Hostname: page-component-586b7cd67f-vdxz6 Total loading time: 0 Render date: 2024-11-27T01:45:34.660Z Has data issue: false hasContentIssue false
  • English
  • Français

Cosmological Simulations with Smoothed Particle Hydrodynamics

Published online by Cambridge University Press:  25 May 2016

Mario G. Abadi ,
Diego G. Lambas  and
Patricia B. Tissera
Mario G. Abadi
Affiliation:
IATE-Observatorio Astronomico Cordoba, Argentina. CONICET, Argentina
Diego G. Lambas
Affiliation:
IATE-Observatorio Astronomico Cordoba, Argentina. CONICET, Argentina
Patricia B. Tissera
Affiliation:
IATE-Observatorio Astronomico Cordoba, Argentina. CONICET, Argentina

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We have developed and tested a code that computes the evolution of a mixed system of gas and dark matter in expanding world models. The gravitational forces are calculated with the Adaptative P3M algorithms developed by H. Couchmann, 1993. The calculation of gas forces follow the standard SPH formalism (Monaghan, 1989).

Type
Part II: Contributed Papers
Information
Symposium - International Astronomical Union , Volume 168: Examining the Big Bang and the Diffuse Background Radiations , 1996 , pp. 577 - 578
Copyright
Copyright © Kluwer 1996