REVIEWS OF TOPICAL PROBLEMS: Population synthesis in astrophysics

Details REVIEWS OF TOPICAL PROBLEMS: Population synthesis in astrophysics REVIEWS OF TOPICAL PROBLEMS: Population synthesis in astrophysics

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007svphu..50.1123p&link_type=abstract

Physics Uspekhi, Volume 50, Issue 11, pp. 1123-1146 (2007).

Physics

6

Scientific paper

Population synthesis is a method for numerical simulation of the population of objects with a complex evolution. This method is widely used in astrophysics. We consider its main applications to studying astronomical objects. Examples of modeling evolution are given for populations of close binaries and isolated neutron stars. The application of the method to studying active galactic nuclei and the integral spectral characteristics of galaxies is briefly discussed. An extensive bibliography on all the topics covered is provided.

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