Measurement of the Time-Integrated CP Asymmetry in D0→ K-K+ Decays

LHCb Collaboration

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Abstract

The time-integrated C P asymmetry in the Cabibbo-suppressed decay D0 → K K+ is measured using proton-proton collision data, corresponding to an integrated luminosity of 5.7 fb−1 collected at a center-of-mass energy of 13 TeV with the LHCb detector. The D0 mesons are required to originate from promptly produced D*+ → D0π+ decays, and the charge of the companion pion is used to determine the flavor of the charm meson at production. The time-integrated CP asymmetry is measured to be ACP (KK+) = [6.8 ± 5.4 ± 1.6] × 10−4 where the first uncertainty is statistical and the second systematic. The direct CP asymmetries in D0 → KK+ and D0 → ππ+ decays, adK−K+ and adπ−π+, are derived by combining ACP(KK+) with the time-integrated CP asymmetry difference, ΔACP = ACP(KK+) − ACP(ππ+), and other inputs, giving adK−K+ = (7.7 ± 5.7) × 10−4, adπ−π+ = (23.2 ± 6.1) × 10−4, with a correlation coefficient corresponding to ρ = 0.88 . The compatibility of these results with CP symmetry is 1.4 and 3.8 standard deviations for D0 → KK+ and D0 → ππ+ decays, respectively. This is the first evidence for direct CP violation in a specific D0 decay. 

Original languageEnglish
Article number91802
Number of pages13
JournalPhysical Review Letters
Volume131
Issue number9
Early online date29 Aug 2023
DOIs
Publication statusPublished - 1 Sept 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); MEN/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 opensource 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 SkłodowskaCurie Actions, and ERC (European Union); A*MIDEX, ANR, IPhU and Labex P2IO, and Region AuvergneRhône-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 and Prog. Atracción Talento, CM (Spain); SRC (Sweden); the Leverhulme Trust, the Royal Society, and UKRI (United Kingdom). ARDC (Australia); Minciencias (Colombia); AvH Foundation (Germany); EPLANET, Marie SkłodowskaCurie Actions, and ERC (European Union); A*MIDEX, ANR, IPhU and Labex P2IO, and R´egion AuvergneRhône-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 and Prog. Atracción Talento, CM (Spain); SRC (Sweden); the Leverhulme Trust, the Royal Society, and UKRI (United Kingdom).

ASJC Scopus subject areas

  • General Physics and Astronomy

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