Supersymmetric Dark Matter
This course was given in the 'First school of Astroparticle Physics in
Argentina' in Buenos Aires, Argentina in March, 1999. The course was
divided into four lectures of 45 minutes each. The transparancies are
given as colour postscript files (gzipped).
- Introduction. (1 page, 29 kB)
- Lecture 1. Introduction to the
MSSM. (22 pages, 235 kB)
- Lecture 2. Accelerator constraints
and relic density calculation. (20 pages, 215 kB)
- Lecture 3. Direct detection and
neutrino-induced muons at neutrino-telescopes. (20 pages, 237 kB)
- Lecture 4. Other indirect
detection methods (signatures from the halo). (21 pages, 314 kB)
- Summary. (2 pages, 37 kB)
- Extra. Some more plots on indirect
and direct detection. (4 pages, 101 kB)
- Details. Feynmann
diagrams for relic density calculation and for gamma lines. (7
pages, 97 kB)
This page was last updated April 16, 1999.