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Advances in High Energy Physics - Volume 2014 2014, Article ID 681312, 19 pages -

Review ArticleInstitut d-Astrophysique, CNRS, UMR 7095 & Université Pierre et Marie Curie, 98 bis Boulevard Arago, 75014 Paris, France

Received 9 January 2014; Accepted 3 February 2014; Published 16 April 2014

Academic Editor: Anselmo Meregaglia

Copyright © 2014 Paolo Panci. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. The publication of this article was funded by SCOAP



I present the status of direct dark matter detection with specific attention to the experimental results and their phenomenological interpretation in terms of dark matter interactions. In particular I review a new and more general approach to study signals in this field based on nonrelativistic operators which parametrize more efficiently the dark matter-nucleus interactions in terms of a very limited number of relevant degrees of freedom. Then I list the major experimental results, pointing out the main uncertainties that affect the theoretical interpretation of the data. Finally, since the underlying theory that describes both the dark matter and the standard model fields is unknown, I address the uncertainties coming from the nature of the interaction. In particular, the phenomenology of a class of models in which the interaction between dark matter particles and target nucleiis of a long range type is discussed.

Author: Paolo Panci



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