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Gravitino production from heavy moduli decay and cosmological moduli problem revived
Open accessAbstract
The cosmological moduli problem for relatively heavy moduli fields is reinvestigated. For this purpose we examine the decay of a modulus field at a quantitative level. The modulus dominantly decays into gauge bosons and gauginos, provided that the couplings among them are not suppressed in the gauge kinetic function. Remarkably the modulus decay into a gravitino pair is unsuppressed generically, with a typical branching ratio of order 0.01. Such a large gravitino yield after the modulus decay causes cosmological difficulties. The constraint from the big-bang nucleosynthesis pushes up the gravitino mass above 105GeV. Furthermore to avoid the over-abundance of the stable neutralino lightest superparticles (LSPs), the gravitino must weigh more than about 106GeV for the wino-like LSP, and even more for other neutralino LSPs. This poses a stringent constraint on model building of low-energy supersymmetry.
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Spergel, D. N., Verde, L., Peiris, H. V., Komatsu, E., Nolta, M. R., Bennett, C. L., Halpern, M., Hinshaw, G., Jarosik, N., Kogut, A., et al. (2003) · The Astrophysical Journal Supplement Series · doi:10.1086/377226 · Cited by 10,976
Cited by
Big-bang nucleosynthesis and gravitinos
Kawasaki, M., Kohri, K., Moroi, T., & Yotsuyanagi, A. (2008) · Physical Review D · doi:10.1103/physrevd.78.065011 · Cited by 458
The QCD axion and moduli stabilisation
Conlon, J. P. (2006) · Journal of High Energy Physics · doi:10.1088/1126-6708/2006/05/078 · Cited by 364
Metadata
- Authors
- Nakamura, S., & Yamaguchi, M.
- Venue
- Physics Letters B
- Publisher
- Elsevier BV
- Published
- 2006-07
- Volume
- 638
- Issue
- 5-6
- Pages
- 389-395
- ISSN
- 0370-2693 (ISSN-L)
- OpenAlex
- W2077458907
- Cited by
- 206
- References
- 1
- FWCI
- 12.49
- Type
- journal article
- Language
- en
- Open access
- hybrid
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- Nakamura, S., & Yamaguchi, M. (2006). Gravitino production from heavy moduli decay and cosmological moduli problem revived. Physics Letters B. https://doi.org/10.1016/j.physletb.2006.05.078
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