Interaction cross sections and matter radii of oxygen isotopes using the Glauber model

2017 ◽  
Vol 95 (5) ◽  
Author(s):  
Suhel Ahmad ◽  
A. A. Usmani ◽  
Shakeb Ahmad ◽  
Z. A. Khan
Keyword(s):  
Oxygen Isotopes ◽  
Cross Sections ◽  
Glauber Model ◽  
Interaction Cross Sections

Modelling Interaction Cross Sections for Intermediate and Low Energy Ions

2002 ◽  
Vol 99 (1) ◽  
pp. 49-51 ◽  
Author(s):  
L. H. Toburen ◽  
J. L. Shinpaugh ◽  
E. L. B. Justiniano
Keyword(s):  
Cross Sections ◽  
Low Energy ◽  
Low Energy Ions ◽  
Interaction Cross Sections

Measurement of interaction cross sections of 0.3?5.0 MeV neutrons with air

1969 ◽  
Vol 26 (5) ◽  
pp. 520-521 ◽  
Author(s):  
V. A. Terekhin ◽  
V. A. Kryzhanovskii ◽  
L. B. Poretskii
Keyword(s):  
Cross Sections ◽  
Interaction Cross Sections

scholarly journals ULTRAHIGH ENERGY NEUTRINO PHYSICS

2004 ◽  
Vol 19 (03) ◽  
pp. 317-340 ◽  
Author(s):  
ANNA M. STAŚTO
Keyword(s):  
Neutrino Physics ◽  
Cross Sections ◽  
High Energy ◽  
Ultrahigh Energy ◽  
Production Rates ◽  
Precise Knowledge ◽  
Detection Probabilities ◽  
Interaction Cross Sections ◽  
The Universe ◽  
Origin Of The Universe

Ultrahigh energy neutrinos can provide important information about the distant astronomical objects and the origin of the Universe. Precise knowledge about neutrino interactions and production rates is essential for estimating background, expected fluxes and detection probabilities. In this paper we review the applications of the high energy QCD to the calculations of the interaction cross-sections of the neutrinos. We also study the production of the ultrahigh energy neutrinos in the atmosphere due to the charm and beauty decays.

INVESTIGATION ON THE NEUTRINO INDUCED MUONS FROM ACTIVE GALACTIC NUCLEI

2000 ◽  
Vol 15 (25) ◽  
pp. 1567-1576
Author(s):  
NAYANTARA GUPTA ◽  
D. P. BHATTACHARYYA
Keyword(s):  
Cross Sections ◽  
Neutrino Flux ◽  
High Energy ◽  
Energy Spectra ◽  
Muon Energy ◽  
Model Calculations ◽  
Charge Current ◽  
Upper Limits ◽  
Total Interaction ◽  
Interaction Cross Sections

The fluxes of neutrino induced muons at different zenith angles have been calculated using the high energy diffused neutrino spectra emitted from blazars. We have used the standard formulation developed by Gaisser based on charge-current interactions in rock and the QED-based energy loss formulation to estimate the spectra of neutrino induced muons. The energy spectra of neutrino flux generated from blazars has been taken from the model calculations of Protheroe. The latest charge-current and total interaction cross-sections at ultrahigh energies from Kwiecinski et al. have been used to find the probability of muon generation from neutrinos and the loss of neutrinos during propagation through the Earth. We find that our derived horizontal neutrino induced muon energy spectra expected from blazar model of Protheroe is comparable with the upper limits as predicted by SOUDAN 2 experiment.

Interaction cross sections and negative pion multiplicities in nucleus-nucleus collisions at 4.2 GeV/c per nucleon

1980 ◽  
Vol 5 (1) ◽  
pp. 1-8 ◽  
Author(s):  
E. O. Abdrahmanov ◽  
A. N. Basina ◽  
I. Ya. Chasnikov ◽  
A. Sh. Gaitinov ◽  
I. S. Streltsov ◽  
...  
Keyword(s):  
Cross Sections ◽  
Negative Pion ◽  
Interaction Cross Sections
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