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Showing 1 to 3 of 3 for “"beta equilibrium"”.
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Dense matter and the compressible liquid drop model
… in the collapsing supernova core. Matter in beta equilibrium is considered at low temperatures; this is the character of the matter that one expects to exist in the inner crust of a cooled neutron star. We obtain for the first time the density range occupied by the non-spherical nuclear …
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Effective interactions and pairing correlations: from nuclei to compact stars
… of different nuclear species in thermal and beta-equilibrium. The resulting specific heat brings to light a strong influence of resonance population at moderate temperatures and in density regions close to the crust-core transition and the importance of an accurate treatment of …
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Neutrino processes in dense matter
Submitted by Carolyn Mead (cmead2@illinois.edu) on 2011-06-16T16:30:51Z No. of bitstreams: 1 1981_iwamoto.pdf: 4398216 bytes, checksum: ca09788c9a5f5d0c309003977f8ed2ab (MD5)