A sample of 3120 K ± → π ± μ+ μ− decay candidates with (3.3 ± 0.7)% background contamination has been collected by the NA48/2 experiment at the CERN SPS, allowing a detailed study of the decay properties. The branching ratio was measured to be BR = (9.62 ± 0.25) × 10−8 . The form factor W(z), where z = ( M(μμ) / M(K) )^2 , was parameterized according to several models. In particular, the slope of the linear form factor W(z) = W0 (1 + δ z) was measured to be δ = 3.11 ± 0.57. Upper limits of 2.9 × 10^-2 and 2.3 × 10^-2 on possible charge asymmetry and forward-backward asymmetry were established at 90% CL. An upper limit BR( K ± → π ∓ μ± μ± ) < 1.1 × 10^-9 was established at 90% CL for the rate of the lepton number violating decay.

New measurement of the K+- -> pi+- mu+ mu- decay / J. R., B., G., K., C., L., D. J., M., M. W., S., S. A., W., R., A., G., B., N., C., A., C., D., C., V., F., M., F., L., G., A., G., W., K., A., N., A., M., M., P., A., P., et al.. - In: PHYSICS LETTERS. SECTION B. - ISSN 0370-2693. - STAMPA. - 697:2(2011), pp. 107-115. [10.1016/j.physletb.2011.01.042]

New measurement of the K+- -> pi+- mu+ mu- decay

BIZZETI, Andrea;
2011

Abstract

A sample of 3120 K ± → π ± μ+ μ− decay candidates with (3.3 ± 0.7)% background contamination has been collected by the NA48/2 experiment at the CERN SPS, allowing a detailed study of the decay properties. The branching ratio was measured to be BR = (9.62 ± 0.25) × 10−8 . The form factor W(z), where z = ( M(μμ) / M(K) )^2 , was parameterized according to several models. In particular, the slope of the linear form factor W(z) = W0 (1 + δ z) was measured to be δ = 3.11 ± 0.57. Upper limits of 2.9 × 10^-2 and 2.3 × 10^-2 on possible charge asymmetry and forward-backward asymmetry were established at 90% CL. An upper limit BR( K ± → π ∓ μ± μ± ) < 1.1 × 10^-9 was established at 90% CL for the rate of the lepton number violating decay.
2011
697
2
107
115
New measurement of the K+- -> pi+- mu+ mu- decay / J. R., B., G., K., C., L., D. J., M., M. W., S., S. A., W., R., A., G., B., N., C., A., C., D., C., V., F., M., F., L., G., A., G., W., K., A., N., A., M., M., P., A., P., et al.. - In: PHYSICS LETTERS. SECTION B. - ISSN 0370-2693. - STAMPA. - 697:2(2011), pp. 107-115. [10.1016/j.physletb.2011.01.042]
J. R., Batley; G., Kalmus; C., Lazzeroni; D. J., Munday; M. W., Slater; S. A., Wotton; R., Arcidiacono; G., Bocquet; N., Cabibbo; A., Ceccucci; D., Cu...espandi
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11380/705356
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