Article(id=1242118715492335697, tenantId=1146029695717560320, journalId=1146031591421210625, issueId=1242118642922488529, articleNumber=null, orderNo=null, doi=null, pmid=null, cstr=null, oa=null, hot=null, price=null, onlineType=0, articleFormat=0, articleType=null, articleTypeStr=null, receivedDate=1096041600000, receivedDateStr=2004-09-25, revisedDate=-2209017600000, revisedDateStr=1900-01-01, acceptedDate=null, acceptedDateStr=null, onlineDate=1100016000000, onlineDateStr=2004-11-10, pubDate=1100016000000, pubDateStr=2004-11-10, doiRegisterDate=null, doiRegisterDateStr=null, onlineIssueDate=1100016000000, onlineIssueDateStr=2004-11-10, onlineJustAcceptDate=null, onlineJustAcceptDateStr=null, onlineFirstDate=null, onlineFirstDateStr=null, sourceXml=null, magXml=null, createTime=1774073779221, creator=sys-migrate, updateTime=1774073779221, updator=sys-migrate, issue=Issue{id=1242118642922488529, tenantId=1146029695717560320, journalId=1146031591421210625, year='2004', volume='22', issue='0411', pageStart='1', pageEnd='65', issueExtLink='null', onlineDate='null', pubDate='1100016000000', pubDateStr='2004-11-10', beforeIssueId=null, nextIssueId=null, price=null, status=1, issueComplete=1, articleOrder=3, issueType=-1, specialIssue=null, createTime=1774073761919, creator='sys-migrate', updateTime=1774073761919, updator='sys-migrate', preIssue=null, nextIssue=null, articleTotal=null, ext=null, issueFiles=null, downloadFileDto=null}, startPage=19, endPage=22, ext={EN=ArticleExt(id=1242118719426597349, articleId=1242118715492335697, tenantId=1146029695717560320, journalId=1146031591421210625, language=EN, title=THEORETICAL EXPLANATIONS FOR THE WEINBERG ANGLE ANOMALY, columnId=1242118638866596547, journalTitle=Science & Technology Review, columnName=论文, runingTitle=null, highlight=null, articleAbstract=Weinberg angle (or weak angle) is so important that it can partly confirm the Standard Model (SM), which has been widely accepted because the predictions in the SM are consistent with the experiment data in the last twenty years. In 2002, the value of Weinberg angle reported by the NuTeV collaboration is different from the world average value measured in other electroweak processes. An extensive attention has been paid to this anomaly, because it would shed light on particle physics whether it can be explained or not within the Standard Model. In order to explain this discrepancy, we obtained the correction to the Paschos-Wolfenstein relation when the distributions of strange quark-antiquark are asymmetric within the SM. In this work, we calculated the asymmetry of strange quark-antiquark distributions in the nucleon by using the light-cone meson-baryon fluctuation model and the chiral quark model and gained similar results. As a result, we found that the correction due to the asymmetry of the strange quark-antiquark distributions can remove the NuTeV anomaly to a great extent, which implies that asymmetric strange-antistrange quark distributions may be a reasonable explanation for the NuTeV defect., authors=DING Yong, MA Bo-qiang, authorsList=DING Yong;MA Bo-qiang, authorCompany=School of Physics, Peking University, Beijing 100871,China, correspAuthors=null, authorNote=null, correspAuthorsNote=null, copyrightStatement=null, copyrightOwner=null, extLink=null, articleAbsUrl=null, sourceXml=null, magXml=null, pdfUrl=null, pdf=OM3u80HKmKyJD/JPVEqUQA==, pdfFileSize=248370, pdfExtLink=null, richHtmlUrl=null, mobilePdfUrl=null, reviewReport=null, pdfFirstPage=null, abstractGraph=null, abstractGraphContent=null, abstractVideo=null, citation=null, cebUrl=null, magXmlContent=null, mapNumber=null, fund=null), CN=ArticleExt(id=1242118717182644692, articleId=1242118715492335697, tenantId=1146029695717560320, journalId=1146031591421210625, language=CN, title=Weinberg角反常现象的理论解释, columnId=1242117055294537731, journalTitle=科技导报, columnName=论文, runingTitle=null, highlight=null, articleAbstract=标准模型在过去20年中经历了大量的实验检验,已被人们所接受。