Metastable pions in dense media
arXiv:1610.05751 · doi:10.1103/PhysRevD.95.096013
Abstract
We study the leptonic decay of charged pions in a compact star environment. Considering leptons as a degenerated Fermi system, pions are tightly constrained to decay into these particles because their Fermi levels are occupied. Thus, pion decay is only possible through thermal fluctuations. Under these circumstances, pion lifetime is larger and hence can be considered to reach a metastable state. We explore restrictions under which such a metastability is possible. We also study conditions under which pions and leptons already in chemical equilibrium can reach simultaneously the thermal equilibrium, and obtain the neutrino emissivity from metastable pions. Scenarios that favor this metastable state are protoneutron stars.
10 pages, 5 figures. Version to appear in Phys. Rev. D
References in corpus (16)
- BEC-BCS Crossover in the Nambu--Jona-Lasinio Model of QCD
- Tables of Hyperonic Matter Equation of State for Core-Collapse Supernovae
- Astrophysical Implications of Equation of State for Hadron-Quark Mixed Phase: Compact Stars and Stellar Collapses
- Pion Condensation in Baryonic Matter: from Sarma Phase to Larkin-Ovchinnikov-Fudde-Ferrell Phase
- Pion and Kaon Condensation at Finite Temperature and Density
- Probing nuclear symmetry energy at high densities using pion, kaon, eta and photon productions in heavy-ion collisions
- The Linear Sigma Model and the formation of a charged pion condensate in the presence of an external magnetic field
- Intriguing aspects of meson condensation
- Pion and muon production in electron-positron photon plasma
- Equation of state of imbalanced cold matter from chiral perturbation theory
- Recent Developments on Kaon Condensation and Its Astrophysical Implications
- In-medium and isospin effects on particle production near threshold energies in heavy-ion collisions
- Duality between chiral symmetry breaking and charged pion condensation at large : Consideration of an NJL model with baryon-, isospin- and chiral isospin chemical potentials
- Possibility of s-wave pion condensates in neutron stars revisited
- Magnetic catalysis of a charged Bose-Einstein condensate
- Pion properties at finite nuclear density based on in-medium chiral perturbation theory
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- Pion crystals hosting topologically stable baryons
- QCD phase diagram at finite isospin chemical potential and temperature in an IR-improved soft-wall AdS/QCD model
- Pions near condensation under compact star conditions