Leonardo Di Giustino , Stanley J. Brodsky , Philip G. Ratcliffe , Sheng-Quan Wang , Xing-Gang Wu
{"title":"利用最大一致性和无限阶尺度设置原理,从射流观测资料中独立确定所有尺度上的QCD运行耦合","authors":"Leonardo Di Giustino , Stanley J. Brodsky , Philip G. Ratcliffe , Sheng-Quan Wang , Xing-Gang Wu","doi":"10.1016/j.physletb.2025.139884","DOIUrl":null,"url":null,"abstract":"<div><div>We present a new approach to determining the strong coupling <span><math><mrow><msub><mi>α</mi><mi>s</mi></msub><mrow><mo>(</mo><mi>Q</mi><mo>)</mo></mrow></mrow></math></span>, over the entire range of validity of perturbative QCD, for scales above <span><math><msub><mstyle><mi>Λ</mi></mstyle><mrow><mi>QCD</mi></mrow></msub></math></span> and up to the Planck scale <span><math><mrow><mo>∼</mo><mn>1.22</mn><mo>·</mo><msup><mn>10</mn><mn>19</mn></msup></mrow></math></span> GeV, with the highest precision and using the data of a single experiment. In particular, we use the results obtained for the thrust (<span><math><mi>T</mi></math></span>) and <span><math><mi>C</mi></math></span>-parameter (<span><math><mi>C</mi></math></span>) distributions in <span><math><mrow><msup><mi>e</mi><mo>+</mo></msup><msup><mi>e</mi><mo>−</mo></msup></mrow></math></span> annihilation at a single annihilation energy <span><math><mrow><msqrt><mi>s</mi></msqrt><mo>=</mo><msub><mi>M</mi><mi>Z</mi></msub></mrow></math></span> (i.e. at the <span><math><msup><mi>Z</mi><mn>0</mn></msup></math></span> peak). This new method is based on the <em>intrinsic conformality</em> (iCF) and on the Infinite-Order Scale Setting, using the Principle of Maximum Conformality (i.e. the PMC<span><math><msub><mrow></mrow><mi>∞</mi></msub></math></span>), which allows a rigorous determination of the renormalization scales for the event-shape variable distributions satisfying all of the requirements of Renormalization Group Invariance, including renormalization-scheme independence and consistency with Abelian theory in the <span><math><mrow><msub><mi>N</mi><mi>C</mi></msub><mo>→</mo><mn>0</mn></mrow></math></span> limit. This new method is based on the scale-invariance of the iCF, which allows determination of <span><math><mrow><msub><mi>α</mi><mi>s</mi></msub><mrow><mo>(</mo><msub><mi>μ</mi><mn>0</mn></msub><mo>)</mo></mrow></mrow></math></span> at any scale <span><math><msub><mi>μ</mi><mn>0</mn></msub></math></span>, and on the Maximum Likelihood statistical approach. We propose a novel approach to determining the best-fitting range by considering all possible intervals over the entire range of bins available in the perturbative region and selecting that which returns the most-likely-lowest <span><math><msubsup><mi>χ</mi><mrow><mi>min</mi></mrow><mn>2</mn></msubsup></math></span>. This new method is designed to eliminate the errors that arise due to selection of the bin-interval and that have been neglected in previous analyses. In particular, using data for thrust and <span><math><mi>C</mi></math></span>-parameter at the <span><math><msup><mi>Z</mi><mn>0</mn></msup></math></span> peak from ALEPH, OPAL, DELPHI and L3 experiments, we obtain the average value: <span><math><mrow><msub><mi>α</mi><mi>s</mi></msub><mrow><mo>(</mo><msub><mi>M</mi><mi>Z</mi></msub><mo>)</mo></mrow><mo>=</mo><mn>0</mn><mo>.</mo><msubsup><mn>1182</mn><mrow><mo>−</mo><mn>0.0007</mn></mrow><mrow><mo>+</mo><mn>0.0007</mn></mrow></msubsup></mrow></math></span>, for the strong coupling. This determination of <span><math><mrow><msub><mi>α</mi><mi>s</mi></msub><mrow><mo>(</mo><msub><mi>M</mi><mi>Z</mi></msub><mo>)</mo></mrow></mrow></math></span> is consistent with the world average and has an improved precision with respect to the values obtained from the analysis of event shape observables currently used in the world average.</div></div>","PeriodicalId":20162,"journal":{"name":"Physics Letters B","volume":"869 ","pages":"Article 139884"},"PeriodicalIF":4.5000,"publicationDate":"2025-09-12","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Scheme-independent determination of the QCD running coupling at all scales from jet observables using the principle of maximum conformality and infinite-order scale setting\",\"authors\":\"Leonardo Di Giustino , Stanley J. Brodsky , Philip G. Ratcliffe , Sheng-Quan Wang , Xing-Gang Wu\",\"doi\":\"10.1016/j.physletb.2025.139884\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><div>We present a new approach to determining the strong coupling <span><math><mrow><msub><mi>α</mi><mi>s</mi></msub><mrow><mo>(</mo><mi>Q</mi><mo>)</mo></mrow></mrow></math></span>, over the entire range of validity of perturbative QCD, for scales above <span><math><msub><mstyle><mi>Λ</mi></mstyle><mrow><mi>QCD</mi></mrow></msub></math></span> and up to the Planck scale <span><math><mrow><mo>∼</mo><mn>1.22</mn><mo>·</mo><msup><mn>10</mn><mn>19</mn></msup></mrow></math></span> GeV, with the highest precision and using the data of a single experiment. In particular, we use the results obtained for the thrust (<span><math><mi>T</mi></math></span>) and <span><math><mi>C</mi></math></span>-parameter (<span><math><mi>C</mi></math></span>) distributions in <span><math><mrow><msup><mi>e</mi><mo>+</mo></msup><msup><mi>e</mi><mo>−</mo></msup></mrow></math></span> annihilation at a single annihilation energy <span><math><mrow><msqrt><mi>s</mi></msqrt><mo>=</mo><msub><mi>M</mi><mi>Z</mi></msub></mrow></math></span> (i.e. at the <span><math><msup><mi>Z</mi><mn>0</mn></msup></math></span> peak). This new method is based on the <em>intrinsic conformality</em> (iCF) and on the Infinite-Order Scale Setting, using the Principle of Maximum Conformality (i.e. the PMC<span><math><msub><mrow></mrow><mi>∞</mi></msub></math></span>), which allows a rigorous determination of the renormalization scales for the event-shape variable distributions satisfying all of the requirements of Renormalization Group Invariance, including renormalization-scheme independence and consistency with Abelian theory in the <span><math><mrow><msub><mi>N</mi><mi>C</mi></msub><mo>→</mo><mn>0</mn></mrow></math></span> limit. This new method is based on the scale-invariance of the iCF, which allows determination of <span><math><mrow><msub><mi>α</mi><mi>s</mi></msub><mrow><mo>(</mo><msub><mi>μ</mi><mn>0</mn></msub><mo>)</mo></mrow></mrow></math></span> at any scale <span><math><msub><mi>μ</mi><mn>0</mn></msub></math></span>, and on the Maximum Likelihood statistical approach. We propose a novel approach to determining the best-fitting range by considering all possible intervals over the entire range of bins available in the perturbative region and selecting that which returns the most-likely-lowest <span><math><msubsup><mi>χ</mi><mrow><mi>min</mi></mrow><mn>2</mn></msubsup></math></span>. This new method is designed to eliminate the errors that arise due to selection of the bin-interval and that have been neglected in previous analyses. In particular, using data for thrust and <span><math><mi>C</mi></math></span>-parameter at the <span><math><msup><mi>Z</mi><mn>0</mn></msup></math></span> peak from ALEPH, OPAL, DELPHI and L3 experiments, we obtain the average value: <span><math><mrow><msub><mi>α</mi><mi>s</mi></msub><mrow><mo>(</mo><msub><mi>M</mi><mi>Z</mi></msub><mo>)</mo></mrow><mo>=</mo><mn>0</mn><mo>.</mo><msubsup><mn>1182</mn><mrow><mo>−</mo><mn>0.0007</mn></mrow><mrow><mo>+</mo><mn>0.0007</mn></mrow></msubsup></mrow></math></span>, for the strong coupling. This determination of <span><math><mrow><msub><mi>α</mi><mi>s</mi></msub><mrow><mo>(</mo><msub><mi>M</mi><mi>Z</mi></msub><mo>)</mo></mrow></mrow></math></span> is consistent with the world average and has an improved precision with respect to the values obtained from the analysis of event shape observables currently used in the world average.</div></div>\",\"PeriodicalId\":20162,\"journal\":{\"name\":\"Physics Letters B\",\"volume\":\"869 \",\"pages\":\"Article 139884\"},\"PeriodicalIF\":4.5000,\"publicationDate\":\"2025-09-12\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Physics Letters B\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/S0370269325006434\",\"RegionNum\":2,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q1\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Physics Letters B","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0370269325006434","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
Scheme-independent determination of the QCD running coupling at all scales from jet observables using the principle of maximum conformality and infinite-order scale setting
We present a new approach to determining the strong coupling , over the entire range of validity of perturbative QCD, for scales above and up to the Planck scale GeV, with the highest precision and using the data of a single experiment. In particular, we use the results obtained for the thrust () and -parameter () distributions in annihilation at a single annihilation energy (i.e. at the peak). This new method is based on the intrinsic conformality (iCF) and on the Infinite-Order Scale Setting, using the Principle of Maximum Conformality (i.e. the PMC), which allows a rigorous determination of the renormalization scales for the event-shape variable distributions satisfying all of the requirements of Renormalization Group Invariance, including renormalization-scheme independence and consistency with Abelian theory in the limit. This new method is based on the scale-invariance of the iCF, which allows determination of at any scale , and on the Maximum Likelihood statistical approach. We propose a novel approach to determining the best-fitting range by considering all possible intervals over the entire range of bins available in the perturbative region and selecting that which returns the most-likely-lowest . This new method is designed to eliminate the errors that arise due to selection of the bin-interval and that have been neglected in previous analyses. In particular, using data for thrust and -parameter at the peak from ALEPH, OPAL, DELPHI and L3 experiments, we obtain the average value: , for the strong coupling. This determination of is consistent with the world average and has an improved precision with respect to the values obtained from the analysis of event shape observables currently used in the world average.
期刊介绍:
Physics Letters B ensures the rapid publication of important new results in particle physics, nuclear physics and cosmology. Specialized editors are responsible for contributions in experimental nuclear physics, theoretical nuclear physics, experimental high-energy physics, theoretical high-energy physics, and astrophysics.