Erratum: “Hydrodynamic Simulations of Tilted Thick‐Disk Accretion onto a Kerr Black Hole” (ApJ, 623, 347 [2005])

  • Fragile P
  • Anninos P
N/ACitations
Citations of this article
6Readers
Mendeley users who have this article in their library.

Abstract

The correct form of equation (6) for the Kerr line element in tilted (t,r,ϑ,ϕ) coordinates should beds2=-(1-2Mr/(ϱ2))dt2+4Mr/(ϱ2)dtdr-(4Marsin2θ)/(ϱ2)P1dtdϑ-(4Marsin2θ)/(ϱ2)P2dtdϕ+(1+2Mr/(ϱ2))dr2-2asin2θ(1+2Mr/(ϱ2))P1drdϑ-2asin2θ(1+2Mr/(ϱ2))P2drdϕ+(ϱ2T21+AP21)dϑ2+2(ϱ2T1T2+AP1P2)dϑdϕ+(ϱ2T22+AP22)dϕ2. (1)This differs from the original form in a sign change inside the parenthesis in the sixth and seventh terms of the equation. In other words, whereas the metric given in our original paper had a factor (1-2Mr/ϱ2) in the grϑ and grϕ terms, the correct factor is (1+2Mr/ϱ2). The results and conclusions of the paper are unaffected by this change.

Cite

CITATION STYLE

APA

Fragile, P. C., & Anninos, P. (2007). Erratum: “Hydrodynamic Simulations of Tilted Thick‐Disk Accretion onto a Kerr Black Hole” (ApJ, 623, 347 [2005]). The Astrophysical Journal, 665(2), 1507–1507. https://doi.org/10.1086/519682

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free