Tidal Tracks and Artificial Disruption of Cold Dark Matter Halos
arXiv:2206.01842 · doi:10.1093/mnras/stac2750
Abstract
We describe a simple extension to existing models for the tidal heating of dark matter subhalos which takes into account second order terms in the impulse approximation for tidal heating. We show that this revised model can accurately match the tidal tracks along which subhalos evolve as measured in high-resolution N-body simulations. We further demonstrate that, when a constant density core is introduced into a subhalo, this model is able to quantitatively reproduce the evolution and artificial disruption of N-body subhalos arising from finite resolution effects. Combining these results we confirm prior work indicating that artificial disruption in N-body simulations can result in a factor two underestimate of the subhalo mass function in the inner regions of host halos, and a 10--20% reduction over the entire virial volume.
9 pages, accepted for publication in MNRAS
References in corpus (10)
- The Tidal Evolution of Local Group Dwarf Spheroidals
- Disruption of Dark Matter Substructure: Fact or Fiction?
- Dark Matter Substructure in Numerical Simulations: A Tale of Discreteness Noise, Runaway Instabilities, and Artificial Disruption
- The asymptotic tidal remnants of cold dark matter subhalos
- The tidal evolution of dark matter substructure -- II. The impact of artificial disruption on subhalo mass functions and radial profiles
- The tidal evolution of dark matter substructure -- I. Subhalo density profiles
- Nonlinear evolution of dark matter subhalos and applications to warm dark matter
- DASH: a library of dynamical subhalo evolution
- Structure and kinematics of tidally limited satellite galaxies in LCDM
- A new calibration method of sub-halo orbital evolution for semi-analytic models
Cited by in corpus (18)
- Symphony: Cosmological Zoom-in Simulation Suites over Four Decades of Host Halo Mass
- Forecasts for Galaxy Formation and Dark Matter Constraints from Dwarf Galaxy Surveys
- Tidal Stripping in the Adiabatic Limit
- Prompt cusps and the dark matter annihilation signal
- Tidal evolution of cored and cuspy dark matter halos
- How the Galaxy-Halo Connection Depends on Large-Scale Environment
- Novel Conservative Methods for Adaptive Force Softening in Collisionless and Multi-Species N-Body Simulations
- Limits on dark matter annihilation in prompt cusps from the isotropic gamma-ray background
- The Effects of Linear Matter Power Spectrum Enhancement on Dark Matter Substructure
- Faster than SAM: An empirical model for the tidal evolution of dark matter substructure around strong gravitational lenses
- Impulsive mixing of stellar populations in dwarf spheroidal galaxies
- Collisionless relaxation from near equilibrium configurations: Linear theory and application to tidal stripping
- Limits on Early Matter Domination from the Isotropic Gamma-Ray Background
- The cusp-halo relation
- New insights on low-mass dark matter subhalo tidal tracks via numerical simulations
- Semianalytic model for decaying dark matter halos
- Constraining the Nature of Dark Matter from Tidal Radii of Cluster Galaxy Subhalos
- The PARADIGM project II: The lifetimes and quenching of satellites in Milky Way-mass haloes