TL;DR
This paper introduces two new methods based on the orbital probability density function (oPDF) to infer the gravitational potential from steady-state tracers, applicable to spherical and potentially non-spherical systems, without assuming specific distribution functions.
Contribution
The paper develops and tests two novel, assumption-free methods for gravitational potential inference using steady-state tracers, based on the oPDF, applicable to arbitrary orbit distributions.
Findings
Methods are unbiased and efficient in dark matter haloes.
The likelihood estimator fits analytical potentials accurately.
The phase-mark method reconstructs potential profiles non-parametrically.
Abstract
We develop two general methods to infer the gravitational potential of a system using steady-state tracers, i.e., tracers with a time-independent phase-space distribution. Combined with the phase-space continuity equation, the time independence implies a universal Orbital Probability Density Function (oPDF) , where is the coordinate of the particle along the orbit. The oPDF is equivalent to Jeans theorem, and is the key physical ingredient behind most dynamical modelling of steady-state tracers. In the case of a spherical potential, we develop a likelihood estimator that fits analytical potentials to the system, and a non-parametric method ("phase-mark") that reconstructs the potential profile, both assuming only the oPDF. The methods involve no extra assumptions about the tracer distribution function and can be applied to…
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