Probability of the most massive cluster under non-Gaussian initial conditions

Very massive high redshift clusters can be used to constrain and test the Lambda CDM model. Taking into account the observational constraints of Jee et al. (2009) we have calculated the probability for the most massive cluster to be found in the range (5.2-7.6)e14 M_sun, between redshifts 1.4-2.2, w...

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Veröffentlicht in:	arXiv.org 2011-03
Hauptverfasser:	Cayón, Laura, Gordon, Christopher, Silk, Joseph
Format:	Artikel
Sprache:	eng
Schlagworte:	Big Bang theory Clusters Constraint modelling Cosmic microwave background Initial conditions Physics - Cosmology and Nongalactic Astrophysics Physics - General Relativity and Quantum Cosmology Physics - High Energy Physics - Phenomenology Physics - High Energy Physics - Theory Red shift
Online-Zugang:	Volltext
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