activity
20182026
most citedSWIFT: A modern highly-parallel gravity and smoothed particle hydrodynamics solver for astrophysical and cosmological applications

106 citations · 473 across the 19 of their papers we have counts for

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11 papers · 1 filter

astro-ph.EP2025

Atmospheric loss during giant impacts: mechanisms and scaling of near- and far-field loss

Matthew J. Roche, Simon J. Lock, Jingyao Dou +3

The primary epoch of planetary accretion concludes with giant impacts - highly energetic collisions between proto-planets that can play a key role in shaping a planet's inventory o…

astro-ph.EP2024★ 2 cited

No dilute core produced in simulations of giant impacts on to Jupiter

T. D. Sandnes, V. R. Eke, J. A. Kegerreis +2

A giant impact has been proposed as a possible formation mechanism for Jupiter's dilute core -- the planet's inferred internal structure in which the transition between its core of…

astro-ph.EP2024★ 12 cited

Origin of Mars's moons by disruptive partial capture of an asteroid

Jacob A. Kegerreis, Jack J. Lissauer, Vincent R. Eke +2

The origin of Mars's small moons, Phobos and Deimos, remains unknown. They are typically thought either to be captured asteroids or to have accreted from a debris disk produced by…

astro-ph.EP2023★ 29 cited

A recent impact origin of Saturn's rings and mid-sized moons

Luís F. A. Teodoro, Jacob A. Kegerreis, Paul R. Estrada +5

We simulate the collision of precursor icy moons analogous to Dione and Rhea as a possible origin for Saturn's remarkably young rings. Such an event could have been triggered a few…

astro-ph.EP2022★ 35 cited

Immediate origin of the Moon as a post-impact satellite

Jacob A. Kegerreis, Sergio Ruiz-Bonilla, Vincent R. Eke +3

The Moon is traditionally thought to have coalesced from the debris ejected by a giant impact onto the early Earth. However, such models struggle to explain the similar isotopic co…

astro-ph.EP2022★ 2 cited

Dealing with density discontinuities in planetary SPH simulations

Sergio Ruiz-Bonilla, Josh Borrow, Vincent R. Eke +4

Density discontinuities cannot be precisely modelled in standard formulations of smoothed particles hydrodynamics (SPH) because the density field is defined smoothly as a kernel-we…

astro-ph.EP2020★ 23 cited

The effect of pre-impact spin on the Moon-forming collision

Sergio Ruiz-Bonilla, Vincent R. Eke, Jacob A. Kegerreis +2

We simulate the hypothesised collision between the proto-Earth and a Mars-sized impactor that created the Moon. Amongst the resulting debris disk in some impacts, we find a self-gr…

astro-ph.EP2020★ 38 cited

Atmospheric Erosion by Giant Impacts onto Terrestrial Planets: A Scaling Law for any Speed, Angle, Mass, and Density

Jacob A. Kegerreis, Vincent R. Eke, David C. Catling +3

We present a new scaling law to predict the loss of atmosphere from planetary collisions for any speed, angle, impactor mass, target mass, and body compositions, in the regime of g…

astro-ph.EP2020★ 39 cited

Atmospheric Erosion by Giant Impacts onto Terrestrial Planets

J. A. Kegerreis, V. R. Eke, R. J. Massey +1

We examine the mechanisms by which atmosphere can be eroded by giant impacts onto Earth-like planets with thin atmospheres, using 3D smoothed particle hydrodynamics simulations wit…

astro-ph.EP2019★ 50 cited

Planetary Giant Impacts: Convergence of High-Resolution Simulations using Efficient Spherical Initial Conditions and SWIFT

J. A. Kegerreis, V. R. Eke, P. G. Gonnet +4

We perform simulations of giant impacts onto the young Uranus using smoothed particle hydrodynamics (SPH) with over 100 million particles. This 100--1000 improvement in par…

astro-ph.EP2018★ 73 cited

Consequences of Giant Impacts on Early Uranus for Rotation, Internal Structure, Debris, and Atmospheric Erosion

J. A. Kegerreis, L. F. A. Teodoro, V. R. Eke +6

We perform a suite of smoothed particle hydrodynamics simulations to investigate in detail the results of a giant impact on the young Uranus. We study the internal structure, rotat…