The DOI matches its Crossref record; 51 of the 51 references it cites were found in a registry or an index.
Constraints on the interacting holographic dark energy model
Open accessAbstract
Abstract We examined the interacting holographic dark energy model in a universe with spatial curvature. Using the near-flatness condition and requiring that the universe is experiencing an accelerated expansion, we have constrained the parameter space of the model and found that the model can accommodate a transition of the dark energy from ω D > − 1 to ω D − 1 .
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Cites
Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
Riess, A. G., Filippenko, A. V., Challis, P., Clocchiatti, A., Diercks, A., Garnavich, P. M., Gilliland, R. L., Hogan, C. J., Jha, S., Kirshner, R. P., et al. (1998) · The Astronomical Journal · doi:10.1086/300499 · Cited by 19,704
Measurements of Ω and Λ from 42 High‐Redshift Supernovae
Perlmutter, S., Aldering, G., Goldhaber, G., Knop, R. A., Nugent, P., Castro, P. G., Deustua, S., Fabbro, S., Goobar, A., Groom, D. E., et al. (1999) · The Astrophysical Journal · doi:10.1086/307221 · Cited by 18,062
The cosmological constant and dark energy
Peebles, P. J. E., & Ratra, B. (2003) · Reviews of Modern Physics · doi:10.1103/revmodphys.75.559 · Cited by 5,213
Cosmological constant—the weight of the vacuum
Padmanabhan, T. (2003) · Physics Reports · doi:10.1016/s0370-1573(03)00120-0 · Cited by 3,195
A flat Universe from high-resolution maps of the cosmic microwave background radiation
de Bernardis, P., Ade, P. A. R., Bock, J. J., Bond, J. R., Borrill, J., Boscaleri, A., Coble, K., Crill, B. P., De Gasperis, G., Farese, P. C., et al. (2000) · Nature · doi:10.1038/35010035 · Cited by 2,518
Cosmological Constant - the Weight of the VacuumPreprint
Padmanabhan, Τ. (2002) · Cited by 2,145
A model of holographic dark energy
Li, M. (2004) · Physics Letters B · doi:10.1016/j.physletb.2004.10.014 · Cited by 1,897
Amendola, L. (2000) · Physical Review D · doi:10.1103/physrevd.62.043511 · Cited by 1,835
A Flat Universe from High-Resolution Maps of the Cosmic Microwave Background \nRadiation
de Bernardis, P., Ade, P. A. R., Bock, J. J., Bond, J. R., Borrill, J., Boscaleri, A., Coble, K., Crill, B. P., de Gasperis, G., Farese, P. C., et al. (2000) · eScholarship (California Digital Library) · Cited by 1,562
Knop, R. A., Aldering, G., Amanullah, R., Astier, P., Blanc, G., Burns, M. S., Conley, A., Deustua, S. E., Doi, M., Ellis, R., et al. (2003) · The Astrophysical Journal · doi:10.1086/378560 · Cited by 1,454
Cited by
Bamba, K., Capozziello, S., Nojiri, S., & Odintsov, S. D. (2012) · Astrophysics and Space Science · doi:10.1007/s10509-012-1181-8 · Cited by 2,387
Barrow holographic dark energy
Saridakis, E. N. (2020) · Physical Review D · doi:10.1103/physrevd.102.123525 · Cited by 266
Metadata
- Authors
- Wang, B., Lin, C.-Y., & Abdalla, E.
- Venue
- Physics Letters B
- Publisher
- Elsevier BV
- Published
- 2006-06
- Volume
- 637
- Issue
- 6
- Pages
- 357-361
- ISSN
- 0370-2693 (ISSN-L)
- OpenAlex
- W2040384286
- Cited by
- 290
- References
- 51
- FWCI
- 13.88
- Type
- journal article
- Language
- en
- Open access
- green
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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.
