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Cited by 231

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Effective equation of state and energy conditions in phantom/tachyon inflationary cosmology perturbed by quantum effects

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Nojiri, Shin'ichi, Odintsov, Sergei D.·2003·Physics Letters B

Abstract

Abstract We discuss the model consisting of tachyon which may have the negative kinetic energy plus scalar phantom and plus conformal quantum matter. It is demonstrated that such a model naturally admits two de Sitter phases where the early universe inflation is produced by quantum effects and the late time accelerating universe is caused by phantom/tachyon. The energy conditions bounds for such cosmology are derived. It is interesting that effective equation of state may change its sign what depends from the proper choice of the combination of phantom/tachyon and quantum effects.

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Metadata

Authors
Nojiri, S., & Odintsov, S. D.
Venue
Physics Letters B
Publisher
Elsevier BV
Published
2003-10
Volume
571
Issue
1-2
Pages
1-10
ISSN
0370-2693 (ISSN-L)
OpenAlex
W2035091607
Cited by
231
References
2
FWCI
17.20
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Effective equation of state and energy conditions in phantom/tachyon inflationary cosmology perturbed by quantum effects. https://app.cochat.ai/papers/10.1016/j.physletb.2003.08.013
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Nojiri, S., & Odintsov, S. D. (2003). Effective equation of state and energy conditions in phantom/tachyon inflationary cosmology perturbed by quantum effects. Physics Letters B. https://doi.org/10.1016/j.physletb.2003.08.013

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.