aμ|l.ohvp, QCD power corrections and αs from e+e− → Hadrons

Stephan Narison
{"title":"aμ|l.ohvp, QCD power corrections and αs from e+e− → Hadrons","authors":"Stephan Narison","doi":"10.1016/j.nuclphysbps.2024.11.007","DOIUrl":null,"url":null,"abstract":"<div><div>In this talk, I review the results obtained recently in Ref. <span><span>[1]</span></span>. <em>First,</em> we estimate the LO hadronic vacuum polarization contribution to the muon and <em>τ</em> anomalous magnetic moments to be: <span><math><msub><mrow><mi>a</mi></mrow><mrow><mi>μ</mi></mrow></msub><msubsup><mrow><mo>|</mo></mrow><mrow><mi>l</mi><mo>.</mo><mi>o</mi></mrow><mrow><mi>h</mi><mi>v</mi><mi>p</mi></mrow></msubsup><mo>=</mo><mo>(</mo><mn>7036.5</mn><mo>±</mo><mn>38.9</mn><mo>)</mo><mo>×</mo><msup><mrow><mn>10</mn></mrow><mrow><mo>−</mo><mn>11</mn></mrow></msup></math></span>, <span><math><msub><mrow><mi>a</mi></mrow><mrow><mi>τ</mi></mrow></msub><msubsup><mrow><mo>|</mo></mrow><mrow><mi>l</mi><mo>.</mo><mi>o</mi></mrow><mrow><mi>h</mi><mi>v</mi><mi>p</mi></mrow></msubsup><mo>=</mo><mo>(</mo><mn>3494.8</mn><mo>±</mo><mn>24.7</mn><mo>)</mo><mo>×</mo><msup><mrow><mn>10</mn></mrow><mrow><mo>−</mo><mn>9</mn></mrow></msup></math></span> (see Table 1) leading to: <span><math><mi>Δ</mi><msub><mrow><mi>a</mi></mrow><mrow><mi>μ</mi></mrow></msub><mo>≡</mo><msubsup><mrow><mi>a</mi></mrow><mrow><mi>μ</mi></mrow><mrow><mi>e</mi><mi>x</mi><mi>p</mi></mrow></msubsup><mo>−</mo><msubsup><mrow><mi>a</mi></mrow><mrow><mi>μ</mi></mrow><mrow><mi>S</mi><mi>M</mi></mrow></msubsup><mo>=</mo><mo>(</mo><mn>143</mn><mo>±</mo><msub><mrow><mn>42</mn></mrow><mrow><mi>t</mi><mi>h</mi></mrow></msub><mo>±</mo><msub><mrow><mn>22</mn></mrow><mrow><mi>e</mi><mi>x</mi><mi>p</mi></mrow></msub><mo>)</mo><mo>×</mo><msup><mrow><mn>10</mn></mrow><mrow><mo>−</mo><mn>11</mn></mrow></msup></math></span> which is about 3<em>σ</em> discrepancy between the SM predictions and experiment. One also finds: <span><math><msup><mrow><mi>α</mi></mrow><mrow><mo>(</mo><mn>5</mn><mo>)</mo></mrow></msup><mo>(</mo><msub><mrow><mi>M</mi></mrow><mrow><mi>Z</mi></mrow></msub><mo>)</mo><msub><mrow><mo>|</mo></mrow><mrow><mi>h</mi><mi>a</mi><mi>d</mi></mrow></msub><mo>=</mo><mo>(</mo><mn>2766.3</mn><mo>±</mo><mn>4.5</mn><mo>)</mo><mo>×</mo><msup><mrow><mn>10</mn></mrow><mrow><mo>−</mo><mn>5</mn></mrow></msup></math></span>. <em>Second,</em> we estimate the QCD power corrections up to dimension 20 from the ratio of Laplace sum rule and from <em>τ</em>-like decay high moments (see Table 3). We do not observe any exponential growth of their size which may not favour a duality violation of the spectral function. We obtain <span><math><mo>〈</mo><msub><mrow><mi>α</mi></mrow><mrow><mi>s</mi></mrow></msub><msup><mrow><mi>G</mi></mrow><mrow><mn>2</mn></mrow></msup><mo>〉</mo><mo>=</mo><mo>(</mo><mn>7.8</mn><mo>±</mo><mn>3.5</mn><mo>)</mo><mo>×</mo><msup><mrow><mn>10</mn></mrow><mrow><mo>−</mo><mn>2</mn></mrow></msup><mspace></mspace><msup><mrow><mtext>GeV</mtext></mrow><mrow><mn>4</mn></mrow></msup></math></span> in