dc.contributor.author | Khachatryan, V. | |
dc.contributor.author | Sirunyan, A. M. | |
dc.contributor.author | Tumasyan, A. | |
dc.date.accessioned | 2023-10-02T05:18:34Z | |
dc.date.available | 2023-10-02T05:18:34Z | |
dc.date.issued | 2016 | |
dc.identifier.issn | 1029-8479 | |
dc.identifier.uri | http://dspace.adiyaman.edu.tr:8080/xmlui/handle/20.500.12414/4550 | |
dc.description.abstract | The decorrelation in the azimuthal angle between the most forward and the most backward jets (Mueller-Navelet jets) is measured in data collected in pp collisions with the CMS detector at the LHC at root s = 7 TeV. The measurement is presented in the form of distributions of azimuthal-angle differences, Delta phi, between the Mueller-Navelet jets, the average cosines of (pi - Delta phi), 2(pi - Delta phi), and 3(pi - Delta phi), and ratios of these cosines. The jets are required to have transverse momenta, p(T), in excess of 35 GeV and rapidities, |y|, of less than 4.7. The results are presented as a function of the rapidity separation, Delta y, between the Mueller-Navelet jets, reaching Delta y up to 9.4 for the first time. The results are compared to predictions of various Monte Carlo event generators and to analytical predictions based on the DGLAP and BFKL parton evolution schemes. | tr |
dc.language.iso | en | tr |
dc.publisher | Springer | tr |
dc.subject | Hadron-Hadron scattering (experiments) | tr |
dc.subject | proton-proton scattering | tr |
dc.subject | Forward physics | tr |
dc.subject | Jets | tr |
dc.subject | Particle correlations and fluctuations | tr |
dc.title | Search ... Results for Adiyaman University (Affiliation) and 2016 (Publication Years) Azimuthal decorrelation of jets widely separated in rapidity in pp collisions at root s=7 TeV 330 of 409 Azimuthal decorrelation of jets widely separated in rapidity in pp collisions at root s=7 TeV | tr |
dc.type | Article | tr |
dc.contributor.department | Yerevan Phys Inst, | tr |
dc.identifier.volume | 8 | tr |
dc.source.title | JOURNAL OF HIGH ENERGY PHYSICS | tr |