scholarly journals Production of bb¯ at forward rapidity in p+p collisions at s=510  GeV

2020 ◽  
Vol 102 (9) ◽  
Author(s):  
U. Acharya ◽  
A. Adare ◽  
C. Aidala ◽  
N. N. Ajitanand ◽  
Y. Akiba ◽  
...  
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2012 ◽  
Vol 20 ◽  
pp. 214-221
Author(s):  
JAMAL JALILIAN-MARIAN

Forward rapidity di-hadron azimuthal angular correlations in high energy proton-nucleus and proton-proton collisions are sensitive to quadrupoles; traceless correlator of 4 Wilson lines whereas single inclusive particle production iNVOLVES only dipoles, traceless correlator of 2 Wilson lines. We discuss the progress made in understanding the energy (rapidity) evolution of the quadrupole as well as its various limits.


2019 ◽  
Vol 210 ◽  
pp. 02009
Author(s):  
Jean-Noël Capdevielle ◽  
Zbigniew Plebaniak ◽  
Barbara Szabelska ◽  
Jacek Szabelski

The model HDPM of CORSIKA has been updated and developed on the base of the recent measurements by ALICE, CMS, TOTEM, LHCb, LHCf... The new model, GHOST, involving a four-source production reproduces correctly the pseudo-rapidity distributions of charged secondaries and has been tested with the data in the mid and forward rapidity region, especially in the complex case of TOTEM, and also with the recent measurements of CMS, up to $ \sqrt s = 13\,{\rm{TeV}} $ (9.0 1016 eV in laboratory system). Special calculations have been devoted to the semi-inclusive data playing an important role in the cosmic ray simulation (fluctuations in earliest collisions, individual cascades measured at high altitude with high energy emulsion chambers). Taking into account the violation of KNO scaling, the negative binomial distribution (NegBin-expressed in terms of scaled elements) $ z = {n \mathord{\left/ {\vphantom {n {\bar {n}}}} \right. \kern-\nulldelimiterspace} {\bar {n}}} $ (n is the number of charged secondaries) has been used pointing out a possible asymptotic behaviour of total charged multiplicities at primary energies exceeding 40 TeV (8.5 1017 eV). Thus, larger reduction of the energies devoted to the leading cluster and very large multiplicity of secondary particles could suggest for EAS generated by primary protons a larger production of muons and a shower maximum at higher altitude.


2019 ◽  
Vol 798 ◽  
pp. 134926 ◽  
Author(s):  
S. Acharya ◽  
D. Adamová ◽  
S.P. Adhya ◽  
A. Adler ◽  
J. Adolfsson ◽  
...  
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2018 ◽  
Vol 780 ◽  
pp. 185-190 ◽  
Author(s):  
Marcin Bury ◽  
Hans Van Haevermaet ◽  
Andreas Van Hameren ◽  
Pierre Van Mechelen ◽  
Krzysztof Kutak ◽  
...  

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