Observation of the decays B0(s) → Ds1(2536)K±

LHCb Collaboration, Daniel Johnson, Cristina Lazzeroni, Marcus Madurai, Niladribihari Sahoo, Mark Slater, Paul Swallow, Daniel Thompson, Nigel Watson

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Abstract

This paper reports the observation of the decays B0(s) → Ds1(2536)K± using proton-proton collision data collected by the LHCb experiment, corresponding to an integrated luminosity of 9 fb−1. The branching fractions of these decays are measured relative to the normalisation channel B0 → D̅0K+K. The Ds1(2536) meson is reconstructed in the D̅*(2007)0K decay channel and the products of branching fractions are measured to be

B (B0s → Ds1(2536)K±) × B (Ds1(2536)− → D̅(2007)0K)
= (2.49 ± 0.11 ± 0.12 ± 0.25 ± 0.06) × 10−5,
B (B→ Ds1(2536)K±) × B (Ds1(2536)− → D̅(2007)0K)
= (0.510 ± 0.021 ± 0.036 ± 0.050) × 10−5.

The first uncertainty is statistical, the second systematic, and the third arises from the uncertainty of the branching fraction of the B0 → D̅0K+K normalisation channel. The last uncertainty in the B0result is due to the limited knowledge of the fragmentation fraction ratio, fs/fd. The significance for the Bsand B0 signals is larger than 10 σ. The ratio of the helicity amplitudes which governs the angular distribution of the Ds1(2536) → D̅*(2007)0K decay is determined from the data. The ratio of the S- and D-wave amplitudes is found to be 1.11 ± 0.15 ± 0.06 and the phase difference between them 0.70 ± 0.09 ± 0.04 rad, where the first uncertainty is statistical and the second systematic.
Original languageEnglish
Article number106
Number of pages25
JournalJHEP
Volume2023
Issue number10
DOIs
Publication statusPublished - 17 Oct 2023

Bibliographical note

Acknowledgments:
We express our gratitude to our colleagues in the CERN accelerator departments for the excellent performance of the LHC. We thank the technical and administrative staff at the LHCb institutes. We acknowledge support from CERN and from the national agencies: CAPES, CNPq, FAPERJ and FINEP (Brazil); MOST and NSFC (China); CNRS/IN2P3 (France); BMBF, DFG and MPG (Germany); INFN (Italy); NWO (Netherlands); MNiSW and NCN (Poland); MCID/IFA (Romania); MICINN (Spain); SNSF and SER (Switzerland); NASU (Ukraine); STFC (United Kingdom); DOE NP and NSF (USA). We acknowledge the computing resources that are provided by CERN, IN2P3 (France), KIT and DESY (Germany), INFN (Italy), SURF (Netherlands), PIC (Spain), GridPP (United Kingdom), CSCS (Switzerland), IFIN-HH (Romania), CBPF (Brazil), Polish WLCG (Poland) and NERSC (USA). We are indebted to the communities behind the multiple open-source software packages on which we depend. Individual groups or members have received support from ARC and ARDC (Australia); Minciencias (Colombia); AvH Foundation (Germany); EPLANET, Marie Skłodowska-Curie Actions, ERC and NextGenerationEU (European Union); A*MIDEX, ANR, IPhU and Labex P2IO, and Région Auvergne-Rhône-Alpes (France); Key Research Program of Frontier Sciences of CAS, CAS PIFI, CAS CCEPP, Fundamental Research Funds for the Central Universities, and Sci. & Tech. Program of Guangzhou (China); GVA, XuntaGal, GENCAT, Inditex, InTalent and Prog. Atracción Talento, CM (Spain); SRC (Sweden); the Leverhulme Trust, the Royal Society and UKRI (United Kingdom).

Keywords

  • B Physics
  • Branching fraction
  • Flavour Physics
  • Hadron-Hadron Scattering

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