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We calculate the bulk-viscous dissipation time for adiabatic density oscillations in nuclear matter at densities of 1-7 times nuclear saturation density and at temperatures ranging from 1 MeV, where corrections to previous low-temperature calculations become important, up to 10 MeV, where the assumption of neutrino transparency is no longer valid.
1903
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2004
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Y.-F. Yuan, Electron positron capture rates and the steady state equilibrium condition for electron-positron plasma with nucleons , Phys. Rev. D72
2005
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2008
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W.-j. Fu, G.-h. Wang and Y.-x. Liu, Electron Capture and Its Reverse Process in Hot and Dense Astronuclear Matter , Astrophys. J. 678
2008
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2016
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2008
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2010
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2010
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2010
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2010
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A. Schmitt, Dense matter in compact stars: A pedagogical introduction , Lect. Notes Phys. 811
2010
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2010
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2011
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M. Hanauske, J. Steinheimer, L. Bovard, A. Mukherjee, S. Schramm, K. Takami et al., Concluding Remarks: Connecting Relativistic Heavy Ion Collisions and Neutron Star Mergers by the Equation of State of Dense Hadron- and Quark Matter as signalled by Gravitational Waves , J. Phys. Conf. Ser. 878
2017
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2017
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2018
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2018
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M. G. Alford and S. P. Harris, Beta equilibrium in neutron star mergers , Phys. Rev. C98
2018
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2018
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2018
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2018
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2018
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2019
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M. Hanauske, J. Steinheimer, A. Motornenko, V. Vovchenko, L. Bovard, E. R. Most et al., Neutron Star Mergers: Probing the EoS of Hot, Dense Matter by Gravitational Waves , Particles 2
2019
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2019
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