B s的研究

IF 1.5 4区 物理与天体物理 Q3 PHYSICS, PARTICLES & FIELDS
Su-Ping Jin, Zhen-Jun Xiao
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We first evaluated all relevant form factors <jats:inline-formula>\n <math xmlns=\"http://www.w3.org/1998/Math/MathML\" id=\"M4\">\n <msub>\n <mrow>\n <mi>F</mi>\n </mrow>\n <mrow>\n <mi>i</mi>\n </mrow>\n </msub>\n <mfenced open=\"(\" close=\")\">\n <mrow>\n <msup>\n <mrow>\n <mi>q</mi>\n </mrow>\n <mrow>\n <mn>2</mn>\n </mrow>\n </msup>\n </mrow>\n </mfenced>\n </math>\n </jats:inline-formula> in the low-<jats:inline-formula>\n <math xmlns=\"http://www.w3.org/1998/Math/MathML\" id=\"M5\">\n <msup>\n <mrow>\n <mi>q</mi>\n </mrow>\n <mrow>\n <mn>2</mn>\n </mrow>\n </msup>\n </math>\n </jats:inline-formula> region using the PQCD approach, and we also took the available lattice QCD results at the high-<jats:inline-formula>\n <math xmlns=\"http://www.w3.org/1998/Math/MathML\" id=\"M6\">\n <msup>\n <mrow>\n <mi>q</mi>\n </mrow>\n <mrow>\n <mn>2</mn>\n </mrow>\n </msup>\n </math>\n </jats:inline-formula> region as additional input to improve the extrapolation of <jats:inline-formula>\n <math xmlns=\"http://www.w3.org/1998/Math/MathML\" id=\"M7\">\n <msub>\n <mrow>\n <mi>F</mi>\n </mrow>\n <mrow>\n <mi>i</mi>\n </mrow>\n </msub>\n <mfenced open=\"(\" close=\")\">\n <mrow>\n <msup>\n <mrow>\n <mi>q</mi>\n </mrow>\n <mrow>\n <mn>2</mn>\n </mrow>\n </msup>\n </mrow>\n </mfenced>\n </math>\n </jats:inline-formula> from the low-<jats:inline-formula>\n <math xmlns=\"http://www.w3.org/1998/Math/MathML\" id=\"M8\">\n <msup>\n <mrow>\n <mi>q</mi>\n </mrow>\n <mrow>\n <mn>2</mn>\n </mrow>\n </msup>\n </math>\n </jats:inline-formula> region to the endpoint <jats:inline-formula>\n <math xmlns=\"http://www.w3.org/1998/Math/MathML\" id=\"M9\">\n <msubsup>\n <mrow>\n <mi>q</mi>\n </mrow>\n <mrow>\n <mi mathvariant=\"normal\">max</mi>\n </mrow>\n <mrow>\n <mn>2</mn>\n </mrow>\n </msubsup>\n </math>\n </jats:inline-formula>. We then calculated the branching ratios and many other physical observables <jats:inline-formula>\n <math xmlns=\"http://www.w3.org/1998/Math/MathML\" id=\"M10\">\n <msubsup>\n <mrow>\n <mi>A</mi>\n </mrow>\n <mrow>\n <mtext>FB</mtext>\n </mrow>\n <mrow>\n <mi>l</mi>\n </mrow>\n </msubsup>\n </math>\n </jats:inline-formula>, <jats:inline-formula>\n <math xmlns=\"http://www.w3.org/1998/Math/MathML\" id=\"M11\">\n <msubsup>\n <mrow>\n <mi>F</mi>\n </mrow>\n <mrow>\n <mi>L</mi>\n </mrow>\n <mrow>\n <mi>ϕ</mi>\n </mrow>\n </msubsup>\n </math>\n </jats:inline-formula>, <jats:inline-formula>\n <math xmlns=\"http://www.w3.org/1998/Math/MathML\" id=\"M12\">\n <msub>\n <mrow>\n <mi>S</mi>\n </mrow>\n <mrow>\n <mn>3</mn>\n <mo>,</mo>\n <mn>4</mn>\n <mo>,</mo>\n <mn>7</mn>\n </mrow>\n </msub>\n </math>\n </jats:inline-formula>, and <jats:inline-formula>\n <math xmlns=\"http://www.w3.org/1998/Math/MathML\" id=\"M13\">\n <msub>\n <mrow>\n <mi>A</mi>\n </mrow>\n <mrow>\n <mn>5</mn>\n <mo>,</mo>\n <mn>6</mn>\n <mo>,</mo>\n <mn>8</mn>\n <mo>,</mo>\n <mn>9</mn>\n </mrow>\n </msub>\n </math>\n </jats:inline-formula> and the clean angular observables <jats:inline-formula>\n <math xmlns=\"http://www.w3.org/1998/Math/MathML\" id=\"M14\">\n <msub>\n <mrow>\n <mi>P</mi>\n </mrow>\n <mrow>\n <mn>1</mn>\n ","PeriodicalId":7498,"journal":{"name":"Advances in High Energy Physics","volume":" ","pages":""},"PeriodicalIF":1.5000,"publicationDate":"2021-11-09","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":"{\"title\":\"Study of \\n \\n \\n B\\n \\n \\n s\\n \\n \\n ⟶\\n ϕ\\n \\n \",\"authors\":\"Su-Ping Jin, Zhen-Jun Xiao\",\"doi\":\"10.1155/2021/3840623\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<jats:p>In this paper, we studied systematically the semileptonic decays <jats:inline-formula>\\n <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\" id=\\\"M2\\\">\\n <msub>\\n <mrow>\\n <mi>B</mi>\\n </mrow>\\n <mrow>\\n <mi>s</mi>\\n </mrow>\\n </msub>\\n <mo>⟶</mo>\\n <mi>ϕ</mi>\\n <msup>\\n <mrow>\\n <mi>l</mi>\\n </mrow>\\n <mrow>\\n <mo>+</mo>\\n </mrow>\\n </msup>\\n <msup>\\n <mrow>\\n <mi>l</mi>\\n </mrow>\\n <mrow>\\n <mo>−</mo>\\n </mrow>\\n </msup>\\n </math>\\n </jats:inline-formula> with <jats:inline-formula>\\n <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\" id=\\\"M3\\\">\\n <msup>\\n <mrow>\\n <mi>l</mi>\\n </mrow>\\n <mrow>\\n <mo>−</mo>\\n </mrow>\\n </msup>\\n <mo>=</mo>\\n <mfenced open=\\\"(\\\" close=\\\")\\\">\\n <mrow>\\n <msup>\\n <mrow>\\n <mi>e</mi>\\n </mrow>\\n <mrow>\\n <mo>−</mo>\\n </mrow>\\n </msup>\\n <mo>,</mo>\\n <msup>\\n <mrow>\\n <mi>μ</mi>\\n </mrow>\\n <mrow>\\n <mo>−</mo>\\n </mrow>\\n </msup>\\n <mo>,</mo>\\n <msup>\\n <mrow>\\n <mi>τ</mi>\\n </mrow>\\n <mrow>\\n <mo>−</mo>\\n </mrow>\\n </msup>\\n </mrow>\\n </mfenced>\\n </math>\\n </jats:inline-formula> by using the perturbative QCD (PQCD) and the “PQCD+Lattice” factorization approach, respectively. 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We then calculated the branching ratios and many other physical observables <jats:inline-formula>\\n <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\" id=\\\"M10\\\">\\n <msubsup>\\n <mrow>\\n <mi>A</mi>\\n </mrow>\\n <mrow>\\n <mtext>FB</mtext>\\n </mrow>\\n <mrow>\\n <mi>l</mi>\\n </mrow>\\n </msubsup>\\n </math>\\n </jats:inline-formula>, <jats:inline-formula>\\n <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\" id=\\\"M11\\\">\\n <msubsup>\\n <mrow>\\n <mi>F</mi>\\n </mrow>\\n <mrow>\\n <mi>L</mi>\\n </mrow>\\n <mrow>\\n <mi>ϕ</mi>\\n </mrow>\\n </msubsup>\\n </math>\\n </jats:inline-formula>, <jats:inline-formula>\\n <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\" id=\\\"M12\\\">\\n <msub>\\n <mrow>\\n <mi>S</mi>\\n </mrow>\\n <mrow>\\n <mn>3</mn>\\n <mo>,</mo>\\n <mn>4</mn>\\n <mo>,</mo>\\n <mn>7</mn>\\n </mrow>\\n </msub>\\n </math>\\n </jats:inline-formula>, and <jats:inline-formula>\\n <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\" id=\\\"M13\\\">\\n <msub>\\n <mrow>\\n <mi>A</mi>\\n </mrow>\\n <mrow>\\n <mn>5</mn>\\n <mo>,</mo>\\n <mn>6</mn>\\n <mo>,</mo>\\n <mn>8</mn>\\n <mo>,</mo>\\n <mn>9</mn>\\n </mrow>\\n </msub>\\n </math>\\n </jats:inline-formula> and the clean angular observables <jats:inline-formula>\\n <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\" id=\\\"M14\\\">\\n <msub>\\n <mrow>\\n <mi>P</mi>\\n </mrow>\\n <mrow>\\n <mn>1</mn>\\n \",\"PeriodicalId\":7498,\"journal\":{\"name\":\"Advances in High Energy Physics\",\"volume\":\" \",\"pages\":\"\"},\"PeriodicalIF\":1.5000,\"publicationDate\":\"2021-11-09\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"1\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Advances in High Energy Physics\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://doi.org/10.1155/2021/3840623\",\"RegionNum\":4,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q3\",\"JCRName\":\"PHYSICS, PARTICLES & FIELDS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Advances in High Energy Physics","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1155/2021/3840623","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"PHYSICS, PARTICLES & FIELDS","Score":null,"Total":0}
引用次数: 1

摘要

在本文中,我们系统地研究了半光子衰减B s+ l−with l−= e−,μ−,τ−分别采用微扰QCD (PQCD)和“PQCD+晶格”分解方法。我们首先评估了所有相关的外形因素F i q2在低q2区域使用PQCD方法,并且我们还将高q2区域的可用晶格QCD结果作为额外输入,以改进的外推F i q 2从低q2区域到端点qMax 2。 然后,我们计算了分支比率和许多其他物理观察结果,F l φ,S 3 4 7,和A 5,6,8,9和干净角观测值p1
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Study of B s ⟶ ϕ
In this paper, we studied systematically the semileptonic decays B s ϕ l + l with l = e , μ , τ by using the perturbative QCD (PQCD) and the “PQCD+Lattice” factorization approach, respectively. We first evaluated all relevant form factors F i q 2 in the low- q 2 region using the PQCD approach, and we also took the available lattice QCD results at the high- q 2 region as additional input to improve the extrapolation of F i q 2 from the low- q 2 region to the endpoint q max 2 . We then calculated the branching ratios and many other physical observables A FB l , F L ϕ , S 3 , 4 , 7 , and A 5 , 6 , 8 , 9 and the clean angular observables P 1
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来源期刊
Advances in High Energy Physics
Advances in High Energy Physics PHYSICS, PARTICLES & FIELDS-
CiteScore
3.40
自引率
5.90%
发文量
55
审稿时长
6-12 weeks
期刊介绍: Advances in High Energy Physics publishes the results of theoretical and experimental research on the nature of, and interaction between, energy and matter. Considering both original research and focussed review articles, the journal welcomes submissions from small research groups and large consortia alike.
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