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Cited by 823Pulsars and Gravitational Waves ResearchAstrophysical Phenomena and ObservationsGamma-ray bursts and supernovae

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Physics of strongly magnetized neutron stars

Open access
Harding, Alice K, Lai, Dong·2006·Reports on Progress in Physics
DOI 10.1088/0034-4885/69/9/r03
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Abstract

There has recently been growing evidence for the existence of neutron stars possessing magnetic fields with strengths that exceed the quantum critical field strength of 4.4 × 10 13 G, at which the cyclotron energy equals the electron rest mass. Such evidence has been provided by new discoveries of radio pulsars having very high spin-down rates and by observations of bursting gamma-ray sources termed magnetars. This paper will discuss the exotic physics of this high-field regime, where a new array of processes becomes possible and even dominant and where familiar processes acquire unusual properties. We review the physical processes that are important in neutron star interiors and magnetospheres, including the behaviour of free particles, atoms, molecules, plasma and condensed matter in strong magnetic fields, photon propagation in magnetized plasmas, free-particle radiative processes, the physics of neutron star interiors and field evolution and decay mechanisms. Application of such processes in astrophysical source models, including rotation-powered pulsars, soft gamma-ray repeaters, anomalous x-ray pulsars and accreting x-ray pulsars will also be discussed. Throughout this review, we will highlight the observational signatures of high magnetic field processes, as well as the theoretical issues that remain to be understood.

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Research works printed but not linked: 62

