We discuss possible large contributions to B→Xsγ, which can occur at the next-to-leading order in supersymmetric models. They can originate from terms enhanced by tan β factors, when the ratio between the two Higgs vacuum expectation values is large, or by logarithm of MSUSY/MW, when the supersymmetric particles are considerably heavier than the W boson. We give compact formulae which include all potentially large higher-order contributions. We find that tan β terms at the next-to-leading order do not only appear from the Hall-Rattazzi-Sarid effect (the modified relation between the bottom mass and Yukawa coupling), but also from an analogous effect in the top-quark Yukawa coupling. Finally, we show how next-to-leading order corrections, in the large tan β region, can significantly reduce the limit on the charged-Higgs mass, even if supersymmetric particles are very heavy.

B→Xsγ in supersymmetry: large contributions beyond the leading order

GAMBINO, Paolo;
2000-01-01

Abstract

We discuss possible large contributions to B→Xsγ, which can occur at the next-to-leading order in supersymmetric models. They can originate from terms enhanced by tan β factors, when the ratio between the two Higgs vacuum expectation values is large, or by logarithm of MSUSY/MW, when the supersymmetric particles are considerably heavier than the W boson. We give compact formulae which include all potentially large higher-order contributions. We find that tan β terms at the next-to-leading order do not only appear from the Hall-Rattazzi-Sarid effect (the modified relation between the bottom mass and Yukawa coupling), but also from an analogous effect in the top-quark Yukawa coupling. Finally, we show how next-to-leading order corrections, in the large tan β region, can significantly reduce the limit on the charged-Higgs mass, even if supersymmetric particles are very heavy.
2000
0012
009
-
http://iopscience.iop.org/1126-6708/2000/12/009/
Giuseppe Degrassi; Paolo Gambino; Gian Francesco Giudice
File in questo prodotto:
Non ci sono file associati a questo prodotto.

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2318/104602
Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus 297
  • ???jsp.display-item.citation.isi??? 331
social impact