Работы, цитирующие эту работу

Работ: 3

Работа: Equation of state for dense nucleon matter

1. Crustal oscillations of slowly rotating relativistic stars

   M. Vavoulidis, Kostas D. Kokkotas, A. Stavridis

   СтатьяPulsars and Gravitational Waves ResearchMonthly Notices of the Royal Astronomical Society2008Цитирований: 2

   ABIABI:AkademIndex/openalex/2008.article.000020

2. Rotating stars in relativity

   Vasileios Paschalidis, Nikolaos Stergioulas

   СтатьяPulsars and Gravitational Waves ResearchLiving Reviews in Relativity2017Цитирований: 2

   ABIABI:AkademIndex/openalex/2017.article.000003

3. Constraining the high-density behavior of the nuclear symmetry energy with the tidal polarizability of neutron stars

   F. J. Fattoyev, J. Carvajal, William G. Newton +1

   СтатьяPulsars and Gravitational Waves ResearchPhysical Review C2013Цитирований: 0

   ABIABI:AkademIndex/openalex/2013.article.000005