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Current status and future prospects
Top and QCD Current status and future prospects Y. Sumino (Tohoku Univ.)
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โPlan of Talk Introduction: Pert. QCD and Top quark
2. Status of pert. QCD (top processes) 3. Towards precision ๐ ๐ก determinations 4. Vision of quantum corrections at frontiers 5. Conclusions and future prospects
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p (้ฝๅญ) p (้ฝๅญ) LHC ๏ผฌ๏ผจ๏ผฃๅฎ้จใซใใใๅๅฟใใผใฟ
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ๅผทใๅ _ u u _ u _ u u u โฅโฅใฏใฉใผใฏใ้ฝๅญใปไธญๆงๅญใฎไธญใซ้ใ่พผใใฆใใๅ ใฏใฉใผใฏใ้ฝๅญใปไธญๆงๅญใฎไธญใใๅใๅบใใใจใฏ
ใงใใชใ๏ผใใฏใฉใผใฏใฎ้ใ่พผใใ _ u u ไธญ้ๅญ ๆ ธๅญ๏ผ้ฝๅญใปไธญๆงๅญใชใฉ๏ผ ๆฑบใใฆๅไฝใฎใฏใฉใผใฏใฏๅใๅบใใชใใ ๅธธใซ ใๆ ธๅญ๏ผใฏใฉใผใฏ๏ผใคใงๅบๆฅใฆใใ๏ผ ใไธญ้ๅญ๏ผใฏใฉใผใฏใปๅใฏใฉใผใฏใฎๅฏพใงๅบๆฅใฆใใ๏ผ ใฎไธญใซๅ
ฅใฃใฆใใใ _ u _ u u u ไธญ้ๅญ ไธญ้ๅญ
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d u d u u u ้ฝๅญ ้ฝๅญ ๏ผ่ก็ชใจใใซใฎใผ๏ผ๏ผ๏ผ้ฝๅญใฎ่ณช้รc2๏ผ ใใใใฎๆฐใฎ ๆ ธๅญใไธญ้ๅญใ็ๆใใใใ
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p (้ฝๅญ) p (้ฝๅญ) LHC ๏ผฌ๏ผจ๏ผฃๅฎ้จใซใใใใใใฐใน็ฒๅญ็ๆใ ๅซใไบ่ฑกใฎใทใใฅใฌใผใทใงใณ ๆๅ๏ผฑ๏ผฃ๏ผคใซๅบใฅใ
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Whatโs Pert. QCD? 3 types of so-called โPert. QCD predictionsโ : Confusing (i) Predict observable in series expansion in ๐ผ ๐ IR safe obs., intrinsic uncertainties ~ (ฮ QCD / ๐ธ) ๐ (ii) Predict observable in the framework of Wilsonian EFT OPE, uncertainties of (i) replaced by non-pert. matrix elements Most accurate, future applications (iii) Predict observable assisted by model predictions Many obs in high-energy experiments depend on hadronization models, PDF. Necessary (in MC) to compare with experimental data Systematic uncertainties difficult to control, O(5-10%) accuracy at LHC
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โ ๐๐ถ๐ท ( ๐ผ ๐ , ๐ ๐ ;๐) Pert. QCD Theory of quarks and gluons
renormalization scale โ ๐๐ถ๐ท ( ๐ผ ๐ , ๐ ๐ ;๐) Theory of quarks and gluons Same input parameters as full QCD. Systematic: own way to estimate errors (๐-dep.) Differs from a model ! Predictable observables ๐, ๐ |๐,๐ ๐,๐| = โ๐๐๐. |โ๐๐๐. โ๐๐๐.| = 1 testable hypothesis (a) Inclusive observables (hadronic inclusive) โฏ insensitive to hadronization ๐
๐ธ โก ๐ ๐ + ๐ โ โโ๐๐๐๐๐๐ ;๐ธ ๐ ๐ + ๐ โ โ ๐ + ๐ โ ;๐ธ โข Inclusive cross sections/decay widths e.g. โข Distributions of non-colored particles, โ, ๐พ, ๐,๐ป,โฏ (b) Observables of heavy quarkonium states (only individual hadronic states) โข spectrum, leptonic decay width, transition rates
