Resolving the mass--anisotropy degeneracy of the spherically symmetric Jeans equation I: theoretical foundation

TL;DR

This paper develops a theoretical foundation for a method that removes the mass--anisotropy degeneracy in spherical Jeans modeling, enabling unbiased and unique mass estimates of stellar systems by reconstructing kinematic profiles using flexible B-spline functions.

Contribution

It introduces a novel theoretical approach that reconstructs unique kinematic profiles, overcoming the mass--anisotropy degeneracy in spherical Jeans equation analysis.

Findings

Successfully recovers unique kinematic profiles from synthetic data.

Removes degeneracy to allow unbiased mass estimates.

Demonstrates the method's effectiveness with an isotropic King model.

Abstract

A widely employed method for estimating the mass of stellar systems with apparent spherical symmetry is dynamical modelling using the spherically symmetric Jeans equation. Unfortunately this approach suffers from a degeneracy between the assumed mass density and the second order velocity moments. This degeneracy can lead to significantly different predictions for the mass content of the system under investigation, and thus poses a barrier for accurate estimates of the dark matter content of astrophysical systems. In a series of papers we describe an algorithm that removes this degeneracy and allows for unbiased mass estimates of systems of constant or variable mass-to-light ratio. The present contribution sets the theoretical foundation of the method that reconstructs a unique kinematic profile for some assumed free functional form of the mass density. The essence of our method lies in using flexible B-spline functions for the representation of the radial velocity dispersion in the spherically symmetric Jeans equation. We demonstrate our algorithm through an application to synthetic data for the case of an isotropic King model with fixed mass-to-light ratio, recovering excellent fits of theoretical functions to observables and a unique solution. The mass-anisotropy degeneracy is removed to the extent that, for an assumed functional form of the potential and mass density pair $(\Phi,\rho)$, and a given set of line-of-sight velocity dispersion $\sigma_{los}^2$ observables, we recover a unique profile for $\sigma_{rr}^2$ and $\sigma_{tt}^2$. Our algorithm is simple, easy to apply and provides an efficient means to reconstruct the kinematic profile.