A new algorithm traces filament evolution in simulations and finds suppressed halo mass accretion plus non-random spin alignment changes near dense filaments.
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2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
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astro-ph.CO 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Galaxy properties in IllustrisTNG form a continuum across the multiscale caustic skeleton, with formation time of web components influencing colors and star formation activity.
citing papers explorer
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The impact of evolving cosmic filaments on mass and spin evolution of dark matter halos
A new algorithm traces filament evolution in simulations and finds suppressed halo mass accretion plus non-random spin alignment changes near dense filaments.
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Galaxy Populations in the IllustrisTNG Caustic Skeleton
Galaxy properties in IllustrisTNG form a continuum across the multiscale caustic skeleton, with formation time of web components influencing colors and star formation activity.