collaborators

6 papers

astro-ph.CO2026

Cosmological discrete self-similarity in primordial black hole formation

Luis E. Padilla, Tomohiro Harada, Ethan Milligan +1

We demonstrate that discrete self-similarity (DSS), originally discovered in the collapse of a massless scalar field in an asymptotically flat system, survives in primordial black…

astro-ph.CO2026

Decoupling of large-scale, adiabatic inflationary perturbations from enhanced small-scale modes at one-loop

Laura Iacconi, David Mulryne, David Seery

We reconsider back-reaction from large amplitude, short-scale perturbations onto a long wavelength adiabatic mode. In a loop expansion of the long-mode power spectrum, this back-re…

astro-ph.CO2025

Primordial Black Hole Formation in a Scalar Field Dominated Universe: Investigation of the Critical nature of the Collapse

Luis E. Padilla, Ethan Milligan, David J. Mulryne +1

In this paper, we investigate the critical collapse leading to primordial black hole (PBH) formation in a universe dominated by a self-interacting scalar field with a quartic poten…

astro-ph.CO2025

Suppression of the induced gravitational wave background due to third-order perturbations

Raphael Picard, Luis E. Padilla, Karim A. Malik +1

In this work, we revisit and evaluate new source terms which contribute to the induced gravitational wave background. We study their respective contributions to the stochastic grav…

astro-ph.CO2025

Primordial Black Hole Formation in a Scalar Field Dominated Universe

Ethan Milligan, Luis E. Padilla, David J. Mulryne +1

We present a numerical code that solves the Misner-Sharp system for a spherically symmetric cosmological model containing both a scalar field and a perfect fluid. While the code is…

astro-ph.CO2025

Primordial correlators from multi-point propagators

Andrea Costantini, Laura Iacconi, David J. Mulryne

A key step in the comparison between inflationary predictions and cosmological observations is the computation of primordial correlators. Numerical methods have been developed that…