Panda, P. K. [UNESP]Sahu, R.Mishra, S.2014-05-272014-05-272000-11-01Physical Review C - Nuclear Physics, v. 62, n. 5, p. 558021-558028, 2000.0556-2813http://hdl.handle.net/11449/66273We study the equation of state for neutron matter using the Walecka model including quantum corrections for baryons and sigma mesons through a realignment of the vacuum. We next use this equation of state to calculate the radius, mass, and other properties of rotating neutron stars.558021-558028engEffects of vacuum structure on neutron starsArtigo10.1103/PhysRevC.62.055802WOS:000165369400065Acesso restrito2-s2.0-00390001752-s2.0-0039000175.pdf