Transition to hot quark matter in relativistic heavy-ion collision

1978 ◽  
Vol 78 (5) ◽  
pp. 552-555 ◽  
Author(s):  
S.A. Chin
Keyword(s):  
Quark Matter ◽  
Heavy Ion ◽  
Heavy Ion Collision ◽  
Relativistic Heavy Ion Collision ◽  
Hot Quark Matter ◽  
Ion Collision

scholarly journals Bremsstrahlung pair production in relativistic heavy ion collision

1998 ◽  
Vol 2 (4) ◽  
pp. 741 ◽  
Author(s):  
Helmar Meier ◽  
Kai Hencken ◽  
Dirk Trautmann ◽  
Gerhard Baur
Keyword(s):  
Pair Production ◽  
Heavy Ion ◽  
Heavy Ion Collision ◽  
Relativistic Heavy Ion Collision ◽  
Ion Collision

scholarly journals Development of the Detector for Relativistic Heavy-Ion-Collision Experiments

2010 ◽  
Vol 19 (1/2) ◽  
pp. 32
Author(s):  
Youngil KWON ◽  
Young-Jin KIM ◽  
In-Kwon YOO ◽  
Byungsik HONG
Keyword(s):  
Heavy Ion ◽  
Heavy Ion Collision ◽  
Relativistic Heavy Ion Collision ◽  
Ion Collision

scholarly journals Search for DCC in relativistic heavy-ion collision through event shape analysis

1999 ◽  
Vol 449 (1-2) ◽  
pp. 109-113 ◽  
Author(s):  
B.K. Nandi ◽  
G.C. Mishra ◽  
B. Mohanty ◽  
D.P. Mahapatra ◽  
T.K. Nayak
Keyword(s):  
Shape Analysis ◽  
Heavy Ion ◽  
Event Shape ◽  
Heavy Ion Collision ◽  
Relativistic Heavy Ion Collision ◽  
Ion Collision

scholarly journals MAGIC - how MAtter’s extreme phases can be revealed in Gravitational wave observations and in relativistic heavy Ion Collision experiments

2019 ◽  
Vol 1271 ◽  
pp. 012023 ◽  
Author(s):  
Matthias Hanauske ◽  
Luke Bovard ◽  
Jan Steinheimer ◽  
Anton Motornenko ◽  
Volodymyr Vovchenko ◽  
...  
Keyword(s):  
Gravitational Wave ◽  
Heavy Ion ◽  
Heavy Ion Collision ◽  
Relativistic Heavy Ion Collision ◽  
Ion Collision

scholarly journals STRANGENESS IN NEUTRON STARS

2007 ◽  
Vol 16 (02n03) ◽  
pp. 231-245 ◽  
Author(s):  
FRIDOLIN WEBER ◽  
ALEXANDER HO ◽  
RODRIGO P. NEGREIROS ◽  
PHILIP ROSENFIELD
Keyword(s):  
Neutron Stars ◽  
Quark Matter ◽  
Strange Quark ◽  
Baryon Number ◽  
Heavy Ion ◽  
Strange Quark Matter ◽  
Relativistic Heavy Ion Collision ◽  
Quark Deconfinement ◽  
Ion Collision ◽  
High Pressure Environment

It is generally agreed on that the tremendous densities reached in the centers of neutron stars provide a high-pressure environment in which several intriguing particles processes may compete with each other. These range from the generation of hyperons to quark deconfinement to the formation of kaon condensates and H-matter. There are theoretical suggestions of even more exotic processes inside neutron stars, such as the formation of absolutely stable strange quark matter. In the latter event, neutron stars would be largely composed of strange quark matter possibly enveloped in a thin nuclear crust. This paper gives a brief overview of these striking physical possibilities with an emphasis on the role played by strangeness in neutron star matter, which constitutes compressed baryonic matter at ultra-high baryon number density but low temperature which is not accessible to relativistic heavy ion collision experiments.

Sign in / Sign up

Export Citation Format

Share Document