Analytic solutions of the geodesic equation in higher dimensional static spherically symmetric space-times

TL;DR

This paper provides complete analytical solutions for the geodesic equations of massive particles in various higher-dimensional static spherically symmetric spacetimes, revealing complex orbit structures depending on multiple parameters.

Contribution

It introduces explicit solutions using Kleinian sigma functions for geodesics in higher-dimensional Schwarzschild, Reissner-Nordstroem, and (anti)de Sitter spacetimes, extending previous work to up to 11 dimensions.

Findings

Explicit analytical solutions for geodesics in dimensions up to 11.

Rich variety of orbits only in four and five dimensions.

Bound and escape orbits can traverse different universes in Reissner--Nordstroem spacetimes.

Abstract

The complete analytical solutions of the geodesic equation of massive test particles in higher dimensional Schwarzschild, Schwarzschild-(anti)de Sitter, Reissner-Nordstroem and Reissner-Nordstroem-(anti)de Sitter space--times are presented. Using the Jacobi inversion problem restricted to the theta divisor the explicit solution is given in terms of Kleinian sigma functions. The derived orbits depend on the structure of the roots of the characteristic polynomials which depend on the particle's energy and angular momentum, on the mass and the charge of the gravitational source, and the cosmological constant. We discuss the general structure of the orbits and show that due to the specific dimension-independent form of the angular momentum and the cosmological force a rich variety of orbits can emerge only in four and five dimensions. We present explicit analytical solutions for orbits up to 11 dimensions. A particular feature of Reissner--Nordstroem space-times is that bound and escape orbits traverse through different universes.