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 ...

(RHIC) in

Brookhaven National Laboratory Brookhaven National Laboratory (BNL) is a United States Department of Energy national laboratories, United States Department of Energy national laboratory located in Upton, New York, a hamlet of the Brookhaven, New York, Town of Brookhaven. It w ...

, 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 Quark–gluon plasma (QGP or quark soup) is an interacting localized assembly of quarks and gluons at Thermodynamic equilibrium#Local and global equilibrium, thermal (local kinetic) and (close to) chemical (abundance) equilibrium. The word ''plasm ...

(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 is a physical theory that describes how the universe expanded from an initial state of high density and temperature. Various cosmological models based on the Big Bang concept explain a broad range of phenomena, including th ...

, 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 A gluon ( ) is a type of massless elementary particle that mediates the strong interaction between quarks, acting as the exchange particle for the interaction. Gluons are massless vector bosons, thereby having a spin of 1. Through the s ...

. In today's cool universe, quarks and gluons are confined and exist only within composite particles (bound states) – the

hadrons In particle physics, a hadron is a composite subatomic particle made of two or more quarks held together by the strong nuclear force. Pronounced , the name is derived . They are analogous to molecules, which are held together by the electric ...

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

viscosity Viscosity is a measure of a fluid's rate-dependent drag (physics), resistance to a change in shape or to movement of its neighboring portions relative to one another. For liquids, it corresponds to the informal concept of ''thickness''; for e ...

, and to investigate

macroscopic quantum phenomena Macroscopic quantum phenomena are processes showing Quantum mechanics, quantum behavior at the macroscopic scale, rather than at the Atom, atomic scale where quantum effects are prevalent. The best-known examples of macroscopic quantum phenomena ar ...

, such as the chiral magnetic effect.

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

* 2023-present Spokespeople : Frank Geurts (Rice), Lijuan Ruan (BNL) ** Deputies: ShinIchi Esumi (Tsukuba), Qinghua Xu (Shandong) * 2020–2023 Spokespeople : Helen Caines (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 (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 Bielčíková (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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