Noncommutative effects in astrophysical objects: a survey
classification
🌀 gr-qc
keywords
starsastrophysicalmain-sequencenoncommutativityobjectsappliedcalculatedcanonical
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The main implications of noncommutativity over astrophysical objects are examined. Noncommutativity is introduced through a deformed dispersion relation $E^{2}=p^{2}c^{2}(1+\lambda E)^{2} + m^{2}c^{4}$ and the relevant thermodynamical quantities are calculated using the grand canonical ensemble formalism. These results are applied to simple physical models describing main-sequence stars, white-dwarfs and neutron stars. The stability of main-sequence stars and white dwarfs is discussed.
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