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 |