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Whatโs Pert. QCD? 3 types of so-called โPert. QCD predictionsโ : Confusing (i) Predict observable in series expansion in ๐ผ ๐ IR safe obs., intrinsic uncertainties ~ (ฮ QCD / ๐ธ) ๐ (ii) Predict observable in the framework of Wilsonian EFT OPE, uncertainties of (i) replaced by non-pert. matrix elements Most accurate, future applications (iii) Predict observable assisted by model predictions Many obs in high-energy experiments depend on hadronization models, PDF. Necessary (in MC) to compare with experimental data Systematic uncertainties difficult to control, O(5-10%) accuracy at LHC
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Remarkable progress of computational technologies in the last 10-20 years
Higher-loop corrections Numerical and analytical methods Intersection with frontiers of mathematics Factorization of scales in loop corrections Provide powerful and precise foundation for theory predictions PDFs Radiator fn Matrix element ๐ ๐+๐โ๐ ๐ = ๐,๐ ๐ ๐ฅ ๐ ๐ฅ 2 ๐ ๐/๐ ๐ฅ 1 , ๐ ๐น ๐ ๐/๐ ๐ฅ 2 , ๐ ๐น ๐๐ง ๐
๐๐ ๐ง, ๐ ๐น , ๐ ๐ ๐๐โ๐ ๐ 2 =๐ง ๐ฅ 1 ๐ฅ 2 ๐ 2 ๐ ๐/๐ ๐ ๐/๐ ๐ ๐น ๐ ๐ ๐ ๐=๐ ๐=๐ Separation of scales
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Tree-level Higgs potential
Role of top quark in the SM vacuum structure 1-loop corrections Tree-level Higgs potential ๐ฃ ๐ป ๐๐ป 1 4๐ ๐ ๐ป ฮฆ โ ฮฆโ ๐ ๐ป log ๐ ๐ป ฮฆ โ ฮฆโ ๐ ๐ป 2 ๐ 2 ๐ ๐ป ฮฆ โ ฮฆโ ๐ ๐ป log 3 ๐ ๐ป ฮฆ โ ฮฆโ ๐ ๐ป 2 ๐ 2 ๐ ๐ป 1 4๐ ๐ ฮฆ โ ฮฆ 2 log ๐ ฮฆ โ ฮฆ ๐ 2 ๐ 2 + ๐ โฒ2 2 ฮฆ โ ฮฆ 2 log ๐ 2 + ๐ โฒ2 2 ฮฆ โ ฮฆ ๐ 2 ๐,๐,๐พ = 246 GeV ๐ ฮฆ =โ ๐ ๐ป 2 ฮฆ โ ฮฆ+ ๐ ๐ป ฮฆ โ ฮฆ 2 ๐ก 1 4๐ 2 โ3 ๐ฆ ๐ก 2 ฮฆ โ ฮฆ 2 log ๐ฆ ๐ก 2 ฮฆ โ ฮฆ ๐ 2 ฮฆ= ๐ฃ ๐ป +โ
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Tree-level Higgs potential
Role of top quark in the SM vacuum structure 1-loop corrections Tree-level Higgs potential 1 4๐ ๐ ๐ป ฮฆ โ ฮฆโ ๐ ๐ป log ๐ ๐ป ฮฆ โ ฮฆโ ๐ ๐ป 2 ๐ 2 ๐ ๐ป ฮฆ โ ฮฆโ ๐ ๐ป log 3 ๐ ๐ป ฮฆ โ ฮฆโ ๐ ๐ป 2 ๐ 2 tree top loop ๐,๐ loop 1 4๐ ๐ ฮฆ โ ฮฆ 2 log ๐ ฮฆ โ ฮฆ ๐ 2 ๐ 2 + ๐ โฒ2 2 ฮฆ โ ฮฆ 2 log ๐ 2 + ๐ โฒ2 2 ฮฆ โ ฮฆ ๐ 2 Higgs loop ๐,๐,๐พ ๐ ๐ [GeV] ๐ ฮฆ =โ ๐ ๐ป 2 ฮฆ โ ฮฆ+ ๐ ๐ป ฮฆ โ ฮฆ 2 ๐ก 1 4๐ 2 โ3 ๐ฆ ๐ก 2 ฮฆ โ ฮฆ 2 log ๐ฆ ๐ก 2 ฮฆ โ ฮฆ ๐ 2 ฮฆ= ๐ฃ ๐ป +โ
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๐ก ๐ก production at LHC ๐ ๐ NNLO predictions Czakon, Heymes, Mitov
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Slide from Kimโs talk
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Anomaly in top FB asymmetry has disappeared.
