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Delos,An analytical description of substructure-induced gravitational perturbations in stellar systems,Mon

3 Pith papers cite this work. Polarity classification is still indexing.

3 Pith papers citing it

fields

astro-ph.CO 3

years

2025 3

representative citing papers

Growth of Structure in Multi-species Wave Dark Matter

astro-ph.CO · 2025-10-20 · unverdicted · novelty 7.0

Derives the power spectrum evolution and cross-spectra for arbitrary multi-species wave and particle dark matter, incorporating free-streaming, Jeans scales, and intrinsic fluctuations.

Multi-species Dark Matter with Warmth and Randomness

astro-ph.CO · 2025-10-16 · unverdicted · novelty 7.0

Presents a general analytic framework based on truncated BBGKY hierarchy solved via Volterra equations for computing power spectra in multi-species dark matter with finite velocity dispersion and Poisson fluctuations.

Early Growth of Structure in Warm Wave Dark Matter

astro-ph.CO · 2025-06-13 · conditional · novelty 6.0

Derives suppression of adiabatic perturbations and scale-dependent growth of isocurvature power in warm wave dark matter, verifies with Schrödinger-Poisson simulations, and proposes an analytic halo mass function.

citing papers explorer

Showing 3 of 3 citing papers.

  • Growth of Structure in Multi-species Wave Dark Matter astro-ph.CO · 2025-10-20 · unverdicted · none · ref 78

    Derives the power spectrum evolution and cross-spectra for arbitrary multi-species wave and particle dark matter, incorporating free-streaming, Jeans scales, and intrinsic fluctuations.

  • Multi-species Dark Matter with Warmth and Randomness astro-ph.CO · 2025-10-16 · unverdicted · none · ref 10

    Presents a general analytic framework based on truncated BBGKY hierarchy solved via Volterra equations for computing power spectra in multi-species dark matter with finite velocity dispersion and Poisson fluctuations.

  • Early Growth of Structure in Warm Wave Dark Matter astro-ph.CO · 2025-06-13 · conditional · none · ref 36

    Derives suppression of adiabatic perturbations and scale-dependent growth of isocurvature power in warm wave dark matter, verifies with Schrödinger-Poisson simulations, and proposes an analytic halo mass function.