V. S. Beskin, “Radio pulsars: already fifty years!”, UFN, 188:4 (2018), 377–408; Phys. Usp., 61:4 (2018), 353

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Uspekhi Fizicheskikh Nauk, 2018, Volume 188, Number 4, Pages 377–408
DOI: https://doi.org/10.3367/UFNr.2017.10.038216 (Mi ufn6088)

This article is cited in 72 scientific papers (total in 77 papers)

100 YEARS OF THE "USPEKHI FIZICHESKIKH NAUK" JOURNAL. REVIEWS OF TOPICAL PROBLEMS

Radio pulsars: already fifty years!

V. S. Beskin^ab

^a Lebedev Physical Institute, Russian Academy of Sciences, Moscow
^b Moscow Institute of Physics and Technology (State University), Dolgoprudnyi, Moscow region

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DOI: https://doi.org/10.3367/UFNr.2017.10.038216

Abstract: Although fifty years have passed 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 as yet no consensus on key issues, such as the nature of coherent radio emission or the conversion mechanism of the electromagnetic energy of the pulsar wind into particle energy. In this review, we present the main theoretical results on the magnetosphere of neutron stars. We formulate a number of apparently simple questions, which nevertheless remain unanswered since the very beginning of the field and which must be resolved before any further progress can be made.

Funding agency	Grant number
Russian Foundation for Basic Research	17-02-00788
This study was supported by the Russian Foundation for Basic Research grant 17-02-00788.

Received: July 31, 2017
Revised: October 3, 2017
Accepted: October 5, 2017

English version:
Physics–Uspekhi, 2018, Volume 61, Issue 4, Pages 353–380
DOI: https://doi.org/10.3367/UFNe.2017.10.038216

Bibliographic databases:

Document Type: Article

PACS: 01.65.+g, 95.30.Qd, 97.60.Gb

Language: Russian

Citation: V. S. Beskin, “Radio pulsars: already fifty years!”, UFN, 188:4 (2018), 377–408; Phys. Usp., 61:4 (2018), 353–380

Citation in format AMSBIB

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https://www.mathnet.ru/eng/ufn6088

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This publication is cited in the following 77 articles:

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K. A. Postnov, N. K. Porayko, M. S. Pshirkov, “Precision methods of pulsar timing and polarimetry: results and prospects”, Phys. Usp., 68:2 (2025), 146–162
Guy Pelletier, “Generation of ultralight axions by a Kerr black hole. II. The favorable magnetospheric physics”, Phys. Rev. D, 111:6 (2025)
Patrick Chi-Kit Cheong, Antonios Tsokaros, Milton Ruiz, Fabrizio Venturi, Juno Chun Lung Chan, Anson Ka Long Yip, Kōji Uryū, “General-relativistic resistive-magnetohydrodynamics simulations of self-consistent magnetized rotating neutron stars”, Phys. Rev. D, 111:6 (2025)
Jan Benáček, Patricio A. Muñoz, Jörg Büchner, Axel Jessner, “Streaming instability in neutron star magnetospheres: No indication of soliton-like waves”, A&A, 683 (2024), A69
Joonas Nättilä, Jari J. E. Kajava, Handbook of X-ray and Gamma-ray Astrophysics, 2024, 4177
Biao‐Peng Li, Wen‐Qi Ma, Zhi‐Fu Gao, “A short review of the pulsar magnetic inclination angles (II)”, Astron Nachr, 345:2-3 (2024)
Zhengli Wang, Jiguang Lu, Jingchen Jiang, Shunshun Cao, Weiyang Wang, Enwei Liang, Renxin Xu, “Non‐symmetrical sparking may hint “zits” on a pulsar surface”, Astron Nachr, 345:2-3 (2024)
Zhengli Wang, Jiguang Lu, Jinchen Jiang, Shunshun Cao, Kejia Lee, Enwei Liang, Lunhua Shang, Weiyang Wang, Renxin Xu, Weiwei Zhu, “Radio Pulsar B0950+08: Radiation in the Magnetosphere and Sparks above the Surface”, ApJ, 963:1 (2024), 65
Pavel Abolmasov, Anton Biryukov, Sergei B. Popov, “Spin Evolution of Neutron Stars”, Galaxies, 12:1 (2024), 7
M.D. Afonina, A.V. Biryukov, S.B. Popov, “Early accretion onset in long-period isolated pulsars”, Publ. Astron. Soc. Aust., 41 (2024)
S. Riggi, G. Umana, C. Trigilio, C. Bordiu, F. Bufano, A. Ingallinera, F. Cavallaro, Y. Gordon, R.P. Norris, G. Gürkan, P. Leto, C. Buemi, S. Loru, A.M. Hopkins, M.D. Filipović, T. Cecconello, “Classification of compact radio sources in the Galactic plane with supervised machine learning”, Publ. Astron. Soc. Aust., 41 (2024)
V. V. Kocharovsky, V. V. Vdovin, A. S. Gavrilov, E. R. Kocharovskaya, S. V. Logvinenko, E. M. Loskutov, V. M. Malofeev, “The Method of Periodic Principal Components for the Dynamic Spectrum of Radio Pulsars and Faraday Rotation of Nine Pulse Components of PSR B0329+54”, Astron. Lett., 50:2 (2024), 120
A. Ahmad, S. Dai, E. Lenc, M. D. Filipović, L. Barnes, G. Hobbs, J. C. F. Balzan, L. Zhang, “Wideband polarization and spectral properties of 18 high Galactic latitude pulsars”, Astrophys Space Sci, 369:6 (2024)
Zhen Yan, Zhiqiang Shen, Yajun Wu, Rongbing Zhao, Jie Liu, Zhipeng Huang, Rui Wang, Xiaowei Wang, Qinghui Liu, Bin Li, Jinqing Wang, Weiye Zhong, Wu Jiang, Bo Xia, “Shanghai Tianma Radio Telescope and Its Role in Pulsar Astronomy”, Universe, 10:5 (2024), 195
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M. V. Popov, “Microstructure in Radio Emission of the Pulsar B1133+16 at a Frequency of 111 MHz”, Astron. Rep., 68:5 (2024), 514
L. A. Bakaleinikov, V. I. Kuznetsov, E. Yu. Flegontova, D. P. Barsukov, I. K. Morozov, “Steady state stability features of the electron–positron plasma diode in a mode with particle reflection from potential extrema”, Physics of Plasmas, 31:9 (2024)
Zonghai Li, Junji Jia, “Deflection of charged signals in a dipole magnetic field in Kerr background”, Eur. Phys. J. C, 84:9 (2024)
V. V. Kocharovskii, V. V. Vdovin, A. S. Gavrilov, E. R. Kocharovskaya, S. V. Logvinenko, E. M. Loskutov, V. M. Malofeev, “Metod periodicheskikh glavnykh komponent dinamicheskogo spektra radiopulsarov i faradeevskoe vraschenie devyati sostavlyayuschikh impulsa PSR B0329+54”, Pisʹma v Astronomičeskij žurnal, 50:2 (2024), 142

Citing articles in Google Scholar: Russian citations, English citations
Related articles in Google Scholar: Russian articles, English articles

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