Hadron-quark phase transition at nonzero isospin density: The effect of quark pairing
Creators
- 1. Institut fuer Theoretische Physik, Ruprecht-Karls-Universitaet, Philosophenweg 16, D-69120, Heidelberg (Germany)
Description
We compute the mixed phase of nuclear matter and 2SC matter for different temperatures and proton fractions. After showing that the symmetry energy of the 2SC phase is, to a good approximation, 3 times larger than the one of the normal quark phase, we discuss and compare all the properties of the mixed phase with a 2SC component or a normal quark matter component. In particular, the local isospin densities of the nuclear and the quark component and the stiffness of the mixed phase are significantly different whether the 2SC phase or the normal quark phase are considered. If a strong diquark pairing is adopted for the 2SC phase, there is a possibility to eventually enter in the nuclear matter 2SC matter mixed phase in low energy heavy ions collisions experiments. Possible observables able to discern between the formation of the 2SC phase or the normal quark phase are finally discussed.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.81.094024;
- arXiv
- arXiv:1003.1017v1;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 81
- Journal Issue
- 9
- Journal Page Range
- p. 094024-094024.10
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 42003108
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- APPROXIMATIONS; COMPARATIVE EVALUATIONS; DENSITY; HEAVY ION REACTIONS; ISOSPIN; NUCLEAR MATTER; PAIR PRODUCTION; PHASE TRANSFORMATIONS; PROTONS; QUARK MATTER; QUARKS; SYMMETRY
- Descriptors DEC
- BARYONS; CALCULATION METHODS; ELEMENTARY PARTICLES; EVALUATION; FERMIONS; HADRONS; INTERACTIONS; MATTER; NUCLEAR REACTIONS; NUCLEONS; PARTICLE PRODUCTION; PARTICLE PROPERTIES; PHYSICAL PROPERTIES
Optional Information
- Notes
- (c) 2010 The American Physical Society