observed suppression. Different quarkonium states with different binding energies are expected to dissociate at different temperatures, and therefore measurement of this “sequential melting” can help constrain the temperature of the medium. In this seminar, I will present and discuss the latest measurements of quarkonium (J/psi and Upsilon) production in p+p, p+Au and Au+Au collisions at √sNN = 200 GeV with the STAR experiment.

Frank Geurts appointed Deputy Spokesperson STAR Collaboration

July 17th, 2017 by geurts

Frank Geurts, associate professor of physics and astronomy, has been appointed deputy spokesperson for the STAR Collaboration, a group of more than 600 high-energy nuclear physicists from 63 institutes in 13 countries. The collaboration conducts research at the Relativistic Heavy Ion Collider (RHIC) at the U.S. Department of Energy’s Brookhaven National Laboratory in Upton, N.Y. STAR refers to the Solenoid Tracker at RHIC, one of the largest and most sophisticated experiments at the Long Island particle collider.

 

taken from: Rice News

NPP Seminar by Daniel Cebra (UC Davis)

March 9th, 2017 by geurts

Date: Friday, March 9, 2017  at 4pm
Location: 223 Herman Brown Hall, Rice University

Title: Studying The Phase Diagram Of Qcd Matter: The Beam Energy Scan Program At RHIC
Speaker: Daniel Cebra (UC Davis)

Abstract: As nuclear matter is compressed and heated to extreme temperatures, eventually a point is reached where the quarks and gluons are no longer bound within their hadrons but are instead constituents of a larger mass of deconfined matter, a QCD plasma. This matter interacts through the bare color force. Theoretical studies of the properties of matter require Lattice QCD. The current understanding is that the nature of the transition from a state of hot hadronic gas to a plasma depends on the baryon chemical potential, which is a measure of the ratio of quarks to anti-quarks. A cross-over transition is expected at low baryon chemical potential, while at high baryon chemical potential the transition is expected to be first order. A systematic study of heavy-ion collisions across a broad range of beam energy can create QCD plasma with a broad spectrum of chemical potentials. The RHIC facility has embarked on such a study to try to experimentally map out the nature of the QCD phase diagram. Follow-up studies are planned in 2019 and 2020. The energy range of this follow-up scan can be extended with a fixed-target program.

 

NPP Seminar by Hongwei Ke (BNL)

February 16th, 2017 by geurts

Date: Thursday, February 23, 2017  at 4pm
Location: 223 Herman Brown Hall, Rice University

Title: STAR High Level Trigger
Speaker: Hongwei Ke (BNL)
Abstract: We implemented a High-Level Trigger (HLT) system for the STAR experiment to better utilize the luminosity delivered by RHIC. By reconstructing tracks and assembling data from multiple detectors, STAR HLT can select events of great physics interests online, which will reduce the data volume to tape, speed up offline physics analysis and provide vital online monitoring information. In the past a few years, a series of important physics achievements and programs of STAR have benefited from HLT, including the discovery of anti-alpha particles, the first J/\Psi elliptic flow measurement, the Beam Energy Scan program phase I and more recently the STAR heavy flavor tracker and muon telescope detector program. Currently, STAR HLT has 10 times of the computing resources than we had in 2012, which contains about 1200 CPU cores and 45 Xeon Phi (KNC) coprocessors. In this talk, I will discuss the development of STAR HLT, lessons we learned of using such a heterogeneous system and most importantly the physics opportunities opened with these resources.

