Population synthesis in astrophysics

S.B. Popov, M.E. Prokhorov
Lomonosov Moscow State University, Shternberg State Astronomical Institute, Universitetskii prosp. 13, Moscow, 119889, Russian Federation

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.

PACS: 97.10.−q, 97.60.Jd, 97.80.−d (all)
DOI: 10.1070/PU2007v050n11ABEH006179
URL: https://ufn.ru/en/articles/2007/11/b/
Web of Science

000253900700002
Scopus

2-s2.0-40449120542
ADS NASA

2007PhyU...50.1123P
Citation: Popov S B, Prokhorov M E "Population synthesis in astrophysics" Phys. Usp. 50 1123–1146 (2007)

BibTexBibNote ® (generic)BibNote ® (RIS)MedlineRefWorks

Оригинал: Попов С Б, Прохоров М Е «Популяционный синтез в астрофизике» УФН 177 1179–1206 (2007); DOI: 10.3367/UFNr.0177.200711b.1179

References (202) Cited by (42) Similar articles (20) ↓

A.Yu. Potekhin “The physics of neutron stars” Phys. Usp. 53 1235–1256 (2010)
A.M. Cherepashchuk “Search for black holes” Phys. Usp. 46 335–371 (2003)
L.P. Grishchuk, V.M. Lipunov et al “Gravitational wave astronomy: in anticipation of first sources to be detected” Phys. Usp. 44 1–51 (2001)
A.V. Tutukov, A.M. Cherepashchuk “Evolution of close binary stars: theory and observations” Phys. Usp. 63 209–244 (2020)
V.L. Ginzburg, V.V. Zheleznyakov, V.V. Zaitsev “Coherent radio-emission mechanisms and magnetic pulsar models” Sov. Phys. Usp. 12 378–398 (1969)
A.G. Zhilkin, D.V. Bisikalo, A.A. Boyarchuk “Flow structure in magnetic close binary stars” Phys. Usp. 55 115–136 (2012)
A.M. Cherepashchuk “Masses of black holes in binary stellar systems” Phys. Usp. 39 759–780 (1996)
V.S. Beskin “Radio pulsars --- already fifty years!” Phys. Usp. 61 353–380 (2018)
D.G. Yakovlev, K.P. Levenfish, Yu.A. Shibanov “Cooling of neutron stars and superfluidity in their cores” Phys. Usp. 42 737 (1999)
G.S. Bisnovatyi-Kogan, V.M. Chechetkin “Nonequilibrium shells of neutron stars and their role in sustaining x-ray emission and nucleosynthesis” Sov. Phys. Usp. 22 89–108 (1979)
D.M. Sedrakyan, K.M. Shakhabasyan “Superfluidity and the magnetic field of pulsars” Sov. Phys. Usp. 34 (7) 555–571 (1991)
Yu.N. Efremov, A.D. Chernin “Large-scale star formation in galaxies” Phys. Usp. 46 1–20 (2003)
V.L. Ginzburg “PULSARS (Theoretical Concepts)” Sov. Phys. Usp. 14 83–103 (1971)
V.S. Beskin “Radio pulsars” Phys. Usp. 42 1071 (1999)
A.M. Fridman, D.V. Bisikalo “The nature of accretion disks of close binary stars: overreflection instability and developed turbulence” Phys. Usp. 51 551–576 (2008)
V.S. Beskin “Magnetohydrodynamic models of astrophysical jets” Phys. Usp. 53 1199–1233 (2010)
V.S. Imshennik “Rotational explosion mechanism for collapsing supernovae and the two-stage neutrino signal from supernova 1987A in the Large Magellanic Cloud” Phys. Usp. 53 1081–1092 (2010)
V.I. Dokuchaev “Birth and life of massive black holes” Sov. Phys. Usp. 34 (6) 447–470 (1991)
A.Y. Potekhin “Atmospheres and radiating surfaces of neutron stars” Phys. Usp. 57 735–770 (2014)
V.E. Panchuk, Yu.Yu. Balega et al “Study of exoplanets by spectroscopic methods” Phys. Usp. 63 562–582 (2020)

The list is formed automatically.