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Consequences of a strong phase transition in the dense matter equation of state for the rotational evolution of neutron stars
M. Bejger · D. Blaschke · P. Haensel · J. L. Zdunik · M. Fortin · ↳ astro-ph.HE
Nuclear Theory·nucl-th
5 papers—3 primary·2 cross-listed
M. Bejger · D. Blaschke · P. Haensel · J. L. Zdunik · M. Fortin · ↳ astro-ph.HE
Martha Constantinou🇺🇸 · ↳ hep-lat
first authorsco-authorsvia INSPIRE