Constraints on holographic dark energy from X-ray gas mass fraction of galaxy clusters
Authors:
- Zhe ChangZCZhe Chang
- Feng-Quan WuFWFeng-Quan Wu
- Xin ZhangXin Zhang
Open Access
- 1 February 2006
- journal article
- research article
- Published by Elsevier in Physics Letters B
- Vol. 633 (1) , 14-18
Abstract
No abstract availableKeywords
All Related Versions
This publication has 61 references indexed in Scilit:
- The Three‐Dimensional Power Spectrum of Galaxies from the Sloan Digital Sky SurveyThe Astrophysical Journal, 2004
- Cosmological parameters from SDSS and WMAPPhysical Review D, 2004
- First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Preliminary Maps and Basic ResultsThe Astrophysical Journal Supplement Series, 2003
- First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Determination of Cosmological ParametersThe Astrophysical Journal Supplement Series, 2003
- Cosmological constant—the weight of the vacuumPhysics Reports, 2003
- The cosmological constant and dark energyReviews of Modern Physics, 2003
- The Cosmological ConstantLiving Reviews in Relativity, 2001
- Measurements of Ω and Λ from 42 High‐Redshift SupernovaeThe Astrophysical Journal, 1999
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological ConstantThe Astronomical Journal, 1998
- The cosmological constant problemReviews of Modern Physics, 1989