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Radial modes of rotating neutron stars in the Chandrasekhar-Friedman formalism

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dc.contributor.authorDatta, Bhaskar
dc.contributor.authorHasan, S.S.
dc.contributor.authorSahu, P.K.
dc.contributor.authorPrasanna, A.R.
dc.date.accessioned2008-02-01T11:07:41Z
dc.date.available2008-02-01T11:07:41Z
dc.date.issued1998-02
dc.descriptionRestricted Access.en
dc.description.abstractEigenfrequencies of radial pulsations of "slowly" rotating neutron stars are calculated in a general relativistic formalism given by Chandrasekhar & Friedman. It is found that the square of the frequencies are always a decreasing function of the central density of the neutron star. The decrease of the squared frequency is sensitive to the equation of state of neutron star matter, and is illustrated using realistic models.en
dc.format.extent762341 bytes
dc.format.mimetypeapplication/pdf
dc.identifier.citationInternational Journal of Modern Physics D, 1998, Vol.7, p49-59en
dc.identifier.issn0218-2718
dc.identifier.urihttp://hdl.handle.net/2289/3409
dc.language.isoenen
dc.publisherWorld Scientific Publishing Companyen
dc.relation.urihttp://dx.doi.org/10.1142/S021827189800005Xen
dc.rights1998. World Scientific Publishing Companyen
dc.titleRadial modes of rotating neutron stars in the Chandrasekhar-Friedman formalismen
dc.typeArticleen

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