Abstract
The cosmological relic densities of stable particles are calculated to high precision. The results depend on assumptions made about the quark-hadron phase transition. We discuss in detail the calculation of the thermally averaged annihilation cross section. We consider the specific cases of photinos, higgsinos, and Dirac and Majorana neutrinos.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 693-713 |
| Number of pages | 21 |
| Journal | Nuclear Physics, Section B |
| Volume | 310 |
| Issue number | 3-4 |
| DOIs | |
| State | Published - Dec 12 1988 |
Bibliographical note
Funding Information:The work of M.S. and R.W. was supported in part by NSF Grant No. PHY-86-14185. M.S. also acknowledges the receipt of a Research Fellowship from the Alfred P. Sloan Foundation. The work of K.A.O. was supported in part by DOE Grant No. DE-AC02-83ER-40105, and by a Presidential Young Investigator Award.