Towards a Noncommutative Astrophysics
arXiv:0908.4196 · doi:10.1103/PhysRevD.81.025005
Abstract
We consider astrophysical objects such as main-sequence stars, white-dwarfs and neutron stars in a noncommutative context. Noncommutativity is implemented via a deformed dispersion relation from which we obtain noncommutative corrections to the pressure, particle number and energy densities for radiation and for a degenerate fermion gas. The main implications of noncommutativity for the considered astrophysical objects are examined and discussed.
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References in corpus (5)
Cited by in corpus (27)
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