agreement with the more precise one from heavy quark sum rules, while <span><math><mi>ρ</mi><msub><mrow><mi>α</mi></mrow><mrow><mi>s</mi></mrow></msub><msup><mrow><mo>〈</mo><mover><mrow><mi>ψ</mi></mrow><mrow><mo>¯</mo></mrow></mover><mi>ψ</mi><mo>〉</mo></mrow><mrow><mn>2</mn></mrow></msup><mo>=</mo><mo>(</mo><mn>5.98</mn><mo>±</mo><mn>0.64</mn><mo>)</mo><mo>×</mo><msup><mrow><mn>10</mn></mrow><mrow><mo>−</mo><mn>4</mn></mrow></msup><mspace></mspace><msup><mrow><mtext>GeV</mtext></mrow><mrow><mn>6</mn></mrow></msup></math></span> confirms a violation of the four-quark condensate factorization by a factor <span><math><mi>ρ</mi><mo>≃</mo><mn>6</mn></math></span>. <em>Third</em>, using the previous values of the condensates, we re-extract <span><math><msub><mrow><mi>α</mi></mrow><mrow><mi>s</mi></mrow></msub></math></span> from the lowest <em>τ</em>-decay Braaten-SN-Pich (BNP) moment and find to order <span><math><msubsup><mrow><mi>α</mi></mrow><mrow><mi>s</mi></mrow><mrow><mn>4</mn></mrow></msubsup><mo>:</mo><msub><mrow><mi>α</mi></mrow><mrow><mi>s</mi></mrow></msub><mo>(</mo><msub><mrow><mi>M</mi></mrow><mrow><mi>τ</mi></mrow></msub><mo>)</mo><mo>=</mo><mn>0.3081</mn><mo>(</mo><mn>86</mn><mo>)</mo><mspace></mspace><mo>[</mo><mrow><mi>resp</mi><mo>.</mo></mrow><mspace></mspace><mn>0.3260</mn><mo>(</mo><mn>79</mn><mo>)</mo><mo>]</mo><mo>⟶</mo><mspace></mspace><mo>∘</mo><mspace></mspace><mspace></mspace><msub><mrow><mi>α</mi></mrow><mrow><mi>s</mi></mrow></msub><mo>(</mo><msub><mrow><mi>M</mi></mrow><mrow><mi>Z</mi></mrow></msub><mo>)</mo><mo>=</mo><mn>0.1170</mn><mo>(</mo><mn>7</mn><mo>)</mo><mspace></mspace><mo>[</mo><mrow><mi>resp</mi><mo>.</mo></mrow><mspace></mspace><mn>0.1192</mn><mo>(</mo><mn>7</mn><mo>)</mo><mo>]</mo></math></span> for Fixed Order (FO) [resp. Contour Improved (CI)] PT series. We also show that the contributions beyond the Shifman-Vainshtein-Zakharov (SVZ)-expansion are negligible.</div></div>","PeriodicalId":37968,"journal":{"name":"Nuclear and Particle Physics Proceedings","volume":"347 ","pages":"Pages 105-115"},"PeriodicalIF":0.0000,"publicationDate":"2024-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Nuclear and Particle Physics Proceedings","FirstCategoryId":"1085","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S2405601424001718","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"Physics and Astronomy","Score":null,"Total":0}
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Abstract

