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dc.contributor.author
de Florian, Daniel Enrique  
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Mahakhud, Maguni  
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Mathews, Prakash  
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Mazzitelli, Javier Sebastián  
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Ravindran, V.  
dc.date.available
2017-06-15T18:26:26Z  
dc.date.issued
2014-04  
dc.identifier.citation
de Florian, Daniel Enrique; Mahakhud, Maguni; Mathews, Prakash; Mazzitelli, Javier Sebastián; Ravindran, V.; Next-to-next-to-leading order QCD corrections in models of TeV-scale gravity; Springer; Journal Of High Energy Physics; 2014; 28; 4-2014; 1-18  
dc.identifier.issn
1029-8479  
dc.identifier.uri
http://hdl.handle.net/11336/18265  
dc.description.abstract
We compute the next-to-next-to-leading order QCD corrections to the graviton production in models of TeV-scale gravity, within the soft-virtual approximation. For the Arkani-Hamed, Dimopoulos and Dvali (ADD) model we evaluate the contribu-tion to the Drell-Yan cross section, and we present distributions for the di-lepton invariant mass at the LHC with a center-of-mass energy sH−−−√sH = 14 TeV. We find a large K factor (K ≃ 1.8) for large values of invariant mass, which is the region where the ADD graviton contribution dominates the cross section. The increase in the cross section with respect to the previous order result is larger than 10% in the same invariant mass region. We also observe a substantial reduction in the scale uncertainty. For the Randall-Sundrum (RS) model we computed the total single graviton production cross section at the LHC. We find an increase between 10% and 13% with respect to the next-to-leading order prediction, depending on the model parameters. We provide an analytic expression for the NNLO K factor as a function of the lightest RS graviton mass.  
dc.format
application/pdf  
dc.language.iso
eng  
dc.publisher
Springer  
dc.rights
info:eu-repo/semantics/openAccess  
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https://creativecommons.org/licenses/by-nc-sa/2.5/ar/  
dc.subject
Gravity  
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Nnlo  
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Qcd  
dc.subject.classification
Física de Partículas y Campos  
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Ciencias Físicas  
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CIENCIAS NATURALES Y EXACTAS  
dc.title
Next-to-next-to-leading order QCD corrections in models of TeV-scale gravity  
dc.type
info:eu-repo/semantics/article  
dc.type
info:ar-repo/semantics/artículo  
dc.type
info:eu-repo/semantics/publishedVersion  
dc.date.updated
2017-06-09T14:15:34Z  
dc.journal.volume
2014  
dc.journal.number
28  
dc.journal.pagination
1-18  
dc.journal.pais
Alemania  
dc.journal.ciudad
Berlin  
dc.description.fil
Fil: de Florian, Daniel Enrique. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina  
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Fil: Mahakhud, Maguni. Harish-Chandra Research Institute; India  
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Fil: Mathews, Prakash. Saha Institute of Nuclear Physics; India  
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Fil: Mazzitelli, Javier Sebastián. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina  
dc.description.fil
Fil: Ravindran, V.. Institute of Mathematical Sciencies; India  
dc.journal.title
Journal Of High Energy Physics  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1007/JHEP04(2014)028  
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info:eu-repo/semantics/altIdentifier/url/https://link.springer.com/article/10.1007%2FJHEP04%282014%29028  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1312.7173