Paul Singer
Technion – Israel Institute of Technology
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Publication
Featured researches published by Paul Singer.
Physics Letters B | 1984
L. Bergström; E. Massó; Paul Singer; D. Wyler
Abstract We study a class of diagrams, that has previously been overlooked, contributing to the (dispersive) electromagnetic part of the K L → μ + μ − amplitude. The strength of this extra contribution can be estimated in different models and could be measured in related processes. By combining these results with those coming from the K 0 K 0 transition (evaluated in the Kobayashi-Maskawa scheme) we obtain rather strong constraints on the t quark mass and the B meson lifetime. The recently measured value for the B meson lifetime is difficult to accommodate unless the t quark is very heavy; m t > 100 GeV could be natural values according to the analysis.
European Physical Journal C | 2003
Svjetlana Fajfer; Paul Singer; Jure Zupan
Abstract. We present a calculation of the rare decay modes
European Physical Journal C | 1999
S. Fajfer; S. Prelovšek; Paul Singer
D^0 \to e^+ e^- \gamma
Physics Letters B | 1986
Lars Bergström; Paul Singer
and
Physical Review D | 1997
S. Fajfer; Paul Singer
D^0 \to \mu^+\mu^- \gamma
Physical Review D | 1996
Gad Eilam; A. Ioannissian; R. R. Mendel; Paul Singer
in the framework of the standard model. For the short distance part we have derived QCD corrections to the Wilson coefficients involved, including C9. The latter is found to be strongly suppressed by the corrections, leading to diminished values for the
Physical Review D | 1998
Svjetlana Fajfer; Sasa Prelovsek; Paul Singer
c\to u l^+l^-
Physics Letters B | 2000
Svjetlana Fajfer; Sasa Prelovsek; Paul Singer; Daniel Wyler
branching ratios in the 10-10 range. Within SM the exclusive decays are dominated by long distance effects. Non-resonant contributions are estimated using heavy quark and chiral symmetries to be at the level of
Physical Review D | 2000
S. Fajfer; Paul Singer
10\%
Physics Letters B | 1999
Katri Huitu; Cai-Dian Lü; Paul Singer; Da-Xin Zhang
, compared to the contributions arising from