Role of Initial Data in Higher Dimensional Quasi-Spherical Gravitational Collapse

Details Role of Initial Data in Higher Dimensional Quasi-Spherical Gravitational Collapse Role of Initial Data in Higher Dimensional Quasi-Spherical Gravitational Collapse

2003-08-12

arxiv.org/abs/gr-qc/0308037v1

Gen.Rel.Grav. 37 (2005) 225-232

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

7 Latex Pages, RevTex Style, No figures

Scientific paper

10.1007/s10714-005-0011-5

We study the gravitational collapse in ($n+2$)-D quasi-spherical Szekeres space-time (which possess no killing vectors) with dust as the matter distribution. Instead of choosing the radial coordinate `$r$' as the initial value for the scale factor $R$, we consider a power function of $r$ as the initial scale for the radius $R$. We examine the influence of initial data on the formation of singularity in gravitational collapse.

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