The DOI matches its Crossref record; 19 of the 19 references it cites were found in a registry or an index.
Supernova constraints on a holographic dark energy model
Open accessAbstract
In this paper, we use the type Ia supernova data to constrain the model of holographic dark energy. For d = 1, the best fit result is Ω m 0 = 0.25, the equation of the state of the holographic dark energy w Λ 0 = −0.91 and the transition between the decelerating expansion and the accelerating expansion happened when the cosmological red-shift was z T = 0.72. If we set d as a free parameter, the best fit results are d = 0.21, Ω m 0 = 0.46, w Λ 0 = −2.67, which sounds like a phantom today, and the transition red-shift is z T = 0.28.
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Cites
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Cited by
Quintom cosmology: Theoretical implications and observations
Cai, Y.-F., Saridakis, E. N., Setare, M. R., & Xia, J.-Q. (2010) · Physics Reports · doi:10.1016/j.physrep.2010.04.001 · Cited by 868
Constraints on the interacting holographic dark energy model
Wang, B., Lin, C.-Y., & Abdalla, E. (2006) · Physics Letters B · doi:10.1016/j.physletb.2006.04.009 · Cited by 290
Metadata
- Authors
- Huang, Q.-G., & Gong, Y.
- Venue
- Journal of Cosmology and Astroparticle Physics
- Publisher
- IOP Publishing
- Published
- 2004-08-10
- Volume
- 2004
- Issue
- 08
- Pages
- 006-006
- ISSN
- 1475-7508 (ISSN-L)
- 1475-7516
- OpenAlex
- W2062958117
- Cited by
- 275
- References
- 19
- FWCI
- 12.80
- Type
- journal article
- Language
- en
- Open access
- bronze
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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