SU(3)F sum rules for CP asymmetries of D(s) decays

IF 5 2区 物理与天体物理 Q1 Physics and Astronomy
Syuhei Iguro, Ulrich Nierste, Emil Overduin, Maurice Schüßler
{"title":"SU(3)F sum rules for CP asymmetries of D(s) decays","authors":"Syuhei Iguro, Ulrich Nierste, Emil Overduin, Maurice Schüßler","doi":"10.1103/physrevd.111.035023","DOIUrl":null,"url":null,"abstract":"Charge-parity (C</a:mi>P</a:mi></a:math>) asymmetries in charm decays are extremely suppressed in the Standard Model and may well be dominated by new-physics contributions. The LHCb Collaboration reported the results of direct <c:math xmlns:c=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><c:mi>C</c:mi><c:mi>P</c:mi></c:math> asymmetry measurements in <e:math xmlns:e=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><e:mrow><e:msup><e:mrow><e:mi>D</e:mi></e:mrow><e:mrow><e:mn>0</e:mn></e:mrow></e:msup><e:mo stretchy=\"false\">→</e:mo><e:msup><e:mrow><e:mi>K</e:mi></e:mrow><e:mrow><e:mo>+</e:mo></e:mrow></e:msup><e:msup><e:mrow><e:mi>K</e:mi></e:mrow><e:mrow><e:mo>−</e:mo></e:mrow></e:msup></e:mrow></e:math> and <h:math xmlns:h=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><h:msup><h:mi>D</h:mi><h:mn>0</h:mn></h:msup><h:mo stretchy=\"false\">→</h:mo><h:msup><h:mi>π</h:mi><h:mo>+</h:mo></h:msup><h:msup><h:mi>π</h:mi><h:mo>−</h:mo></h:msup></h:math> decays with unprecedented accuracy: <k:math xmlns:k=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><k:msub><k:mi>a</k:mi><k:mrow><k:mi>C</k:mi><k:mi>P</k:mi></k:mrow></k:msub><k:mo stretchy=\"false\">(</k:mo><k:msup><k:mi>K</k:mi><k:mo>+</k:mo></k:msup><k:msup><k:mi>K</k:mi><k:mo>−</k:mo></k:msup><k:mo stretchy=\"false\">)</k:mo><k:mo>=</k:mo><k:mo stretchy=\"false\">(</k:mo><k:mn>7.7</k:mn><k:mo>±</k:mo><k:mn>5.7</k:mn><k:mo stretchy=\"false\">)</k:mo><k:mo>×</k:mo><k:msup><k:mn>10</k:mn><k:mrow><k:mo>−</k:mo><k:mn>4</k:mn></k:mrow></k:msup></k:math> and <q:math xmlns:q=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><q:mrow><q:msub><q:mrow><q:mi>a</q:mi></q:mrow><q:mrow><q:mi>C</q:mi><q:mi>P</q:mi></q:mrow></q:msub><q:mo stretchy=\"false\">(</q:mo><q:msup><q:mrow><q:mi>π</q:mi></q:mrow><q:mrow><q:mo>+</q:mo></q:mrow></q:msup><q:msup><q:mrow><q:mi>π</q:mi></q:mrow><q:mrow><q:mo>−</q:mo></q:mrow></q:msup><q:mo stretchy=\"false\">)</q:mo><q:mo>=</q:mo><q:mo stretchy=\"false\">(</q:mo><q:mn>23.2</q:mn><q:mo>±</q:mo><q:mn>6.1</q:mn><q:mo stretchy=\"false\">)</q:mo><q:mo>×</q:mo><q:msup><q:mrow><q:mn>10</q:mn></q:mrow><q:mrow><q:mo>−</q:mo><q:mn>4</q:mn></q:mrow></q:msup></q:mrow></q:math>, with the latter quantity inferred from the precise measurement of <w:math xmlns:w=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><w:mrow><w:mi mathvariant=\"normal\">Δ</w:mi><w:msub><w:mrow><w:mi>a</w:mi></w:mrow><w:mrow><w:mi>C</w:mi><w:mi>P</w:mi></w:mrow></w:msub><w:mo>=</w:mo><w:msub><w:mrow><w:mi>a</w:mi></w:mrow><w:mrow><w:mi>C</w:mi><w:mi>P</w:mi></w:mrow></w:msub><w:mo stretchy=\"false\">(</w:mo><w:msup><w:mrow><w:mi>K</w:mi></w:mrow><w:mrow><w:mo>+</w:mo></w:mrow></w:msup><w:msup><w:mrow><w:mi>K</w:mi></w:mrow><w:mrow><w:mo>−</w:mo></w:mrow></w:msup><w:mo stretchy=\"false\">)</w:mo><w:mo>−</w:mo><w:msub><w:mrow><w:mi>a</w:mi></w:mrow><w:mrow><w:mi>C</w:mi><w:mi>P</w:mi></w:mrow></w:msub><w:mo stretchy=\"false\">(</w:mo><w:msup><w:mrow><w:mi>π</w:mi></w:mrow><w:mrow><w:mo>+</w:mo></w:mrow></w:msup><w:msup><w:mrow><w:mi>π</w:mi></w:mrow><w:mrow><w:mo>−</w:mo></w:mrow></w:msup><w:mo