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20242026
most citedSIDM Concerto: Compilation and Data Release of Self-interacting Dark Matter Zoom-in Simulations

11 citations · 14 across the 5 of their papers we have counts for

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astro-ph.CO202511 cited

SIDM Concerto: Compilation and Data Release of Self-interacting Dark Matter Zoom-in Simulations

Ethan O. Nadler, Demao Kong, Daneng Yang +1

We present SIDM Concerto: cosmological zoom-in simulations in cold dark matter (CDM) and self-interacting dark matter (SIDM) models based on the Symphony and Milky Way-est sui…

astro-ph.CO2025

A Universal Analytic Model for Gravitational Lensing by Self-Interacting Dark Matter Halos

Siyuan Hou, Daneng Yang, Nan Li +1

We present a model for analytically calculating gravitational lensing by self-interacting dark matter (SIDM) halos. Leveraging the universal behavior of SIDM halos during gravother…

astro-ph.CO2025

Diversifying halo structures in two-component self-interacting dark matter models via mass segregation

Daneng Yang, Yue-Lin Sming Tsai, Yi-Zhong Fan

Self-interacting dark matter (SIDM), through gravothermal evolution driven by elastic self-scatterings, offers a compelling explanation for the observed diversity of inner halo den…

astro-ph.CO2025

COZMIC. III. Cosmological Zoom-in Simulations of Self-interacting Dark Matter with Suppressed Initial Conditions

Ethan O. Nadler, Rui An, Daneng Yang +3

We present eight cosmological dark matter (DM)--only zoom-in simulations of a Milky Way--like system that include suppression of the linear matter power spectrum , and/or vel…

astro-ph.GA2025

EDEN: Exploring Disks Embedded in N-body simulations of Milky-Way-mass halos from Symphony

Yunchong Wang, Philip Mansfield, Ethan O. Nadler +4

We investigate the impact of galactic disks on the tidal stripping of cold dark matter subhalos within Milky Way (MW)-mass halos () using…

astro-ph.CO2025

SASHIMI-SIDM: Semi-analytical subhalo modelling for self-interacting dark matter at sub-galactic scales

Shin'ichiro Ando, Shunichi Horigome, Ethan O. Nadler +2

We combine the semi-analytical structure formation model, SASHIMI, which predicts subhalo populations in collisionless, cold dark matter (CDM), with a parametric model that maps CD…