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Volumn 71, Issue 8, 2005, Pages 1-10

Shining on an orbifold

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; COSMOLOGICAL PHENOMENA; COSMOS; GRAVITY; MATHEMATICAL ANALYSIS; MATHEMATICAL PARAMETERS; NUCLEAR PHYSICS; THEORETICAL MODEL;

EID: 18444419133     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.71.085013     Document Type: Article
Times cited : (1)

References (23)
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    • 0030524154 scopus 로고    scopus 로고
    • The only problem with the Polonyi model is that it might conflict with cosmological constraints such as big bang nucleosynthesis. For a nice description on how to fix such problems, see T. Moroi, Prog. Theor. Phys. Suppl. 123, 457 (1996).
    • (1996) Prog. Theor. Phys. Suppl. , vol.123 , pp. 457
    • Moroi, T.1
  • 18
    • 0002973180 scopus 로고
    • E. Cremmer, S. Ferrara, C. Kounnas, and D.V. Nanopoulos, Phys. Lett. 133B, 61 (1983); J. Bagger, E. Poppitz, and L. Randall, Nucl. Phys. B455, 59 (1995).
    • (1995) Nucl. Phys. , vol.B455 , pp. 59
    • Bagger, J.1    Poppitz, E.2    Randall, L.3
  • 20
    • 0004057466 scopus 로고
    • University of Chicago Press, Chicago
    • R. M. Wald, General Relativity (University of Chicago Press, Chicago, 1984).
    • (1984) General Relativity
    • Wald, R.M.1
  • 23
    • 84927781096 scopus 로고    scopus 로고
    • note
    • This actually only works if you ignore the gravitational dynamics. For instance, the action in Eq. (2) includes the term φ∂ μφ∂μB5 + h.c., which is not 5D Lorentz invariant or gauge invariant. In this paper, however, we are only dealing with constant fields and therefore this error is not a problem. I thank M. Son and M. Luty for bringing this to my attention.


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