stretchy=\"false\">)</w:mo><w:mo>=</w:mo><w:mspace linebreak=\"goodbreak\"/><w:mo stretchy=\"false\">(</w:mo><w:mo>−</w:mo><w:mn>15.7</w:mn><w:mo>±</w:mo><w:mn>2.9</w:mn><w:mo stretchy=\"false\">)</w:mo><w:mo>×</w:mo><w:msup><w:mrow><w:mn>10</w:mn></w:mrow><w:mrow><w:mo>−</w:mo><w:mn>4</w:mn></w:mrow></w:msup></w:mrow></w:math>. When interpreted within the Standard Model, these values indicate a breakdown of the approximate <gb:math xmlns:gb=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><gb:mi>U</gb:mi></gb:math>-spin symmetry of QCD. If, however, this symmetry holds and the data stem from new physics, other <ib:math xmlns:ib=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><ib:mi>C</ib:mi><ib:mi>P</ib:mi></ib:math> asymmetries should be enhanced as well. We derive <kb:math xmlns:kb=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><kb:mi>C</kb:mi><kb:mi>P</kb:mi></kb:math> asymmetry sum rules based on SU(3) flavor symmetry for <mb:math xmlns:mb=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><mb:mi>D</mb:mi></mb:math> meson decays into a pair of pseudoscalar mesons as well as a pair of a pseudoscalar and a vector meson for two generic scenarios, with <ob:math xmlns:ob=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><ob:mi mathvariant=\"normal\">Δ</ob:mi><ob:mi>U</ob:mi><ob:mo>=</ob:mo><ob:mn>0</ob:mn></ob:math> and <rb:math xmlns:rb=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><rb:mo stretchy=\"false\">|</rb:mo><rb:mi mathvariant=\"normal\">Δ</rb:mi><rb:mi>U</rb:mi><rb:mo stretchy=\"false\">|</rb:mo><rb:mo>=</rb:mo><rb:mn>1</rb:mn></rb:math> interactions, respectively. The correlations implied by the sum rules can be used to check the consistency between different measurements and to discriminate between these scenarios with future data. For instance, we find <wb:math xmlns:wb=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><wb:mrow><wb:msub><wb:mrow><wb:mi>a</wb:mi></wb:mrow><wb:mrow><wb:mi>C</wb:mi><wb:mi>P</wb:mi></wb:mrow></wb:msub><wb:mo stretchy=\"false\">(</wb:mo><wb:msup><wb:mrow><wb:mi>π</wb:mi></wb:mrow><wb:mrow><wb:mo>+</wb:mo></wb:mrow></wb:msup><wb:msup><wb:mrow><wb:mi>K</wb:mi></wb:mrow><wb:mrow><wb:mo>*</wb:mo><wb:mn>0</wb:mn></wb:mrow></wb:msup><wb:mo stretchy=\"false\">)</wb:mo><wb:mo>+</wb:mo><wb:msub><wb:mrow><wb:mi>a</wb:mi></wb:mrow><wb:mrow><wb:mi>C</wb:mi><wb:mi>P</wb:mi></wb:mrow></wb:msub><wb:mo stretchy=\"false\">(</wb:mo><wb:msup><wb:mrow><wb:mi>K</wb:mi></wb:mrow><wb:mrow><wb:mo>+</wb:mo></wb:mrow></wb:msup><wb:msup><wb:mrow><wb:mover accent=\"true\"><wb:mrow><wb:mi>K</wb:mi></wb:mrow><wb:mrow><wb:mo stretchy=\"false\">¯</wb:mo></wb:mrow></wb:mover></wb:mrow><wb:mrow><wb:mo>*</wb:mo><wb:mn>0</wb:mn></wb:mrow></wb:msup><wb:mo stretchy=\"false\">)</wb:mo><wb:mo>=</wb:mo><wb:mn>0</wb:mn></wb:mrow></wb:math> for <ec:math xmlns:ec=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><ec:mi mathvariant=\"normal\">Δ</ec:mi><ec:mi>U</ec:mi><ec:mo>=</ec:mo><ec:mn>0</ec:mn></ec:math> new physics and the opposite relative sign for the <hc:math xmlns:hc=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><hc:mo stretchy=\"false\">|</hc:mo><hc:mi mathvariant=\"normal\">Δ</hc:mi><hc:mi>U</hc:mi><hc:mo stretchy=\"false\">|</hc:mo><hc:mo>=</hc:mo><hc:mn>1</hc:mn></hc:math> case. One sum rule, connecting four