Weinberg角(或称弱角)是标准模型中一个极其重要的物理量,它的精确值对于检验标准模型有着至关重要的作用。2002年,NuTeV实验组报道了他们测量到的Weinberg角的值与在其它电弱过程中测量到的该角的值不同。这一反常现象引起了人们极大的关注,无论能否在标准模型内解释这种现象,对粒子物理都将是一个推进。为了解释这种反常现象,本文在标准模型的框架下,推导了核子海中奇异-反奇异夸克分布不对称对Paschos-Wolfenstein关系的修正,并计算了光锥介子-重子波动模型和手征夸克模型下,奇异-反奇异夸克分布的不对称性,考查了这种不对称性对Weinberg角测量值的影响。结果表明,核子海中奇异-反奇异夸克分布的不对称性所引起的修正,能够在很大程度上降低NuTeV测量到的Weinberg角的值与标准模型预言值之间的差异,可以作为NuTeV反常现象的一种合理的解释。, authors=丁勇, 马伯强, authorsList=丁勇;马伯强, authorCompany=北京大学物理学院,北京100871, correspAuthors=null, authorNote=null, correspAuthorsNote=null, copyrightStatement=null, copyrightOwner=null, extLink=null, articleAbsUrl=null, sourceXml=null, magXml=null, pdfUrl=null, pdf=q5sZTAi3hAtQOZAm3bqjHA==, pdfFileSize=248370, pdfExtLink=null, richHtmlUrl=null, mobilePdfUrl=null, reviewReport=null, pdfFirstPage=null, 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Weinberg角反常现象的理论解释
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科技导报 | 论文 2004,22(0411): 19-22
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科技导报 |论文 2004 , 22 (0411) : 19 -22
Weinberg角反常现象的理论解释
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丁勇, 马伯强
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    北京大学物理学院,北京100871
THEORETICAL EXPLANATIONS FOR THE WEINBERG ANGLE ANOMALY
  • DING Yong, MA Bo-qiang
  • Affiliations
      School of Physics, Peking University, Beijing 100871,China
    出版时间: 2004-11-10
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    标准模型在过去20年中经历了大量的实验检验,已被人们所接受。Weinberg角(或称弱角)是标准模型中一个极其重要的物理量,它的精确值对于检验标准模型有着至关重要的作用。2002年,NuTeV实验组报道了他们测量到的Weinberg角的值与在其它电弱过程中测量到的该角的值不同。这一反常现象引起了人们极大的关注,无论能否在标准模型内解释这种现象,对粒子物理都将是一个推进。为了解释这种反常现象,本文在标准模型的框架下,推导了核子海中奇异-反奇异夸克分布不对称对Paschos-Wolfenstein关系的修正,并计算了光锥介子-重子波动模型和手征夸克模型下,奇异-反奇异夸克分布的不对称性,考查了这种不对称性对Weinberg角测量值的影响。结果表明,核子海中奇异-反奇异夸克分布的不对称性所引起的修正,能够在很大程度上降低NuTeV测量到的Weinberg角的值与标准模型预言值之间的差异,可以作为NuTeV反常现象的一种合理的解释。
    Paschos-Wolfenstein关系  /  温伯格角  /  核子海  /  奇异反奇异夸克分布不对称
    Weinberg angle (or weak angle) is so important that it can partly confirm the Standard Model (SM), which has been widely accepted because the predictions in the SM are consistent with the experiment data in the last twenty years. In 2002, the value of Weinberg angle reported by the NuTeV collaboration is different from the world average value measured in other electroweak processes. An extensive attention has been paid to this anomaly, because it would shed light on particle physics whether it can be explained or not within the Standard Model. In order to explain this discrepancy, we obtained the correction to the Paschos-Wolfenstein relation when the distributions of strange quark-antiquark are asymmetric within the SM. In this work, we calculated the asymmetry of strange quark-antiquark distributions in the nucleon by using the light-cone meson-baryon fluctuation model and the chiral quark model and gained similar results. As a result, we found that the correction due to the asymmetry of the strange quark-antiquark distributions can remove the NuTeV anomaly to a great extent, which implies that asymmetric strange-antistrange quark distributions may be a reasonable explanation for the NuTeV defect.
    Paschos-Wolfenstein relation  /  Weinberg angle  /  nucleon sea  /  asymmetry of strange-antistrange quark distribution
    丁勇;马伯强. Weinberg角反常现象的理论解释. 科技导报, 2004 , 22 (0411) : 19 -22 .
    DING Yong;MA Bo-qiang. THEORETICAL EXPLANATIONS FOR THE WEINBERG ANGLE ANOMALY[J]. Science & Technology Review, 2004 , 22 (0411) : 19 -22 .

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    • 接收时间:2004-09-25
    • 首发时间:2004-11-10
    • 出版时间:2004-11-10
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    小菇科 Mycenaceae 2 12 5.74 丝盖伞属 Inocybe 5 2.39
    多孔菌科 Polyporaceae 8 14 6.70 蜡蘑属 Laccaria 5 2.39
    红菇科 Russulaceae 3 23 11.00 小皮伞属 Marasmius 6 2.87
    小菇属 Mycena 11 5.26
    光柄菇属 Pluteus 5 2.39
    红菇属 Russula 17 8.13
    栓菌属 Trametes 5 2.39
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