The Physics and Detectors of the Relativistic Heavy Ion Collider (RHIC).

The Physics and Detectors of the Relativistic Heavy Ion Collider (RHIC).
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Total Pages: 5
Release: 1996
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In mid-1999 the Relativistic Heavy Ion Collider (RHIC) facility will begin accelerating 197Au nuclei to 100 A GeV. The effective temperature in the dense region of overlap when two nuclei collide nearly head on at this energy will reach 1012 degrees Kelvin. At this temperature a basic restructuring of matter is expected to occur, in which the quark and gluon constituents normally confined in hadronic matter form a chirally symmetric deconfined plasma. There are many signatures to help isolate evidence of a transition to a deconfined phase of matter. These include, for example: (1) strangeness saturation on a time scale too short to be accounted for by strangeness exchange interactions in a hadron gas, (2) color screening (vector meson suppression) in the plasma phase, (3) in-medium effects on the mass/lifetime of the vector mesons, (4) the observation of thermodynamic/chemical equilibrium, (5) thermal radiation from a hot plasma, (6) excess heavy flavor production, (7) a discontinuity or change in the correlation between energy density and entropy density, (8) the observation of a long hadronization time, (9) disoriented chiral condensate behavior (isospin or low pt correlations). Each of the RHIC detectors is optimized for the measurement of a number of the above signatures. It is therefore possible because of the very high particle densities at RHIC for these detectors to correlate multiple observables in a single event or in a sample of events. It will thus be possible to isolate events which exhibit correlated non-statistical fluctuations in several observables simultaneously. It will be possible at RHIC to make a self-consistent measurement of the initial conditions, and in particular the gluon distribution in the nucleus. This affords optimal use of perturbative QCD in providing guidance as to the evolution of the early stages of the collision. We review the design and capabilities of the four detectors at RHIC: BRAHMS, PHENIX, PHOBOS, and STAR.

Fourth Workshop on Experiments and Detectors for a Relativistic Heavy Ion Collider

Fourth Workshop on Experiments and Detectors for a Relativistic Heavy Ion Collider
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Total Pages: 442
Release: 1990
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This report contains papers on the following topics: physics at RHIC; flavor flow from quark-gluon plasma; space-time quark-gluon cascade; jets in relativistic heavy ion collisions; parton distributions in hard nuclear collisions; experimental working groups, two-arm electron/photon spectrometer collaboration; total and elastic pp cross sections; a 4[pi] tracking TPC magnetic spectrometer; hadron spectroscopy; efficiency and background simulations for J/[psi] detection in the RHIC dimuon experiment; the collision regions beam crossing geometries; Monte Carlo simulations of interactions and detectors; proton-nucleus interactions; the physics of strong electromagnetic fields in collisions of relativistic heavy ions; a real time expert system for experimental high energy/nuclear physics; the development of silicon multiplicity detectors; a pad readout detector for CRID/tracking; RHIC TPC R D progress and goals; development of analog memories for RHIC detector front-end electronic systems; calorimeter/absorber optimization for a RHIC dimuon experiment; construction of a highly segmented high resolution TOF system; progress report on a fast, particle-identifying trigger based on ring-imaging and highly integrated electronics for a TPC detector.

The Physics and Experimental Program of the Relativistic Heavy Ion Collider (RHIC).

The Physics and Experimental Program of the Relativistic Heavy Ion Collider (RHIC).
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Release: 2005
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The primary motivation for studying nucleus-nucleus collisions at relativistic and ultrarelativistic energies is to investigate matter at high energy densities ([var-epsilon] [much-gt] 1 GeV/fm[sup 3]). Early speculations of possible exotic states of matter focused on the astrophysical implications of abnormal states of dense nuclear matter. Field theoretical calculations predicted abnormal nuclear states and excitation of the vacuum. This generated an initial interest among particle and nuclear physicists to transform the state of the vacuum by using relativistic nucleus-nucleus collisions. Extremely high temperatures, above the Hagedorn limiting temperature, were expected and a phase transition to a system of deconfined quarks and gluons, the Quark-Gluon Plasma (QGP), was predicted. Such a phase of matter would have implications for both early cosmology and stellar evolution. The understanding of the behavior of high temperature nuclear matter is still in its early stages. However, the dynamics of the initial stages of these collisions, which involve hard parton-parton interactions, can be calculated using perturbative QCD. Various theoretical approaches have resulted in predictions that a high temperature (T [approximately] 500 MeV) gluon gas will be formed in the first instants (within 0.3 fm/c) of the collision. Furthermore, QCD lattice calculations exhibit a phase transition between a QGP and hadronic matter at a temperature near 250 MeV. Such phases of matter may have existed shortly after the Big Bang and may exist in the cores of dense stars. An important question is whether such states of matter can be created and studied in the laboratory. The Relativistic Heavy Ion Collider (RHIC) and a full complement of detector systems are being constructed at Brookhaven National Laboratory to investigate these new and fundamental properties of matter.

