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http://hdl.handle.net/2289/3409
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DC Field | Value | Language |
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dc.contributor.author | Datta, Bhaskar | - |
dc.contributor.author | Hasan, S.S. | - |
dc.contributor.author | Sahu, P.K. | - |
dc.contributor.author | Prasanna, A.R. | - |
dc.date.accessioned | 2008-02-01T11:07:41Z | - |
dc.date.available | 2008-02-01T11:07:41Z | - |
dc.date.issued | 1998-02 | - |
dc.identifier.citation | International Journal of Modern Physics D, 1998, Vol.7, p49-59 | en |
dc.identifier.issn | 0218-2718 | - |
dc.identifier.uri | http://hdl.handle.net/2289/3409 | - |
dc.description | Restricted Access. | en |
dc.description.abstract | Eigenfrequencies 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.extent | 762341 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | World Scientific Publishing Company | en |
dc.relation.uri | http://dx.doi.org/10.1142/S021827189800005X | en |
dc.rights | 1998. World Scientific Publishing Company | en |
dc.title | Radial modes of rotating neutron stars in the Chandrasekhar-Friedman formalism | en |
dc.type | Article | en |
Appears in Collections: | Research Papers (A&A) |
Files in This Item:
File | Description | Size | Format | |
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1998 Int. Jou. of Mod. Phys. D V7 p49-59.pdf Restricted Access | Restricted Access | 744.47 kB | Adobe PDF | View/Open Request a copy |
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