Tidal Stripping in the Adiabatic Limit

TL;DR

This paper introduces a model for adiabatic tidal stripping of dark matter haloes, accurately predicting remnant properties and mass loss limits based on initial structure and tidal field, with applications to dark matter annihilation predictions.

Contribution

The paper presents an exact model for tidal stripping of NFW haloes in the adiabatic limit, enabling predictions of remnant properties and mass loss solely from initial conditions and tidal field parameters.

Findings

Model reproduces NFW halo remnants under adiabatic tidal fields.

Predicts asymptotic mass loss limits based on initial structure and tidal field.

NFW haloes cannot be fully disrupted adiabatically.

Abstract

We present a model for the remnants of haloes that have gone through an adiabatic tidal stripping process. We show that this model exactly reproduces the remnant of an NFW halo that is exposed to a slowly increasing isotropic tidal field and approximately for an anisotropic tidal field. The model can be used to predict the asymptotic mass loss limit for orbiting subhaloes, solely as a function of the initial structure of the subhalo and the value of the tidal field at pericentre. Predictions can easily be made for differently concentrated host-haloes with and without baryonic components, which differ most notably in their relation between pericentre radius and tidal field. The model correctly predicts several empirically measured relations such as the `tidal track' and the `orbital frequency relation' that was reported by Errani & Navarro (2021) for the case of an isothermal sphere. Further, we propose applications of the `structure-tide' degeneracy which implies that increasing the concentration of a subhalo has exactly the same impact on tidal stripping as reducing the amplitude of the tidal field. Beyond this, we find that simple relations hold for the bound mass, truncation radius, WIMP annihilation luminosity and tidal ratio of tidally stripped NFW haloes in relation to quantities measured at the radius of maximum circular velocity. Finally, we note that NFW haloes cannot be completely disrupted when exposed adiabatically to tidal fields of arbitrary magnitudes. We provide an open-source implementation of our model and suggest that it can be used to improve predictions of dark matter annihilation.