activity
20122023
most citedLong-lived transient structure in collisionless self-gravitating systems

18 citations · 120 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.CO2023

Testing growth rate dependence in cosmological perturbation theory using scale-free models

Azrul Pohan, Michael Joyce, David Benhaiem +1

We generalize previously derived analytic results for the one-loop power spectrum (PS) in scale-free models (with linear PS ) to a broader class of such models in…

astro-ph.GA2019★ 18 cited

Long-lived transient structure in collisionless self-gravitating systems

David Benhaiem, Francesco Sylos Labini, Michael Joyce

The evolution of self-gravitating systems, and long-range interacting systems more generally, from initial configurations far from dynamical equilibrium is often described as a sim…

astro-ph.GA2018★ 11 cited

Nonaxisymmetric models of galaxy velocity maps

Francesco Sylos Labini, David Benhaiem, Sebastien Comeron +1

Galaxy velocity maps often show the typical pattern of a rotating disk, consistent with the dynamical model where emitters rotate in circular orbits around the galactic center. The…

astro-ph.GA2017★ 16 cited

Transient spiral arms from far out of equilibrium gravitational evolution

David Benhaiem, Michael Joyce, Francesco Sylos Labini

We describe how a simple class of out of equilibrium, rotating and asymmetrical mass distributions evolve under their self-gravity to produce a quasi-planar spiral structure surrou…

astro-ph.CO2017★ 9 cited

Particle number dependence in the non-linear evolution of N-body self-gravitating systems

David Benhaiem, Michael Joyce, Francesco Sylos Labini +1

Simulations of purely self-gravitating N-body systems are often used in astrophysics and cosmology to study the collisionless limit of such systems. Their results for macroscopic q…

astro-ph.GA2016★ 5 cited

Formation of satellites from cold collapse

David Benhaiem, Francesco Sylos Labini

We study the collapse of an isolated, initially cold, irregular (but almost spherical) and (slightly) inhomogeneous cloud of self-gravitating particles. The cloud is driven towards…