Pith. sign in

REVIEW 1 cited by

UV/IR Mixing and Black Hole Thermodynamics

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 0708.1220 v1 pith:2GINWIDZ submitted 2007-08-09 gr-qc

classification gr-qc
keywords blackholeenergymdrsmixingdispersionevaporationfinal
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

The goal of this paper is to investigate the final stage of black hole evaporation process in the framework of Lorentz violating Modified Dispersion Relations(MDRs). As a consequence of MDRs, the high energy sector of the underlying field theory does not decouple from the low energy sector, the phenomenon which is known as UV/IR mixing. In the absence of exact supersymmetry, we derive a modified dispersion relation which shows UV/IR mixing by a novel energy dependence. Then we investigate the effects of these type of MDRs on the thermodynamics of a radiating noncommutative Schwarzschild black hole. The final stage of black hole evaporation obtained in this framework is compared with existing pictures.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Perturbative black-hole and horizon solutions in gravity with explicit spacetime-symmetry breaking

    gr-qc 2024-11 conditional novelty 6.0 of 10

    New perturbative black hole solutions in an explicit spacetime-symmetry-breaking gravity EFT, with derived observables including three-horizon metrics when two coefficients are active.

Pith tools