B(s)→s (a0(1450), K0*(1430), f0(1500)))螺旋形因子符合QCD光锥求和规则

IF 5.3 2区 物理与天体物理 Q1 Physics and Astronomy
Yi Zhang, Wei Cheng, Jia-Wei Zhang, Tao Zhong, Hai-Bing Fu, Li-Sheng Geng
{"title":"B(s)→s (a0(1450), K0*(1430), f0(1500)))螺旋形因子符合QCD光锥求和规则","authors":"Yi Zhang, Wei Cheng, Jia-Wei Zhang, Tao Zhong, Hai-Bing Fu, Li-Sheng Geng","doi":"10.1103/27kn-4xz2","DOIUrl":null,"url":null,"abstract":"In this paper, we investigate the helicity form factors (HFFs) of the B</a:mi>(</a:mo>s</a:mi>)</a:mo></a:mrow></a:msub></a:math>-meson decay into a scalar meson with a mass larger than 1 GeV, i.e., <e:math xmlns:e=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><e:mi>B</e:mi><e:mo stretchy=\"false\">→</e:mo><e:msub><e:mi>a</e:mi><e:mn>0</e:mn></e:msub><e:mo stretchy=\"false\">(</e:mo><e:mn>1450</e:mn><e:mo stretchy=\"false\">)</e:mo></e:math>, <j:math xmlns:j=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><j:msub><j:mi>B</j:mi><j:mrow><j:mo stretchy=\"false\">(</j:mo><j:mi>s</j:mi><j:mo stretchy=\"false\">)</j:mo></j:mrow></j:msub><j:mo stretchy=\"false\">→</j:mo><j:msubsup><j:mi>K</j:mi><j:mn>0</j:mn><j:mo>*</j:mo></j:msubsup><j:mo stretchy=\"false\">(</j:mo><j:mn>1430</j:mn><j:mo stretchy=\"false\">)</j:mo></j:math>, and <q:math xmlns:q=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><q:msub><q:mi>B</q:mi><q:mi>s</q:mi></q:msub><q:mo stretchy=\"false\">→</q:mo><q:msub><q:mi>f</q:mi><q:mn>0</q:mn></q:msub><q:mo stretchy=\"false\">(</q:mo><q:mn>1500</q:mn><q:mo stretchy=\"false\">)</q:mo></q:math> by using the light-cone sum rules approach. We take the standard currents for correlation functions. To enhance the precision of our calculations, we incorporate the next-to-leading order (NLO) corrections and retain the scalar meson twist-3 light-cone distribution amplitudes. Furthermore, we extend the HFFs to the entire physical <v:math xmlns:v=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><v:msup><v:mi>q</v:mi><v:mn>2</v:mn></v:msup></v:math> region employing a simplified <x:math xmlns:x=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><x:mi>z</x:mi></x:math>-series expansion. At the point of <z:math xmlns:z=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><z:mrow><z:msup><z:mrow><z:mi>q</z:mi></z:mrow><z:mn>2</z:mn></z:msup><z:mo>=</z:mo><z:mn>1</z:mn><z:mtext> </z:mtext><z:mtext> </z:mtext><z:msup><z:mrow><z:mi>GeV</z:mi></z:mrow><z:mn>2</z:mn></z:msup></z:mrow></z:math>, all NLO contributions to the HFFs are negative, with the maximum contribution around 25%. Then, as applications of these HFFs, we analyze the differential decay widths, branching ratios, and lepton polarization asymmetries for the semileptonic <bb:math xmlns:bb=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><bb:msub><bb:mi>B</bb:mi><bb:mrow><bb:mo stretchy=\"false\">(</bb:mo><bb:mi>s</bb:mi><bb:mo stretchy=\"false\">)</bb:mo></bb:mrow></bb:msub><bb:mo stretchy=\"false\">→</bb:mo><bb:mi>S</bb:mi><bb:mo>ℓ</bb:mo><bb:msub><bb:mover accent=\"true\"><bb:mi>ν</bb:mi><bb:mo stretchy=\"false\">¯</bb:mo></bb:mover><bb:mo>ℓ</bb:mo></bb:msub></bb:math>, FCNC <ib:math xmlns:ib=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><ib:msub><ib:mi>B</ib:mi><ib:mrow><ib:mo stretchy=\"false\">(</ib:mo><ib:mi>s</ib:mi><ib:mo stretchy=\"false\">)</ib:mo></ib:mrow></ib:msub><ib:mo stretchy=\"false\">→</ib:mo><ib:mi>S</ib:mi><ib:mo>ℓ</ib:mo><ib:mover accent=\"true\"><ib:mo>ℓ</ib:mo><ib:mo stretchy=\"false\">¯</ib:mo></ib:mover></ib:math> and rare <pb:math