Indirect Detection of Neutralino Dark Matter

@inproceedings{Dalberg1999IndirectDO,
  title={Indirect Detection of Neutralino Dark Matter},
  author={Eva Dalberg},
  year={1999}
}
Since neutralinos are Majorana particles, they can annihilate pair-wise and form standard model matter. This can be done either in the dark matter halo itself or once the neutralinos have been gravitationally trapped and have accumulated in the center of the Sun or the Earth. The annihilation products can form detectable uxes, for example in the form of anti-protons or neutrinos. Some characteristics of these signals will be reviewed. Examples of ongoing and future experimental e orts to detect… CONTINUE READING

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