Supersymmetric scenarios with dominant radiative neutralino decay
- Randall Physics Laboratory, University of Michigan, Ann Arbor, Michigan 48109-1120 (United States)
- INFN, Sezione di Roma 1 and University La Sapienza, Rome (Italy)
The radiative decay of the next-to-lightest neutralino into a lightest neutralino and a photon is analyzed in the minimal supersymmetric standard model. We find that significant regions of the supersymmetric parameter space with large radiative branching ratios (up to about 100{percent}) do exist. The radiative channel turns out to be enhanced when the neutralino tree-level decays are suppressed either {open_quotes}kinematically{close_quotes} or {open_quotes}dynamically.{close_quotes} In general, in the regions allowed by data from CERN LEP and not characterized by asymptotic values of the supersymmetric parameters, the radiative enhancement requires tan{beta}{approx_equal}1 and/or M{sub 1}{approx_equal}M{sub 2}, and negative values of {mu}. We present typical scenarios where these conditions are satisfied, relaxing the usual relation M{sub 1}=(5/3)tan{sup 2}{theta}{sub W}M{sub 2}, i.e., gaugino mass unification at the grand unified theory scale. The influence of varying the top-squark masses and mixing angle when the radiative decay is enhanced is also considered. Some phenomenological consequences of the above picture are discussed. {copyright} {ital 1997} {ital The American Physical Society}
- OSTI ID:
- 450545
- Journal Information:
- Physical Review, D, Journal Name: Physical Review, D Journal Issue: 3 Vol. 55; ISSN 0556-2821; ISSN PRVDAQ
- Country of Publication:
- United States
- Language:
- English
Similar Records
Relic density of neutralino dark matter in supergravity models
Supersymmetric dark matter in the light of CERN LEP and the Fermilab Tevatron collider
Role of W-ino content in neutralino dark matter
Journal Article
·
Sat Feb 28 23:00:00 EST 1998
· Physical Review, D
·
OSTI ID:615340
Supersymmetric dark matter in the light of CERN LEP and the Fermilab Tevatron collider
Journal Article
·
Sun Oct 01 00:00:00 EDT 2000
· Physical Review. D, Particles Fields
·
OSTI ID:20217744
Role of W-ino content in neutralino dark matter
Journal Article
·
Sun Jul 01 00:00:00 EDT 2001
· Physical Review D
·
OSTI ID:40204485