Systematic estimation of theoretical uncertainties in the calculation of the pion-photon transition form factor using light-cone sum rules
We consider the calculation of the pion-photon transition form factor F super([gamma]*[gamma][pi]0)(Q super(2)) within light-cone sum rules focusing attention to the low-mid region of momenta. The central aim is to estimate the theoretical uncertainties which originate from a wide variety of sources...
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Veröffentlicht in: | Physical review. D 2016-06, Vol.93 (11), Article 114018 |
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description | We consider the calculation of the pion-photon transition form factor F super([gamma]*[gamma][pi]0)(Q super(2)) within light-cone sum rules focusing attention to the low-mid region of momenta. The central aim is to estimate the theoretical uncertainties which originate from a wide variety of sources related to (i) the relevance of next-to-next-to-leading order radiative corrections (ii) the influence of the twist-four and the twist-six term (iii) the sensitivity of the results on auxiliary parameters, like the Borel scale M super(2), (iv) the role of the phenomenological description of resonances, and (v) the significance of a small but finite virtuality of the quasireal photon. Predictions for F super([gamma]*[gamma][pi]0)(Q super(2)) are presented which include all these uncertainties and found to comply within the margin of experimental error with the existing data in the Q super(2) range between 1 and 5GeV super(2), thus justifying the reliability of the applied calculational scheme. This provides a solid basis for confronting theoretical predictions with forthcoming data bearing small statistical errors. |
doi_str_mv | 10.1103/PhysRevD.93.114018 |
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V. ; Pimikov, A. V. ; Stefanis, N. G.</creator><creatorcontrib>Mikhailov, S. V. ; Pimikov, A. V. ; Stefanis, N. G.</creatorcontrib><description>We consider the calculation of the pion-photon transition form factor F super([gamma]*[gamma][pi]0)(Q super(2)) within light-cone sum rules focusing attention to the low-mid region of momenta. The central aim is to estimate the theoretical uncertainties which originate from a wide variety of sources related to (i) the relevance of next-to-next-to-leading order radiative corrections (ii) the influence of the twist-four and the twist-six term (iii) the sensitivity of the results on auxiliary parameters, like the Borel scale M super(2), (iv) the role of the phenomenological description of resonances, and (v) the significance of a small but finite virtuality of the quasireal photon. Predictions for F super([gamma]*[gamma][pi]0)(Q super(2)) are presented which include all these uncertainties and found to comply within the margin of experimental error with the existing data in the Q super(2) range between 1 and 5GeV super(2), thus justifying the reliability of the applied calculational scheme. This provides a solid basis for confronting theoretical predictions with forthcoming data bearing small statistical errors.</description><identifier>ISSN: 2470-0010</identifier><identifier>EISSN: 2470-0029</identifier><identifier>DOI: 10.1103/PhysRevD.93.114018</identifier><language>eng</language><subject>Cosmology ; Errors ; Focusing ; Form factors ; Mathematical analysis ; Photons ; Sum rules ; Uncertainty</subject><ispartof>Physical review. 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D</title><description>We consider the calculation of the pion-photon transition form factor F super([gamma]*[gamma][pi]0)(Q super(2)) within light-cone sum rules focusing attention to the low-mid region of momenta. The central aim is to estimate the theoretical uncertainties which originate from a wide variety of sources related to (i) the relevance of next-to-next-to-leading order radiative corrections (ii) the influence of the twist-four and the twist-six term (iii) the sensitivity of the results on auxiliary parameters, like the Borel scale M super(2), (iv) the role of the phenomenological description of resonances, and (v) the significance of a small but finite virtuality of the quasireal photon. Predictions for F super([gamma]*[gamma][pi]0)(Q super(2)) are presented which include all these uncertainties and found to comply within the margin of experimental error with the existing data in the Q super(2) range between 1 and 5GeV super(2), thus justifying the reliability of the applied calculational scheme. This provides a solid basis for confronting theoretical predictions with forthcoming data bearing small statistical errors.