{"title":"有限温度下同位旋非对称致密共振物质中的介子和反介子","authors":"Manpreet Kaur, Arvind Kumar","doi":"10.1103/physrevd.110.114054","DOIUrl":null,"url":null,"abstract":"We study the in-medium properties of kaons and antikaons in isospin asymmetric hot and dense resonance matter within the chiral SU(3) hadronic mean field model. Along with nucleons and hyperons, the interactions of K</a:mi></a:math> and <c:math xmlns:c=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><c:mover accent=\"true\"><c:mi>K</c:mi><c:mo stretchy=\"false\">¯</c:mo></c:mover></c:math> mesons with all decuplet baryons (<g:math xmlns:g=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><g:msup><g:mi mathvariant=\"normal\">Δ</g:mi><g:mrow><g:mo>+</g:mo><g:mo>+</g:mo><g:mo>,</g:mo><g:mo>+</g:mo><g:mo>,</g:mo><g:mn>0</g:mn><g:mo>,</g:mo><g:mo>−</g:mo></g:mrow></g:msup><g:mo>,</g:mo><g:msup><g:mi mathvariant=\"normal\">Σ</g:mi><g:mrow><g:mo>*</g:mo><g:mo>±</g:mo><g:mo>,</g:mo><g:mn>0</g:mn></g:mrow></g:msup><g:mo>,</g:mo><g:msup><g:mi mathvariant=\"normal\">Ξ</g:mi><g:mrow><g:mo>*</g:mo><g:mn>0</g:mn><g:mo>,</g:mo><g:mo>−</g:mo></g:mrow></g:msup><g:mo>,</g:mo><g:msup><g:mi mathvariant=\"normal\">Ω</g:mi><g:mo>−</g:mo></g:msup></g:math>) are explicitly considered in the dispersion relations. The properties of mesons in the chiral SU(3) model are modified at finite density and temperature of asymmetric resonance matter through the exchange of scalar fields <m:math xmlns:m=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><m:mrow><m:mi>σ</m:mi></m:mrow></m:math>, <o:math xmlns:o=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><o:mrow><o:mi>ζ</o:mi></o:mrow></o:math>, and <q:math xmlns:q=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><q:mi>δ</q:mi></q:math> and the vector fields <s:math xmlns:s=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><s:mrow><s:mi>ω</s:mi></s:mrow></s:math>, <u:math xmlns:u=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><u:mrow><u:mi>ρ</u:mi></u:mrow></u:math>, and <w:math xmlns:w=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><w:mi>ϕ</w:mi></w:math>. The presence of resonance baryons in the medium at finite temperature is observed to modify significantly the effective masses of <y:math xmlns:y=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><y:mi>K</y:mi></y:math> and K</ab:mi>¯</ab:mo></ab:mover></ab:math> mesons. We also calculated the optical potentials of kaons and antikaons as a function of momentum in resonance matter. The present study of in-medium masses and optical potentials of kaons and antikaons will be important for understanding the experimental observables from the heavy-ion collision experiments where hot and dense matter may be produced. Our results indicate that when resonance baryons are present within the medium at finite baryonic density, the mass reduction of kaons and antikaons becomes more pronounced as the temperature of the medium increases from zero to 100 and 150 MeV. The study of the optical potentials of kaons and antikaons reveals a stronger correlation with strangeness fraction compared to isospin asymmetry. <jats:supplementary-material> <jats:copyright-statement>Published by the American Physical Society</jats:copyright-statement> <jats:copyright-year>2024</jats:copyright-year> </jats:permissions> </jats:supplementary-material>","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"3 1","pages":""},"PeriodicalIF":5.3000,"publicationDate":"2024-12-30","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Kaons and antikaons in isospin asymmetric dense resonance matter at finite temperature\",\"authors\":\"Manpreet Kaur, Arvind Kumar\",\"doi\":\"10.1103/physrevd.110.114054\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"We study the in-medium properties of kaons and antikaons in isospin asymmetric hot and dense resonance matter within the chiral SU(3) hadronic mean field model. Along with nucleons and hyperons, the interactions of K</a:mi></a:math> and <c:math xmlns:c=\\\"http://www.w3.org/1998/Math/MathML\\\" display=\\\"inline\\\"><c:mover accent=\\\"true\\\"><c:mi>K</c:mi><c:mo stretchy=\\\"false\\\">¯</c:mo></c:mover></c:math> mesons with all decuplet baryons (<g:math xmlns:g=\\\"http://www.w3.org/1998/Math/MathML\\\" display=\\\"inline\\\"><g:msup><g:mi mathvariant=\\\"normal\\\">Δ</g:mi><g:mrow><g:mo>+</g:mo><g:mo>+</g:mo><g:mo>,</g:mo><g:mo>+</g:mo><g:mo>,</g:mo><g:mn>0</g:mn><g:mo>,</g:mo><g:mo>−</g:mo></g:mrow></g:msup><g:mo>,</g:mo><g:msup><g:mi mathvariant=\\\"normal\\\">Σ</g:mi><g:mrow><g:mo>*</g:mo><g:mo>±</g:mo><g:mo>,</g:mo><g:mn>0</g:mn></g:mrow></g:msup><g:mo>,</g:mo><g:msup><g:mi