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Properties and Dynamics of Neutron Stars and Proto-Neutron Stars

Following new developments in the measurement of gravitational waves from neutron–star mergers and the modification or construction of particle colliders to reach larger densities, we are entering a new era, during which we can begin to understand dense and hot matter for the first time. This, toge...

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Guardado en:
Formato: Online
Lenguaje:inglés
Publicado: MDPI - Multidisciplinary Digital Publishing Institute 2022
Materias:
neutron stars
equations of state
relativistic models
gravitational waves
neutron star
equation of state
universal relation
hybrid star
color superconductivity
diquark
dense matter
neutrinos
hyperons
nuclear matter
neutron star merger
beta equilibration
weak interaction
n/a
chiral symmetry
axion QED
quark–hole pairing
cold-dense QCD
magnetic DCDW
quark stars
dark matter
radial oscillations
nuclear matter aspects
quark deconfinement
quark-gluon plasma production
phase-transition
neutron star crust
meson interactions
quantum molecular dynamics
thema EDItEUR::G Reference, Information and Interdisciplinary subjects::GP Research and information: general
thema EDItEUR::P Mathematics and Science::PH Physics
Acceso en línea:ONIX_20221025_9783036553993_123
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ONIX_20221025_9783036553993_123

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