Cosmic distance duality relation and the shape of galaxy clusters

DOI10.1051/0004-6361/201015547zbMath1260.85132arXiv1003.5906OpenAlexW2164310534WikidataQ68998071 ScholiaQ68998071MaRDI QIDQ4905687

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Publication date: 20 February 2013

Published in: Astronomy & Astrophysics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1003.5906

zbMATH Keywords

X-raysdistance scalecosmic background radiationgalaxies: clustersSunyaev-Zeldovich effect (SZE)

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Galactic and stellar dynamics (85A05) Equations of motion in general relativity and gravitational theory (83C10) General questions in astronomy and astrophysics (85A04) Astrophysical cosmology (85A40)

Related Items (6)

Testing the distance-duality relation from Hubble, galaxy clusters and type ia supernovae data with model independent methods ⋮ Testing the violation of the equivalence principle in the electromagnetic sector and its consequences in f(T) gravity ⋮ Galaxy clusters, cosmic chronometers and the Einstein equivalence principle ⋮ Improved constraints on violations of the Einstein equivalence principle in the electromagnetic sector with complementary cosmic probes ⋮ New constraints on \(H _{0}\) and \(\Omega _{m }\) from SZE/X-ray data and baryon acoustic oscillations ⋮ CONSTRAINTS ON THE HUBBLE PARAMETER FROM GALAXY CLUSTERS AND THE VALIDITY OF THE COSMIC DISTANCE DUALITY RELATION

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