Introduction To Relativistic Heavy Ion Physics

Introduction To Relativistic Heavy Ion Physics
Author: Bartke Jerzy
Publisher: World Scientific
Total Pages: 240
Release: 2008-12-22
Genre:
ISBN: 9813104562

This book attempts to cover the fascinating field of physics of relativistic heavy ions, mainly from the experimentalist's point of view. After the introductory chapter on quantum chromodynamics, basic properties of atomic nuclei, sources of relativistic nuclei, and typical detector set-ups are described in three subsequent chapters. Experimental facts on collisions of relativistic heavy ions are systematically presented in 15 consecutive chapters, starting from the simplest features like cross sections, multiplicities, and spectra of secondary particles and going to more involved characteristics like correlations, various relatively rare processes, and newly discovered features: collective flow, high pT suppression and jet quenching. Some entirely new topics are included, such as the difference between neutron and proton radii in nuclei, heavy hypernuclei, and electromagnetic effects on secondary particle spectra.Phenomenological approaches and related simple models are discussed in parallel with the presentation of experimental data. Near the end of the book, recent ideas about the new state of matter created in collisions of ultrarelativistic nuclei are discussed. In the final chapter, some predictions are given for nuclear collisions in the Large Hadron Collider (LHC), now in construction at the site of the European Organization for Nuclear Research (CERN), Geneva. Finally, the appendix gives us basic notions of relativistic kinematics, and lists the main international conferences related to this field. A concise reference book on physics of relativistic heavy ions, it shows the present status of this field.

Physics with the STAR Detector at RHIC.

Physics with the STAR Detector at RHIC.
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Total Pages: 12
Release: 1998
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The Relativistic Heavy Ion Collider (RHIC) at Brookhaven National Laboratory will collide beams of nuclei (as light as protons and as heavy as gold) at energies of up to 200 GeV per nucleon. At these energies, the probability of detecting a phase transition to a state of matter where quarks and gluons are not confined to nucleons is large. (The nuclear densities are approaching nucleon densities) Additionally, the collision is occurring in a kinematic regime where perturbative QCD is expected to be reliable. I discuss the capabilities of the STAR detector at RHIC and a subset of the physics program the STAR collaboration hopes to undertake with this detector.

Exploring New Frontiers in Nuclear and Particle Physics with the STAR Detector at RHIC.

Exploring New Frontiers in Nuclear and Particle Physics with the STAR Detector at RHIC.
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Total Pages: 17
Release: 1996
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The Solenoidal Tracker At RHIC (STAR) is a large acceptance collider detector scheduled to begin operation at the Relativistic Heavy Ion Collider (RHIC) at Brookhaven National Laboratory in the fall of 1999. In the sections which follow, details of the STAR detector and physics program, as well as the status of the RHIC construction project will be presented.

High Energy Heavy Ion Collisions and the RHIC (Relativistic Heavy Ion Collider) Project at Brookhaven

High Energy Heavy Ion Collisions and the RHIC (Relativistic Heavy Ion Collider) Project at Brookhaven
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Total Pages: 9
Release: 1989
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The most spectacular of the new high energy approaches to nuclear physics is the field of relativistic heavy ion collisions, for which it is anticipated that construction of the Relativistic Heavy Ion Collider (RHIC) facility will begin soon. Here the goal is to subject large volumes of nuclear matter to such extreme conditions of temperature and pressure that a new form of matter is produced in which the recognizable components are not the familiar neutrons and protons, but are quarks. This paper discusses the RHIC project of the experiments and detectors associated with it. 10 refs., 4 figs.

Physics with the Collider Detectors at RHIC and the LHC.

Physics with the Collider Detectors at RHIC and the LHC.
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Total Pages: 212
Release: 1995
Genre:
ISBN:

On January 8, 1995, over 180 participants gathered to hear the QM95 preconference workshop on 'Physics with the Collider Detectors at RHIC and the LHC'. The goal was to bring together the experimentalists from a wide community of hadron and heavy ion collider detector collaborations. The speakers were encouraged to present the current status of their detectors, with all the blemishes, and the audience was encouraged to share their successes and failures in approaching similar detector design issues. The presentations were excellent and the discussions were lively and stimulating. The editors hope that the reader will find these proceedings to be equally stimulating. Separate abstracts have been submitted to the energy database from articles in this report.