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Volumn 51, Issue 5, 1995, Pages 2421-2427

Vacuum oscillations in the supersymmetric standard model

Author keywords

[No Author keywords available]

Indexed keywords


EID: 0001709205     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.51.2421     Document Type: Article
Times cited : (166)

References (47)
  • 1
    • 84927505926 scopus 로고    scopus 로고
    • A. Yu. Smirnov, ICTP Report No. IC/93/388 (unpublished);
  • 8
    • 84927463746 scopus 로고    scopus 로고
    • a recent review can be found in D. P. Roy, invited talk at the X Symposium in High Energy Physics, Bombay, India (unpublished).
  • 24
    • 84927465694 scopus 로고    scopus 로고
    • JETP 64, 4 (1986)
  • 38
    • 84927479531 scopus 로고    scopus 로고
    • Note that the sneutrino VEV is constrained to be < 10 ; keV from stellar cooling in models with spontaneous violation of R parity. The neutrino masses fall in this case in the range appropriate for the MSW solution to the solar neutrino problem.
  • 40
    • 84927482576 scopus 로고    scopus 로고
    • This scenario is, however, not viable in view of the LEP constraints on the invisible width.
  • 42
    • 84927497691 scopus 로고    scopus 로고
    • The nonobservation of the neutralino puts a somewhat more stringent restriction than that of the chargino displayed in Figs. 1 and 2. See, e.g., [18].
  • 46
    • 84927497391 scopus 로고    scopus 로고
    • and further references therein.
  • 47
    • 84927459165 scopus 로고    scopus 로고
    • This follows from the fact that all Oα 4,Oα 5,Oα 6 appear in Eq. (28) and the LSP is never a pure tildeH2; see cite2.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.