Radial pulsation frequencies of slowly rotating neutron stars

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dc.creatorSahu, P. K.
dc.creatorPrasanna, A. R.
dc.date1996-03-20
dc.date.accessioned2026-07-07T02:21:02Z
dc.date.available2026-07-07T02:21:02Z
dc.descriptionWe study the radial pulsation frequencies of slowly rotating neutron stars in general relativistic formalism using realistic equations of state. It is found that the pulsation frequencies are always an increasing function of rotation rate. The increasing rate of frequency depends on the nature of equations of state.
dc.description15 pages (LaTex), two postscript figures
dc.identifierhttps://arxiv.org/abs/astro-ph/9603107
dc.identifierhttp://arxiv.org/abs/astro-ph/9603107
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10410
dc.subjectAstrophysics
dc.titleRadial pulsation frequencies of slowly rotating neutron stars
dc.typetext

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