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Volumn 597, Issue 3-4, 2004, Pages 321-327

δT/T and neutrino masses in SU(5)

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PROTON;

EID: 4344618071     PISSN: 03702693     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.physletb.2004.07.030     Document Type: Article
Times cited : (12)

References (71)
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    • C.L. Bennett Astrophys. J. 464 1996 L1 astro-ph/9601067 There is some (weak) evidence for a running spectral index with d n s / d ln k ≈ - 5 × 10 - 2. We will consider the simplest models which yield d n s / d ln k ≲ - 10 - 3. However, more complicated scenarios would yield more than one inflationary epoch, in which case d n s / d ln k could be significantly larger
    • (1996) Astrophys. J. , vol.464
    • Bennett, C.L.1
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    • For an earlier discussion see L. Covi, G. Mangano, A. Masiero, and G. Miele Phys. Lett. B 424 1998 253 hep-ph/9707405 The U (1) R symmetry was not fully exploited in this Letter
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    • Covi, L.1    Mangano, G.2    Masiero3    Miele, G.A.4
  • 19
    • 84862415345 scopus 로고    scopus 로고
    • See also T. Watari, and T. Yanagida hep-ph/0402125
    • Watari1    Yanagida2
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    • 4243734527 scopus 로고    scopus 로고
    • Superkamiokande CollaborationFukuda S.*et al.
    • Superkamiokande Collaboration S. Fukuda Phys. Rev. Lett. 85 2000 3999
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    • Q. Shafi, and A. Vilenkin Phys. Rev. D 29 1984 1870 This paper discusses inflation with SU (5) × U (1) X in a non-supersymmetric setting
    • (1984) Phys. Rev. D , vol.29 , pp. 1870
    • Shafi1    Vilenkin, A.Q.2
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    • Harvard preprint HUTP-80/A031 (1980) University of New Hampshire, April 10-12
    • E. Witten, Harvard preprint HUTP-80/A031 (1980), presented at First Workshop on Grand Unification, University of New Hampshire, April 10-12, 1980
    • (1980) First Workshop on Grand Unification
    • Witten, E.1
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    • For leptogenesis in the context of GUT inflation, see G. Lazarides, and Q. Shafi Phys. Lett. B 258 1991 305
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    • Lazarides1    Shafi, Q.G.2
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    • (in Russian), the bound T r < 3 × 10 6 GeV is obtained from the observed Li-6 abundance
    • M.Yu. Khlopov, Yu.L. Levitan, E.V. Sedelnikov, and I.M. Sobol Phys. At. Nucl. 57 1994 1393 Yad. Fiz. 57 1994 1466 (in Russian), the bound T r < 3 × 10 6 GeV is obtained from the observed Li-6 abundance
    • (1994) Yad. Fiz. , vol.57 , pp. 1466
  • 51
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    • This can be satisfied in inflationary models discussed in V.N. Senoguz, and Q. Shafi hep-ph/0403294
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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.