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Aspects of spin-dependent dark matter search

  • NANP-2003 Proceedings of the Fourth International Conference on “Nonaccelerator New Physics” Joint Institute for Nuclear Research Dubna, Russia June 23–28, 2003
  • Dark Matter
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Abstract

The Weakly Interacting Massive Particle (WIMP) is the main candidate for the relic dark matter. A set of exclusion curves currently obtained for cross sections of spin-dependent WIMP-proton and WIMP-neutron interaction is given. A two-orders-of-magnitude improvement of the sensitivity of the dark matter experiment is needed to reach the SUSY predictions for relic neutralinos. It is noted that new experiments with the high-spin isotope 73Ge can yield a new important constraint on the neutralino-neutron effective coupling and the SUSY parameter space.

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Authors and Affiliations

  1. Joint Institute for Nuclear Research, Dubna, Moscow oblast, 141980, Russia

    V. A. Bednyakov

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  1. V. A. Bednyakov
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Additional information

From Yadernaya Fizika, Vol. 67, No. 11, 2004, pp. 1957–1966.

Original English Text Copyright © 2004 by Bednyakov.

This article was submitted by the author in English.

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Bednyakov, V.A. Aspects of spin-dependent dark matter search. Phys. Atom. Nuclei 67, 1931–1941 (2004). https://doi.org/10.1134/1.1825508

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  • DOI: https://doi.org/10.1134/1.1825508

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