Higgs-mediated K{yields}{pi}{nu}{nu} in the MSSM at large tan{beta}
Journal Article
·
· Physical Review. D, Particles Fields
- INFN, Laboratori Nazionali di Frascati, I-00044 Frascati (Italy)
- INFN, Sezione di Roma II and Dipartimento di Fisica, Universita di Roma 'Tor Vergata', I-00133 Rome (Italy)
We analyze the impact of Higgs-mediated amplitudes on the rare decays K{sub L}{yields}{pi}{sup 0}{nu}{nu} and K{sup +}{yields}{pi}{sup +}{nu}{nu} in the MSSM with large tan{beta} and general flavor mixing. We point out that, going beyond the minimal flavor violation hypothesis, Z-penguin amplitudes generated by charged-Higgs exchange can induce sizable modifications of K{yields}{pi}{nu}{nu} rates. Interestingly, these effects scale as tan{sup 4}{beta} at the amplitude level. For large values of tan{beta}, this mechanism allows deviations from the SM expectations even for tiny (Cabibbo-Kobayashi-Maskawa-type) off-diagonal mixing terms in the right-handed squark sector.
- OSTI ID:
- 20776904
- Journal Information:
- Physical Review. D, Particles Fields, Vol. 73, Issue 5; Other Information: DOI: 10.1103/PhysRevD.73.055017; (c) 2006 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA); ISSN 0556-2821
- Country of Publication:
- United States
- Language:
- English
Similar Records
b{yields}s{nu}{nu} decay in the MSSM: Implication of b{yields}s{gamma} at large tan{beta}
Branching ratios and CP asymmetries of B{yields}a{sub 1}(1260){pi} and a{sub 1}(1260)K decays
Charm quark contribution to K+ ---> pi+ nu anti-nu at next-to-next-to-leading order
Journal Article
·
Tue Jan 01 00:00:00 EST 2008
· Physical Review. D, Particles Fields
·
OSTI ID:20776904
Branching ratios and CP asymmetries of B{yields}a{sub 1}(1260){pi} and a{sub 1}(1260)K decays
Journal Article
·
Thu Nov 01 00:00:00 EDT 2007
· Physical Review. D, Particles Fields
·
OSTI ID:20776904
Charm quark contribution to K+ ---> pi+ nu anti-nu at next-to-next-to-leading order
Journal Article
·
Wed Mar 01 00:00:00 EST 2006
· JHEP 0611:002,2006
·
OSTI ID:20776904
+1 more