A search for the rare decays B0s → τ+τ− and B0 → τ+τ− is performed using proton–proton collision data collected with the LHCb detector. The data sample corresponds to an integrated luminosity of 3 fb−1 collected in 2011 and 2012. The τ leptons are reconstructed through the decay τ− → π−π+π−ντ. Assuming no contribution from B0 → τ+τ− decays, an upper limit is set on the branching fraction B(B0s → τ+τ−) < 6.8 × 10−3 at the 95% confidence level. If instead no contribution from B0s → τ+τ− decays is assumed, the limit is B(B0 → τ+τ−) < 2.1 × 10−3 at the 95% confidence level. These results correspond to the first direct limit on B(B0s → τ+τ−) and the world’s best limit on B(B0 → τ+τ−)

Aaij, R., Adeva, B., Adinolfi, M., Ajaltouni, Z., Akar, S., Albrecht, J., et al. (2017). Search for the Decays B0s →τ+τ− and B0 →τ+τ−. PHYSICAL REVIEW LETTERS, 118(25) [10.1103/PhysRevLett.118.251802].

Search for the Decays B0s →τ+τ− and B0 →τ+τ−

Belloli, N.;Borgheresi, A.;Borsato, M.;Calvi, M.;Carniti, P.;Cassina, L.;Fazzini, D.;Gotti, C.
;
Grillo, L.;Martinelli, M.;Matteuzzi, C.;Petruzzo, M.;
2017

Abstract

A search for the rare decays B0s → τ+τ− and B0 → τ+τ− is performed using proton–proton collision data collected with the LHCb detector. The data sample corresponds to an integrated luminosity of 3 fb−1 collected in 2011 and 2012. The τ leptons are reconstructed through the decay τ− → π−π+π−ντ. Assuming no contribution from B0 → τ+τ− decays, an upper limit is set on the branching fraction B(B0s → τ+τ−) < 6.8 × 10−3 at the 95% confidence level. If instead no contribution from B0s → τ+τ− decays is assumed, the limit is B(B0 → τ+τ−) < 2.1 × 10−3 at the 95% confidence level. These results correspond to the first direct limit on B(B0s → τ+τ−) and the world’s best limit on B(B0 → τ+τ−)
Articolo in rivista - Articolo scientifico
Physics and Astronomy (all)
English
2017
118
25
251802
none
Aaij, R., Adeva, B., Adinolfi, M., Ajaltouni, Z., Akar, S., Albrecht, J., et al. (2017). Search for the Decays B0s →τ+τ− and B0 →τ+τ−. PHYSICAL REVIEW LETTERS, 118(25) [10.1103/PhysRevLett.118.251802].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/10281/181714
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