z-logo
open-access-imgOpen Access
Search for Dark Matter with space experiments
Author(s) -
A. Morselli
Publication year - 2006
Publication title -
aip conference proceedings
Language(s) - English
Resource type - Conference proceedings
SCImago Journal Rank - 0.177
H-Index - 75
eISSN - 1551-7616
pISSN - 0094-243X
DOI - 10.1063/1.2409075
Subject(s) - dark matter , physics , milky way , annihilation , antiproton , positron , particle physics , halo , dark matter halo , astrophysics , scalar field dark matter , astronomy , nuclear physics , cosmology , galaxy , electron , dark energy , proton
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.

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom