We report on the first next-to-leading BFKL study of the cross section and azimuthal decorrellation of Mueller Navelet jets. This includes next-to-leading corrections to the Green's function as well as next-to-leading corrections to the Mueller Navelet vertices. The obtained results for standard observables proposed for studies of Mueller Navelet jets show that both sources of corrections are of equal and big importance for final magnitude and final behavior of observables, in particular for the LHC kinematics investigated here in detail. The astonishing conclusion of our analysis is that the observables obtained within the complete next-lo-leading order BFKL framework of the present contribution are quite similar to the same observables obtained within next-to-leading logarithm DGLAP type treatment. The only noticeable difference is the ratio the azimuthal angular moments 〈cos2φ〉/〈cosφ〉 which still differs in both treatments.

The first complete NLL BFKL study of Mueller Navelet jets at LHC / Colferai D.; Schwennsen F.; Szymanowski L.; Wallon S.. - In: POS PROCEEDINGS OF SCIENCE. - ISSN 1824-8039. - ELETTRONICO. - 2011-:(2011), pp. 0-0. ( 21st International Europhysics Conference on High Energy Physics, EPS-HEP 2011 fra 2011).

The first complete NLL BFKL study of Mueller Navelet jets at LHC

Colferai D.
Membro del Collaboration Group
;
2011

Abstract

We report on the first next-to-leading BFKL study of the cross section and azimuthal decorrellation of Mueller Navelet jets. This includes next-to-leading corrections to the Green's function as well as next-to-leading corrections to the Mueller Navelet vertices. The obtained results for standard observables proposed for studies of Mueller Navelet jets show that both sources of corrections are of equal and big importance for final magnitude and final behavior of observables, in particular for the LHC kinematics investigated here in detail. The astonishing conclusion of our analysis is that the observables obtained within the complete next-lo-leading order BFKL framework of the present contribution are quite similar to the same observables obtained within next-to-leading logarithm DGLAP type treatment. The only noticeable difference is the ratio the azimuthal angular moments 〈cos2φ〉/〈cosφ〉 which still differs in both treatments.
2011
Proceedings of Science
21st International Europhysics Conference on High Energy Physics, EPS-HEP 2011
fra
2011
Colferai D.; Schwennsen F.; Szymanowski L.; Wallon S.
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Utilizza questo identificatore per citare o creare un link a questa risorsa: https://hdl.handle.net/2158/1448333
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