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Volumn 56, Issue 2, 1997, Pages 1324-1327

Supersymmetric inflation with constraints on superheavy neutrino masses

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Indexed keywords


EID: 0000810627     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.56.1324     Document Type: Article
Times cited : (139)

References (23)
  • 3
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    • Phys. Rev. D 49, 748 (1994).
    • (1994) Phys. Rev. D , vol.49 , pp. 748
  • 5
    • 0003753693 scopus 로고
    • Harwood Academic, Switzerland
    • Supersymmetric inflation has a long history and there are several reviews available, see, e.g., A. D. Linde, Particle Physics and Inflationary Cosmology (Harwood Academic, Switzerland, 1990).
    • (1990) Particle Physics and Inflationary Cosmology
    • Linde, A.D.1
  • 6
    • 85038338025 scopus 로고    scopus 로고
    • The soft supersymmetry-breaking scalar masses can be safely ignored
    • The soft supersymmetry-breaking scalar masses can be safely ignored.
  • 8
    • 85038330633 scopus 로고    scopus 로고
    • The supergravity-induced inflaton mass remains exactly zero even if we include in (Formula presented) all possible nonrenormalizable terms involving (Formula presented), (Formula presented), (Formula presented) allowed by the gauge and (Formula presented) symmetries, and with a minimal Kähler potential [see first reference in [3
    • The supergravity-induced inflaton mass remains exactly zero even if we include in (Formula presented) all possible nonrenormalizable terms involving (Formula presented), (Formula presented), (Formula presented) allowed by the gauge and (Formula presented) symmetries, and with a minimal Kähler potential [see first reference in and
  • 9
    • 33748954944 scopus 로고
    • The fact that (Formula presented) plays a crucial role if higher order terms are included in the Kähler potential. The inflaton mass can then be kept (Formula presented) with only a mild tuning of just one parameter [G. Dvali (private communication)]. In many other inflationary scenarios one needs to adjust an infinite number of parameters
    • E. D. Stewart, Phys. Rev. D 51, 6847 (1995).] The fact that (Formula presented) plays a crucial role if higher order terms are included in the Kähler potential. The inflaton mass can then be kept (Formula presented) with only a mild tuning of just one parameter [G. Dvali (private communication)]. In many other inflationary scenarios one needs to adjust an infinite number of parameters.
    • (1995) Phys. Rev. D , vol.51 , pp. 6847
    • Stewart, E.D.1
  • 12
    • 85038321822 scopus 로고    scopus 로고
    • K. S. Babu (private communication).
    • Babu, K.S.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.