Constraining the gravitational redshift of a neutron star from the Σ-meson well depth View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

2011-03

AUTHORS

Xian-Feng Zhao

ABSTRACT

The effect of the Σ-meson well depth on the gravitational redshift is examined within the framework of relativistic mean field theory for the baryon octet system. It is found that, for a stable neutron star, the gravitational redshift increases with the central energy density increase or with the mass increase but decreases as the radius increases. Considering a change of from −30 MeV to 30 MeV, for a stable neutron star the gravitational redshift near to the maximum mass increases. In addition, it is also found that the growth of the makes the gravitational redshift as a function of Mmax /R increase, the higher the the less the change in the gravitational redshift. More... »

PAGES

139-144

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/s10509-010-0498-4

DOI

http://dx.doi.org/10.1007/s10509-010-0498-4

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1016937405


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