Matematicheskoe modelirovanie
RUS  ENG    JOURNALS   PEOPLE   ORGANISATIONS   CONFERENCES   SEMINARS   VIDEO LIBRARY   PACKAGE AMSBIB  
General information
Latest issue
Archive
Impact factor

Search papers
Search references

RSS
Latest issue
Current issues
Archive issues
What is RSS


Matem. Mod.:
Year:
Volume:
Issue:
Page:
Find




Personal entry:
Login:
Password:
Save password
Enter
Forgotten password?
Register

Matematicheskoe modelirovanie, 2017, Volume 29, Number 11, Pages 131–139 (Mi mm3912)  
This article is cited in 5 scientific papers (total in 5 papers)

Mathematical simulation of a massive star evolution on the basis of a gasdynamical model

A. V. Babakova, M. V. Popovbc, V. M. Chechetkindec

a Institute for Computer Aided Design of RAS, Moscow
b École Normale Supérieure de Lyon, CRAL (UMR CNRS 5574), Université de Lyon 1, France
c Keldysh Institute of Applied Mathematics of RAS, Moscow
d National Research Nuclear University MEPhI, Moscow
e Kurchatov Institute of Atomic Energy, Moscow
Full-text PDF (469 kB) Citations (5)
References:
PDF
HTML
Abstract: The FLOW method, coupled with an algorithm for self-gravity computations, is applied for three-dimensional modeling of astrophysical flows. This method is based on difference approximations of conservation laws, written for finite volumes. It is implemented within the simulation tool box FLUX, designed for computer systems of cluster architecture. The problem of hydrodynamic simulation in a model of a massive star of third generation (Pop III), which is a progenitor of pair instability supernova (PISN), is considered. Large-scale convective structures are produced under the neutral equilibrium conditions that significantly affect the process of a supernova explosion.
Keywords: mathematical modeling, conservative difference schemes, numerical methods, parallel algorithms, aerohydrodynamics, astrophysics, supernovae, gravity, vortex structures.
Funding agency Grant number
Russian Science Foundation 16-11-10339
Received: 06.10.2016
English version:
Mathematical Models and Computer Simulations, 2018, Volume 10, Issue 3, Pages 357–362
DOI: https://doi.org/10.1134/S2070048218030031
Bibliographic databases:
Document Type: Article
Language: Russian
Citation: A. V. Babakov, M. V. Popov, V. M. Chechetkin, “Mathematical simulation of a massive star evolution on the basis of a gasdynamical model”, Matem. Mod., 29:11 (2017), 131–139; Math. Models Comput. Simul., 10:3 (2018), 357–362
Citation in format AMSBIB
\Bibitem{BabPopChe17}
\by A.~V.~Babakov, M.~V.~Popov, V.~M.~Chechetkin
\paper Mathematical simulation of a massive star evolution on the basis of a gasdynamical model
\jour Matem. Mod.
\yr 2017
\vol 29
\issue 11
\pages 131--139
\mathnet{http://mi.mathnet.ru/mm3912}
\elib{https://elibrary.ru/item.asp?id=30462934}
\transl
\jour Math. Models Comput. Simul.
\yr 2018
\vol 10
\issue 3
\pages 357--362
\crossref{https://doi.org/10.1134/S2070048218030031}
\scopus{https://www.scopus.com/record/display.url?origin=inward&eid=2-s2.0-85048113431}
Linking options:
  • https://www.mathnet.ru/eng/mm3912
  • https://www.mathnet.ru/eng/mm/v29/i11/p131
    • This publication is cited in the following 5 articles:
    Citing articles in Google Scholar: Russian citations, English citations
    Related articles in Google Scholar: Russian articles, English articles
    		Математическое моделирование
    Statistics & downloads:
    Abstract page:255
    Full-text PDF :76
    References:34
    First page:15
     
      Contact us:
    		  Terms of Use  Registration to the website  Logotypes © Steklov Mathematical Institute RAS, 2024