1995
DOI: 10.1103/physrevlett.74.2885
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First Measurement of the Rate for the Inclusive Radiative Penguin Decaybsγ

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Cited by 603 publications
(412 citation statements)
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“…SUSY can accommodate the observed flavor mixing [8,9,10] and thus, the LFV processes (15), (16) and (17) would arise in these models. A study conducted at the LHC showed that an upper bound of 0.6 × 10 −6 on the τ ± → µ ± γ branching ratio can be achieved with an integrated luminosity of 30 fb −1 while theoretical estimates are at the level of 10 −9 or less [10,32].…”
Section: Collider Experimentsmentioning
confidence: 99%
See 1 more Smart Citation
“…SUSY can accommodate the observed flavor mixing [8,9,10] and thus, the LFV processes (15), (16) and (17) would arise in these models. A study conducted at the LHC showed that an upper bound of 0.6 × 10 −6 on the τ ± → µ ± γ branching ratio can be achieved with an integrated luminosity of 30 fb −1 while theoretical estimates are at the level of 10 −9 or less [10,32].…”
Section: Collider Experimentsmentioning
confidence: 99%
“…One of the most stringent test of the 2HDM type I and type II comes from the measurement of the b → sγ decay rate which receives substantial enhancement (over the SM prediction) in the 2HDM in a large region of the (m H ± , tan β) parameter space [13,14,15]. The measured b → sγ decay rate from CLEO [16] and ALEPH [17] leads to a model dependent indirect lower bound of the charged Higgs mass as function of tan β [18]. In the 2HDM-III, no discrete symmetries are present and in general FCNC exist in this model [19,20].…”
mentioning
confidence: 99%
“…Fits to the semileptonic decay spectrum at CLEO [16] suggest a value of β = 0.287GeV ; m b = 4.87GeV . In our results we consider β = .15 − .45GeV , though in most cases the branching ratios are not strongly dependent on β.…”
Section: Introduction 2 Role Of the Anomalymentioning
confidence: 99%
“…When the cut is imposed however, the fraction passing the cut is strongly dependent on m b . Following CLEO (b → sγ) [16] we vary m b over the range of 4.7 to 4.9GeV . Using β = 0.3 GeV we find that for m b = 4.7 GeV the branching fraction which passes the cut is 6.7 × 10 −4 while if m b = 4.9GeV then the corresponding branching fraction is 9.8 × 10 −4 .…”
Section: Introduction 2 Role Of the Anomalymentioning
confidence: 99%
“…Recall first the CLEO observation [104] Br(B → X s γ) = (2.32 ± .57 ± .35) × 10 −4 and the corresponding 95% CL bounds of 1 × 10 −4 < Br(B → X s γ) < 4.2 × 10 −4 . These were updated by CLEO to read Br(B → X s γ) < (3.11 ± 0.8 ± 0.72) × 10 −4 where, at 95% CL, 2.0 × 10 −4 < Br(B → X s γ) < 4.5 × 10 −4 [105,106].…”
Section: Hdm With Cp Nonconservation and No Fcncmentioning
confidence: 99%