# Evolution of the Carter constant for inspirals into a black hole: effect of the black hole quadrupole

## TL;DR

This paper investigates how gravitational radiation reaction affects the Carter constant for generic orbits around axisymmetric bodies with a quadrupole moment, revealing effects on orbit shape and orientation, and challenging the existence of such constants in general spacetimes.

## Contribution

It provides the first calculation of the quadrupole's effect on the Carter constant's evolution and demonstrates the absence of a Carter-like constant in most axisymmetric vacuum spacetimes.

## Key findings

- Quadrupole effects circularize eccentric orbits.
- Quadrupole influences orbital plane orientation.
- No Carter constant exists for generic axisymmetric spacetimes except special cases.

## Abstract

We analyze the effect of gravitational radiation reaction on generic orbits around a body with an axisymmetric mass quadrupole moment Q to linear order in Q, to the leading post-Newtonian order, and to linear order in the mass ratio. This system admits three constants of the motion in absence of radiation reaction: energy, angular momentum, and a third constant analogous to the Carter constant. We compute instantaneous and time-averaged rates of change of these three constants. For a point particle orbiting a black hole, Ryan has computed the leading order evolution of the orbit's Carter constant, which is linear in the spin. Our result, when combined with an interaction quadratic in the spin (the coupling of the black hole's spin to its own radiation reaction field), gives the next to leading order evolution. The effect of the quadrupole, like that of the linear spin term, is to circularize eccentric orbits and to drive the orbital plane towards antialignment with the symmetry axis. In addition we consider a system of two point masses where one body has a single mass multipole or current multipole. To linear order in the mass ratio, to linear order in the multipole, and to the leading post-Newtonian order, we show that there does not exist an analog of the Carter constant for such a system (except for the cases of spin and mass quadrupole). With mild additional assumptions, this result falsifies the conjecture that all vacuum, axisymmetric spacetimes posess a third constant of geodesic motion.