Results from RHIC with Implications for LHC
Book
·
OSTI ID:989746
High energy nucleus-nucleus collisions provide the means of creating nuclear matter in conditions of extreme temperature and density. The kinetic energy of the incident projectiles would be dissipated in the large volume of nuclear matter involved in the reaction. At large energy or baryon density, a phase transition is expected from a state of nucleons containing confined quarks and gluons to a state of 'deconfined' (from their individual nucleons) quarks and gluons, in chemical and thermal equilibrium, covering a volume that is many units of the confining length scale. This state of nuclear matter was originally given the name Quark Gluon Plasma (QGP), a plasma being an ionized gas. However the results at RHIC indicated that instead of behaving like a gas of free quarks and gluons, the matter created in heavy ion collisions at nucleon-nucleon c.m. energy {radical}s{sub NN} = 200 GeV appears to be more like a liquid. This matter interacts much more strongly than originally expected, as elaborated in peer reviewed articles by the 4 RHIC experiments, which inspired the theorists to give it the new name 'sQGP' (strongly interacting QGP).
- Research Organization:
- Brookhaven National Laboratory (BNL) Relativistic Heavy Ion Collider
- Sponsoring Organization:
- Doe - Office Of Science
- DOE Contract Number:
- AC02-98CH10886
- OSTI ID:
- 989746
- Report Number(s):
- BNL--93946-2010-BC; KB0201021
- Country of Publication:
- United States
- Language:
- English
Similar Records
RHIC and the QGP at 10: from the 'age of discovery' to the 'age of exploration'
Heavy Ion Physics at RHIC
Looking for quark-gluon plasma with strange hadrons
Journal Article
·
Mon May 23 00:00:00 EDT 2011
· AIP Conference Proceedings
·
OSTI ID:21513240
Heavy Ion Physics at RHIC
Journal Article
·
Mon May 04 00:00:00 EDT 2009
· AIP Conference Proceedings
·
OSTI ID:21304769
Looking for quark-gluon plasma with strange hadrons
Journal Article
·
Fri Oct 01 00:00:00 EDT 1993
· Bulletin of the American Physical Society
·
OSTI ID:387230