{"title":"Roles of the N(1535) and a0(980) in the process Λc+→π+ηn","authors":"Meng-Yuan Li, Wen-Tao Lyu, Li-Juan Liu, En Wang","doi":"10.1103/physrevd.111.034046","DOIUrl":null,"url":null,"abstract":"We have investigated the process Λ</a:mi>c</a:mi>+</a:mo></a:msubsup>→</a:mo>π</a:mi>+</a:mo></a:msup>η</a:mi>n</a:mi></a:math> by taking into account the contributions from the nucleon resonance <e:math xmlns:e=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><e:mi>N</e:mi><e:mo stretchy=\"false\">(</e:mo><e:mn>1535</e:mn><e:mo stretchy=\"false\">)</e:mo></e:math> and the scalar meson <i:math xmlns:i=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><i:msub><i:mi>a</i:mi><i:mn>0</i:mn></i:msub><i:mo stretchy=\"false\">(</i:mo><i:mn>980</i:mn><i:mo stretchy=\"false\">)</i:mo></i:math>, which could be dynamically generated by the interaction of the <m:math xmlns:m=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><m:mi>S</m:mi></m:math>-wave pseudoscalar meson-octet baryon and the <o:math xmlns:o=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><o:mi>S</o:mi></o:math>-wave pseudoscalar meson-pseudoscalar meson, respectively. Our results show that, in <q:math xmlns:q=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><q:mi>η</q:mi><q:mi>n</q:mi></q:math> invariant mass distribution, there is a significant near-threshold enhancement structure, which could be associated with <s:math xmlns:s=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><s:mi>N</s:mi><s:mo stretchy=\"false\">(</s:mo><s:mn>1535</s:mn><s:mo stretchy=\"false\">)</s:mo></s:math>. On the other hand, one can find a clear cusp structure of <w:math xmlns:w=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><w:msub><w:mi>a</w:mi><w:mn>0</w:mn></w:msub><w:mo stretchy=\"false\">(</w:mo><w:mn>980</w:mn><w:mo stretchy=\"false\">)</w:mo></w:math> in π</ab:mi>+</ab:mo></ab:msup>η</ab:mi></ab:math> invariant mass distribution. We further estimate the ratio <cb:math xmlns:cb=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><cb:mrow><cb:mi>R</cb:mi><cb:mo>=</cb:mo><cb:mi mathvariant=\"script\">B</cb:mi><cb:mo stretchy=\"false\">(</cb:mo><cb:msubsup><cb:mrow><cb:mi mathvariant=\"normal\">Λ</cb:mi></cb:mrow><cb:mrow><cb:mi>c</cb:mi></cb:mrow><cb:mrow><cb:mo>+</cb:mo></cb:mrow></cb:msubsup><cb:mo stretchy=\"false\">→</cb:mo><cb:msub><cb:mrow><cb:mi>a</cb:mi></cb:mrow><cb:mrow><cb:mn>0</cb:mn></cb:mrow></cb:msub><cb:mo stretchy=\"false\">(</cb:mo><cb:mn>980</cb:mn><cb:msup><cb:mrow><cb:mo stretchy=\"false\">)</cb:mo></cb:mrow><cb:mrow><cb:mo>+</cb:mo></cb:mrow></cb:msup><cb:mi>n</cb:mi><cb:mo stretchy=\"false\">)</cb:mo><cb:mo>/</cb:mo><cb:mi mathvariant=\"script\">B</cb:mi><cb:mo stretchy=\"false\">(</cb:mo><cb:msubsup><cb:mrow><cb:mi mathvariant=\"normal\">Λ</cb:mi></cb:mrow><cb:mrow><cb:mi>c</cb:mi></cb:mrow><cb:mrow><cb:mo>+</cb:mo></cb:mrow></cb:msubsup><cb:mo stretchy=\"false\">→</cb:mo><cb:msup><cb:mrow><cb:mi>π</cb:mi></cb:mrow><cb:mrow><cb:mo>+</cb:mo></cb:mrow></cb:msup><cb:mi>η</cb:mi><cb:mi>n</cb:mi><cb:mo stretchy=\"false\">)</cb:mo><cb:mo>≈</cb:mo><cb:mn>0.313</cb:mn></cb:mrow></cb:math>. Our results can be tested by BESIII, Belle II, and the proposed Super Tau-Charm Facility experiments in the future. <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":"130 1","pages":""},"PeriodicalIF":5.0000,"publicationDate":"2025-02-27","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.111.034046","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}
Roles of the N(1535) and a0(980) in the process Λc+→π+ηn
We have investigated the process Λc+→π+ηn by taking into account the contributions from the nucleon resonance N(1535) and the scalar meson a0(980), which could be dynamically generated by the interaction of the S-wave pseudoscalar meson-octet baryon and the S-wave pseudoscalar meson-pseudoscalar meson, respectively. Our results show that, in ηn invariant mass distribution, there is a significant near-threshold enhancement structure, which could be associated with N(1535). On the other hand, one can find a clear cusp structure of a0(980) in π+η invariant mass distribution. We further estimate the ratio R=B(Λc+→a0(980)+n)/B(Λc+→π+ηn)≈0.313. Our results can be tested by BESIII, Belle II, and the proposed Super Tau-Charm Facility experiments in the future. Published by the American Physical Society2025
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.