Ynogkm: A new public code for calculating time-like geodesics in the Kerr-Newman spacetime

15Citations
Citations of this article
9Readers
Mendeley users who have this article in their library.

Abstract

In this paper, we present a new public code, named ynogkm (Yun-Nan observatories geodesic in a Kerr-Newman spacetime for massive particles), for the fast calculation of time-like geodesics in the Kerr-Newman (K-N) spacetime, which is a direct extension of ynogk (Yun-Nan observatories geodesic Kerr) calculating null geodesics in a Kerr spacetime. Following the strategies used in ynogk, we also solve the equations of motion analytically and semi-analytically by using Weierstrass' and Jacobi's elliptic functions and integrals in which the Boyer-Lidquist (B-L) coordinates r, θ, φ, t and the proper time σ are expressed as functions of an independent variable p (Mino time). All of the elliptic integrals are computed by Carlson's elliptic integral method, which guarantees the fast speed of the code. Finally, the code is applied to a couple of toy problems. © 2014 ESO.

Cite

CITATION STYLE

APA

Yang, X. L., & Wang, J. C. (2014). Ynogkm: A new public code for calculating time-like geodesics in the Kerr-Newman spacetime. Astronomy and Astrophysics, 561. https://doi.org/10.1051/0004-6361/201322565

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