activity
20082021
most citedWIMPs and stellar-mass primordial black holes are incompatible

137 citations · 1.3k across the 30 of their papers we have counts for

collaborators

30 papers

hep-th2021

Inflation in a Gaussian Random Landscape

Lerh Feng Low, Richard Easther, Shaun Hotchkiss

Random, multifield functions can set generic expectations for landscape-style cosmologies. We consider the inflationary implications of a landscape defined by a Gaussian random fun…

hep-th2020★ 5 cited

The Distribution of Vacua in Random Landscape Potentials

Lerh Feng Low, Shaun Hotchkiss, Richard Easther

Landscape cosmology posits the existence of a convoluted, multidimensional, scalar potential -- the "landscape" -- with vast numbers of metastable minima. Random matrices and rando…

astro-ph.CO2019★ 60 cited

Lighting the Dark: The Evolution of the Post-Inflationary Universe

Nathan Musoke, Shaun Hotchkiss, Richard Easther

In simple inflationary cosmological scenarios the near-exponential growth can be followed by a long period in which the Universe is dominated by the oscillating inflaton condensate…

astro-ph.CO2019★ 137 cited

WIMPs and stellar-mass primordial black holes are incompatible

Julian Adamek, Christian T. Byrnes, Mateja Gosenca +1

We recently showed that postulated ultracompact minihalos with a steep density profile do not form in realistic simulations with enhanced initial perturbations. In this paper we as…

astro-ph.CO2018★ 77 cited

PyUltraLight: A Pseudo-Spectral Solver for Ultralight Dark Matter Dynamics

Faber Edwards, Emily Kendall, Shaun Hotchkiss +1

PyUltraLight simulates the dynamics of ultralight dark matter in a non-expanding background. PyUltraLight can describe the evolution of several interacting ultralight dark matter h…

astro-ph.CO2017★ 57 cited

3D simulations with boosted primordial power spectra and ultracompact minihalos

Mateja Gosenca, Julian Adamek, Christian T. Byrnes +1

We perform three-dimensional simulations of structure formation in the early Universe, when boosting the primordial power spectrum on approximately kpc scales. We demonstrate that…