Radio pulsars --- already fifty years!

V.S. Beskin^a, b
^aMoscow Institute of Physics and Technology (National Research University), Institutskii per. 9, Dolgoprudny, Moscow Region, 141701, Russian Federation
^bLebedev Physical Institute, Russian Academy of Sciences, Leninsky prosp. 53, Moscow, 119991, Russian Federation

Despite fifty years since the discovery of radio pulsars, there is still no satisfactory understanding of how these amazing objects operate. While there has been significant progress in understanding the basic properties of radio pulsars, there is yet no consensus on key issues such as the nature of coherent radio emission or the conversion mechanism of the electromagnetic energy of pulsar wind into particle energy. This review attempts to present the main theoretical results on the magnetosphere of neutron stars. A number of questions are formulated which, while seemingly fairly simple, have remained unanswered since the very beginning of the field and which should necessarily be resolved before any further progress can be made.

Keywords: radio pulsars, pulsar magnetosphere, pulsar wind
PACS: 01.65.+g, 95.30.Qd, 97.60.Gb (all)
DOI: 10.3367/UFNe.2017.10.038216
URL: https://ufn.ru/en/articles/2018/4/b/
Web of Science

000439002500002
Scopus

2-s2.0-85050609219
ADS NASA

2018PhyU...61..353B
Citation: Beskin V S "Radio pulsars --- already fifty years!" Phys. Usp. 61 353–380 (2018)

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Received: 31st, July 2017, revised: 3rd, October 2017, accepted: 5th, October 2017

Оригинал: Бескин В С «Радиопульсары — уже пятьдесят лет!» УФН 188 377–408 (2018); DOI: 10.3367/UFNr.2017.10.038216

References (259) Cited by (57) Similar articles (20) ↓

V.S. Beskin “Magnetohydrodynamic models of astrophysical jets” 53 1199–1233 (2010)
M.A. Liberman, B. Johansson “Properties of matter in ultrahigh magnetic fields and the structure of the surface of neutron stars” 38 117–136 (1995)
A.Y. Potekhin “Atmospheres and radiating surfaces of neutron stars” 57 735–770 (2014)
A.Yu. Potekhin “The physics of neutron stars” 53 1235–1256 (2010)
V.S. Beskin “Radio pulsars” 42 1071 (1999)
V.S. Beskin, A.V. Gurevich, Ya.N. Istomin “Physics of pulsar magnetospheres” 29 946–970 (1986)
V.S. Beskin, V.I. Krauz, S.A. Lamzin “Laboratory modeling of jets from young stars using plasma focus facilities” 66 327–359 (2023)
S.B. Popov, M.E. Prokhorov “Population synthesis in astrophysics” 50 1123–1146 (2007)
B.M. Bolotovskii, V.L. Ginzburg “The Vavilov-Cerenkov Effect and the Doppler Effect in the Motion of Sources with Superluminal Velocity in Vacuum” 15 184–192 (1972)
V.S. Beskin “Axisymmetric stationary flows in compact astrophysical objects” 40 659–688 (1997)
V.L. Ginzburg “PULSARS (Theoretical Concepts)” 14 83–103 (1971)
E.D. Eidelman, A.V. Arkhipov “Field emission from carbon nanostructures: models and experiment” 63 648–667 (2020)
D.M. Sedrakyan, K.M. Shakhabasyan “Superfluidity and the magnetic field of pulsars” 34 (7) 555–571 (1991)
B.M. Vladimirskii, A.M. Gal’per et al “Cygnus X-3: a powerful galactic source of hard radiation” 28 153–169 (1985)
Ya.B. Zel’dovich, I.D. Novikov “Relativistic astrophysics. II” 8 522–577 (1966)
A.P. Pyatakov, A.K. Zvezdin “Magnetoelectric and multiferroic media” 55 557–581 (2012)
B.S. Ishkhanov, I.M. Kapitonov “Giant dipole resonance of atomic nuclei. Prediction, discovery, and research” 64 141–156 (2021)
D.F. Alferov, Yu.A. Bashmakov, P.A. Cherenkov “Radiation from relativistic electrons in a magnetic undulator” 32 200–227 (1989)
Ya.B. Zel’dovich “Interaction of free electrons with electromagnetic radiation” 18 79–98 (1975)
A.V. Tutukov, A.M. Cherepashchuk “Evolution of close binary stars: theory and observations” 63 209–244 (2020)

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