activity
20022026
most citedHigh Performance Direct Gravitational N-body Simulations on Graphics Processing Units -- II: An implementation in CUDA

210 citations · 678 across the 40 of their papers we have counts for

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Showing astro-ph.EPShow all

13 papers · 1 filter

astro-ph.EP2026

Star Cluster Ecology VIII. -- Dynamically Forming S-Type and Centauri-like Systems

Erwan Hochart, Simon Portegies Zwart

Aims: To analyse the impact of dynamically formed binaries emerging naturally from various star cluster environments on already established planetary systems. Methods: Numerical si…

astro-ph.EP2026

Planet-moon ejections in close stellar encounters

Yannick Badoux, Simon Portegies Zwart

Free-floating planet-moon pairs (FFPMs) may form when planetary systems experience close stellar encounters. We quantify moon-retention probabilities and ejection cross sections fo…

astro-ph.EP2026

Oort Cloud Ecology -- IV. Exchanging Asteroids

Erwan Hochart, Simon Portegies Zwart

Aims. Investigate the influence of cluster environments on asteroids, with special attention towards captured material. Methods. Using numerical methods, a sub-virial fractally dis…

astro-ph.EP2025

A Systematic North-South asymmetry in the Steady-state Climate of rapidly-rotating Oblique Water Worlds

Y Wu, S. Portegies Zwart, H Dijkstra

Planetary obliquity (axial tilt) plays an important role in regulating the climate evolution and habitability of water-covered planets. Despite the suspicion of large obliquities i…

astro-ph.EP2025

A Resonant Beginning for the Solar System Terrestrial Planets

Shuo Huang, Chris Ormel, Simon Portegies Zwart +2

In the past two decades, transit surveys have revealed a class of planets with thick atmospheres -- sub-Neptunes -- that must have completed their accretion in protoplanet disks. W…

astro-ph.EP2025★ 1 cited

Stability of a cluster-disrupted mean-motion resonance (chain) in HR 8799 and PDS 70

Brent Maas, Shuo Huang, Simon Portegies Zwart

HR~8799 is a planetary system with four planets potentially in a mean-motion resonance chain. It is unclear from the observations if they are in mean-motion resonance. Similarly, P…

astro-ph.EP2025★ 3 cited

Oort Cloud Ecology. III. The Sun left the parent star cluster shortly after the giant planets formed

Simon Portegies Zwart, Shuo Huang

The Sun was born in a clustered environment with 10,000 other stars. Being an isolated star today, the Sun must have left the nest. We do not directly know when that happened, how…

astro-ph.EP2024

He awa whiria: the tidal streams of interstellar objects

John C. Forbes, Michele T. Bannister, Chris Lintott +5

Upcoming surveys are likely to discover a new sample of interstellar objects (ISOs) within the Solar System, but questions remain about the origin and distribution of this populati…

astro-ph.EP2024★ 6 cited

On the origin of transition disk cavities: Pebble-accreting protoplanets vs Super-Jupiters

Shuo Huang, Nienke van der Marel, Simon Portegies Zwart

Protoplanetary disks surrounding young stars are the birth places of planets. Among them, transition disks with inner dust cavities of tens of au are sometimes suggested to host ma…

astro-ph.EP2024★ 14 cited

On the suppression of giant planet formation around low-mass stars in clustered environments

Shuo Huang, Simon Portegies Zwart, Maite J. C. Wilhelm

Context: Current exoplanet formation studies tend to overlook the birth environment of stars in clustered environments. The effect of this environment on the planet-formation proce…

astro-ph.EP2024★ 12 cited

Isles of regularity in a sea of chaos amid the gravitational three-body problem

Alessandro Alberto Trani, Nathan W. C. Leigh, Tjarda C. N. Boekholt +1

The three-body problem (3BP) poses a longstanding challenge in physics and celestial mechanics. Despite the impossibility of obtaining general analytical solutions, statistical the…

astro-ph.EP2023★ 6 cited

A hybrid approach for solving the gravitational N-body problem with Artificial Neural Networks

Veronica Saz Ulibarrena, Philipp Horn, Simon Portegies Zwart +3

Simulating the evolution of the gravitational N-body problem becomes extremely computationally expensive as N increases since the problem complexity scales quadratically with the n…

astro-ph.EP2018★ 42 cited

The Formation of Solar System Analogs in Young Star Clusters

Simon Portegies Zwart

The Solar system was once rich in the short-lived radionuclide (SLR) Al\, but deprived in Fe. Several models have been proposed to explain these anomalous abundances…