运动功率修正深度虚拟康普顿散射到扭转六精度

IF 5.3 2区 物理与天体物理 Q1 Physics and Astronomy
V. M. Braun, Yao Ji, A. N. Manashov
{"title":"运动功率修正深度虚拟康普顿散射到扭转六精度","authors":"V. M. Braun, Yao Ji, A. N. Manashov","doi":"10.1103/physrevd.111.076011","DOIUrl":null,"url":null,"abstract":"We calculate (</a:mo>−</a:mo>t</a:mi></a:mrow></a:msqrt>/</a:mo>Q</a:mi>)</a:mo>k</a:mi></a:msup></a:math> and <e:math xmlns:e=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><e:mo stretchy=\"false\">(</e:mo><e:mi>m</e:mi><e:mo>/</e:mo><e:mi>Q</e:mi><e:msup><e:mo stretchy=\"false\">)</e:mo><e:mi>k</e:mi></e:msup></e:math> power corrections with <i:math xmlns:i=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><i:mi>k</i:mi><i:mo>≤</i:mo><i:mn>4</i:mn></i:math>, where <k:math xmlns:k=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><k:mi>m</k:mi></k:math> is the target mass and <m:math xmlns:m=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><m:mi>t</m:mi></m:math> is the momentum transfer, to several key observables in deeply virtual Compton scattering (DVCS). We find that the power expansion is well convergent up to <o:math xmlns:o=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><o:mo stretchy=\"false\">|</o:mo><o:mi>t</o:mi><o:mo stretchy=\"false\">|</o:mo><o:mo>/</o:mo><o:msup><o:mi>Q</o:mi><o:mn>2</o:mn></o:msup><o:mo>≲</o:mo><o:mn>1</o:mn><o:mo>/</o:mo><o:mn>4</o:mn></o:math> for most of the observables, but is naturally organized in terms of <s:math xmlns:s=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><s:mn>1</s:mn><s:mo>/</s:mo><s:mo stretchy=\"false\">(</s:mo><s:msup><s:mi>Q</s:mi><s:mn>2</s:mn></s:msup><s:mo>+</s:mo><s:mi>t</s:mi><s:mo stretchy=\"false\">)</s:mo></s:math> rather than the nominal hard scale <w:math xmlns:w=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><w:mn>1</w:mn><w:mo>/</w:mo><w:msup><w:mi>Q</w:mi><w:mn>2</w:mn></w:msup></w:math>. We also argue that target mass corrections remain under control and do not endanger quantum chromodynamics (QCD) factorization for coherent DVCS on nuclei. These results remove an important source of uncertainties due to the frame dependence and violation of electromagnetic Ward identities in the QCD predictions for the DVCS amplitudes in the leading-twist approximation. <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":"183 1","pages":""},"PeriodicalIF":5.3000,"publicationDate":"2025-04-14","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Kinematic power corrections to deeply virtual Compton scattering to twist-six accuracy\",\"authors\":\"V. M. Braun, Yao Ji, A. N. Manashov\",\"doi\":\"10.1103/physrevd.111.076011\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"We calculate (</a:mo>−</a:mo>t</a:mi></a:mrow></a:msqrt>/</a:mo>Q</a:mi>)</a:mo>k</a:mi></a:msup></a:math> and <e:math xmlns:e=\\\"http://www.w3.org/1998/Math/MathML\\\" display=\\\"inline\\\"><e:mo stretchy=\\\"false\\\">(</e:mo><e:mi>m</e:mi><e:mo>/</e:mo><e:mi>Q</e:mi><e:msup><e:mo stretchy=\\\"false\\\">)</e:mo><e:mi>k</e:mi></e:msup></e:math> power corrections with <i:math xmlns:i=\\\"http://www.w3.org/1998/Math/MathML\\\" display=\\\"inline\\\"><i:mi>k</i:mi><i:mo>≤</i:mo><i:mn>4</i:mn></i:math>, where <k:math xmlns:k=\\\"http://www.w3.org/1998/Math/MathML\\\" display=\\\"inline\\\"><k:mi>m</k:mi></k:math> is the target mass and <m:math xmlns:m=\\\"http://www.w3.org/1998/Math/MathML\\\" display=\\\"inline\\\"><m:mi>t</m:mi></m:math> is the momentum transfer, to several key observables in deeply virtual Compton scattering (DVCS). We find that the power expansion is well convergent up to <o:math xmlns:o=\\\"http://www.w3.org/1998/Math/MathML\\\" display=\\\"inline\\\"><o:mo stretchy=\\\"false\\\">|</o:mo><o:mi>t</o:mi><o:mo stretchy=\\\"false\\\">|</o:mo><o:mo>/</o:mo><o:msup><o:mi>Q</o:mi><o:mn>2</o:mn></o:msup><o:mo>≲</o:mo><o:mn>1</o:mn><o:mo>/</o:mo><o:mn>4</o:mn></o:math> for most of the observables, but is naturally organized in terms of <s:math xmlns:s=\\\"http://www.w3.org/1998/Math/MathML\\\" display=\\\"inline\\\"><s:mn>1</s:mn><s:mo>/</s:mo><s:mo stretchy=\\\"false\\\">(</s:mo><s:msup><s:mi>Q</s:mi><s:mn>2</s:mn></s:msup><s:mo>+</s:mo><s:mi>t</s:mi><s:mo stretchy=\\\"false\\\">)</s:mo></s:math> rather than the nominal hard scale <w:math xmlns:w=\\\"http://www.w3.org/1998/Math/MathML\\\" display=\\\"inline\\\"><w:mn>1</w:mn><w:mo>/</w:mo><w:msup><w:mi>Q</w:mi><w:mn>2</w:mn></w:msup></w:math>. We also argue that target mass corrections remain under control and do not endanger quantum chromodynamics (QCD) factorization for coherent DVCS on nuclei. These results remove an important source of uncertainties due to the frame dependence and violation of electromagnetic Ward identities in the QCD predictions for the DVCS amplitudes in the leading-twist approximation. <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\":\"183 1\",\"pages\":\"\"},\"PeriodicalIF\":5.3000,\"publicationDate\":\"2025-04-14\",\"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.111.076011\",\"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.111.076011","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}
引用次数: 0