decay modes, holds in both scenarios. We further extend our sum rules to certain differences of <mc:math xmlns:mc=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><mc:mi>C</mc:mi><mc:mi>P</mc:mi></mc:math> asymmetries from which the <oc:math xmlns:oc=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><oc:mi>D</oc:mi></oc:math> production asymmetries drop out. <jats:supplementary-material> <jats:copyright-statement>Published by the American Physical Society</jats:copyright-statement> <jats:copyright-year>2025</jats:copyright-year> </jats:permissions> </jats:supplementary-material>","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"21 1","pages":""},"PeriodicalIF":5.0000,"publicationDate":"2025-02-24","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Physical Review D","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1103/physrevd.111.035023","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"Physics and Astronomy","Score":null,"Total":0}
引用次数: 0

Abstract

Charge-parity (CP) asymmetries in charm decays are extremely suppressed in the Standard Model and may well be dominated by new-physics contributions. The LHCb Collaboration reported the results of direct CP asymmetry measurements in D0K+K and D0π+π decays with unprecedented accuracy: aCP(K+K)=(7.7±5.7)×104 and aCP(π+π)=(23.2±6.1)×104, with the latter quantity inferred from the precise measurement of ΔaCP=aCP(K+K)aCP(π+π)=(15.7±2.9)×104. When interpreted within the Standard Model, these values indicate a breakdown of the approximate U-spin symmetry of QCD. If, however, this symmetry holds and the data stem from new physics, other CP asymmetries should be enhanced as well. We derive CP asymmetry sum rules based on SU(3) flavor symmetry for D meson decays into a pair of pseudoscalar mesons as well as a pair of a pseudoscalar and a vector meson for two generic scenarios, with ΔU=0 and |ΔU|=1 interactions, respectively. The correlations implied by the sum rules can be used to check the consistency between different measurements and to discriminate between these scenarios with future data. For instance, we find aCP(π+K*0)+aCP(K+K¯*0)=0 for ΔU=0 new physics and the opposite relative sign for the |ΔU|=1 case. One sum rule, connecting four decay modes, holds in both scenarios. We further extend our sum rules to certain differences of CP asymmetries from which the D production asymmetries drop out. Published by the American Physical Society 2025
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来源期刊
Physical Review D
Physical Review D 物理-天文与天体物理
CiteScore
9.20
自引率
36.00%
发文量
0
审稿时长
2 months
期刊介绍: Physical Review D (PRD) is a leading journal in elementary particle physics, field theory, gravitation, and cosmology and is one of the top-cited journals in high-energy physics. PRD covers experimental and theoretical results in all aspects of particle physics, field theory, gravitation and cosmology, including: Particle physics experiments, Electroweak interactions, Strong interactions, Lattice field theories, lattice QCD, Beyond the standard model physics, Phenomenological aspects of field theory, general methods, Gravity, cosmology, cosmic rays, Astrophysics and astroparticle physics, General relativity, Formal aspects of field theory, field theory in curved space, String theory, quantum gravity, gauge/gravity duality.
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