A MODEL OF HOLOGRAPHIC DARK ENERGY
By Miao Li. 2004
1,729 citations recorded by the source corpus.
A model for holographic dark energy is proposed, following the idea that the short distance cut-off is related to the infrared cut-off. We assume that the infrared cut-off relevant to the dark energy is the size of the event horizon. With the input Omega(Lambda) = 0.73, we predict the equation of state of the dark energy at the present time be characterized by w = -0.90. The cosmic coincidence problem can be resolved by inflation in our scenario, provided we assume the minimal number of e-foldings. (C) 2004 Elsevier B.V. All rights reserved.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/a151e6bc400c4f8049d7911912dcecd669cc520e
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In Astronomy and Astrophysics
- Emmanuel N. Saridakis
- Sergei D. Odintsov
- Shuang Wang
- Yi Wang
- Ratbay Myrzakulov
- Xin Zhang
- Kazuharu Bamba
- Miao Li
In Nuclear and High Energy Physics
- Emmanuel N. Saridakis
- Sergei D. Odintsov
- Shuang Wang
- Yi Wang
- Ratbay Myrzakulov
- Kazuharu Bamba
- Xin Zhang
- Miao Li
Citations in the corpus
- Categorizing Different Approaches to the Cosmological Constant Problem (2004, background): “More recently however, another proposal was made [41] where instead L is taken to be proportional to the size of the future event horizon:”