Gravitational Field of A Radiating Star in Higher Dimensions

Simple item page
dc.creatorPaul, B. C.
dc.creatorChattopadhyay, P. K.
dc.date2007-08-06
dc.date.accessioned2026-07-07T08:22:21Z
dc.date.available2026-07-07T08:22:21Z
dc.descriptionWe obtain fields of a relativistic radiating star of non-static mass in the framework of higher dimensional spacetime. Assuming energy-momentum tensor in Higher dimensions analogous to that considered by Vaidya in 4 dimensions we obtain solution of a radiating spherically symmetric star. The solution obtained here is new in higher dimensions which however reduces to that obtained by Vaidya in 4 dimensions. It is also different in form from that obtained by Iyer and Vishveshwara. The interesting observation is that the radius of a radiating star in higher dimensions oscillates. The radial size of radiating star oscillates with a period which depends on the modes of vibration and dimensions of the space-time.
dc.description16 pages, no figure
dc.identifierhttps://arxiv.org/abs/0708.0793
dc.identifierhttp://arxiv.org/abs/0708.0793
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/135625
dc.subjectAstrophysics
dc.titleGravitational Field of A Radiating Star in Higher Dimensions
dc.typetext

Files

Collections

arXiv