SHARD is a collision-resolution framework that interpolates SPH results for remnants and clusters unresolved debris into N-body fragments while enforcing mass and water conservation for planet formation simulations.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.EP 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Revised mass of 0.503 M_Earth and radius of 0.736 R_Earth for GJ 367 b give a density of 6.9 g cm^{-3} and an iron fraction of 50-70% via new tidal and composition modeling.
citing papers explorer
-
Clustering SPH Debris into N-body Fragments: A Collisional Code for Planet Formation
SHARD is a collision-resolution framework that interpolates SPH results for remnants and clusters unresolved debris into N-body fragments while enforcing mass and water conservation for planet formation simulations.
-
Revisiting the Exo-Mercury Candidate GJ 367 b with ESPRESSO and a Self-Consistent Tidal Distortion Model
Revised mass of 0.503 M_Earth and radius of 0.736 R_Earth for GJ 367 b give a density of 6.9 g cm^{-3} and an iron fraction of 50-70% via new tidal and composition modeling.