  1. Alford M, 2001, Phys. Rev., D64, 075017
  2. Ashcroft N W, 1976, Solid State Phys.
  3. Baring M G, 1991, Astron. Astrophys., 249, 581
  4. Baring M G Harding A K Schrader C R, 1992, Proc. 2nd GRO Science Workshop, 245
  5. Basko M M, 1975, Astron. Astrophys., 42, 311
  6. Bhattacharya D, 1992, Astron. Astrophys., 254, 198
  7. Bisnovati-Kogan G S, 1975, Sov. Astron., 18, 217
  8. Bonazzola S, 1979, Astron. Astrophys., 78, 53
  9. Brinkmann W, 1980, Astron. Astrophys., 82, 352
  10. Bulik T, 1998, Acta Astron., 48, 695
  11. Camilo F, 2006, Nature
  12. Canuto V, 1977, Fundam. Cosm. Phys., 2, 203
  13. Cheng K S, 1994, Toward a Major Atmospheric Cherenkov Detector, 25
  14. Faucher-Giguéré C, 2006, Astrophys. J.
  15. Gnedin Yu N, 1974, Sov. Phys. JETP, 38, 903
  16. Gnedin Yu N, 1978, JETP Lett., 27, 305
  17. Haberl F Briel U G Sembay S Read A, 2005, Proc. 2005 EPIC XMM-Newton Consortium Meeting
  18. Haensel P, 1990, Astron. Astrophys., 222, 353
  19. Harding A K, 2003, Pulsars, AXPs and SGRs Observed with BeppoSAX, 127
  20. den Hartog P R, 2004, Astron. Tel., 293
  21. Herold H, 1982, Astron. Astrophys., 115, 90
  22. Heyl J Chen P, 2005, Proc. 22nd Texas Symposium on Relativistic Astrophysics at Stanford University
  23. Hurley K, 1999, Astrophys. J., 510, L110
  24. Kadomtsev B B, 1970, Zh. Eksp. Teor. Fiz., 58, 1765
  25. Kadomtsev B B, 1970, Sov. Phys. JETP, 31, 945
  26. Kadomtsev B B, 1971, Pis'ma Zh. Eksp. Teor. Fiz., 13, 61
  27. Kadomtsev B B, 1971, Sov. Phys. JETP Lett., 13, 42
  28. Khersonskii V K, 1987, Sov. Astron., 31, 225
  29. Kirk J G, 1985, Astron. Astrophys., 142, 430
  30. Klepikov N P, 1954, Zh. Eksp. Teor. Fiz., 26, 19
  31. Kössl D, 1988, Astron. Astrophys., 205, 347
  32. Kozlenkov A A, 1987, Sov. Phys. JETP, 64, 1173
  33. Kretschmar P, 2005, Astron. Tel, 601
  34. Landau L D, 1980, Statistical Physics
  35. Medin Z, 2006, Phys. Rev.
  36. Melrose D B, 1986, Astron. Astrophys., 156, 268
  37. Melrose D B, 1981, Astron. Astrophys., 95, 86
  38. Miller M C, 1995, Astrophys. J., 488, L29
  39. Nagase F, 1989, Publ. Astron. Soc. Japan, 41, 1
  40. Nice D J, 2005, Astrophys. J.
  41. Paczynski B, 1992, Acta Astron., 42, 145
  42. Pavlov G G Sanwal D Teter M A Camilo F Gaensler B M, 2003, Young Neutron Stars and their Environments IAU Symp. 218
  43. Pavlov G G, 1976, Sov. Phys. JETP, 43, 389
  44. Petrova S A, 2000, Astrophys. J., 355, 1168
  45. Potekhin A Y, 1999, Astron. Astrophys., 351, 787
  46. Potekhin A Y, 1999, Phys. Rev. E, 63, 01990
  47. Ruderman M, 2003, X-ray and gamma-ray astrophysics of galactic sources, 27
  48. Schaaf M E, 1990, Astron. Astrophys., 227, 61
  49. Shibanov Y A, 1992, Astron. Astrophys., 266, 313
  50. Soffel M, 1983, Astron. Astrophys., 126, 251
  51. Srinivasan G, 1990, Curr. Sci., 59, 31
  52. Urpin V A, 1980, Sov. Astron., 24, 425
  53. Usov N A, 1980, Sov. Phys.-JETP, 51, 148
  54. van Adelsberg M, 2006, Mon. Not. R. Astron. Soc.
  55. Wang C, 2006, Astrophys. J.
  56. Wiebicke H-J, 1996, Astron. Astrophys., 309, 203
  57. Wunner G, 1979, Phys. Rev., 42, 79
  58. Wunner G, 1986, Astron. Astrophys., 170, 179
  59. Zavlin V E, 1996, Astron. Astrophys., 315, 141
  60. Zavlin V E Pavlov G G Becker W, 2002, Proc. 270 WE-Heraeus Seminar on Neutron Stars, Pulsars and Supernova Remnants
  61. Zhang B, 1998, Astron. Astrophys., 338, 62
  62. Zhang B, 1996, Astron. Astrophys., 310, 135

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Metadata

Authors
Harding, A. K., & Lai, D.
Affiliations
  • Goddard Space Flight Center (US)
  • Cornell University (US)
ORCID
Venue
Reports on Progress in Physics
Publisher
IOP Publishing
Published
2006-08-23
Volume
69
Issue
9
Pages
2631-2708
ISSN
  • 0034-4885 (ISSN-L)
  • 1361-6633
DOI
10.1088/0034-4885/69/9/r03
OpenAlex
W2084824827
Cited by
823
References
430
Citations by year
2026: 35 · 2025: 50 · 2024: 46 · 2023: 34 · 2022: 32 · 2021: 35 · 2020: 49 · 2019: 53 · 2018: 38 · 2017: 49 · 2016: 52 · 2015: 42 · 2014: 43 · 2013: 35 · 2012: 43
FWCI
22.38
Type
journal article
Language
en
Open access
Locations
  • Reports on Progress in Physics (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
  • arXiv (Cornell University)
Funders
National Science Foundation (0307252)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Pulsars and Gravitational Waves Research
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysical Phenomena and Observations
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Gamma-ray bursts and supernovae
Keywords
magnetars, neutron star structure, neutron star magnetospheres, magnetized plasma, photon propagation, magnetic field evolution, field decay, rotation-powered pulsars, soft gamma repeaters, anomalous X-ray pulsars, accreting X-ray pulsars, radio pulsars, spin-down rate

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