Please use this identifier to cite or link to this item: https://doi.org/10.1051/epjconf/201920609013
Title: Hubble parameter measurement constraints on holographic dark energy
Authors: Lum You Sheng, P.
Ng Shao Chin, C. 
Issue Date: 2018
Publisher: INSPIRE
Citation: Lum You Sheng, P., Ng Shao Chin, C. (2018). Hubble parameter measurement constraints on holographic dark energy. Proceedings - 48th International Symposium on Multiparticle Dynamics, ISMD 2018 : 9013. ScholarBank@NUS Repository. https://doi.org/10.1051/epjconf/201920609013
Rights: Attribution 4.0 International
Abstract: We review and attempt to constrain the ?CDM and XCDM models using 26 Hubble parameter against redshift data points from [1], [2], [3], [4] and [5]. Also known as the cosmic chronometers approach, these constraints are now almost as restrictive as or less than those from Type 1a Supernova (SN1a) apparent magnitude versus redshift data [6]. Then, we attempt to constrain the Holographic Dark Energy model [7] using the aforementioned 26 H(z) measurement. Although interesting, errors for the H(z) could be less well estimated as it is a relatively new measure relative to SN1a data, which has been studied for a much longer time. © The Authors, published by EDP Sciences.
Source Title: Proceedings - 48th International Symposium on Multiparticle Dynamics, ISMD 2018
URI: https://scholarbank.nus.edu.sg/handle/10635/212562
DOI: 10.1051/epjconf/201920609013
Rights: Attribution 4.0 International
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