Published September 2011
| public
Journal Article
Direct Detection of Vector Dark Matter
Chicago
Abstract
In this paper, we complete formulae for the elastic scattering cross section of general vector dark matter with nucleons in the direct detection at the leading order of the strong coupling constant α_s, assuming that the dark matter is composed of vector particles and interacts with heavy fermions with color charge as well as standard-model quark. As an application of our formulae, the direct detection of the first Kaluza-Klein photon in the minimal universal extra dimension model is discussed. It is found that the scattering cross section is larger than those in the previous works by up to a factor of ten.
Additional Information
© 2011 Progress of Theoretical Physics. Received June 28, 2011. The work was supported in part by Grants-in-Aid from the Ministry of Education, Culture, Sports, Science and Technology (MEXT), Government of Japan, No. 20244037, No. 2054252, and No. 2244021 (J.H.). The work of J.H. is also supported by the World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan. This work was also supported in part by the U.S. Department of Energy under contract No. DE-FG02-92ER40701, and by the Gordon and Betty Moore Foundation (K.I.).Additional details
- Eprint ID
- 27651
- DOI
- 10.1143/PTP.126.435
- Resolver ID
- CaltechAUTHORS:20111107-115404879
- Ministry of Education, Culture, Sports, Science and Technology (MEXT), Government of Japan
- 20244037
- Ministry of Education, Culture, Sports, Science and Technology (MEXT), Government of Japan
- 2054252
- Ministry of Education, Culture, Sports, Science and Technology (MEXT), Government of Japan
- 2244021
- World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan
- Department of Energy (DOE)
- DE-FG02-92ER40701
- Gordon and Betty Moore Foundation
- Created
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2011-11-08Created from EPrint's datestamp field
- Updated
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2021-11-09Created from EPrint's last_modified field
- Caltech groups
- Caltech Theory, Moore Center for Theoretical Cosmology and Physics