Parameters of radiation defect clusters in silicon irradiated by high-energy γ-rays

1985 ◽  
Vol 87 (1) ◽  
pp. 15-22
Author(s):  
V. I. Kuznetsov ◽  
P. F. Lugakov ◽  
V. V. Shusha
Keyword(s):  
Radiation Defect ◽  
High Energy ◽  
Defect Clusters ◽  
Γ Rays

Introduction of defect clusters in GaAs by high-energy γ-rays

1979 ◽  
Vol 56 (1) ◽  
pp. 387-393 ◽  
Author(s):  
T. I. Kolchenko ◽  
V. M. Lomako ◽  
I. G. Tarutin
Keyword(s):  
High Energy ◽  
Defect Clusters ◽  
Γ Rays

Introduction of Defect Clusters in GaAs by High-Energy γ-Rays

1979 ◽  
pp. 387-394
Author(s):  
T. I. Kolchenko ◽  
V. M. Lomako ◽  
I. G. Tarutin
Keyword(s):  
High Energy ◽  
Defect Clusters ◽  
Γ Rays

Radiation damage of BGO crystals due to low energy γ rays, high energy protons and fast neutrons

1983 ◽  
Vol 206 (1-2) ◽  
pp. 107-117 ◽  
Author(s):  
Masaaki Kobayashi ◽  
Kenjiro Kondo ◽  
Hiromi Hirabayashi ◽  
Shin-ichi Kurokawa ◽  
Mitsuhiko Taino ◽  
...  
Keyword(s):  
Radiation Damage ◽  
High Energy ◽  
Low Energy ◽  
Fast Neutrons ◽  
Γ Rays

scholarly journals Low frequency radio counterparts of HESS J1731−347 a.k.a SNR G353.6−0.7

2017 ◽  
Vol 12 (S331) ◽  
pp. 201-205
Author(s):  
A. J. Nayana ◽  
Poonam Chandra
Keyword(s):  
Radio Emission ◽  
Radio Telescope ◽  
Supernova Remnants ◽  
Low Frequency ◽  
High Energy ◽  
Spectral Indices ◽  
Thermal Radio Emission ◽  
Very High Energy ◽  
Γ Rays ◽  
Very High

AbstractHESS J1731−347 a.k.a. SNR G353.6−0.7 is one of the five known very high energy (VHE, Energy > 0.1 TeV) shell-type supernova remnants. We carried out Giant Metrewave Radio Telescope (GMRT) observations of this TeV SNR in 1390, 610 and 325 MHz bands. We detected the 325 and 610 MHz radio counterparts of the SNR G353.6−0.7 (Nayana et al. 2017). We also determined the spectral indices of individual filaments and our values are consistent with the non-thermal radio emission. We compared the radio morphology with that of VHE emission. The peak in radio emission corresponds to the faintest feature in the VHE emission. We explain this anti-correlated emission in a possible leptonic origin of the VHE γ-rays.

scholarly journals Molecular Clouds Observed by the EGRET Gamma-Ray Telescope

1997 ◽  
Vol 170 ◽  
pp. 22-24 ◽  
Author(s):  
Seth. W. Digel ◽  
Stanley D. Hunter ◽  
Reshmi Mukherjee ◽  
Eugéne J. de Geus ◽  
Isabelle A. Grenier ◽  
...  
Keyword(s):  
Molecular Mass ◽  
Molecular Clouds ◽  
Gamma Ray ◽  
Angular Resolution ◽  
Cosmic Ray ◽  
High Energy ◽  
Background Rejection ◽  
Γ Rays ◽  
Γ Ray ◽  
Production Mechanisms

EGRET, the high-energy γ-ray telescope on the Compton Gamma-Ray Observatory, has the sensitivity, angular resolution, and background rejection necessary to study diffuse γ-ray emission from the interstellar medium (ISM). High-energy γ rays produced in cosmic-ray (CR) interactions in the ISM can be used to determine the CR density and calibrate the CO line as a tracer of molecular mass. Dominant production mechanisms for γ rays of energies ∼30 MeV–30 GeV are the decay of pions produced in collisions of CR protons with ambient matter and Bremsstrahlung scattering of CR electrons.

Life-Shortening and Disease Incidence in Mice after Exposure to γ Rays or High-Energy Neutrons

1991 ◽  
Vol 128 (1) ◽  
pp. S117 ◽  
Author(s):  
J. R. Maisin ◽  
A. Wambersie ◽  
G. B. Gerber ◽  
G. Mattelin ◽  
M. Lambiet-Collier ◽  
...  
Keyword(s):  
Disease Incidence ◽  
High Energy ◽  
Γ Rays
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