Effects of vacuum structure on neutron stars
Contribuinte(s) |
Universidade Estadual Paulista (UNESP) |
---|---|
Data(s) |
27/05/2014
27/05/2014
01/11/2000
|
Resumo |
We 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. |
Formato |
558021-558028 |
Identificador |
http://dx.doi.org/10.1103/PhysRevC.62.055802 Physical Review C - Nuclear Physics, v. 62, n. 5, p. 558021-558028, 2000. 0556-2813 http://hdl.handle.net/11449/66273 10.1103/PhysRevC.62.055802 WOS:000165369400065 2-s2.0-0039000175 2-s2.0-0039000175.pdf |
Idioma(s) |
eng |
Relação |
Physical Review C: Nuclear Physics |
Direitos |
closedAccess |
Tipo |
info:eu-repo/semantics/article |