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

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3163

Title:	Radial modes of rotating neutron stars in the Chandrasekhar-Friedman formalism
Authors:	Datta, B Hasan, S. S Sahu, P. K Prasanna, A. R
Keywords:	Neutron Stars: Pulsations
Issue Date:	Feb-1998
Publisher:	World Scientific Publishing Company
Citation:	International Journal of Modern Physics D, Vol. 7, No. 1, p. 49 - 59
Abstract:	Eigenfrequencies of radial pulsations of "slowly" rotating neutron stars are calculated in a general relativistic formalism given by Chandrasekhar and Friedman (1972). 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.
URI:	http://hdl.handle.net/2248/3163
ISSN:	0218-2718
Appears in Collections:	IIAP Publications

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