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Vector dark energy and high-z massive clusters

Carlesi, Edoardo ; Knebe, Alexander ; Yepes, Gustavo ; Gottlöber, Stefan ; Jiménez, Jose Beltrán ; Maroto, Antonio L.

In: Monthly Notices of the Royal Astronomical Society, 2011, vol. 418, no. 4, p. 2715-2719

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    Titre
    • Vector dark energy and high-z massive clusters
    Auteur
    • Carlesi, Edoardo. Departamento de Física Teórica, Universidad Autónoma de Madrid, 28049 Cantoblanco, Madrid, Spain
    • Knebe, Alexander. Departamento de Física Teórica, Universidad Autónoma de Madrid, 28049 Cantoblanco, Madrid, Spain
    • Yepes, Gustavo. Departamento de Física Teórica, Universidad Autónoma de Madrid, 28049 Cantoblanco, Madrid, Spain
    • Gottlöber, Stefan. Leibniz Institut für Astrophysik, An der Sternwarte 16, 14482 Potsdam, Germany
    • Jiménez, Jose Beltrán. Institute de Physique Théorique and Center for Astroparticle Physics, Université de Genève, 24 quai E. Ansermet, 1211 Genève, Switzerland
    • Maroto, Antonio L.. Departamento de Física Teórica, Universidad Complutense de Madrid, 28040 Madrid, Spain
    Type de document
    • Postprint
    Langue
    • Inglese
    Publié dans
    • Monthly Notices of the Royal Astronomical Society, 2011, vol. 418, no. 4, p. 2715-2719. Blackwell Publishing Ltd
    Autre version électronique
    Identifiant OAI-PMH
    • oai:doc.rero.ch:298108
    Summary
    The detection of extremely massive clusters at z > 1 such as SPT-CL J0546−5345, SPT-CL J2106−5844 and XMMU J2235.3−2557 has been considered by some authors as a challenge to the standard Λ cold dark matter cosmology. In fact, assuming Gaussian initial conditions, the theoretical expectation of detecting such objects is as low as ≤1 per cent. In this paper we discuss the probability of the existence of such objects in the light of the vector dark energy paradigm, showing by means of a series of N-body simulations that chances of detection are substantially enhanced in this non-standard framework