Population synthesis in astrophysics

2004/11/30 by S. B. Popov, S B Popov, M. E. Prokhorov +1 · 3 citations
Materials Science · Physics and Astronomy · #Chemical and Physical Properties of Materials #Nuclear physics research studies #Pulsars and Gravitational Waves Research #astro-ph #physics.comp-ph

paper · pdf · doi:10.1070/pu2007v050n11abeh006179

published as Phys.Usp.50:1123-1146,2007 · 30 pages, no figures, to appear in proceedings of the Helmholtz International Summer School and Workshop on Hot points in Astrophysics and Cosmology

arxiv created 2004/11/30 · openalex publication_date 2007/11/30 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28

Abstract

We briefly describe different astrophysical applications of a population synthesis method. In some details we discuss the population synthesis of close binary systems and of isolated neutron stars.

Citations

• Neutron star cooling constraints for color superconductivity in hybrid stars
• Intermediate-Mass Black Holes
• Inclusion of binaries in evolutionary population synthesis
• Evolutionary Processes in Close Binary Systems

Cited by

• Modified pulsar current analysis: probing magnetic field evolution
• Where do the progenitors of millisecond pulsars come from?
• The Evolution of Compact Binary Star Systems