<--- Back to Details
First PageDocument Content
Celestial mechanics / Large-scale structure of the cosmos / Galaxy clusters / Dark matter / Galaxy rotation curve / Gravitational lens / N-body simulation / General relativity / Galaxy / Physics / Physical cosmology / Astrophysics
Date: 2013-01-15 09:53:11
Celestial mechanics
Large-scale structure of the cosmos
Galaxy clusters
Dark matter
Galaxy rotation curve
Gravitational lens
N-body simulation
General relativity
Galaxy
Physics
Physical cosmology
Astrophysics

Simulating Coulomb Interacting Dark Matter Colin Lauer, Christopher M. Wells, Ph. D. Department of Physics ● Houghton College ● 1 Willard Avenue ● Houghton, NY

Add to Reading List

Source URL: www.houghton.edu

Download Document from Source Website

File Size: 584,81 KB

Share Document on Facebook

Similar Documents

dark matter in spiral galaxies mass, size and shape of the halo rotation curves • extended (core/cusp: Nancy)

dark matter in spiral galaxies mass, size and shape of the halo rotation curves • extended (core/cusp: Nancy)

DocID: 1gv87 - View Document

Vrije Universiteit Brussel  Faculteit Wetenschappen en Bio-ingenieurswetenschappen Departement Natuurkunde  Study of the sensitivity

Vrije Universiteit Brussel Faculteit Wetenschappen en Bio-ingenieurswetenschappen Departement Natuurkunde Study of the sensitivity

DocID: 1fBZr - View Document

Morphology and Dynamics of Galaxies with Cellular Automata Dr.	
  Brian	
  R.	
  Kent	
  (Na#onal	
  Radio	
  Astronomy	
  Observatory)	
   Abstract Galaxies are among the largest observed physical systems, surpa

Morphology and Dynamics of Galaxies with Cellular Automata Dr.  Brian  R.  Kent  (Na#onal  Radio  Astronomy  Observatory)   Abstract Galaxies are among the largest observed physical systems, surpa

DocID: 1atFt - View Document

CHANGING IT IS TIME FOR WDM Paolo Salucci SISSA  DARK MATTER IN GALAXIES

CHANGING IT IS TIME FOR WDM Paolo Salucci SISSA DARK MATTER IN GALAXIES

DocID: 1acfu - View Document

Galaxy Structure Observations and Cored Density Profiles CHANGING  IT IS TIME FOR WDM

Galaxy Structure Observations and Cored Density Profiles CHANGING IT IS TIME FOR WDM

DocID: 19TDJ - View Document