xmlns:pb=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><pb:msub><pb:mi>B</pb:mi><pb:mrow><pb:mo stretchy=\"false\">(</pb:mo><pb:mi>s</pb:mi><pb:mo stretchy=\"false\">)</pb:mo></pb:mrow></pb:msub><pb:mo stretchy=\"false\">→</pb:mo><pb:mi>S</pb:mi><pb:mi>ν</pb:mi><pb:mover accent=\"true\"><pb:mi>ν</pb:mi><pb:mo stretchy=\"false\">¯</pb:mo></pb:mover></pb:math> decays. Our results are consistent with existing studies within uncertainties. The current data still suffer from large uncertainties and need to be measured more precisely, which can lead to a better understanding of the fundamental properties of light scalar mesons.","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"5 1","pages":""},"PeriodicalIF":5.3000,"publicationDate":"2025-09-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"B(s)→S(a0(1450), K0*(1430), f0(1500)) helicity form factors within QCD light-cone sum rules\",\"authors\":\"Yi Zhang, Wei Cheng, Jia-Wei Zhang, Tao Zhong, Hai-Bing Fu, Li-Sheng Geng\",\"doi\":\"10.1103/27kn-4xz2\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"In this paper, we investigate the helicity form factors (HFFs) of the B</a:mi>(</a:mo>s</a:mi>)</a:mo></a:mrow></a:msub></a:math>-meson decay into a scalar meson with a mass larger than 1 GeV, i.e., <e:math xmlns:e=\\\"http://www.w3.org/1998/Math/MathML\\\" display=\\\"inline\\\"><e:mi>B</e:mi><e:mo stretchy=\\\"false\\\">→</e:mo><e:msub><e:mi>a</e:mi><e:mn>0</e:mn></e:msub><e:mo stretchy=\\\"false\\\">(</e:mo><e:mn>1450</e:mn><e:mo stretchy=\\\"false\\\">)</e:mo></e:math>, <j:math xmlns:j=\\\"http://www.w3.org/1998/Math/MathML\\\" display=\\\"inline\\\"><j:msub><j:mi>B</j:mi><j:mrow><j:mo stretchy=\\\"false\\\">(</j:mo><j:mi>s</j:mi><j:mo stretchy=\\\"false\\\">)</j:mo></j:mrow></j:msub><j:mo stretchy=\\\"false\\\">→</j:mo><j:msubsup><j:mi>K</j:mi><j:mn>0</j:mn><j:mo>*</j:mo></j:msubsup><j:mo stretchy=\\\"false\\\">(</j:mo><j:mn>1430</j:mn><j:mo stretchy=\\\"false\\\">)</j:mo></j:math>, and <q:math xmlns:q=\\\"http://www.w3.org/1998/Math/MathML\\\" display=\\\"inline\\\"><q:msub><q:mi>B</q:mi><q:mi>s</q:mi></q:msub><q:mo stretchy=\\\"false\\\">→</q:mo><q:msub><q:mi>f</q:mi><q:mn>0</q:mn></q:msub><q:mo stretchy=\\\"false\\\">(</q:mo><q:mn>1500</q:mn><q:mo stretchy=\\\"false\\\">)</q:mo></q:math> by using the light-cone sum rules approach. We take the standard currents for correlation functions. To enhance the precision of our calculations, we incorporate the next-to-leading order (NLO) corrections and retain the scalar meson twist-3 light-cone distribution amplitudes. Furthermore, we extend the HFFs to the entire physical <v:math xmlns:v=\\\"http://www.w3.org/1998/Math/MathML\\\" display=\\\"inline\\\"><v:msup><v:mi>q</v:mi><v:mn>2</v:mn></v:msup></v:math> region employing a simplified <x:math xmlns:x=\\\"http://www.w3.org/1998/Math/MathML\\\" display=\\\"inline\\\"><x:mi>z</x:mi></x:math>-series expansion. At the point of <z:math xmlns:z=\\\"http://www.w3.org/1998/Math/MathML\\\" display=\\\"inline\\\"><z:mrow><z:msup><z:mrow><z:mi>q</z:mi></z:mrow><z:mn>2</z:mn></z:msup><z:mo>=</z:mo><z:mn>1</z:mn><z:mtext> </z:mtext><z:mtext> </z:mtext><z:msup><z:mrow><z:mi>GeV</z:mi></z:mrow><z:mn>2</z:mn></z:msup></z:mrow></z:math>, all NLO contributions to the HFFs are negative, with the maximum contribution around 25%. Then, as applications of these HFFs, we analyze the differential decay widths, branching ratios, and lepton polarization asymmetries for the semileptonic <bb:math xmlns:bb=\\\"http://www.w3.org/1998/Math/MathML\\\" display=\\\"inline\\\"><bb:msub><bb:mi>B</bb:mi><bb:mrow><bb:mo