In this talk, I review the results obtained recently in Ref. [1]. First, we estimate the LO hadronic vacuum polarization contribution to the muon and τ anomalous magnetic moments to be: aμ|l.ohvp=(7036.5±38.9)×1011, aτ|l.ohvp=(3494.8±24.7)×109 (see Table 1) leading to: ΔaμaμexpaμSM=(143±42th±22exp)×1011 which is about 3σ discrepancy between the SM predictions and experiment. One also finds: α(5)(MZ)|had=(2766.3±4.5)×105. Second, we estimate the QCD power corrections up to dimension 20 from the ratio of Laplace sum rule and from τ-like decay high moments (see Table 3). We do not observe any exponential growth of their size which may not favour a duality violation of the spectral function. We obtain αsG2=(7.8±3.5)×102GeV4 in agreement with the more precise one from heavy quark sum rules, while ραsψ¯ψ2=(5.98±0.64)×104GeV6 confirms a violation of the four-quark condensate factorization by a factor ρ6. Third, using the previous values of the condensates, we re-extract αs from the lowest τ-decay Braaten-SN-Pich (BNP) moment and find to order αs4:αs(Mτ)=0.3081(86)[resp.0.3260(79)]αs(MZ)=0.1170(7)[resp.0.1192(7)] for Fixed Order (FO) [resp. Contour Improved (CI)] PT series. We also show that the contributions beyond the Shifman-Vainshtein-Zakharov (SVZ)-expansion are negligible.
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一个μl |。e+e− → 强子的ohvp, QCD功率修正和αs
在这次演讲中,我回顾了最近在Ref. b[1]中获得的结果。首先,我们估计LO强子真空极化对μ子和τ异常磁矩的贡献为:aμ|l.ohvp=(7036.5±38.9)×10−11,aτ|l.ohvp=(3494.8±24.7)×10−9(见表1),导致:Δaμ≡aμexp−aμSM=(143±42±22exp)×10−11,这与SM预测和实验之间的误差约为3σ。α(5)(MZ)| =(2766.3±4.5)×10−5。其次,我们从拉普拉斯和规则的比率和τ样衰减高矩(见表3)估计到20维的QCD功率修正。我们没有观察到它们的大小的任何指数增长,这可能不利于谱函数的对偶性违反。我们得到< αsG2 > =(7.8±3.5)×10−2GeV4符合重夸克和规则,而ραs < ψ¯ψ > 2=(5.98±0.64)×10−4GeV6证实了一个因子ρ≃6违反了四夸克凝聚分解。第三,利用先前的凝析油值,从最低τ-衰变braten - sn - pich (BNP)矩中重新提取αs,得到αs4阶:αs(Mτ)=0.3081(86)[resp.0.3260(79)]。轮廓改进(CI)] PT系列。我们还证明了超出Shifman-Vainshtein-Zakharov (SVZ)展开式的贡献可以忽略不计。
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Nuclear and Particle Physics Proceedings
Nuclear and Particle Physics Proceedings Physics and Astronomy-Nuclear and High Energy Physics
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期刊介绍: Nuclear and Particle Physics Proceedings is the premier publication outlet for the proceedings of key conferences on nuclear and high-energy physics and related areas. The series covers both large international conferences and topical meetings. The newest discoveries and the latest developments, reported at carefully selected meetings, are published covering experimental as well as theoretical particle physics, nuclear and hadronic physics, cosmology, astrophysics and gravitation, field theory and statistical systems, and physical mathematics.
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QCD aspects in W and Z production with ATLAS aμ|l.ohvp, QCD power corrections and αs from e+e− → Hadrons Forward physics at LHC: Intersections with astrophysics Recent results on hadron spectroscopy at LHCb Closing Address—QCD24 Proceedings
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