One-Temperature Model for Chemically Non-equilibrium Gas Mixtures

Author(s):  
Ekaterina Nagnibeda ◽  
Elena Kustova
1989 ◽  
Vol 8 ◽  
pp. 217-221
Author(s):  
Hitoshi Hanami ◽  
Tatsuo Yoshida

AbstractThe X-ray emission from the interaction of the ejecta with circumstellar matter (CSM) for SN1987A is investigated. The electron and the ion temperatures seem to be in non-equilibrium in the early phase of a SN remnant. We have studied the two-temperature model in the early phase of SNR and discuss the X-ray emission from SN1987A and its CSM.


2021 ◽  
Author(s):  
Shaon Talukdar ◽  
Md. Monir Hossain ◽  
Rajagopalan V. Ranganathan ◽  
Mruthunjaya Uddi

2016 ◽  
Vol 61 (1) ◽  
pp. 197-207 ◽  
Author(s):  
K. Konishi ◽  
M. Shigeta ◽  
M. Tanaka ◽  
A. Murata ◽  
T. Murata ◽  
...  

2012 ◽  
Vol 30 (4) ◽  
pp. 517-523 ◽  
Author(s):  
Bishnupriya Nayak ◽  
S.V.G. Menon

AbstractConditions for thermonuclear ignition are determined by three parameters: fuel density, temperature and hot-spot size. A simple three temperature model is developed to calculate the critical burn-up parameter or the minimum ρR product. Extensive results obtained are compared with earlier one temperature model for DT and DD fuels. While the two approaches are found to provide similar results for DT fuel except at low temperature regime (~10 keV), three temperature modeling is found to be necessary for DD fuel. This is argued to be due to the lower fusion reactivity and energy production in DD reactions.


2018 ◽  
Author(s):  
M. M. Kuznetsov ◽  
Yu. D. Kuleshova ◽  
Yu. G. Reshetnikova ◽  
L. V. Smotrova

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