arXiv High Energy Astrophysical Phenomena
arXiv High Energy Astrophysical Phenomena
5 years ago

Pions in hot dense matter and their astrophysical implications. (arXiv:1911.02632v1 [astro-ph.HE])

Bryce Fore, Sanjay Reddy
We study the role of pions in hot dense matter encountered in astrophysics. We find that strong interactions enhance the number density of negatively charged pions and that this enhancement can be calculated reliably for a relevant range of density and temperature using the virial expansion. We assess the influence of pions and muons on the equation of state (EOS) and weak interaction rates in hot dense matter. We find that thermal pions increase the proton fraction and soften the EOS. We also find that charged current weak reactions involving pions and muons and make an important contribution to the opacity of muon neutrinos. This could influence the dynamics of core-collapse supernovae and neutron star mergers. Finally, we note that pion-nucleon reactions can alter the evolution of the proton fraction when weak interactions are not in equilibrium.

Publisher URL: http://arxiv.org/abs/1911.02632

DOI: arXiv:1911.02632v1

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