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.
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3 Pith papers cite this work. Polarity classification is still indexing.
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UNVERDICTED 3representative citing papers
Simulations tie the deep-mantle primordial neon reservoir to an initial embryo mass of ~0.3 Earth masses assembled during solar-nebula dispersal.
Multi-technique observations constrain the configuration of the ξ Tau system, detecting orbital oscillations on multiple timescales and suggesting component C is itself a binary.
citing papers explorer
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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.
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Constructing Earth Formation History Using Deep Mantle Noble Gas Reservoirs
Simulations tie the deep-mantle primordial neon reservoir to an initial embryo mass of ~0.3 Earth masses assembled during solar-nebula dispersal.
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Configuration of the $\xi$ Tau system constrained by multi-technique observations
Multi-technique observations constrain the configuration of the ξ Tau system, detecting orbital oscillations on multiple timescales and suggesting component C is itself a binary.