Effects of vacuum structure on neutron star


Autoria(s): Panda, P. K.; Sahu, R.; Mishra, S.; Navarra, F. S.; Robilotta, M. R.; Krein, G.
Contribuinte(s)

Universidade Estadual Paulista (UNESP)

Data(s)

20/05/2014

20/05/2014

01/01/2001

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 star.

Formato

405-408

Identificador

International Workshop on Hadron Physics 2000. Singapore: World Scientific Publ Co Pte Ltd, p. 405-408, 2001.

http://hdl.handle.net/11449/23111

WOS:000172097700040

Idioma(s)

eng

Publicador

World Scientific Publ Co Pte Ltd

Relação

International Workshop on Hadron Physics 2000

Direitos

closedAccess

Tipo

info:eu-repo/semantics/conferencePaper