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Vector dark energy and high-z massive clusters

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arxiv 1108.4173 v3 pith:X3HKJA4S submitted 2011-08-21 astro-ph.CO

Edoardo Carlesi , Alexander Knebe , Gustavo Yepes , Stefan Gottloeber , Jose Beltran Jimenez , Antonio L. Maroto This is my paper · ORCID
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keywords clustersdarkdetectionenergymassiveobjectsspt-clvector
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abstract

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 \LCDM$\;$cosmology. In fact,assuming Gaussian initial conditions, the theoretical expectation of detecting such objects is as low as $\leq 1%$. In this \textit{Letter} we discuss the probability of the existence of such objects in the light of the Vector Dark Energy (VDE) paradigm, showing by means of a series of $N$-body simulations that chances of detection are substantially enhanced in this non-standard framework.

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