NPP Seminar by Li Yi (Yale)

February 1st, 2017 by geurts

Date: Thursday, February 16, 2017  at 2pm
Location: 223 Herman Brown Hall, Rice University

Title:Underlying-event Activity in Proton+Proton Collisions at
sqrt(s_NN) = 200GeV with the STAR Detector at RHIC
Speaker: Li Yi (Yale)
Abstract: Underlying-event activity is defined as the soft particle production
in proton+proton collisions which is not directly related to the final
fragmentation of hard-scattered partons. Underlying-event measurements
therefore provide a tool to study non-factorizable and
non-perturbative phenomena. Systematic measurements of the
relationship between the underlying event and jet processes  are
crucial for a complete description of both soft and hard QCD processes
at hadron colliders and for Monte Carlo modeling. In this talk, we
will report the progress of underlying-event measurements in
proton+proton collisions at RHIC by STAR and its comparison with Monte
Carlo tuning. The comparison between RHIC and LHC energy
underlying-event activities will also be discussed.

P&A Colloquium: Mike Lisa (OSU)

March 7th, 2016 by geurts

Date: Wednesday March 16, 2016  at 4pm
Location: 101 Brockman Hall, Rice University

Title:FROM THE STARS TO STAR: Intensity Interferometry from HBT to Heavy Ions
Speaker: Mike Lisa (OSU)
Abstract: Sixty years ago, two radio engineers emerged from the frenzy of World War II and entered the new field of radio astronomy. Hanbury Brown and Twiss developed an entirely new instrument and technique, based on “correlated noise,” to measure the angular radius of previously un-resolvable stars. Initially greeted with skepticism, their work led directly to the birth of quantum optics. At nearly the same time, Goldhaber et al discovered a tiny unexpected correlation in the first true particle physics experiments; until recently, the “GGLP effect” played a minor role in particle physics. It would take another 15 years until the connection between these apparently disparate phenomena was realized by Shuryak, Gyulassy and others around 1976, just as the new field of heavy ion physics was emerging. Thus did Hanbury Brown’s discovery give birth to femtoscopy, the most direct method to probe the highly non-trivial dynamic space-time structure of a heavy ion collision. I will discuss the structures and insights that femtoscopy has revealed in ultra-relativistic ion collisions at RHIC and the LHC and how it is leading to a fresh look at high-energy proton collisions

Ph.D. Thesis Defense Kefeng Xin

November 23rd, 2015 by geurts

 

Date & Time: November  23, 2015 at 1pm-4pm
Location: 300 Brockman Hall for Physics

Abstract: Dileptons, e.g. dimuons, have been proved to be very important tools to explore the hot and dense matter created at heavy-ion collider experiments. The first dimuon excess observation at the STAR experiment from Au + Au collisions at sqrt(sNN) = 200 GeV/c will be presented. Muonic atoms are bound hadron-muon states. In ultrarelativistic heavy-ion experiments, muonic atoms can be a perfect tool to access the muon thermal emission of a hot quantum chromodynamics (QCD) system as only thermal muons or muons from short-lived resonances are able to form muonic atoms. Among muonic atoms, the antimatter muonic hydrogen and the hyper-muonic atom, K^0_L, have been predicted but not yet discovered. STAR’s first measurement of muonic atom production will be presented.

Antimatter not so different after all

November 4th, 2015 by geurts

reproduced from Rice News

Rice University scientists help make first measurement of antiproton attraction.

Due to the diligence of a Rice University student and his calculations, humanity now knows a little more about the universe.

Kefeng Xin, a graduate student at Rice, is one of a handful of primary authors who revealed evidence this week that the attractive force between antiprotons is similar to that between protons — and measured it.

Specifically, the team measured two important parameters: the scattering length and the effective range of interaction between two antiprotons. This gave scientists a fundamental new way to understand the force that holds together the nuclei in antimatter and how this compares to matter.

“This is about the subtle difference in the way matter and antimatter interact with each other,” said Rice physicist Frank Geurts.

Rice University physicist Frank Geurts, left, and graduate student Kefeng Xin are part of the team that made the first measurements of the attractive force between antiprotons. Xin is a primary author of the paper that appears this week in Nature. Photo by Jeff Fitlow

Antiprotons carry the opposite electrical charge and spin that protons do. Like all matter and antimatter, both were created at the instant of the Big Bang. Physicists are still trying to understand why they see so few antiparticles in nature even though particles and antiparticles were produced in equal amounts and annihilate each other on contact.

