Evolution from Spherically Symmetric Primordial Overdensities
Using the standard cosmological parameters for λ-CDM Cosmology and adiabatic model, we show three animations:
(a) Spatial Mass Profile and Velocity Evolution
(b) Spatial Mass Profile Evolution
(c) Baryon, CDM and Drift Velocity Fluctuation Power Spectrum Evolution
for each of the following perturbations:
1. Point-like Perturbation
2. 1 Mpc Radius Top-hat Perturbation
3. 10 Mpc Radius Top-hat Perturbation
4. 20 Mpc Radius Top-hat Perturbation
5. 60 Mpc Radius Top-hat Perturbation
We also show the Baryon, CDM and Drift Velocity Power Spectrum for PLANCK primordial power spectrum
Note: The mass profile scale is arbitrary, but are correctly scaled between the panels for synchronous gauge. The amplitude of all the initial perturbations have been normalized such that the density-rms is same as that for the PLANCK primordial power spectrum at the redshift of 50,000 . For details on the proportionality of amplitude of perturbation with the power spectrum, mass profile and velocity profile click here .
1. Point-like Perturbation
(a) Spatial Mass Profile and Velocity Evolution
Video also available here . (mp4)
(b) Spatial Mass Profile Evolution
Video also available here . (mp4)
(c) Baryon, CDM and Drift Velocity Fluctuation Power Spectrum Evolution
Video also available here . (mp4)
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2. 1 Mpc Radius Top-hat Perturbation
(a) Spatial Mass Profile and Velocity Evolution
Video also available here . (mp4)
(b) Spatial Mass Profile Evolution
Video also available here . (mp4)
(c) Baryon, CDM and Drift Velocity Fluctuation Power Spectrum Evolution
Video also available here . (mp4)
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3. 10 Mpc Radius Top-hat Perturbation
(a) Spatial Mass Profile and Velocity Evolution
Video also available here . (mp4)
(b) Spatial Mass Profile Evolution
Video also available here . (mp4)
(c) Baryon, CDM and Drift Velocity Fluctuation Power Spectrum Evolution
Video also available here . (mp4)
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4. 20 Mpc Radius Top-hat Perturbation
(a) Spatial Mass Profile and Velocity Evolution
Video also available here . (mp4)
(b) Spatial Mass Profile Evolution
Video also available here . (mp4)
(c) Baryon, CDM and Drift Velocity Fluctuation Power Spectrum Evolution
Video also available here . (mp4)
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5. 60 Mpc Radius Top-hat Perturbation
(a) Spatial Mass Profile and Velocity Evolution
Video also available here . (mp4)
(b) Spatial Mass Profile Evolution
Video also available here . (mp4)
(c) Baryon, CDM and Drift Velocity Fluctuation Power Spectrum Evolution
Video also available here . (mp4)
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6. Velocity Power Spectrum for Planck primordial power spectrum
Video also available here . (mp4)