scholarly journals CALCULATION OF SECONDARY PARTICLES IN ATMOSPHERE AND HADRONIC INTERACTIONS

2002 ◽  
Author(s):  
G. BATTISTONI ◽  
A. FERRARI ◽  
P. R. SALA
Keyword(s):  
Hadronic Interactions ◽  
Secondary Particles

scholarly journals CALCULATION OF SECONDARY PARTICLES IN ATMOSPHERE AND HADRONIC INTERACTIONS

2002 ◽  
Vol 17 (12n13) ◽  
pp. 1743-1754
Author(s):  
G. BATTISTONI ◽  
A. FERRARI ◽  
P. R. SALA
Keyword(s):  
Cosmic Rays ◽  
Particle Production ◽  
Microscopic Approach ◽  
Hadronic Interactions ◽  
Earth’S Atmosphere ◽  
Secondary Particles ◽  
Production Models ◽  
Explicit Reference ◽  
Earth's Atmosphere

Calculation of secondary particles produced by the interaction of cosmic rays with the nuclei of Earth's atmosphere pose important requirements to particle production models. Here we summarize the important features of hadronic simulations, stressing the importance of the so called "microscopic" approach, making explicit reference to the case of the FLUKA code. Benchmarks are also presented.

Unravelling high volumetric capacity of Co3O4 nanograin-interconnected secondary particles for lithium-ion battery anodes

2021 ◽  
Author(s):  
Joon Ha Chang ◽  
Jun Young Cheong ◽  
Yoonsu Shim ◽  
Jae Yeol Park ◽  
Sung Joo Kim ◽  
...  
Keyword(s):  
Lithium Ion Battery ◽  
Anode Material ◽  
Secondary Particle ◽  
Lithium Ion ◽  
Secondary Particles ◽  
Volumetric Capacity ◽  
Battery Anode

Co3O4 nanograins-interconnected secondary particle (Co3O4 NISP) is proposed as lithium-ion battery anode material that can offer high volumetric capacity by less formation of insulating CoO during lithiation process.

scholarly journals The leading effect explains the forward-backward multiplicity correlations in hadronic interactions

1983 ◽  
Vol 38 (10) ◽  
pp. 359-366 ◽  
Author(s):  
M. Basile ◽  
G. Bonvicini ◽  
G. Cara Romeo ◽  
L. Cifarelli ◽  
A. Contin ◽  
...  
Keyword(s):  
Hadronic Interactions

scholarly journals High energy cosmic ray interactions and UHECR composition problem

2019 ◽  
Vol 210 ◽  
pp. 02001
Author(s):  
Sergey Ostapchenko
Keyword(s):  
Experimental Data ◽  
Monte Carlo ◽  
Cosmic Rays ◽  
Cosmic Ray ◽  
High Energy ◽  
Ultra High Energy ◽  
Hadronic Interactions ◽  
High Energy Cosmic Rays ◽  
Cosmic Ray Interactions ◽  
Composition Problem

The differences between contemporary Monte Carlo generators of high energy hadronic interactions are discussed and their impact on the interpretation of experimental data on ultra-high energy cosmic rays (UHECRs) is studied. Key directions for further model improvements are outlined. The prospect for a coherent interpretation of the data in terms of the UHECR composition is investigated.

scholarly journals Elementary hadronic interactions at the CERN SPS

2003 ◽  
Vol 715 ◽  
pp. 118c-128c ◽  
Author(s):  
H.G. Fischer
Keyword(s):  
Hadronic Interactions

Erratum: Unified model of current-hadronic interactions

1974 ◽  
Vol 9 (11) ◽  
pp. 3216-3216
Author(s):  
J. W. Moffat ◽  
C. D. Wright
Keyword(s):  
Unified Model ◽  
Hadronic Interactions

ALIGNMENT PHENOMENON IN GAMMA FAMILIES WITH ENERGIES 100–1000 TEV

2005 ◽  
Vol 20 (29) ◽  
pp. 7032-7034 ◽  
Author(s):  
T. S. YULDASHBAEV ◽  
KH. NURITDINOV
Keyword(s):  
Experimental Data ◽  
Energy Dependence ◽  
Energetic Particles ◽  
Emulsion Chamber ◽  
X Ray ◽  
Secondary Particles ◽  
String Models

According to Pamir X-ray Emulsion Chamber (XEC) experimental data at the energies E est > 2 × 1016 eV the fraction of events with four "aligned" most energetic particles increases sharply for families without leading secondary particles. That energy dependence is not described by Quark Gluon String Models.

SYSTEMATIC COMPARISON OF THE EXPERIMENTAL DATA WITH THE FRITIOF MODEL IN NUCLEUS–NUCLEUS INTERACTIONS WITH LIGHT AND HEAVY TARGET NUCLEI IN NUCLEAR EMULSION AT 4.5A Gev/c

2002 ◽  
Vol 11 (02) ◽  
pp. 161-175 ◽  
Author(s):  
M. MOHERY ◽  
N. N. ABD-ALLAH
Keyword(s):  
Experimental Data ◽  
Nuclear Emulsion ◽  
Multiplicity Distribution ◽  
Angular Distributions ◽  
Target Groups ◽  
Systematic Comparison ◽  
Secondary Particles ◽  
Heavy Target ◽  
Light Target ◽  
Fritiof Model

The characteristics of the interactions of 4.5 A GeV/c 28 Si nuclei with emulsion have been investigated. The method of separating interactions into those with hydrogen, light and heavy target nuclei has been discussed. The multiplicity distribution, average multiplicities, multiplicity correlation and the angular distributions of the secondary particles emitted in 28 Si -emulsion are calculated according to the Modified Fritiof Model and compared with the experimental data and with other available data for p, 12 C , 24 Mg at the same energy. It has been found that the modified Fritiof model can describe the multiplicity characteristics of the different emitted particles in the above-mentioned interaction with different target groups. The comparison of the experimental data with the modified Fritiof model shows no clear preference for the case of the light target while it seems to be nearer to the experimental data in the case of the heavy target and the emulsion

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