Mathematical Research Data Initiative
Main page
Recent changes
Random page
Help about MediaWiki
Create a new Item
Create a new Property
Merge two items
In other projects
Discussion
View source
View history
Purge
English
Log in

A statistical-mechanical explanation of dark matter halo properties

From MaRDI portal
Publication:4905579
Jump to:navigation, search

DOI10.1051/0004-6361/201015057zbMath1260.85134arXiv1012.1003OpenAlexW3100226146WikidataQ68997189 ScholiaQ68997189MaRDI QIDQ4905579

No author found.

Publication date: 19 February 2013

Published in: Astronomy & Astrophysics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1012.1003


zbMATH Keywords

dark matterhydrodynamicsmethods: analyticalgalaxies: statistics


Mathematics Subject Classification ID

Applications of statistics to physics (62P35) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Computational methods for problems pertaining to astronomy and astrophysics (85-08) Stability and instability of geophysical and astrophysical flows (76E20) Astrophysical cosmology (85A40)


Related Items (3)

Deep learning of CMB radiation temperature ⋮ Cosmic ``adiabatic photon creation: temperature law and blackbody spectrum ⋮ Equilibrium statistical mechanics for self-gravitating systems of two species







This page was built for publication: A statistical-mechanical explanation of dark matter halo properties

Retrieved from "https://portal.mardi4nfdi.de/w/index.php?title=Publication:4905579&oldid=19295667"
Tools
What links here
Related changes
Special pages
Printable version
Permanent link
Page information
MaRDI portal item
This page was last edited on 8 February 2024, at 06:10.
Privacy policy
About MaRDI portal
Disclaimers
Imprint
Powered by MediaWiki