001     419179
005     20211110153543.0
024 7 _ |a arXiv:1812.08690
|2 arXiv
024 7 _ |a 10.3204/PUBDB-2019-00961
|2 datacite_doi
024 7 _ |a inspire:1710427
|2 inspire
037 _ _ |a PUBDB-2019-00961
041 _ _ |a English
088 1 _ |a DESY-18-209; arXiv:1812.08690
088 _ _ |a DESY-18-209
|2 DESY
088 _ _ |a arXiv:1812.08690
|2 arXiv
100 1 _ |a Bell, Guido
|b 0
245 _ _ |a Generic dijet soft functions at two-loop order: correlated emissions
260 _ _ |c 2018
336 7 _ |a Preprint
|b preprint
|m preprint
|0 PUB:(DE-HGF)25
|s 1550218695_7571
|2 PUB:(DE-HGF)
336 7 _ |a WORKING_PAPER
|2 ORCID
336 7 _ |a Electronic Article
|0 28
|2 EndNote
336 7 _ |a preprint
|2 DRIVER
336 7 _ |a Report
|0 PUB:(DE-HGF)29
|2 PUB:(DE-HGF)
|m report
336 7 _ |a ARTICLE
|2 BibTeX
336 7 _ |a Output Types/Working Paper
|2 DataCite
520 _ _ |a We present a systematic algorithm for the perturbative computation of soft functions that are defined in terms of two light-like Wilson lines. Our method is based on a universal parametrisation of the phase-space integrals, which we use to isolate the singularities in Laplace space. The observable-dependent integrations can then be performed numerically, and they are implemented in the new, publicly available package SoftSERVE that we use to derive all of our numerical results. Our algorithm applies to both SCET-1 and SCET-2 soft functions, and in the current version it can be used to compute two out of three NNLO colour structures associated with the so-called correlated-emission contribution. We confirm existing two-loop results for about a dozen $e^+e^-$ and hadron-collider soft functions, and we obtain new predictions for the C-parameter as well as thrust-axis and broadening-axis angularities.
536 _ _ |0 G:(DE-HGF)POF3-611
|c POF3-611
|f POF III
|x 0
|a 611 - Fundamental Particles and Forces (POF3-611)
588 _ _ |a Dataset connected to arXivarXiv
693 _ _ |0 EXP:(DE-MLZ)NOSPEC-20140101
|5 EXP:(DE-MLZ)NOSPEC-20140101
|e No specific instrument
|x 0
700 1 _ |a Rahn, Rudi
|0 P:(DE-HGF)0
|b 1
|e Corresponding author
700 1 _ |a Talbert, Jim
|0 P:(DE-H253)PIP1031711
|b 2
856 4 _ |y OpenAccess
|u https://bib-pubdb1.desy.de/record/419179/files/1812.08690.pdf
856 4 _ |y OpenAccess
|x icon
|u https://bib-pubdb1.desy.de/record/419179/files/1812.08690.gif?subformat=icon
856 4 _ |y OpenAccess
|x icon-1440
|u https://bib-pubdb1.desy.de/record/419179/files/1812.08690.jpg?subformat=icon-1440
856 4 _ |y OpenAccess
|x icon-180
|u https://bib-pubdb1.desy.de/record/419179/files/1812.08690.jpg?subformat=icon-180
856 4 _ |y OpenAccess
|x icon-640
|u https://bib-pubdb1.desy.de/record/419179/files/1812.08690.jpg?subformat=icon-640
856 4 _ |y OpenAccess
|x pdfa
|u https://bib-pubdb1.desy.de/record/419179/files/1812.08690.pdf?subformat=pdfa
909 C O |o oai:bib-pubdb1.desy.de:419179
|p openaire
|p open_access
|p VDB
|p driver
|p dnbdelivery
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 2
|6 P:(DE-H253)PIP1031711
913 1 _ |a DE-HGF
|b Forschungsbereich Materie
|l Materie und Universum
|1 G:(DE-HGF)POF3-610
|0 G:(DE-HGF)POF3-611
|2 G:(DE-HGF)POF3-600
|x 0
|4 G:(DE-HGF)POF
|v Fundamental Particles and Forces
|3 G:(DE-HGF)POF3
914 1 _ |y 2018
915 _ _ |a OpenAccess
|0 StatID:(DE-HGF)0510
|2 StatID
915 _ _ |a Published
|0 StatID:(DE-HGF)0580
|2 StatID
920 1 _ |0 I:(DE-H253)T-20120731
|k T
|l Theorie-Gruppe
|x 0
980 _ _ |a preprint
980 _ _ |a VDB
980 _ _ |a UNRESTRICTED
980 _ _ |a report
980 _ _ |a I:(DE-H253)T-20120731
980 1 _ |a FullTexts


LibraryCollectionCLSMajorCLSMinorLanguageAuthor
Marc 21