scholarly journals Perturbative Charm Production and the Prompt Atmospheric Neutrino Flux in light of RHIC and LHC

2020 ◽  
Author(s):  
Atri Bhattacharya ◽  
Rikard Enberg ◽  
Mary Hall Reno ◽  
Ina Sarcevic ◽  
Anna Stasto
2015 ◽  
Vol 2015 (6) ◽  
Author(s):  
Atri Bhattacharya ◽  
Rikard Enberg ◽  
Mary Hall Reno ◽  
Ina Sarcevic ◽  
Anna Stasto

2017 ◽  
Author(s):  
Yu Seon Jeong ◽  
Atri Bhattacharya ◽  
Rikard Enberg ◽  
C.S. Kim ◽  
Mary Hall Reno ◽  
...  

2019 ◽  
Author(s):  
Morihiro Honda ◽  
M Sajjad Athar ◽  
T. Kajita ◽  
K. Kasahara ◽  
S. Midorikawa ◽  
...  

2019 ◽  
Vol 208 ◽  
pp. 07001
Author(s):  
Morihiro Honda

It is well known that the correlation of atmospheric neutrinos and muons are simply correlated in the energy region of 1–10 GeV, and used for the test bench of the hadronic interaction model used for the calculation of the atmospheric neutrino flux. However, the correlation becomes unclear for neutrinos in the energy range below 1 GeV, which is important for the study of mass ordering of neutrino and CP phase of the neutrino mass. We extend the study of the correlation to the lower neutrino energies and find that the atmospheric muon flux observed at high altitude shows a good correlation to the atmospheric neutrino flux, and could be used to calibrate the hadronic interaction model.


2019 ◽  
Vol 199 ◽  
pp. 04007
Author(s):  
Rafał Maciuła

We consider unfavoured light quark/antiquark to D meson fragmentation. We discuss nonperturbative effects for small transverse momenta. The asymmetry for D+ and D- production measured by the LHCb collaboration provides natural constraints on the parton (quark/antiquark) fragmentation functions. We find that already a fraction of $q/\overline q \to D$ fragmentation probability is sufficient to account for the measured asymmetry. Large D-meson production asymmetries are found for large xF which is related to dominance of light quark/antiquark $q/\overline q \to D$ fragmentation over the standard c → D fragmentation. As a consequence, prompt atmospheric neutrino flux at high neutrino energies can be much larger than for the conventional c → D fragmentation. The latter can constitute a sizeable background for the cosmic neutrinos claimed to be observed recently by the IceCube Observatory.


Sign in / Sign up

Export Citation Format

Share Document