Strangeness driven phase transitions in compressed baryonic matter and their relevance for neutron stars and core collapsing supernovae

2015 ◽  
Author(s):  
Ad. R. Raduta ◽  
F. Gulminelli ◽  
M. Oertel
Keyword(s):  
Phase Transitions ◽  
Neutron Stars ◽  
Baryonic Matter ◽  
Compressed Baryonic Matter

The compressed baryonic matter experiment at FAIR

Open Physics ◽  
2012 ◽  
Vol 10 (6) ◽  
Author(s):  
Peter Senger
Keyword(s):  
Phase Diagram ◽  
Phase Transitions ◽  
Equation Of State ◽  
High Energy ◽  
Baryonic Matter ◽  
Lepton Pairs ◽  
Chiral Phase ◽  
Qcd Phase Diagram ◽  
Compressed Baryonic Matter ◽  
Large Acceptance

AbstractThe Compressed Baryonic Matter (CBM) experiment will be one of the major scientific pillars of the future Facility for Antiproton and Ion Research (FAIR) in Darmstadt. The goal of the CBM research program is to explore the QCD phase diagram in the region of high baryon densities using high-energy nucleus-nucleus collisions. This includes the study of the equation-of-state of nuclear matter at high densities, and the search for the deconfinement and chiral phase transitions. The CBM detector is designed to measure both bulk observables with large acceptance and rare diagnostic probes such as charmed particles and vector mesons decaying into lepton pairs.

scholarly journals Exploring Cosmic Matter in the Laboratory—The Compressed Baryonic Matter Experiment at FAIR

Particles ◽  
2019 ◽  
Vol 2 (4) ◽  
pp. 499-510
Author(s):  
Peter Senger
Keyword(s):  
Phase Transitions ◽  
Neutron Star ◽  
Baryonic Matter ◽  
Heavy Nuclei ◽  
Quantum Chromo Dynamics ◽  
The Core ◽  
Compressed Baryonic Matter ◽  
Chemical Potentials ◽  
Massive Neutron Star ◽  
Density Equation

The Compressed Baryonic Matter (CBM) experiment is one of four scientific pillars of the future Facility for Antiproton and Ion Research (FAIR) in Darmstadt. In collisions between heavy nuclei at FAIR energies, it is expected that the matter in the reaction zone is compressed to more than five times saturation density, corresponding to the density in the core of a massive neutron star. This offers the unique opportunity to study in the laboratory the high-density equation-of-state (EOS) of nuclear matter, and to search for new phases of Quantum Chromo Dynamics (QCD) matter at large baryon-chemical potentials. Promising experimental observables sensitive to the EOS and to possible phase transitions will be discussed, together with a brief description of the CBM experiment.

A high-performance silicon tracker for the Compressed Baryonic Matter experiment at FAIR

2005 ◽  
Vol 55 (12) ◽  
pp. 1649-1653 ◽  
Author(s):  
Johann M. Heuser ◽  
Walter F.J. Muller ◽  
Peter Senger ◽  
Christian Muntz ◽  
Joachim Stroth
Keyword(s):  
High Performance ◽  
Baryonic Matter ◽  
Compressed Baryonic Matter

scholarly journals Phase transitions in rotating neutron stars cores: back bending, stability, corequakes, and pulsar timing

2006 ◽  
Vol 450 (2) ◽  
pp. 747-758 ◽  
Author(s):  
J. L. Zdunik ◽  
M. Bejger ◽  
P. Haensel ◽  
E. Gourgoulhon
Keyword(s):  
Phase Transitions ◽  
Neutron Stars ◽  
Pulsar Timing

Dense Baryonic Matter in the Cores of Neutron Stars

2020 ◽  
pp. 85-152
Author(s):  
William M. Spinella ◽  
Fridolin Weber
Keyword(s):  
Neutron Stars ◽  
Baryonic Matter
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