Czakon, Heymes, Fiedler, Mitov Soon full NNLO prod.+decay corr. will bring investigations of top quark to a new phase.
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Towards precise top mass determinations
๐ก ๐พ,๐ e+ ๐ก ILC LHC Weight function method ๐ก ๐ก threshold at ILC ๐ก ๐ก threshold at up-graded LHC and beyond
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Slides from Kawabataโs talk
Kawabata, Shimizu, YS, Yokoya
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Result of LO simulation analysis using ๐+4-jets mode
S. Kawabata, [hep-ph] LHC 100fb-1 Currently NLO simulation analysis is being performed. NLO production NLO decay NLO prod.+decay (dilepton) [GeV] Our current goal: โ ๐ pole <1 GeV With this method many theoretical problems should go away, except non-pert. effects of background color charge distr. on top decays.
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Precision ๐ ๐ก measurement near ๐ก ๐ก threshold at ๐ + ๐ โ collider
After many years of endeavor, computation of NNNLO corrections to ๐ + ๐ โ โ๐ก ๐ก cross section near threshold has recently been completed. ๐ 1๐ Beneke,Kiyo,Marquard, Penin,Piclum,Steinhauser ๐ ๐ก color-singlet 1S resonance Our estimate: โ ๐ ๐ก =20-30 MeV Kiyo, Mishima, YS
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Slide from Kiyoโs talk
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LHC 3 ab-1 โ ๐ ๐ก โ2 GeV FCC 100 TeV โ ๐ ๐ก โ0.2 GeV @ 1 ab-1 โ ๐ ๐ก โ0.06 GeV @ 10 ab-1 ๐พ ๐ก ๐ ๐ก = +
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A new vision of loop integral based on Baikovโs method
Baikov rep. of loop integral: ๐ ๐ท ๐ 1 โฏ ๐ ๐ท ๐ ๐ฟ ๐ท 1 ๐ 1 โฏ ๐ท ๐ ๐ ๐ = ๐ถ ๐ ๐ฅ 1 ๐ฅ 1 ๐ 1 โฏ ๐ถ ๐ ๐ ๐ฅ ๐ ๐ฅ ๐ ๐ ๐ ๐ ๐ฅ 1 ,โฏ, ๐ฅ ๐ (๐ทโ๐ธโ๐ฟโ1)/2 ๐ฅ ๐ c.f. Mahler measure ๐ถ ๐ As ๐ทโโ, branch points turn to saddle points and using saddle-point approx. coefficients of 1/๐ท expansion can be computed by Gauss integrals. Most difficult computation of 5-loop QCD beta fn. relies on this technique.
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Conclusions and future prospects
Predictability of pert. QCD is rapidly developing and will continue further. A current task is to determine ๐ผ ๐ ( ๐ ๐ ) accurately (among others). Soon scrutiny of top quark will start at LHC, however, cannot be completely free from the unclean environment. Eventually ๐ + ๐ โ machine is necessary for precision physics. Hints for deeper understanding on quantum nature of field theory from progressing theories of radiative corrections. โ ๐ ๐ก <1 GeV probably reachable
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Slide from Heymesโs talk
Loops&Legs2016
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Slide from Mitovโs talk
KEK-PH2016 Anomaly in top FB asymmetry is gone. Czakon, Heymes, Fiedler, Mitov
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Slides from Kawabataโs talk
TopWS2015
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