Conversion of nuclear to 2-flavour quark matter in rotating compact stars: A general relativistic perspective

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dc.creatorMallick, Ritam
dc.creatorBhattachryya, Abhijit
dc.creatorGhosh, Sanjay K.
dc.creatorRaha, Sibaji
dc.date2008-06-11
dc.date.accessioned2026-07-07T09:43:42Z
dc.date.available2026-07-07T09:43:42Z
dc.descriptionThe conversion of neutron star to strange star is argued to be a two step process. The first process involves the deconfinement of nuclear to two-flavour quark matter. The GR results shows that the propagating front breaks up into fragments which propagate with different velocities along different directions. The time taken for this conversion to happen is of the order of few $ms$. This calculation indicates the inadequacy of non-relativistic (NR) or even Special Relativistic (SR) treatments for these cases.
dc.description4 pages, 4 figures
dc.identifierhttps://arxiv.org/abs/0806.1800
dc.identifierhttp://arxiv.org/abs/0806.1800
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/162658
dc.subjectAstrophysics
dc.titleConversion of nuclear to 2-flavour quark matter in rotating compact stars: A general relativistic perspective
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