Phase transition from nuclear matter to color superconducting quark matter: the effect of the isospin
arXiv:1003.1017 · doi:10.1103/PhysRevD.81.094024
Abstract
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, three 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.
9 pages, 8 figures
References in corpus (15)
- Color superconductivity in dense quark matter
- Susceptibilities and the Phase Structure of a Chiral Model with Polyakov Loops
- Hadron Production in Ultra-relativistic Nuclear Collisions: Quarkyonic Matter and a Triple Point in the Phase Diagram of QCD
- Isospin effects on sub-threshold kaon production at intermediate energies
- Quark Number Fluctuations in a Chiral Model at Finite Baryon Chemical Potential
- Testing Deconfinement at High Isospin Density
- Production of K+ and of K- Mesons in Heavy-Ion Collisions from 0.6 to 2.0 AGeV Incident Energy
- Stability of CFL cores in Hybrid Stars
- Conditions for Phase Equilibrium in Supernovae, Proto-Neutron and Neutron Stars
- Color-superconductivity in the strong-coupling regime of Landau gauge QCD
- Softening of the equation of state of matter at large densities and temperatures: chiral symmetry restoration vs. quark deconfinement
- The quark core of protoneutron stars in the phase diagram of quark matter
- Color neutrality effects in the phase diagram of the PNJL model
- A chiral lagrangian with Broken Scale: testing the restoration of symmetries in astrophysics and in the laboratory
- Is a soft nuclear equation of state extracted from heavy-ion data incompatible with pulsar data?
Cited by in corpus (19)
- Core-collapse supernova explosions triggered by a quark-hadron phase transition during the early post-bounce phase
- Probing the Nuclear Symmetry Energy with Heavy Ion Collisions
- Quark matter symmetry energy and quark stars
- Quark stars under strong magnetic fields
- Phase diagrams in the Hadron-PNJL model
- Influence of vector interactions on the hadron-quark/gluon phase transition
- Symmetry energy systematics and its high density behavior
- Isovector properties of quark matter and quark stars in an isospin-dependent confining model
- Hadron-quark phase transition in asymmetric matter with dynamical quark masses
- Phase transition of strongly interacting matter with a chemical potential dependent Polyakov loop potential
- Phase transitions of hadronic to quark matter at finite T and μ_B
- Warm asymmetric quark matter and proto-quark stars within the confined-isospin-density-dependent mass model
- Flavor Symmetry and Topology Change in Nuclear Symmetry Energy for Compact Stars
- Symmetry energy in cold dense matter
- Dense Stellar Matter with Strange Quark Matter Driven by Kaon Condensation
- Quark matter symmetry energy effect on equation of state for neutron stars
- Formation of quark phases in protoneutron stars: the transition from the 2SC to the normal quark phase
- Triple layered compact star with strange quark matter
- Can a supernova bang twice?