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From the 3 of 24 linked papers with an AI index.

collaborators

24 papers

hep-ph2026

Ubiquitous Corotation of Dark Matter Halos: Implications for Direct Detection

Dylan Folsom, Carlos Blanco, Mariangela Lisanti +1

Cosmological simulations have recently begun to quantify the halo-to-halo variance in the phase-space distribution of dark matter around the Sun. We use a sample of nearly one hund…

astro-ph.HE2026

Semi-analytic Inference of Satellite Densities in the Cold Dark Matter Model Part II. Implications for Dark Matter Indirect Detection Constraints

Kailash Raman, Dylan Folsom, Manoj Kaplinghat +2

The paper updates the astrophysical J‑factors for Milky Way dwarf spheroidal galaxies using a calibrated semi‑analytic satellite model and new stellar kinematic data, and shows how…

astro-ph.GA2026

Semi-analytic Inference of Satellite Densities in the Cold Dark Matter Model Part I. Comparison to Ultra-faint Dwarf Kinematics

Kailash Raman, Dylan Folsom, Manoj Kaplinghat +2

The paper uses a semi‑analytic model of Milky Way satellite galaxies to predict their dark‑matter density profiles and compares these predictions to measurements of stellar velocit…

astro-ph.CO2026

Non-linear Evolution of Dark Plasma Subhalos

Andrew Liu, Anirudh Prabhu, Akaxia Cruz +1

The paper uses particle-in-cell simulations to study how electrostatic plasma instabilities in dark-matter subhalos orbiting the Milky Way grow non‑linearly, causing turbulent heat…

astro-ph.GA2026

How to Build an Empirical Speed Distribution for Dark Matter in the Solar Neighborhood

Tal Shpigel, Dylan Folsom, Mariangela Lisanti +3

The dark matter flux in a direct detection experiment depends on its local speed distribution. This distribution has been inferred from simulations of Milky Way-like galaxies, but…

astro-ph.GA2026

Mergers Matter: Gravothermal Collapse in Dwarf Halos with Self-Interacting Dark Matter

Maya Silverman, Abdelaziz Hussein, Arpit Arora +8

Self-Interacting Dark Matter (SIDM) models with large cross sections at relative velocities below can be tested with dwarf galaxy observations. We ana…