scholarly journals Investigation of the beam energy dependence of particle production in gold-gold collisions performed at NICA energy range

2021 ◽  
Author(s):  
Elena A. Pervyshina ◽  
Alexey Aparin
Keyword(s):  
Energy Range ◽  
Energy Dependence ◽  
Beam Energy ◽  
Particle Production ◽  
Gold Collisions

scholarly journals Energy Dependence of Total Cross Sections for Reactions with 4, 6he, 6, 7, 9li Nuclei

KnE Energy ◽  
2018 ◽  
Vol 3 (1) ◽  
pp. 21
Author(s):  
Yu Penionzhkevich ◽  
Yu Sobolev ◽  
V Samarin ◽  
M Naumenko
Keyword(s):  
Experimental Data ◽  
Energy Range ◽  
Numerical Solution ◽  
Energy Dependence ◽  
Cross Sections ◽  
Beam Energy ◽  
Microscopic Analysis ◽  
Time Dependent ◽  
Total Cross Sections ◽  
Good Agreement

The paper presents the results of measurement of the total cross sections for reactions 4,6He + Si and 6,7,9Li + Si in the beam energy range 5−50 A⋅MeV. The enhancements of the total cross sections for reaction 6He + Si compared with reaction 4He + Si, and 9Li + Si compared with reactions 6,7Li + Si have been observed. The performed microscopic analysis of total cross sections for reactions 6He + Si and 9Li + Si based on numerical solution of the time-dependent Schrödinger equation for external neutrons of projectile nuclei 6He and 9Li yielded good agreement with experimental data.

ON THE ENERGY AND MASS DEPENDENCE OF THE MULTIPLICITY IN RELATIVISTIC HEAVY-ION INTERACTIONS

1990 ◽  
Vol 05 (03) ◽  
pp. 169-174 ◽  
Author(s):  
M. I. ADAMOVICH ◽  
Y. A. ALEXANDROV ◽  
M. M. CHERNYAVSKY ◽  
S. G. GERASSIMOV ◽  
S. P. KHARLAMOV ◽  
...  
Keyword(s):  
Energy Range ◽  
Energy Dependence ◽  
Nuclear Emulsion ◽  
Particle Production ◽  
Heavy Ion ◽  
Mass Dependence ◽  
Ion Interactions ◽  
Binary Collisions ◽  
Singly Charged ◽  
Relativistic Particles

The average multiplicities of singly charged relativistic particles in oxygen-induced interactions with a nuclear emulsion target are studied over the energy range 2.1–200 A GeV. A similar energy dependence as for proton-induced interactions is observed. Both the number of participating nucleons and the number of binary collisions are shown to be of importance for the particle production.

Microscopic analysis of the energy dependence of the 6He, 6Li + 28Si total reaction cross sections in the energy range E = 5−50 A MeV

2008 ◽  
Vol 72 (3) ◽  
pp. 356-360
Author(s):  
K. V. Lukyanov ◽  
E. V. Zemlyanaya ◽  
V. K. Lukyanov ◽  
I. N. Kukhtina ◽  
Yu. E. Penionzhkevich ◽  
...  
Keyword(s):  
Energy Range ◽  
Energy Dependence ◽  
Cross Sections ◽  
Microscopic Analysis ◽  
Reaction Cross ◽  
Total Reaction ◽  
Reaction Cross Sections

scholarly journals Beam-energy dependence of the production of light nuclei in Au + Au collisions

2020 ◽  
Vol 102 (4) ◽  
Author(s):  
Wenbin Zhao ◽  
Chun Shen ◽  
Che Ming Ko ◽  
Quansheng Liu ◽  
Huichao Song
Keyword(s):  
Energy Dependence ◽  
Beam Energy ◽  
Light Nuclei

scholarly journals Laser beam energy dependence of martensitic transformation in SLM fabricated NiTi shape memory alloy

Materialia ◽  
2019 ◽  
Vol 6 ◽  
pp. 100305 ◽  
Author(s):  
Y. Yang ◽  
J.B. Zhan ◽  
B. Li ◽  
J.X. Lin ◽  
J.J. Gao ◽  
...  
Keyword(s):  
Martensitic Transformation ◽  
Shape Memory Alloy ◽  
Laser Beam ◽  
Shape Memory ◽  
Energy Dependence ◽  
Beam Energy ◽  
Niti Shape Memory Alloy

scholarly journals On the origin of the TeV gamma-ray emission from Cygnus X-3

2019 ◽  
Vol 208 ◽  
pp. 14008
Author(s):  
V.G. Sinitsyna ◽  
V.Y. Sinitsyna
Keyword(s):  
Energy Range ◽  
Particle Production ◽  
Cosmic Ray ◽  
High Energy ◽  
Wide Energy Range ◽  
Electromagnetic Spectrum ◽  
Essential Information ◽  
Wide Range ◽  
Γ Ray ◽  
Very High

Cygnus X-3 binary system is a famous object studied over the wide range of electromagnetic spectrum. Early detections of ultra-high energy gamma-rays from Cygnus X-3 by Kiel, Havera Park and then by Akeno triggered the construction of several large air shower detectors. Also, Cygnus X-3 has been proposed to be one of the most powerful sources of charged cosmic ray particles in the Galaxy. The results of twenty-year observations of the Cyg X-3 binary at energies 800 GeV - 85 TeV are presented with images, spectra during periods of flaring activity and at low flux periods. The correlation of TeV flux increases with flaring activity at the lower energy range of X-ray and radio emission from the relativistic jets of Cygnus X-3 is found as well as 4.8-hour orbital modulation of TeV γ-ray intensity. Detected modulation of TeV γ-ray emission with orbit and important characteristics of Cyg X-3 such as the high luminosity of the companion star and the close orbit leads to an efficient generation of γ-ray emission through inverse Compton scattering in this object. The different type variability of very high-energy γ-emission and correlation of radiation activity in the wide energy range can provide essential information on the mechanism of particle production up to very high energies.

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