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Volumn 61, Issue 3, 2000, Pages

Constraints on mixing angles of Majorana neutrinos

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EID: 18144430635     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.61.031301     Document Type: Article
Times cited : (22)

References (51)
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    • K. Zuber, Phys. Rep. 305, 295 (1998) we have corrected some printing errors in the mixing matrix given in this report.
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    • Zuber, K.1
  • 25
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    • H. Päs (private communication).
    • Päs, H.1
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    • Although the observations of high redshift supernovae have been interpreted
    • Although the observations of high redshift supernovae have been interpreted 19 in terms of a nonvanishing cosmological constant (Formula presented) cosmological models with (Formula presented) do not provide good fit to the structure data (CMBR anisotropies and the large-scale structure). Leaving this puzzle to be resolved by the cosmologists, we shall stick to Eq. (6) and deduce the consequences for neutrino physics.
  • 33
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    • B.P. Schmidt, astro-ph/9805200.
    • Schmidt, B.P.1
  • 34
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    • Although specific value for (Formula presented) is mentioned here as well as below, it must be scaled suitably if the calculated value of the nuclear matrix element in neutrinoless double beta decay changes or if the experimental limit on this decay improves, since only the ratio of the upper limit of (Formula presented) to (Formula presented) enters into our analysis
    • Although specific value for (Formula presented) is mentioned here as well as below, it must be scaled suitably if the calculated value of the nuclear matrix element in neutrinoless double beta decay changes or if the experimental limit on this decay improves, since only the ratio of the upper limit of (Formula presented) to (Formula presented) enters into our analysis.
  • 35
  • 44
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    • fact this has already happened; according to Reference
    • In fact this has already happened; according to Reference 25, (Formula presented) at 90% C.L.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.