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Volumn 68, Issue 2, 2003, Pages

Disk accretion flow driven by large-scale magnetic fields: Solutions with constant specific energy

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; ELECTROMAGNETIC FIELD; ENERGY; MAGNETIC FIELD; MAGNETISM; MATHEMATICAL ANALYSIS; MATHEMATICAL MODEL;

EID: 4544282004     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.68.024022     Document Type: Article
Times cited : (4)

References (60)
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    • 0002167157 scopus 로고
    • edited by C. DeWitt and B.S. DeWitt Gordon and Breach, New York
    • I.D. Novikov and K.S. Thorne, in Black Holes, edited by C. DeWitt and B.S. DeWitt (Gordon and Breach, New York, 1973), p. 343.
    • (1973) Black Holes , pp. 343
    • Novikov, I.D.1    Thorne, K.S.2
  • 6
    • 33750283528 scopus 로고    scopus 로고
    • note
    • Throughout the paper we use geometrized units G = c=1, where G is the Newtonian gravitational constant, c is the speed of light.
  • 10
    • 33750291599 scopus 로고    scopus 로고
    • M. Kishimoto, R. Antonucci, and O. Blaes, astro-ph/0304118
    • M. Kishimoto, R. Antonucci, and O. Blaes, astro-ph/0304118.
  • 17
    • 33750374021 scopus 로고    scopus 로고
    • I.V. Igumenshchev, R. Narayan, and M.A. Abramowicz, astro-ph/0301402
    • I.V. Igumenshchev, R. Narayan, and M.A. Abramowicz, astro-ph/0301402.
  • 20
    • 33750309855 scopus 로고    scopus 로고
    • O.M. Blaes, astro-ph/0211368
    • O.M. Blaes, astro-ph/0211368.
  • 28
    • 0000272453 scopus 로고    scopus 로고
    • A large-scale magnetic field in an accretion disk can arise in at least two ways: (1) Inherited from the progenitor of the disk. For example, the merger of a magnetized neutron star with a black hole will naturally lead to the formation of a disk with a large-scale magnetic field. (2) Generated from small-scale magnetic fields through reconnection. See, e.g., C. A. Tout and J. E. Pringle, Mon. Not. R. Astron. Soc. 281, 219 (1996).
    • (1996) Mon. Not. R. Astron. Soc. , vol.281 , pp. 219
    • Tout, C.A.1    Pringle, J.E.2
  • 38
    • 33750310610 scopus 로고    scopus 로고
    • J.P. De Villiers and J.F. Hawley, astro-ph/0210518
    • J.P. De Villiers and J.F. Hawley, astro-ph/0210518.
  • 39
    • 33750307025 scopus 로고    scopus 로고
    • note
    • In this paper we use the word "sonic" to refer to "magnetosonic" since we have assumed that the gas pressure is zero.
  • 41
    • 0004057466 scopus 로고
    • The University of Chicago Press, Chicago
    • R.M. Wald, General Relativity (The University of Chicago Press, Chicago, 1984).
    • (1984) General Relativity
    • Wald, R.M.1
  • 42
    • 85107714081 scopus 로고    scopus 로고
    • note
    • n+1 or higher.
  • 45
    • 85107714961 scopus 로고    scopus 로고
    • note
    • r=0 here so must be located at r=∞ and is not relevant.
  • 50
    • 33750292741 scopus 로고    scopus 로고
    • N. Afshordi and B. Paczyński, astro-ph/0202409
    • N. Afshordi and B. Paczyński, astro-ph/0202409.
  • 51
    • 33750353176 scopus 로고    scopus 로고
    • The contour plot is drawn with MATHEMATICA
    • The contour plot is drawn with MATHEMATICA.
  • 59
    • 0004148601 scopus 로고    scopus 로고
    • Oxford University Press, New York
    • L. Mestel, Stellar Magnetism (Oxford University Press, New York, 1999).
    • (1999) Stellar Magnetism
    • Mestel, L.1
  • 60
    • 85107713195 scopus 로고    scopus 로고
    • note
    • φ|≪1 at large radii.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.