Gravitational collapse of spherically symmetric stars in noncommutative general relativity
arXiv:0910.2777 · doi:10.1140/epjc/s10052-010-1342-2
Abstract
Gravitational collapse of a class of spherically symmetric stars are investigated. We quantise the geometries describing the gravitational collapse by a deformation quantisation procedure. This gives rise to noncommutative spacetimes with gravitational collapse.
19 pages, final version, to appear in Eur. Phys. J. C.