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20112026
most citedDisruption of Dark Matter Substructure: Fact or Fiction?

317 citations · 1.2k across the 32 of their papers we have counts for

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Showing astro-ph.COShow all

9 papers · 1 filter

astro-ph.CO2026

Dynamical evolution of dark matter subhaloes in the Milky Way: role of the Galactic disc

Junnan Shen, Go Ogiya, Jens Stücker

Dark matter (DM) subhaloes orbiting inside the Milky Way (MW) are promising targets for DM searches, and reliable predictions for the detectability and spatial distribution of thei…

astro-ph.CO2023★ 14 cited

Examining the effects of dark matter spikes on eccentric intermediate mass ratio inspirals using N-body simulations

Diptajyoti Mukherjee, A. Miguel Holgado, Go Ogiya +1

Recent studies suggest that dark matter (DM) spikes around intermediate-mass black holes could cause observable dephasing in gravitational wave (GW) signals from Intermediate Mass…

astro-ph.CO2023★ 15 cited

The effect of stellar encounters on the dark matter annihilation signal from prompt cusps

Jens Stücker, Go Ogiya, Simon D. M. White +1

Prompt cusps are the densest quasi-equilibrium dark matter objects; one forms at the instant of collapse within every isolated peak of the initial cosmological density field. They…

astro-ph.CO2022★ 33 cited

Tidal Stripping in the Adiabatic Limit

Jens Stücker, Go Ogiya, Raul E. Angulo +2

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 tha…

astro-ph.CO2017★ 45 cited

What sets the central structure of dark matter haloes?

Go Ogiya, Oliver Hahn

Dark matter (DM) haloes forming near the thermal cut-off scale of the density perturbations are unique, since they are the smallest objects and form through monolithic gravitationa…

astro-ph.CO2016★ 41 cited

Dynamical Evolution of Primordial Dark Matter Haloes through Mergers

Go Ogiya, Daisuke Nagai, Tomoaki Ishiyama

Primordial dark matter (DM) haloes are the smallest gravitationally bound DM structures from which the first stars, black holes, and galaxies form and grow in the early universe. H…

astro-ph.CO2013★ 26 cited

The connection between the cusp-to-core transformation and observational universalities of DM halos

Go Ogiya, Masao Mori, Tomoaki Ishiyama +1

Observations have revealed interesting universal properties of dark matter (DM) halos especially around low-mass galaxies. Strigari et al. (2008) showed that DM halos have common e…

astro-ph.CO2012★ 59 cited

The Core-Cusp Problem in Cold Dark Matter Halos and Supernova Feedback: Effects of Oscillation

Go Ogiya, Masao Mori

This study investigates the dynamical response of dark matter (DM) halos to recurrent starbursts in forming less-massive galaxies to solve the core-cusp problem. The gas, which is…

astro-ph.CO2011★ 44 cited

The core-cusp problem in cold dark matter halos and supernova feedback: Effects of Mass Loss

Go Ogiya, Masao Mori

The core-cusp problem remains as one of the unsolved discrepancies between observations and theories predicted by the standard paradigm of cold dark matter (CDM) cosmology. To solv…