摘要

我们计算了深度虚康普顿散射(DVCS)中几个关键观测值在k≤4时的(- t/Q)k和(m/Q)k功率修正,其中m为目标质量,t为动量传递。我们发现,对于大多数可观测值,幂展开式可以很好地收敛到|/Q2 > 1/4,但自然地以1/(Q2+t)而不是名义上的硬尺度1/Q2组织。我们还认为目标质量修正仍然在控制之下,并且不会危及核上相干DVCS的量子色动力学(QCD)分解。这些结果消除了一个重要的不确定性来源,这是由于前导扭转近似中对DVCS振幅的QCD预测中的坐标系依赖和电磁沃德恒等的违反。2025年由美国物理学会出版
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Kinematic power corrections to deeply virtual Compton scattering to twist-six accuracy
We calculate (−t/Q)k and (m/Q)k power corrections with k4, where m is the target mass and t is the momentum transfer, to several key observables in deeply virtual Compton scattering (DVCS). We find that the power expansion is well convergent up to |t|/Q21/4 for most of the observables, but is naturally organized in terms of 1/(Q2+t) rather than the nominal hard scale 1/Q2. We also argue that target mass corrections remain under control and do not endanger quantum chromodynamics (QCD) factorization for coherent DVCS on nuclei. These results remove an important source of uncertainties due to the frame dependence and violation of electromagnetic Ward identities in the QCD predictions for the DVCS amplitudes in the leading-twist approximation. Published by the American Physical Society 2025
求助全文
通过发布文献求助,成功后即可免费获取论文全文。 去求助
来源期刊
Physical Review D
Physical Review D 物理-天文与天体物理
CiteScore
9.20
自引率
36.00%
发文量
0
审稿时长
2 months
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.
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:604180095
Book学术官方微信