id	author	title	date	pages	extension	mime	words	sentences	flesch	summary	cache	txt
work_b675xqoacfcg7b5a2m3jx4ezoa	Roni Harnik	Atmospheric neutrinos can make beauty strange	2004	32	.pdf	application/pdf	10484	1884	83	assumes that these new large mixing angles do not appear in the CKM matrix because the right-handed charged-current interaction is broken at the neutrino mixing angle may appear in the squark mass matrices as a large The squark mass matrix we consider is motivated by models where a large large values of µtanβ, a smaller b̃R-s̃R mixing is allowed. We find, however, that there is a portion of parameter space above the smallest experimentally allowed value of µ tanβ where the right-right mixing diagrams are dominant. The leading Standard Model contribution to Bs mixing is induced by a to have a very large contribution to SφK, one is pushed into a region of parameter space where the gluino, and at least one of the down-type squarks is masses are high, both of which disfavor large contributions to Bs mixing. LR+RR contributions dominate SφK, since in that case large squark masses	./cache/work_b675xqoacfcg7b5a2m3jx4ezoa.pdf	./txt/work_b675xqoacfcg7b5a2m3jx4ezoa.txt