Interacting holographic phantom
By M. Setare. 2007
221 citations recorded by the source corpus.
In this paper we consider the holographic model of interacting dark energy in non-flat universe. With the choice of c≤0.84, the interacting holographic dark energy can be described by a phantom scalar field. Then we show this phantomic description of the holographic dark energy with c≤0.84 and reconstruct the potential of the phantom scalar field.
Subfields: Applied Mathematics, Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/d9187636d6b8a2fee283c93a8e6176eb49118a94
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In Applied Mathematics
In Astronomy and Astrophysics
- Yi Wang
- Shuang Wang
- Miao Li
- M. Setare
- Emmanuel N. Saridakis
- Xin Zhang
- Ahmad Sheykhi
- Fotios Anagnostopoulos
In Nuclear and High Energy Physics
- Yi Wang
- Shuang Wang
- Miao Li
- M. Setare
- Emmanuel N. Saridakis
- Xin Zhang
- Ahmad Sheykhi
- Fotios Anagnostopoulos
Citations in the corpus
- Holographic dark energy (2016, methodology): “However, it is interesting to note that with non-trivial potentials, one can use scalar field to reconstruct HDE [365, 366, 367, 368, 369, 370, 371, 372, 373, 374, 375, 376, 377].”
- The holographic dark energy in non-flat Brans–Dicke cosmology (2006, background): “Finally I must mention that in recent work [ 35 ] I have associated the interacting holographic dark energy in non-flat universe with a phantom scalar field.”