Zhurnal Vychislitel'noi Matematiki i Matematicheskoi Fiziki
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



Zh. Vychisl. Mat. Mat. Fiz.:
Year:
Volume:
Issue:
Page:
Find






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


Zhurnal Vychislitel'noi Matematiki i Matematicheskoi Fiziki, 2020, Volume 60, Number 10, Pages 1787–1794
DOI: https://doi.org/10.31857/S0044466920100142
(Mi zvmmf11151)
 

This article is cited in 2 scientific papers (total in 2 papers)

Mathematical physics

Simulation of the interaction of oppositely directed particle flows

S. Ya. Stepanova, T. V. Sal'nikovaba

a Dorodnicyn Computing Center, Federal Research Center "Computer Science and Control", Russian Academy of Sciences, Moscow, 119333 Russia
b Faculty of Mechanics and Mathematics, Lomonosov Moscow State University, Moscow, 119991 Russia
Citations (2)
References:
Abstract: A mathematical model of the early stage of the formation of interstellar clouds resulting from the interaction of oppositely directed cosmic particle flows and evolution of the clouds into planetary systems is proposed. An important role in the evolution is played by mechanical energy dissipation caused mainly by particle collisions. The simulation is based on the classical $n$-body problem and the Newtonian theory of instantaneous collisions of rigid bodies with a relative velocity recovery factor smaller than unity. The performed computations suggest that this model is applicable in cosmogonic theories of planetary system formation.
Key words: cosmogony, planetary system, evolution, impact.
Received: 07.05.2020
Revised: 07.05.2020
Accepted: 09.06.2020
English version:
Computational Mathematics and Mathematical Physics, 2020, Volume 60, Issue 10, Pages 1730–1736
DOI: https://doi.org/10.1134/S0965542520100139
Bibliographic databases:
Document Type: Article
UDC: 517.93
Language: Russian
Citation: S. Ya. Stepanov, T. V. Sal'nikova, “Simulation of the interaction of oppositely directed particle flows”, Zh. Vychisl. Mat. Mat. Fiz., 60:10 (2020), 1787–1794; Comput. Math. Math. Phys., 60:10 (2020), 1730–1736
Citation in format AMSBIB
\Bibitem{SteSal20}
\by S.~Ya.~Stepanov, T.~V.~Sal'nikova
\paper Simulation of the interaction of oppositely directed particle flows
\jour Zh. Vychisl. Mat. Mat. Fiz.
\yr 2020
\vol 60
\issue 10
\pages 1787--1794
\mathnet{http://mi.mathnet.ru/zvmmf11151}
\crossref{https://doi.org/10.31857/S0044466920100142}
\elib{https://elibrary.ru/item.asp?id=44008029}
\transl
\jour Comput. Math. Math. Phys.
\yr 2020
\vol 60
\issue 10
\pages 1730--1736
\crossref{https://doi.org/10.1134/S0965542520100139}
\isi{https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=Publons&SrcAuth=Publons_CEL&DestLinkType=FullRecord&DestApp=WOS_CPL&KeyUT=WOS:000594502400013}
\scopus{https://www.scopus.com/record/display.url?origin=inward&eid=2-s2.0-85096453076}
Linking options:
  • https://www.mathnet.ru/eng/zvmmf11151
  • https://www.mathnet.ru/eng/zvmmf/v60/i10/p1787
  • This publication is cited in the following 2 articles:
    Citing articles in Google Scholar: Russian citations, English citations
    Related articles in Google Scholar: Russian articles, English articles
    Журнал вычислительной математики и математической физики Computational Mathematics and Mathematical Physics
     
      Contact us:
     Terms of Use  Registration to the website  Logotypes © Steklov Mathematical Institute RAS, 2024