mathvariant=\\\"normal\\\">Ξ</g:mi><g:mrow><g:mo>*</g:mo><g:mn>0</g:mn><g:mo>,</g:mo><g:mo>−</g:mo></g:mrow></g:msup><g:mo>,</g:mo><g:msup><g:mi mathvariant=\\\"normal\\\">Ω</g:mi><g:mo>−</g:mo></g:msup></g:math>) are explicitly considered in the dispersion relations. The properties of mesons in the chiral SU(3) model are modified at finite density and temperature of asymmetric resonance matter through the exchange of scalar fields <m:math xmlns:m=\\\"http://www.w3.org/1998/Math/MathML\\\" display=\\\"inline\\\"><m:mrow><m:mi>σ</m:mi></m:mrow></m:math>, <o:math xmlns:o=\\\"http://www.w3.org/1998/Math/MathML\\\" display=\\\"inline\\\"><o:mrow><o:mi>ζ</o:mi></o:mrow></o:math>, and <q:math xmlns:q=\\\"http://www.w3.org/1998/Math/MathML\\\" display=\\\"inline\\\"><q:mi>δ</q:mi></q:math> and the vector fields <s:math xmlns:s=\\\"http://www.w3.org/1998/Math/MathML\\\" display=\\\"inline\\\"><s:mrow><s:mi>ω</s:mi></s:mrow></s:math>, <u:math xmlns:u=\\\"http://www.w3.org/1998/Math/MathML\\\" display=\\\"inline\\\"><u:mrow><u:mi>ρ</u:mi></u:mrow></u:math>, and <w:math xmlns:w=\\\"http://www.w3.org/1998/Math/MathML\\\" display=\\\"inline\\\"><w:mi>ϕ</w:mi></w:math>. The presence of resonance baryons in the medium at finite temperature is observed to modify significantly the effective masses of <y:math xmlns:y=\\\"http://www.w3.org/1998/Math/MathML\\\" display=\\\"inline\\\"><y:mi>K</y:mi></y:math> and K</ab:mi>¯</ab:mo></ab:mover></ab:math> mesons. We also calculated the optical potentials of kaons and antikaons as a function of momentum in resonance matter. The present study of in-medium masses and optical potentials of kaons and antikaons will be important for understanding the experimental observables from the heavy-ion collision experiments where hot and dense matter may be produced. Our results indicate that when resonance baryons are present within the medium at finite baryonic density, the mass reduction of kaons and antikaons becomes more pronounced as the temperature of the medium increases from zero to 100 and 150 MeV. The study of the optical potentials of kaons and antikaons reveals a stronger correlation with strangeness fraction compared to isospin asymmetry. <jats:supplementary-material> <jats:copyright-statement>Published by the American Physical Society</jats:copyright-statement> <jats:copyright-year>2024</jats:copyright-year> </jats:permissions> </jats:supplementary-material>\",\"PeriodicalId\":20167,\"journal\":{\"name\":\"Physical Review D\",\"volume\":\"3 1\",\"pages\":\"\"},\"PeriodicalIF\":5.3000,\"publicationDate\":\"2024-12-30\",\"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.110.114054\",\"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}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Physical Review D","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1103/physrevd.110.114054","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}
Kaons and antikaons in isospin asymmetric dense resonance matter at finite temperature
We study the in-medium properties of kaons and antikaons in isospin asymmetric hot and dense resonance matter within the chiral SU(3) hadronic mean field model. Along with nucleons and hyperons, the interactions of K and K¯ mesons with all decuplet baryons (Δ++,+,0,−,Σ*±,0,Ξ*0,−,Ω−) are explicitly considered in the dispersion relations. The properties of mesons in the chiral SU(3) model are modified at finite density and temperature of asymmetric resonance matter through the exchange of scalar fields σ, ζ, and δ and the vector fields ω, ρ, and ϕ. The presence of resonance baryons in the medium at finite temperature is observed to modify significantly the effective masses of K and K¯ mesons. We also calculated the optical potentials of kaons and antikaons as a function of momentum in resonance matter. The present study of in-medium masses and optical potentials of kaons and antikaons will be important for understanding the experimental observables from the heavy-ion collision experiments where hot and dense matter may be produced. Our results indicate that when resonance baryons are present within the medium at finite baryonic density, the mass reduction of kaons and antikaons becomes more pronounced as the temperature of the medium increases from zero to 100 and 150 MeV. The study of the optical potentials of kaons and antikaons reveals a stronger correlation with strangeness fraction compared to isospin asymmetry. Published by the American Physical Society2024
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.