stretchy=\\\"false\\\">(</bb:mo><bb:mi>s</bb:mi><bb:mo stretchy=\\\"false\\\">)</bb:mo></bb:mrow></bb:msub><bb:mo stretchy=\\\"false\\\">→</bb:mo><bb:mi>S</bb:mi><bb:mo>ℓ</bb:mo><bb:msub><bb:mover accent=\\\"true\\\"><bb:mi>ν</bb:mi><bb:mo stretchy=\\\"false\\\">¯</bb:mo></bb:mover><bb:mo>ℓ</bb:mo></bb:msub></bb:math>, FCNC <ib:math xmlns:ib=\\\"http://www.w3.org/1998/Math/MathML\\\" display=\\\"inline\\\"><ib:msub><ib:mi>B</ib:mi><ib:mrow><ib:mo stretchy=\\\"false\\\">(</ib:mo><ib:mi>s</ib:mi><ib:mo stretchy=\\\"false\\\">)</ib:mo></ib:mrow></ib:msub><ib:mo stretchy=\\\"false\\\">→</ib:mo><ib:mi>S</ib:mi><ib:mo>ℓ</ib:mo><ib:mover accent=\\\"true\\\"><ib:mo>ℓ</ib:mo><ib:mo stretchy=\\\"false\\\">¯</ib:mo></ib:mover></ib:math> and rare <pb:math xmlns:pb=\\\"http://www.w3.org/1998/Math/MathML\\\" display=\\\"inline\\\"><pb:msub><pb:mi>B</pb:mi><pb:mrow><pb:mo stretchy=\\\"false\\\">(</pb:mo><pb:mi>s</pb:mi><pb:mo stretchy=\\\"false\\\">)</pb:mo></pb:mrow></pb:msub><pb:mo stretchy=\\\"false\\\">→</pb:mo><pb:mi>S</pb:mi><pb:mi>ν</pb:mi><pb:mover accent=\\\"true\\\"><pb:mi>ν</pb:mi><pb:mo stretchy=\\\"false\\\">¯</pb:mo></pb:mover></pb:math> decays. Our results are consistent with existing studies within uncertainties. The current data still suffer from large uncertainties and need to be measured more precisely, which can lead to a better understanding of the fundamental properties of light scalar mesons.\",\"PeriodicalId\":20167,\"journal\":{\"name\":\"Physical Review D\",\"volume\":\"5 1\",\"pages\":\"\"},\"PeriodicalIF\":5.3000,\"publicationDate\":\"2025-09-29\",\"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/10.1103/27kn-4xz2\",\"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/10.1103/27kn-4xz2","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

本文用光锥求和法研究了B(s)介子衰变为质量大于1 GeV的标量介子的螺旋形因子(HFFs),即B(s)→a0(1450)、B(s)→K0*(1430)和B→f0(1500)。我们取相关函数的标准电流。为了提高我们的计算精度,我们加入了次领先阶(NLO)修正,并保留了标量介子扭曲-3光锥分布幅度。此外,我们采用简化的z系列展开将HFFs扩展到整个物理q2区域。在q2=1 GeV2时,所有NLO对HFFs的贡献均为负,最大贡献约为25%。然后,作为这些HFFs的应用,我们分析了半光子B(s)→s α ν¯、FCNC B(s)→s α ν¯和稀有B(s)→s α ν¯衰变的微分衰减宽度、分支比和轻子极化不对称性。我们的结果与现有研究在不确定性范围内是一致的。目前的数据仍然存在很大的不确定性,需要更精确地测量,这可以更好地理解光标量介子的基本性质。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
B(s)→S(a0(1450), K0*(1430), f0(1500)) helicity form factors within QCD light-cone sum rules
In this paper, we investigate the helicity form factors (HFFs) of the B(s)-meson decay into a scalar meson with a mass larger than 1 GeV, i.e., Ba0(1450), B(s)K0*(1430), and Bsf0(1500) by using the light-cone sum rules approach. We take the standard currents for correlation functions. To enhance the precision of our calculations, we incorporate the next-to-leading order (NLO) corrections and retain the scalar meson twist-3 light-cone distribution amplitudes. Furthermore, we extend the HFFs to the entire physical q2 region employing a simplified z-series expansion. At the point of q2=1 GeV2, all NLO contributions to the HFFs are negative, with the maximum contribution around 25%. Then, as applications of these HFFs, we analyze the differential decay widths, branching ratios, and lepton polarization asymmetries for the semileptonic B(s)Sν¯, FCNC B(s)S¯ and rare B(s)Sνν¯ decays. Our results are consistent with existing studies within uncertainties. The current data still suffer from large uncertainties and need to be measured more precisely, which can lead to a better understanding of the fundamental properties of light scalar mesons.
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