Calculations of relic densities in the early universe

Mark Srednicki; Richard Watkins; Keith A. Olive

doi:10.1016/0550-3213(88)90099-5

Calculations of relic densities in the early universe

Mark Srednicki, Richard Watkins, Keith A. Olive

Physics and Astronomy (Twin Cities)

Research output: Contribution to journal › Article › peer-review

341 Scopus citations

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	https://doi.org/10.1016/0550-3213(88)90099-5
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.

Publisher link

10.1016/0550-3213(88)90099-5

Find It

Find It at U of M Libraries

Cite this

@article{a88c182e677c44f69e58671f7456a98b,

title = "Calculations of relic densities in the early universe",

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.",

author = "Mark Srednicki and Richard Watkins and Olive, {Keith A.}",

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.",

year = "1988",

month = dec,

day = "12",

doi = "10.1016/0550-3213(88)90099-5",

language = "English (US)",

volume = "310",

pages = "693--713",

journal = "Nuclear Physics, Section B",

issn = "0550-3213",

publisher = "Elsevier",

number = "3-4",

}

TY - JOUR

T1 - Calculations of relic densities in the early universe

AU - Srednicki, Mark

AU - Watkins, Richard

AU - Olive, Keith A.

N1 - 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.

PY - 1988/12/12

Y1 - 1988/12/12

N2 - 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.

AB - 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.

UR - http://www.scopus.com/inward/record.url?scp=44849086566&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=44849086566&partnerID=8YFLogxK

U2 - 10.1016/0550-3213(88)90099-5

DO - 10.1016/0550-3213(88)90099-5

M3 - Article

AN - SCOPUS:44849086566

SN - 0550-3213

VL - 310

SP - 693

EP - 713

JO - Nuclear Physics, Section B

JF - Nuclear Physics, Section B

IS - 3-4

ER -

Calculations of relic densities in the early universe

Abstract

Bibliographical note

Publisher link

Find It

Other files and links

Fingerprint

Cite this