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Dark matter and modified Newtonian dynamics in a sample of high-redshift galaxy clusters observed with Chandra

✍ Scribed by Carl Blaksley; Massimiliano Bonamente


Publisher
Elsevier Science
Year
2010
Tongue
English
Weight
927 KB
Volume
15
Category
Article
ISSN
1384-1076

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✦ Synopsis


We compare the measurement of the gravitational mass of 38 high-redshift galaxy clusters observed by Chandra using Modified Newtonian Dynamics (MOND) and standard Newtonian gravity. Our analysis confirms earlier findings that MOND cannot explain the difference between the baryonic mass and the total mass inferred from the assumption of hydrostatic equilibrium. We also find that the baryon fraction at r 2500 using MOND is consistent with the Wilkinson Microwave Anisotropy Probe (WMAP) value of