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arxiv gr-qc/0403062 v2 pith:4YQKQKK6 submitted 2004-03-15 gr-qc astro-phhep-th

The Chaplygin gas as a model for dark energy

V. Gorini , A. Kamenshchik , U. Moschella , V. Pasquier This is my paper
classification gr-qc astro-phhep-th
keywords chaplygincosmologicalmodelsappearancebasisconsideredcosmologydark
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We review the essential features of the Chaplygin gas cosmological models and provide some examples of appearance of the Chaplygin gas equation of state in modern physics. A possible theoretical basis for the Chaplygin gas in cosmology is discussed. The relation with scalar field and tachyon cosmological models is also considered.

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Cited by 1 Pith paper

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

  1. The Hawking temperature in the context of dark energy for Kerr-Newman and Kerr-Newman-AdS backgrounds

    gr-qc 2019-06 unverdicted novelty 4.0

    Hawking temperatures for emergent gravity metrics of KN and KNAdS are calculated along θ=0, modified by dark energy from DBI k-essence fields, with metrics satisfying Einstein equations at large r.