Near universality of nonlinear transverse and radial velocity responses in spherical collapse with arbitrary radial profiles
astro-ph.CO, gr-qc
Submitted: 2026-08-27
Updated: 2026-08-27
Terminology
Sources
- Weakly Nonlinear Density-Velocity Relation
- Cosmological Perturbation Theory and the Spherical Collapse model - III. The Velocity divergence field and the $\Omega$ dependence
- The velocity-density relation in the spherical model
- Non-linear density-velocity divergence relation from phase space dynamics
- Two is better than one: joint statistics of density and velocity in concentric spheres as a cosmological probe
- Cosmic variance and the measurement of the local Hubble parameter
- Quasi-local variables in spherical symmetry: numerical applications to dark matter and dark energy sources
- Weighed scalar averaging in LTB dust models, part I: statistical fluctuations and gravitational entropy
- Weighed scalar averaging in LTB dust models, part II: a formalism of exact perturbations
- Invariant characterization of the growing and decaying density modes in LTB dust models
- On spherical dust fluctuations: the exact vs. the perturbative approach
- The BEHOMO project: $\Lambda$LTB $N$-body simulations
- Complete solutions to the metric of spherically collapsing dust in an expanding spacetime with a cosmological constant
- On Separate Universes
- Scalar Perturbations on Lemaitre-Tolman-Bondi Spacetimes
- The $\Omega$ Dependence in the Equations of Motion
- Phase Space dynamics of triaxial collapse: Joint density-velocity evolution
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