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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4078
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dc.contributor.authorKrishan, V-
dc.contributor.authorKumar, N-
dc.date.accessioned2008-12-16T14:29:56Z-
dc.date.available2008-12-16T14:29:56Z-
dc.date.issued1978-08-
dc.identifier.citationAstrophysics and Space Science, Vol. 57, No. 1, pp. 241 - 243en
dc.identifier.issn1572-946X-
dc.identifier.urihttp://hdl.handle.net/2248/4078-
dc.descriptionOpen Access-
dc.description.abstractStarting from the exact general relativistic expression for the total energy of selfgravitating spherically distributed matter and using the minimum energy principle, we calculate the upper mass limit for a neutron star to be 3.1 solar masses.en
dc.language.isoenen
dc.publisherD.Reidel Publishing Co.,en
dc.relation.urihttp://adsabs.harvard.edu/abs/1978Ap%26SS..57..241Ken
dc.relation.urihttp://dx.doi.org/10.1007/BF00639060en
dc.rightsD.Reidel Publishing Co.,-
dc.subjectBlack Holes (Astronomy)en
dc.subjectDynamic Stabilityen
dc.subjectGravitational Collapseen
dc.subjectNeutron Starsen
dc.subjectStellar Massen
dc.subjectBaryonsen
dc.subjectRelativityen
dc.subjectSpace-Time Functionsen
dc.titleUpper mass limit for neutron star stability against black hole formationen
dc.typeArticleen
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