activity
20152026
most citedBoosting the annihilation boost: Tidal effects on dark matter subhalos and consistent luminosity modeling

61 citations · 77 across the 10 of their papers we have counts for

collaborators

12 papers

astro-ph.CO2026

Gravitational-wave background from supermassive black holes without merger trees: Tidally regulated mergers and direct inference from the NANOGrav 15 yr data

Shin'ichiro Ando

We present a semi-analytic framework that computes the gravitational-wave background (GWB) from supermassive black hole (SMBH) binaries by direct integration of an -body-recalib…

astro-ph.CO2026

Wave-Optics Imprints of Warm Dark Matter Subhalos with Prompt Cusps on Strongly Lensed Gravitational Waves

Bhashin A. Thakore, Shin'ichiro Ando

Dark matter halos are expected to form with a prompt density cusp at their centres, and in warm dark matter (WDM) cosmologies these cusps can dominate the inner…

astro-ph.CO2026

A lower bound on primordial power spectrum from halo substructure

Shin'ichiro Ando, Nagisa Hiroshima, Koji Ishiwata +1

We investigate how the primordial curvature perturbation of a certain wavelength scale affects the halo and subhalo structure. Primordial power spectrum considered in this paper fe…

astro-ph.CO2026

Wave-optics imprints of dark matter subhalos on strongly lensed gravitational waves. II. Saddle images and detectability

Shin'ichiro Ando

Wave-optics interference in strongly lensed gravitational waves is a new interferometric probe of dark matter substructure: a subhalo population threading a galaxy-scale lens impri…

astro-ph.CO2026

Wave-Optics Imprints of Dark Matter Subhalos on Strongly Lensed Gravitational Waves

Shin'ichiro Ando

Wave-optics effects in strongly lensed gravitational waves (GWs) provide a new interferometric probe of dark matter substructure. We compute the full diffraction integral for GWs p…

astro-ph.CO2025

Comparison of simulations and semi-analytical model for WDM subhalo mass functions

Mizuki Ono, Takashi Okamoto, Shin'ichiro Ando +1

The Cold Dark Matter (CDM) model successfully explains large-scale structure formation, but challenges remain at smaller scales, leading to interest in Warm Dark Matter (WDM) as an…

astro-ph.CO2025

Stringent Constraints on Self-Interacting Dark Matter Using Milky-Way Satellite Galaxies Kinematics

Shin'ichiro Ando, Kohei Hayashi, Shunichi Horigome +2

Self-interacting dark matter (SIDM) has been proposed to address small-scale challenges faced by the cold dark matter (CDM) paradigm, such as the diverse density profiles observed…

astro-ph.CO2024

Supermassive black holes from inflation constrained by dark matter substructure

Shin'ichiro Ando, Shyam Balaji, Malcolm Fairbairn +2

Recent James Webb Space Telescope observations of high-redshift massive galaxy candidates have initiated renewed interest in the important mystery around the formation and evolutio…

astro-ph.SR2024

TeV Solar Gamma Rays as a probe for the Solar Internetwork Magnetic Fields

Kenny C. Y. Ng, Andrew Hillier, Shin'ichiro Ando

The magnetic fields that emerge from beneath the solar surface and permeate the solar atmosphere are the key drivers of space weather and, thus, understanding them is important to…

astro-ph.CO2024★ 11 cited

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…

hep-ph2019★ 5 cited

Smallest Halos in Thermal Wino Dark Matter

Shin'ichiro Ando, Ayuki Kamada, Toyokazu Sekiguchi +1

(Mini) split supersymmetry explains the observed Higgs mass and evades stringent constraints, while keeping good features of TeV-scale supersymmetry other than the little hierarchy…

astro-ph.CO2015★ 61 cited

Boosting the annihilation boost: Tidal effects on dark matter subhalos and consistent luminosity modeling

Richard Bartels, Shin'ichiro Ando

In the cold dark matter paradigm, structures form hierarchically, implying that large structures contain smaller substructures. These subhalos will enhance signatures of dark matte…