</description><subject>Cosmology</subject><subject>Errors</subject><subject>Focusing</subject><subject>Form factors</subject><subject>Mathematical analysis</subject><subject>Photons</subject><subject>Sum rules</subject><subject>Uncertainty</subject><issn>2470-0010</issn><issn>2470-0029</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2016</creationdate><recordtype>article</recordtype><recordid>eNpNkMtKxDAYhYMoOOi8gKss3XRMmrRNljJeYUDxsg5p-ncaaZsxSYV5BZ_ajKPiKh_nHH7Ih9AZJQtKCbt47LbhCT6uFpKlgBMqDtAs5xXJCMnl4R9TcozmIbyRhCWRFaUz9Pm8DREGHa3BEKLdkRuxa3HswHlIue7xNBrwUdsxWgjYjrsSp8JM_f893iTONp2LKYpej8F-t63zA261ic7jKdhxjXu77mJm3Ag4TAP2Uw_hFB21ug8w_3lP0OvN9cvyLls93N4vL1eZyQWJGQhZNbksmSxIXXIt87qpQDJdi0YC1CZveMF4C6aspWgbRqTgpBSMM2pKztkJOt_f3Xj3PqVPq8EGA32vR3BTUFSwopBCMJqm-X5qvAvBQ6s2PinyW0WJ2rlXv-6VZGrvnn0BGDF8nA</recordid><startdate>20160620</startdate><enddate>20160620</enddate><creator>Mikhailov, S. 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G.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c280t-e897d2963950b64a92bd7e93ab8d9eebc2d4534fec6b98fd309840683431c6443</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2016</creationdate><topic>Cosmology</topic><topic>Errors</topic><topic>Focusing</topic><topic>Form factors</topic><topic>Mathematical analysis</topic><topic>Photons</topic><topic>Sum rules</topic><topic>Uncertainty</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Mikhailov, S. V.</creatorcontrib><creatorcontrib>Pimikov, A. V.</creatorcontrib><creatorcontrib>Stefanis, N. G.</creatorcontrib><collection>CrossRef</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Physical review. D</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Mikhailov, S. V.</au><au>Pimikov, A. V.</au><au>Stefanis, N. G.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Systematic estimation of theoretical uncertainties in the calculation of the pion-photon transition form factor using light-cone sum rules</atitle><jtitle>Physical review. D</jtitle><date>2016-06-20</date><risdate>2016</risdate><volume>93</volume><issue>11</issue><artnum>114018</artnum><issn>2470-0010</issn><eissn>2470-0029</eissn><abstract>We consider the calculation of the pion-photon transition form factor F super([gamma]*[gamma][pi]0)(Q super(2)) within light-cone sum rules focusing attention to the low-mid region of momenta. The central aim is to estimate the theoretical uncertainties which originate from a wide variety of sources related to (i) the relevance of next-to-next-to-leading order radiative corrections (ii) the influence of the twist-four and the twist-six term (iii) the sensitivity of the results on auxiliary parameters, like the Borel scale M super(2), (iv) the role of the phenomenological description of resonances, and (v) the significance of a small but finite virtuality of the quasireal photon. Predictions for F super([gamma]*[gamma][pi]0)(Q super(2)) are presented which include all these uncertainties and found to comply within the margin of experimental error with the existing data in the Q super(2) range between 1 and 5GeV super(2), thus justifying the reliability of the applied calculational scheme. This provides a solid basis for confronting theoretical predictions with forthcoming data bearing small statistical errors.</abstract><doi>10.1103/PhysRevD.93.114018</doi></addata></record> |
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subjects | Cosmology Errors Focusing Form factors Mathematical analysis Photons Sum rules Uncertainty |
title | Systematic estimation of theoretical uncertainties in the calculation of the pion-photon transition form factor using light-cone sum rules |
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