Estimates of the Surface Magnetic Field Strength of Radio Pulsars

被引：1
|
作者：
Kim, Vitaliy [1 ,2 ]
Umirbayeva, Adel [1 ,3 ]
Aimuratov, Yerlan [1 ,3 ,4 ]
机构：
[1] Fesenkov Astrophys Inst, Observ 23, Alma Ata 050020, Kazakhstan
[2] Pulkovo Observ, Pulkovoskoe Shosse 65-1, St Petersburg 196140, Russia
[3] Al Farabi Kazakh Natl Univ, Fac Phys & Technol, Dept Theoret & Nucl Phys, Al Farabi Ave 71, Alma Ata 050040, Kazakhstan
[4] Int Ctr Relativist Astrophys Network, Piazza Repubbl 10, I-65122 Pescara, Italy
来源：
UNIVERSE | 2023年 / 9卷 / 07期
关键词：
neutron star; radio pulsar; magnetic dipole radiation; magnetic field; EVOLUTION; ANGLE;
D O I：
10.3390/universe9070334
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We investigate the geometry of the magnetic field of rotation-powered pulsars. A new method for calculating an angle (beta) between the spin and magnetic dipole axes of a neutron star (NS) in the ejector stage is considered within the frame of the magnetic dipole energy loss mechanism. We estimate the surface magnetic field strength (B-ns) for a population of known neutron stars in the radio pulsar (ejector) stage. The evaluated B-ns(beta) may differ by an order of magnitude from the values without considering the angle beta. It is shown that B-ns(beta) lies in the range 10(8)-10(14) G for a known population of short and middle periodic radio pulsars.
引用
收藏
页数：12
相关论文
共 50 条
  • [31] PROBING THE MAGNETIC-FIELD OF RADIO PULSARS - A REEXAMINATION OF POLARIZATION POSITION ANGLE SWINGS
    BARNARD, JJ
    ASTROPHYSICAL JOURNAL, 1986, 303 (01): : 280 - 291
  • [32] The strong magnetic field decay and evolution of radio pulsars on the P-P diagram
    Guseinov, OH
    Ankay, A
    Tagieva, SO
    INTERNATIONAL JOURNAL OF MODERN PHYSICS D, 2004, 13 (09): : 1805 - 1815
  • [33] Evolution of the magnetic fields of isolated radio pulsars
    Wang, ZX
    Lu, T
    CHINESE PHYSICS LETTERS, 1997, 14 (05) : 391 - 394
  • [34] PUTTING CORONAL SEISMOLOGY ESTIMATES OF THE MAGNETIC FIELD STRENGTH TO THE TEST
    De Moortel, I.
    Pascoe, D. J.
    ASTROPHYSICAL JOURNAL LETTERS, 2009, 699 (02): : L72 - L75
  • [35] Most-likely DCF Estimates of Magnetic Field Strength
    Myers, Philip C.
    Stephens, Ian W.
    Coude, Simon
    ASTROPHYSICAL JOURNAL, 2024, 962 (01):
  • [36] Strength of the Solar Coronal Magnetic Field – A Comparison of Independent Estimates Using Contemporaneous Radio and White-Light Observations
    Anshu Kumari
    R. Ramesh
    C. Kathiravan
    T. J. Wang
    Solar Physics, 2017, 292
  • [37] Strength of the Solar Coronal Magnetic Field - A Comparison of Independent Estimates Using Contemporaneous Radio and White-Light Observations
    Kumari, Anshu
    Ramesh, R.
    Kathiravan, C.
    Wang, T. J.
    SOLAR PHYSICS, 2017, 292 (11)
  • [38] Are pulsars born with a hidden magnetic field?
    Torres-Forne, Alejandro
    Cerda-Duran, Pablo
    Pons, Jose A.
    Font, Jose A.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2016, 456 (04) : 3813 - 3826
  • [39] MAGNETIC-FIELD TOPOLOGY IN PULSARS
    ARONS, J
    ASTROPHYSICAL JOURNAL, 1993, 408 (01): : 160 - 166
  • [40] Diquark condensates and the magnetic field of pulsars
    Blaschke, D
    Sedrakian, DM
    Shahabasyan, KM
    ASTRONOMY & ASTROPHYSICS, 1999, 350 (03): : L47 - L50
12345