2006AIP conference proceedingsRequires access

Search for Dark Matter with space experiments

A. Morselli

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Abstract

The detection of gamma‐rays, antiprotons and positrons due to pair annihilation of dark matter particles in the Milky Way halo is a viable tecniques to search for supersymmetric dark matter candidates if there is the possibility to separate the signal from the backgroung generated by standard production mechanisms. Here we discuss the status of this indirect search and the prospective for the experiments GLAST and PAMELA.

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What this paper is about

The detection of gamma‐rays, antiprotons and positrons due to pair annihilation of dark matter particles in the Milky Way halo is a viable tecniques to search for supersymmetric dark matter candidates if there is the possibility to separate the signal from the backgroung generated by standard production mechanisms. Here we discuss the status of this indirect search and the prospective for the experiments GLAST and PAMELA.

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Available abstract

The detection of gamma‐rays, antiprotons and positrons due to pair annihilation of dark matter particles in the Milky Way halo is a viable tecniques to search for supersymmetric dark matter candidates if there is the possibility to separate the signal from the backgroung generated by standard production mechanisms. Here we discuss the status of this indirect search and the prospective for the experiments GLAST and PAMELA.

Key concepts: Dark matter, Physics, Milky Way, Annihilation, Antiproton, Positron, Particle physics, Halo

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