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|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 , , ,  and . 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 . Then, we attempt to constrain the Holographic Dark Energy model  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|
|Appears in Collections:||Staff Publications|
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