Angular Analysis of the B+→K*+μ+μ− Decay; Physical Review Letters; Vol. 126, iss. 16

Podrobná bibliografie
Parent link:Physical Review Letters
Vol. 126, iss. 16.— 2021.— [161802, 11 p.]
Korporace: Национальный исследовательский Томский политехнический университет Инженерная школа информационных технологий и робототехники Отделение автоматизации и робототехники (ОАР), Национальный исследовательский Томский политехнический университет Исследовательская школа физики высокоэнергетических процессов
Další autoři: Aaij R. Roel, Beteta C. A. Carlos Abellan, Eydelman S. I. Semen Isaakovich, Kharisova A. E. Anastasiya Evgenjevna, Panshin G. L. Gennady Leonidovich
Shrnutí:Title screen
We present an angular analysis of the B+→K*+(→K0Sπ+)μ+μ− decay using 9  fb−1 of pp collision data collected with the LHCb experiment. For the first time, the full set of CP-averaged angular observables is measured in intervals of the dimuon invariant mass squared. Local deviations from standard model predictions are observed, similar to those in previous LHCb analyses of the isospin-partner B0→K*0μ+μ− decay. The global tension is dependent on which effective couplings are considered and on the choice of theory nuisance parameters.
Jazyk:angličtina
Vydáno: 2021
Témata:
On-line přístup:http://earchive.tpu.ru/handle/11683/72764
https://doi.org/10.1103/PhysRevLett.126.161802
Médium: Elektronický zdroj Kapitola
KOHA link:https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=666689
Popis
Shrnutí:Title screen
We present an angular analysis of the B+→K*+(→K0Sπ+)μ+μ− decay using 9  fb−1 of pp collision data collected with the LHCb experiment. For the first time, the full set of CP-averaged angular observables is measured in intervals of the dimuon invariant mass squared. Local deviations from standard model predictions are observed, similar to those in previous LHCb analyses of the isospin-partner B0→K*0μ+μ− decay. The global tension is dependent on which effective couplings are considered and on the choice of theory nuisance parameters.
DOI:10.1103/PhysRevLett.126.161802