Constraints on holographic dark energy from X-ray gas mass fraction of galaxy clusters
By Z. Chang, Fengquan Wu, Xin Zhang. 2005
180 citations recorded by the source corpus.
We use the Chandra measurements of the X-ray gas mass fraction of 26 rich clusters released by Allen et al. to perform constraints on the holographic dark energy model. The constraints are consistent with those from other cosmological tests, especially with the results of a joint analysis of supernovae, cosmic microwave background, and large scale structure data. From this test, the holographic dark energy also tends to behave as a quintom-type dark energy. (c) 2005 Elsevier B.V All rights reserved.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/b4014b63032a596bd96dc917cde9501be654a526
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Citations in the corpus
- Constraints on holographic dark energy from the latest supernovae, galaxy clustering, and cosmic microwave background anisotropy observations (2007, methodology): “In previous work, for instance, [64] and [65], the 1-σ range of c obtained can basically exclude the probability of c > 1 giving rise to the quintessence-like behavior, supporting the quintomlike behavior evidently.”
- Holographic dark energy (2016, unknown): “16 [221] Chandra(X-ray gas mass fraction) 0.”