Uspekhi Fizicheskikh Nauk
RUS  ENG    JOURNALS   PEOPLE   ORGANISATIONS   CONFERENCES   SEMINARS   VIDEO LIBRARY   PACKAGE AMSBIB  
General information
Latest issue
Forthcoming papers
Archive
Impact factor
Guidelines for authors
Submit a manuscript

Search papers
Search references

RSS
Latest issue
Current issues
Archive issues
What is RSS



UFN:
Year:
Volume:
Issue:
Page:
Find






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


Uspekhi Fizicheskikh Nauk, 2012, Volume 182, Number 1, Pages 3–18
DOI: https://doi.org/10.3367/UFNr.0182.201201a.0003
(Mi ufn2556)
 

This article is cited in 16 scientific papers (total in 16 papers)

REVIEWS OF TOPICAL PROBLEMS

A solution to the problems of cusps and rotation curves in dark matter halos in the cosmological standard model

A. G. Doroshkevich, V. N. Lukash, E. V. Mikheeva

Astro Space Center, Lebedev Physical Institute, Russian Academy of Sciences
References:
Abstract: We discuss various aspects of the inner structure formation in virialized dark matter (DM) halos that form as primordial density inhomogeneities evolve in the cosmological standard model. The main focus is on the study of central cusps/cores and of the profiles of DM halo rotation curves, problems that reveal disagreements among the theory, numerical simulations, and observations. A method that was developed by the authors to describe equilibrium DM systems is presented, which allows investigating these complex nonlinear structures analytically and relating density distribution profiles within a halo both to the parameters of the initial small-scale inhomogeneity field and to the nonlinear relaxation characteristics of gravitationally compressed matter. It is shown that cosmological random motions of matter ‘heat up’ the DM particles in collapsing halos, suppressing cusp-like density profiles within developing halos, facilitating the formation of DM cores in galaxies, and providing an explanation for the difference between observed and simulated galactic rotation curves. The analytic conclusions obtained within this approach can be confirmed by the N-body model simulation once improved spatial resolution is achieved for central halo regions.
Received: December 28, 2010
Accepted: February 28, 2011
English version:
Physics–Uspekhi, 2012, Volume 55, Issue 1, Pages 3–17
DOI: https://doi.org/10.3367/UFNe.0182.201201a.0003
Bibliographic databases:
Document Type: Article
PACS: 95.35.+d, 98.62.Gq, 98.62.Js
Language: Russian
Citation: A. G. Doroshkevich, V. N. Lukash, E. V. Mikheeva, “A solution to the problems of cusps and rotation curves in dark matter halos in the cosmological standard model”, UFN, 182:1 (2012), 3–18; Phys. Usp., 55:1 (2012), 3–17
Citation in format AMSBIB
\Bibitem{DorLukMik12}
\by A.~G.~Doroshkevich, V.~N.~Lukash, E.~V.~Mikheeva
\paper A solution to the problems of cusps and rotation curves in dark matter halos in the cosmological standard model
\jour UFN
\yr 2012
\vol 182
\issue 1
\pages 3--18
\mathnet{http://mi.mathnet.ru/ufn2556}
\crossref{https://doi.org/10.3367/UFNr.0182.201201a.0003}
\adsnasa{https://adsabs.harvard.edu/cgi-bin/bib_query?2012PhyU...55....3D}
\elib{https://elibrary.ru/item.asp?id=17239668}
\transl
\jour Phys. Usp.
\yr 2012
\vol 55
\issue 1
\pages 3--17
\crossref{https://doi.org/10.3367/UFNe.0182.201201a.0003}
\isi{https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=Publons&SrcAuth=Publons_CEL&DestLinkType=FullRecord&DestApp=WOS_CPL&KeyUT=000303763300001}
\elib{https://elibrary.ru/item.asp?id=17983670}
\scopus{https://www.scopus.com/record/display.url?origin=inward&eid=2-s2.0-84860239205}
Linking options:
  • https://www.mathnet.ru/eng/ufn2556
  • https://www.mathnet.ru/eng/ufn/v182/i1/p3
  • This publication is cited in the following 16 articles:
    Citing articles in Google Scholar: Russian citations, English citations
    Related articles in Google Scholar: Russian articles, English articles
    Успехи физических наук Physics-Uspekhi
    Statistics & downloads:
    Abstract page:449
    Full-text PDF :137
    References:60
    First page:1
     
      Contact us:
     Terms of Use  Registration to the website  Logotypes © Steklov Mathematical Institute RAS, 2024