Shadows of a maximal acceleration
arXiv:gr-qc/0211011 · doi:10.1016/S0375-9601(02)01536-0
Abstract
A quantum mechanical upper limit on the value of particle accelerations, or maximal acceleration (MA), is applied to compact stars. A few MA fermions are at most present in canonical white dwarfs and neutron stars. They drastically alter a star's stability conditions.
11 pages