Precise determination of alpha sub(s) from the C-parameter distribution
We present a global fit for alpha sub(s)(m sub(Z)), analyzing the available C-parameter data measured at center-of-mass energies between Q = 35 and 207 GeV. The experimental data is compared to a N super(3)LL' + ((ProQuest: Formulae and/or non-USASCII text omitted)) + [Omega] sub(1) theoretical...
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Veröffentlicht in: | Physical review. D, Particles, fields, gravitation, and cosmology Particles, fields, gravitation, and cosmology, 2015-05, Vol.91 (9) |
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creator | Hoang, Andre H Kolodrubetz, Daniel W Mateu, Vicent Stewart, Iain W |
description | We present a global fit for alpha sub(s)(m sub(Z)), analyzing the available C-parameter data measured at center-of-mass energies between Q = 35 and 207 GeV. The experimental data is compared to a N super(3)LL' + ((ProQuest: Formulae and/or non-USASCII text omitted)) + [Omega] sub(1) theoretical prediction (up to the missing four-loop cusp anomalous dimension), which includes power corrections coming from a field-theoretical nonperturbative soft function. The dominant hadronic parameter is its first moment [Omega] sub(1), which is defined in a scheme which eliminates the O([Lambda] sub(QCD)) renormalon ambiguity. The resummation region plays a dominant role in the C-parameter spectrum, and in this region a fit for alpha sub(s)(m sub(Z)) and [Omega] sub(1) is sufficient. We find alpha sub(s)(m sub(Z)) = 0.1123 + or - 0.0015 and [Omega] sub(1) = 0.421 + or - 0.063 GeV with chi super(2)/d. o. f. = 0.988 for 404 bins of data. These results agree with the prediction of universality for [Omega] sub(1) between thrust and C-parameter within 1-[sigma]. |
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The experimental data is compared to a N super(3)LL' + ((ProQuest: Formulae and/or non-USASCII text omitted)) + [Omega] sub(1) theoretical prediction (up to the missing four-loop cusp anomalous dimension), which includes power corrections coming from a field-theoretical nonperturbative soft function. The dominant hadronic parameter is its first moment [Omega] sub(1), which is defined in a scheme which eliminates the O([Lambda] sub(QCD)) renormalon ambiguity. The resummation region plays a dominant role in the C-parameter spectrum, and in this region a fit for alpha sub(s)(m sub(Z)) and [Omega] sub(1) is sufficient. We find alpha sub(s)(m sub(Z)) = 0.1123 + or - 0.0015 and [Omega] sub(1) = 0.421 + or - 0.063 GeV with chi super(2)/d. o. f. = 0.988 for 404 bins of data. These results agree with the prediction of universality for [Omega] sub(1) between thrust and C-parameter within 1-[sigma].</description><identifier>ISSN: 1550-7998</identifier><identifier>EISSN: 1550-2368</identifier><language>eng</language><subject>Ambiguity ; Bins ; Cosmology ; Cusps ; Energy measurement ; Gravitation ; Texts ; Thrust</subject><ispartof>Physical review. 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The experimental data is compared to a N super(3)LL' + ((ProQuest: Formulae and/or non-USASCII text omitted)) + [Omega] sub(1) theoretical prediction (up to the missing four-loop cusp anomalous dimension), which includes power corrections coming from a field-theoretical nonperturbative soft function. The dominant hadronic parameter is its first moment [Omega] sub(1), which is defined in a scheme which eliminates the O([Lambda] sub(QCD)) renormalon ambiguity. The resummation region plays a dominant role in the C-parameter spectrum, and in this region a fit for alpha sub(s)(m sub(Z)) and [Omega] sub(1) is sufficient. We find alpha sub(s)(m sub(Z)) = 0.1123 + or - 0.0015 and [Omega] sub(1) = 0.421 + or - 0.063 GeV with chi super(2)/d. o. f. = 0.988 for 404 bins of data. 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D, Particles, fields, gravitation, and cosmology</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Hoang, Andre H</au><au>Kolodrubetz, Daniel W</au><au>Mateu, Vicent</au><au>Stewart, Iain W</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Precise determination of alpha sub(s) from the C-parameter distribution</atitle><jtitle>Physical review. D, Particles, fields, gravitation, and cosmology</jtitle><date>2015-05-01</date><risdate>2015</risdate><volume>91</volume><issue>9</issue><issn>1550-7998</issn><eissn>1550-2368</eissn><abstract>We present a global fit for alpha sub(s)(m sub(Z)), analyzing the available C-parameter data measured at center-of-mass energies between Q = 35 and 207 GeV. The experimental data is compared to a N super(3)LL' + ((ProQuest: Formulae and/or non-USASCII text omitted)) + [Omega] sub(1) theoretical prediction (up to the missing four-loop cusp anomalous dimension), which includes power corrections coming from a field-theoretical nonperturbative soft function. The dominant hadronic parameter is its first moment [Omega] sub(1), which is defined in a scheme which eliminates the O([Lambda] sub(QCD)) renormalon ambiguity. The resummation region plays a dominant role in the C-parameter spectrum, and in this region a fit for alpha sub(s)(m sub(Z)) and [Omega] sub(1) is sufficient. We find alpha sub(s)(m sub(Z)) = 0.1123 + or - 0.0015 and [Omega] sub(1) = 0.421 + or - 0.063 GeV with chi super(2)/d. o. f. = 0.988 for 404 bins of data. These results agree with the prediction of universality for [Omega] sub(1) between thrust and C-parameter within 1-[sigma].</abstract></addata></record> |
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title | Precise determination of alpha sub(s) from the C-parameter distribution |
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