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Cited by 634

The DOI matches its Crossref record; 3 of the 3 references it cites were found in a registry or an index.

Transition of the dark energy equation of state in an interacting holographic dark energy model

Open access
Wang, Bin, Gong, Yungui, Abdalla, Elcio·2005·Physics Letters B

Abstract

Abstract A model of holographic dark energy with an interaction with matter fields has been investigated. Choosing the future event horizon as an IR cutoff, we have shown that the ratio of energy densities can vary with time. With the interaction between the two different constituents of the universe, we observed the evolution of the universe, from early deceleration to late time acceleration. In addition, we have found that such an interacting dark energy model can accommodate a transition of the dark energy from a normal state where w D > − 1 to w D − 1 phantom regimes. Implications of interacting dark energy model for the observation of dark energy transition has been discussed.

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Crossref · 10.1016/j.physletb.2005.08.008

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Metadata

Authors
Wang, B., Gong, Y., & Abdalla, E.
Venue
Physics Letters B
Publisher
Elsevier BV
Published
2005-09
Volume
624
Issue
3-4
Pages
141-146
ISSN
0370-2693 (ISSN-L)
OpenAlex
W2007572894
Cited by
634
References
3
FWCI
21.47
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Transition of the dark energy equation of state in an interacting holographic dark energy model. https://app.cochat.ai/papers/10.1016/j.physletb.2005.08.008
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Wang, B., Gong, Y., & Abdalla, E. (2005). Transition of the dark energy equation of state in an interacting holographic dark energy model. Physics Letters B. https://doi.org/10.1016/j.physletb.2005.08.008

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Bibliographic data: Semantic Scholar, OpenAlex, Crossref.

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.