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CERN Document Server Encontrados 3 registros  La búsqueda tardó 0.57 segundos. 
1.
A solution to the $^7$Li problem by the long lived stau / Jittoh, Toshifumi ; Kohri, Kazunori ; Koike, Masafumi ; Sato, Joe ; Shimomura, Takashi ; Yamanaka, Masato
2008 - Published in : AIP Conf. Proc.: 1006 (2008) , pp. 126-129 External link: Published version from AIP
In : UAE-CERN Workshop on High Energy Physics and Applications, Al Ain, United Arab Emirates, 26 - 28 Nov 2007, pp.126-129
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2.
Black hole formation and slow-roll inflation / Kohri, Kazunori (Lancaster U.) ; Lyth, David H. (Lancaster U.) ; Melchiorri, Alessandro (Rome U. ; INFN, Rome)
Black hole formation may occur if the spectrum of the curvature perturbation \zeta increases strongly as the scale decreases. As no such increase is observed on cosmological scales, black hole formation requires strongly positive running n' of the spectral index n, though the running might only kick in below the `cosmological scales' probed by the CMB anisotropy and galaxy surveys. [...]
arXiv:0711.5006; CERN-PH-TH-2007-242; CERN-PH-TH-2007-242.- 2008 - 11 p. - Published in : JCAP 04 (2008) 038 Fulltext: PDF; External link: Preprint
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3.
Neutralino Warm Dark Matter / Hisano, Junji (KEK, Tsukuba ; CERN) ; Kohri, Kazunori (Kyoto U., Yukawa Inst., Kyoto) ; Nojiri, Mihoko M. (Kyoto U., Yukawa Inst., Kyoto)
In the supersymmetric (SUSY) standard model, the lightest neutralino may be the lightest SUSY particle (LSP), and it is is a candidate of the dark matter in the universe. The LSP dark matter might be produced by the non-thermal process such as heavy particle decay after decoupling of the thermal relic LSP. [...]
hep-ph/0011216; KEK-TH-725; CERN-TH-2000-338; YITP-00-62; CERN-TH-2000-338; KEK-TH-725; YITP-2000-62.- Geneva : CERN, 2001 - 13 p. - Published in : Phys. Lett. B 505 (2001) 169-176 Access to fulltext document: PDF; Fulltext: PDF; External link: Preprint - Please contact the library if you need to access this document.
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Vea también: autores con nombres similares
42 Kohri, K
8 Kohri, K.
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