activity
20242026
most citedCompaction during fragmentation and bouncing produces realistic dust grain porosities in protoplanetary discs

17 citations · 19 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2026

Virial-based extraction of structures in numerical simulations: The vibes tool

Simon Chevalier, Fabien Louvet, Yann Bernard +9

The processes that determine the stellar initial mass function (IMF) and its connection to the core mass function (CMF) are among the major open questions in star formation. The de…

astro-ph.IM2026

Momentum-conserving self-gravity in the Phantom. Parallel dual tree traversal for the fast multipole method

Yann Bernard, Timothée David-Cléris, Daniel J. Price +1

Tree codes that approximate groups of distant particles with multipole expansions accelerate gravitational force calculations. While momentum-conserving fast multipole methods exis…

astro-ph.GA2025★ 2 cited

DAWN. I. Simulating the formation and early evolution of stellar clusters with Phantom N-Body

Yann Bernard, Estelle Moraux, Daniel J. Price +3

Context. Simulating stellar dynamics in a molecular cloud environment is numerically challenging due to the strong coupling between young stars and their surrounding gas, and the l…

astro-ph.IM2024

On shock capturing in smoothed particle hydrodynamics

Daniel J. Price

For the past 20 years, our approach to shock capturing in smoothed particle hydrodynamics (SPH) has been to use artificial viscosity and conductivity terms supplemented by switches…

astro-ph.EP2024★ 17 cited

Compaction during fragmentation and bouncing produces realistic dust grain porosities in protoplanetary discs

Stéphane Michoulier, Jean-François Gonzalez, Daniel J. Price

Context: In protoplanetary discs, micron-sized dust grows to form millimetre- to centimetre-sized pebbles but encounters several barriers during its evolution. Collisional fragment…

astro-ph.HE2024

Decretion disc size in Be/X-ray binaries depends upon the disc aspect ratio

Rebecca G. Martin, Stephen H. Lubow, Philip J. Armitage +1

With three-dimensional hydrodynamical simulations we show that the size of the decretion disc and the structure of the accretion flow onto the neutron star in a Be/X-ray binary str…