{"arxiv_id":"gr-qc/0512083","incoming":{"papers":14,"sentences":17,"groups":[{"kind":"comparison","label":"Compares with it","papers":1,"sentences":1,"quotes":[{"arxiv_id":"0807.4269","title":"Modified dispersion relations and (A)dS Schwarzschild Black holes","url":"/paper/0807.4269","section":"EUP case","sentence":"This situation is similar to the case presented in [ref] while the difference here is that due to EUP, $T∼T_0$ is also bounded from below with a minimum value for large black holes.","intent_p":1.0,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":4,"sentences":4,"quotes":[{"arxiv_id":"1911.08624","title":"Effects of Planck-scale-modified dispersion relations on the thermodynamics of charged black holes","url":"/paper/1911.08624","section":"Introduction","sentence":"Within this framework, the issue of black holes and their thermodynamics has been explored by many authors in several different contexts and background theories of gravity, see for instance [ref] .","intent_p":0.98,"contests_p":null},{"arxiv_id":"1802.00058","title":"Redshift and lateshift from homogeneous and isotropic modified dispersion relations","url":"/paper/1802.00058","section":"Introduction","sentence":"As long as a fundamental theory of quantum gravity is not available to predict this effect from the scattering between gravitons and the probe particles such quantum gravity effects can be modeled phenomenologically by a modification of the relativistic dispersion relation of freely falling point particles, see [ref] and references therein.","intent_p":0.89,"contests_p":null},{"arxiv_id":"2109.12938","title":"Modified regular black holes with time delay and 1-loop quantum correction","url":"/paper/2109.12938","section":"Introduction","sentence":"Before a complete theory of quantum gravity could be established, it is quite desirable to construct regular black hole solutions, which are non-singular everywhere and characterized by a finite Kretschmann scalar curvature, to understand the final stage of star collapse and black hole evaporation [ref] .","intent_p":0.88,"contests_p":null},{"arxiv_id":"0809.4819","title":"Modified (A)dS Schwarzschild black holes in Rainbow spacetime","url":"/paper/0809.4819","section":"Introduction","sentence":"They may be responsible for threshold anomalies of ultra high energy cosmic rays and Gamma ray burst [ref] , contribute corrections to the entropy of black holes [ref] , provide alternatives to inflationary cosmology [ref] , and disclose the nature of dark energy [ref] .","intent_p":0.84,"contests_p":null}]}],"unlabelled_sentences":12},"outgoing":{"papers":0,"sentences":0,"groups":[],"unlabelled_sentences":0},"claims":[],"thresholds":{"intent_p":0.8,"supports_p":0.95,"contests_p":0.7},"method":"Citing sentences come from each paper's LaTeX source; every \\cite marks the sentence and the works it cites. Pith's classifier typed each sentence. A label is shown at intent probability 0.8 or more (0.95 for support), a contest at 0.7 or more. Measured accuracy against two blind model families is at https://pith.science/accuracy. The quoted sentences are the citing authors' own.","held_up":null,"_links":{"html":"https://pith.science/paper/gr-qc/0512083"}}