STAR Detector at Relativistic Heavy Ion Collider

The STAR detector (for Solenoidal Tracker at RHIC) is one of the four experiments at the

Relativistic Heavy Ion Collider The Relativistic Heavy Ion Collider (RHIC ) is the first and one of only two operating heavy-ion colliders, and the only spin-polarized proton collider ever built. Located at Brookhaven National Laboratory (BNL) in Upton, New York, and used by an ...

(RHIC) in Brookhaven National Laboratory, United States.STAR Lite, education and outreach
/ref> The primary scientific objective of STAR is to study the formation and characteristics of the quark–gluon plasma (QGP), a state of matter believed to exist at sufficiently high energy densities. Detecting and understanding the QGP allows physicists to understand better the Universe in the seconds after the

Big Bang The Big Bang event is a physical theory that describes how the universe expanded from an initial state of high density and temperature. Various cosmological models of the Big Bang explain the evolution of the observable universe from the ...

, when the presently-observed symmetries (and asymmetries) of the Universe were established. Unlike other physics experiments where a theoretical prediction can be tested directly by a single measurement, STAR must make use of a variety of simultaneous studies in order to draw strong conclusions about the QGP. This is due both to the complexity of the system formed in the high-energy nuclear collision and the unexplored landscape of the physics studied. STAR therefore consists of several types of detectors, each specializing in detecting certain types of particles or characterizing their motion. These detectors work together in an advanced data acquisition and subsequent physics analysis that allows definitive statements to be made about the collision.

The physics of STAR

In the immediate aftermath of the

, the expanding matter was so hot and dense that protons and neutrons could not exist. Instead, the early universe comprised a plasma of

quarks A quark () is a type of elementary particle and a fundamental constituent of matter. Quarks combine to form composite particles called hadrons, the most stable of which are protons and neutrons, the components of atomic nuclei. All commonly o ...

and gluons, which in today's cool universe are confined and exist only within composite particles (bound states) – the hadrons, such as protons and neutrons. Collisions of heavy nuclei at sufficiently high energies allow physicists to study whether quarks and gluons become deconfined at high densities, and if so, what the properties of this matter (i.e. quark–gluon plasma) are. In particular, STAR studies the collective expansion of the hot quark-gluon matter, such as the

elliptic flow Relativistic heavy-ion collisions produce very large numbers of subatomic particles in all directions. In such collisions, ''flow'' refers to how energy, momentum, and number of these particles varies with direction, and elliptic flow is a measure ...

. This allows to extract the transport coefficients that characterize the quark-gluon matter, including the shear and bulk

viscosity The viscosity of a fluid is a measure of its resistance to deformation at a given rate. For liquids, it corresponds to the informal concept of "thickness": for example, syrup has a higher viscosity than water. Viscosity quantifies the inte ...

, and to investigate

macroscopic quantum phenomena Macroscopic quantum phenomena are processes showing quantum behavior at the macroscopic scale, rather than at the atomic scale where quantum effects are prevalent. The best-known examples of macroscopic quantum phenomena are superfluidity and sup ...

, such as the

chiral magnetic effect Chiral magnetic effect (CME) is the generation of electric current along an external magnetic field induced by chirality imbalance. Fermions are said to be chiral if they keep a definite projection of spin quantum number on momentum. The CME is a ...

Collaboration governance

The governance of STAR is via two branches: the institutional Council which is run by a Chairperson elected from the Council ranks, and elected Spokesperson(s) and their management team. The Spokesperson(s) represent the Collaboration in scientific, technical, and managerial concerns. The Council deals with general issues that concern the collaboration. Examples include the organization and governance of the Collaboration, adoption of bylaws and amendments thereto, the policy on admission of new members institutions to the Collaboration, and Policies for the Publication and Presentation of STAR Results. The term of the office of the Council Chair is nominally two years. The Council elects, a Spokesperson or a team of two Spokespersons who then serve at the discretion of the Council. The normal term of office for the Spokesperson(s) is 3 years, and an individual is eligible to serve at most two consecutive terms as Spokesperson(s). The elected Spokesperson(s) and their team of Deputies, and the Council Chairs of STAR are listed below. The Institute listed indicates the institute the person was at when they held the position.

Spokespersons

* 2020–present Spokespeople :

Helen Caines Helen Louise Caines is a Professor of Physics at Yale University. She studies the quark–gluon plasma and is the co-spokesperson for the STAR experiment. Education Caines studied physics at the University of Birmingham and graduated in 1992. ...

(Yale), Lijuan Ruan (BNL) ** Deputies: Kenneth Barish (UC Riverside), Xin Dong (LBNL) * 2017–2020 Spokespeople : Helen Caines (Yale), Zhangbu Xu (BNL) ** Deputies: Jim Drachenberg (ACU), Frank Geurts (Rice) * 2014–2017 : Zhangbu Xu (BNL) ** Deputies : Helen Caines (Yale), Renee Fatemi (UTK), Ernst Sichtermann (LBNL) * 2011–2014 : Nu Xu (LBNL) ** Deputies: James Dunlop (BNL), Bedangadas Mohanty (VECC/NISER), Scott Wissink (Indiana) * 2008–2011: Nu Xu (LBNL) ** Deputies : James Dunlop (BNL),

Olga Evdokimov Olga Evdokimov is a Russian born professor of physics at the University of Illinois, Chicago (UIC). She is a High Energy Nuclear Physicist, who currently collaborates on two international experiments; the Solenoidal Tracker At RHIC (STAR) experi ...

(UIC), Berndt Surrow (MIT) * 2005–2008 : Tim Hallman (BNL) ** Deputies : Carl Gagliardi (Texas A&M), Hans Georg Ritter (LBNL), Helen Caines (Yale) (2007 - 2008) * 2002–2005 : Tim Hallman (BNL) ** Deputies : Jim Thomas (LBNL), Steven Vigdor (Indiana) * 1991–2002 : John Harris (Yale) ** Deputies : Rene Bellwied (Wayne State) (2001-2002), Tim Hallman (BNL) (1999-2000)

Council Chairpersons

* 2021–present : Jana Bielcikova (NPI, CAS) * 2016–2021 : Olga Evdokimov (UIC) * 2014–2016 : Huan Huang (UCLA) * 2009–2014 : Gary Westfall (MSU) * 2005–2008 : Hank Crawford (UC Berkeley) * 2003–2005 : Bill Christie (BNL) * 2000–2003 : Jay Marx (LBNL)

References

{{reflist

External Links

STAR experiment
record on

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