“It could have been that antimatter didn’t have the same attractive force as matter and would have helped explain how these differences, during the initial part of the Big Bang, might have resulted in antimatter not having survived in the shape of stars and planets, as matter did,” Geurts said.

“That’s where this research is helpful. The interactions between two antimatter particles turn out to be quite similar to matter particles. It may not give us a solution to the bigger problem, but we most definitely removed one option,” he said.

The find was reported in Nature on behalf of the more than 500 scientists, including Geurts, who work on the STAR experiment, part of the Relativistic Heavy Ion Collider (RHIC) at the U.S. Department of Energy’s Brookhaven National Laboratory. Brookhaven’s story on the discovery appears here.

The scattering length is a measurement of how particles deviate as they travel from source to destination; their paths are visible as three-dimensional traces captured by STAR (which is short for Solenoid Tracker at RHIC). The effective range indicates how close particles need to be for their charges to influence each other, like magnets.

Both are measured in femtometers. One femtometer is one-millionth of a nanometer; a nanometer is one-billionth of a meter.

For antiprotons measured at RHIC, the scattering length was roughly 7.41 femtometers, and the effective range was 2.14 femtometers, nearly equivalent to their proton counterparts. Measuring distances that small involves both sophisticated equipment and sophisticated calculations.

Scientists working at Brookhaven National Laboratory, including physicists at Rice, have announced the first measurements of the attractive force between antiprotons.

Scientists working at Brookhaven National Laboratory, including physicists at Rice, have announced the first measurements of the attractive force between antiprotons. The discovery gives physicists new ways to look at the forces that bind matter and antimatter. Courtesy of Brookhaven National Laboratory

“This discovery isn’t a surprise,” said Xin, whose Ph.D. thesis focuses on rather exotic systems called muonic atoms. “We’ve been studying the interaction between nucleons (particles that make up an atom’s nucleus) for decades, and we’ve always thought the forces between antimatter particles are the same as for matter. But this is the first time we’ve been able to quantify it.”

Xin, a student of Geurts, applied methods developed in his thesis to the analysis. The first task was to determine which particles produced in a collision were indeed antiprotons and whether any two were in close enough proximity to influence each other. Then came correlating their momentum from creation to destruction, typically a few nanoseconds.

“All of the data we collected in 2011 is from 500 million events (collisions between two heavy gold ions),” Xin said. “Pretty much every event can contribute.”

Antimatter can be created in small amounts with a collider like RHIC and analyzed. The collider accelerates the nuclei of heavy atoms to nearly the speed of light and smashes them together to produce elemental particles, antiparticles and exotic materials like quarks, muons and plasmas. All of these can be characterized by tools built at Rice and elsewhere as part of STAR.

RHIC smashed gold ions to produce hundreds of millions of particles, which can be detected by the ionization traces they leave in a gas-filled cylinder that surrounds the collision and a “time-of-flight” sensor. The instrument, the construction of which was led by Rice, tells researchers how many nanoseconds it takes particles to travel from the point of impact to sensors at the outer boundaries of the collider.

“RHIC is ideal for this kind of experiment because it allows us to dump a boatload of energy into a very small volume and have many particles come out of it,” Geurts said. “The multiplicity is important. If you don’t make a lot of particles, the odds of having them interact with each other is slim.”

Researchers from 52 institutions that are part of the STAR collaboration are co-authors of the Nature paper. Rice co-authors include graduate students Daniel Brandenburg, Joey Butterworth and Nick Luttrell; research scientist Geary Eppley; and Pablo Yepes, a senior faculty fellow in physics and astronomy. Geurts is an associate professor of physics and astronomy.

The research is funded primarily by the Department of Energy Office of Science.

– See more at: http://news.rice.edu/2015/11/04/antimatter-not-so-different-after-all-2/#sthash.MJ7A84cH.dpuf