Severe gas expulsion and expansion in a primordial star cluster, combined with a top-heavy IMF, can reproduce the high velocity dispersion and broad stream of C-19 without dark matter subhalos.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
representative citing papers
The authors reformulate frictionless smooth rigid-body contact as an adaptively augmented ReLCP that enforces nonpenetration directly on smooth geometry, with termination proofs for convex bodies and reduction to classical SNSD LCP at small timesteps.
Catastrophic disruption of differentiated asteroids creates a sheet-like mix of core and mantle fragments with uniform iron-rock ratios that reaccumulate into iron-rich rubble piles if the core is molten.
citing papers explorer
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The formation of the C-19 progenitor: a primordial cluster heated by gas expulsion
Severe gas expulsion and expansion in a primordial star cluster, combined with a top-heavy IMF, can reproduce the high velocity dispersion and broad stream of C-19 without dark matter subhalos.
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Smooth-Rigid-Body Contact as a ReLCP: A Recursively Generated Linear Complementarity Problem
The authors reformulate frictionless smooth rigid-body contact as an adaptively augmented ReLCP that enforces nonpenetration directly on smooth geometry, with termination proofs for convex bodies and reduction to classical SNSD LCP at small timesteps.
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Reaccumulation process after a catastrophic disruption event on a differentiated asteroid
Catastrophic disruption of differentiated asteroids creates a sheet-like mix of core and mantle fragments with uniform iron-rock ratios that reaccumulate into iron-rich rubble piles if the core is molten.