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arxiv: 0908.4196 · v2 · pith:U54R6U3Mnew · submitted 2009-08-28 · 🌀 gr-qc · astro-ph.SR· hep-ph· hep-th

Towards a Noncommutative Astrophysics

classification 🌀 gr-qc astro-ph.SRhep-phhep-th
keywords noncommutativeastrophysicalnoncommutativityobjectsstarsastrophysicsconsiderconsidered
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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 $E^{2}=p^{2}c^{2}(1+\lambda E)^{2}+m^{2}c^{4}$ 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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