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20242026
most citedStochastic Inflation in Numerical Relativity

2 citations · 2 across the 1 of their papers we have counts for

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9 papers

gr-qc20262 cited

Stochastic Inflation in Numerical Relativity

Yoann L. Launay, Gerasimos I. Rigopoulos, E. Paul S. Shellard

A set of 3+1 equations for stochastic inflation incorporating all metric and scalar matter degrees of freedom, first presented in previous work, are re-derived in a gauge invariant…

gr-qc2026

Inflaton perturbations through an Ultra-Slow Roll transition and Hamilton-Jacobi attractors

Tomislav Prokopec, Gerasimos Rigopoulos

We examine the behaviour of the gauge invariant scalar field perturbations in an analytic inflationary model that transitions from slow-roll to an ultra-slow-roll (USR) phase. We f…

astro-ph.CO2026

Dynamical reconstruction of SPARC galactic halos within self-interacting fuzzy dark matter

Milos Indjin, I-Kang Liu, Nick P. Proukakis +2

Fuzzy Dark Matter with non-zero quartic self-interaction (SFDM) is shown to be a viable model for simultaneously fitting 17 dark-matter-dominated galaxies from the SPARC database w…

astro-ph.CO2025

Fuzzy dark matter halos with repulsive self-interactions: coherent soliton and halo vortex network with moderate self-coupling

Milos Indjin, Nick Keepfer, I-Kang Liu +2

We examine the impact of moderate repulsive self-interactions on fuzzy dark matter halos generated by merging smaller Gaussian density concentrations. We study the size of the core…

cond-mat.quant-gas2025

Dynamical Dipolar Condensate Finite Temperature Stochastic Gross--Pitaevskii--Boltzmann Model

Nick P. Proukakis, Gerasimos Rigopoulos, Alex Soto

We formulate a generalized self-consistent stochastic quantum kinetic theory for finite-temperature ultracold Bose gases interacting via a generic long-range interaction, applicabl…

gr-qc2025

Bunch-Davies initial conditions and non-perturbative inflationary dynamics in Numerical Relativity

Yoann L. Launay, Gerasimos I. Rigopoulos, E. Paul S. Shellard

We show that it is possible to simulate realistic inhomogeneities during cosmological inflation with high precision using {Numerical Relativity}. Stochastic initial conditions are…