2020
DOI: 10.1088/1361-6382/ab7ac7
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Force-free electrodynamics near rotation axis of a Kerr black hole

Abstract: Despite their potential importance for understanding astrophysical jets, physically realistic exact solutions for magnetospheres around Kerr black holes have not been found, even in the force-free approximation. Instead approximate analytical solutions such as the Blandford-Znajek (split-)monopole, as well as numerical solutions, have been constructed. In this paper we consider a new approach to the analysis and construction of such magnetospheres. We consider force-free electrodynamics close to the rotation a… Show more

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Cited by 11 publications
(26 citation statements)
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“…(Ref. [11] further demonstrates the need for matched asymptotic expansions.) Our work shows that the monopole flux function is jointly C 3 in (ǫx, 1/x), where x = r/M , 11 with similar statements for the other quantities.…”
Section: Comparison With Previous Workmentioning
confidence: 99%
See 1 more Smart Citation
“…(Ref. [11] further demonstrates the need for matched asymptotic expansions.) Our work shows that the monopole flux function is jointly C 3 in (ǫx, 1/x), where x = r/M , 11 with similar statements for the other quantities.…”
Section: Comparison With Previous Workmentioning
confidence: 99%
“…Tanabe and Nagataki [7] computed the subleading correction to the energy extraction rate, but noted the full subleading solution could not be determined from their method. More recently, there have been conflicting claims of a high-order solution [8,9] and that the expansion is inconsistent [10,11].…”
Section: Introductionmentioning
confidence: 99%
“…In recent years, there has been renewed interest in extending these perturbative constructions [14][15][16][17][18][19][20] and exploring other profiles [21][22][23][24][25]. The BZ mechanism has been investigated in the intermediate-spin regime [26][27][28][29][30][31][32] using numerical simulations.…”
Section: Introduction and Summary Of The Resultsmentioning
confidence: 99%
“…Among the static magnetospheres, there are configurations with monopole [1], paraboloidal [1], hyperbolic [23] and vertical [4,21] magnetic field line profiles. We refer the reader to [19] for a classification of the asymptotic behaviour. Typically, in solving Eq.…”
Section: Blandford-znajek Split-monopole In the Slow-spin Regimementioning
confidence: 99%
“…in active galactic nuclei and quasars. For more recent discussions on the consistency of the BZ mechanism, see [2][3][4].…”
Section: Jhep12(2020)018mentioning
confidence: 99%