activity
20062023
most citedNonperturbative Dynamics Of Reheating After Inflation: A Review

503 citations · 5.3k across the 71 of their papers we have counts for

collaborators

73 papers

astro-ph.CO2023★ 31 cited

Kinetic relaxation and Bose-star formation in multicomponent dark matter- I

Mudit Jain, Mustafa A. Amin, Jonathan Thomas +1

Using wave kinetics, we estimate the emergence time-scale of gravitating Bose-Einstein condensates/Bose stars in the kinetic regime for a general multicomponent Schrödinger-Poisson…

astro-ph.CO2023★ 1 cited

A novel integrated Sachs-Wolfe effect from Early Dark Energy

Tristan L. Smith, John T. Giblin, Mustafa A. Amin +4

We study the nonlinear effects of minimally coupled, massless, cosmological scalar fields on the cosmic microwave background (CMB). These fields can exhibit post-recombination para…

astro-ph.CO2023★ 44 cited

Cosmological Structure Formation and Soliton Phase Transition in Fuzzy Dark Matter with Axion Self-Interactions

Philip Mocz, Anastasia Fialkov, Mark Vogelsberger +11

We investigate cosmological structure formation in Fuzzy Dark Matter (FDM) with an attractive self-interaction (SI) with numerical simulations. Such a SI would arise if the FDM bos…

hep-ph2023★ 21 cited

Photons from dark photon solitons via parametric resonance

Mustafa A. Amin, Andrew J. Long, Enrico D. Schiappacasse

Wave-like dark matter made of spin-1 particles (dark photons) is expected to form ground state clumps called "vector solitons", which can have different polarizations. In this work…

astro-ph.CO2022★ 16 cited

i-SPin: An integrator for multicomponent Schrödinger-Poisson systems with self-interactions

Mudit Jain, Mustafa A. Amin

We provide an algorithm and a publicly available code to numerically evolve multicomponent Schrödinger-Poisson (SP) systems with a SO() symmetry, including attractive or repulsi…

hep-ph2022★ 4 cited

A lower bound on dark matter mass

Mustafa A. Amin, Mehrdad Mirbabayi

We argue that there is a lower bound of order eV on dark matter mass if it is produced after inflation via a process with finite correlation length. We rely on non-detec…