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The streaming velocity damps density perturbations on the acoustic oscillation scale at recombination, i.e. in the range (simeq5mbox100mbox { Mpc}).
Crayfish did not have any influence on the survival rate of trout, which was positively related to streaming velocity instead.
After recombination, the effective sound speed drops to that of a gas with a temperature of ({sim}10^{4}mbox { K}), such that the streaming velocity becomes supersonic.
As the streaming velocity is increased, the halos retain less gas, the central gas density is reduced, and less gas is able to cool and form stars.
Following recombination, the relative velocity decreases (propto a^{-1}), such that at (zgtrsim 20) the streaming velocity is close to (1mbox { km}mbox { s}^{-1}).
The transparent SAW devices have also demonstrated their ability to induce a strong acoustic streaming in a water droplet with a streaming velocity up to 2.27 cm/s.
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These include HD cooling, cosmic rays, streaming velocities, DM annihilation, and alternative cosmologies.
I also discuss the influence of additional physical processes, such as magnetic fields and streaming velocities.
Figure 8 Baryonic mass available for star formation in minihalos in a cosmological simulation that includes streaming velocities.
Similarly, Tanaka and Li (2014) suggest that streaming velocities may suppress halo collapse and molecule formation until the atomic cooling threshold is surpassed.
Since the streaming velocities are sourced by acoustic oscillations before recombination, this leads to a modulation of Population III star formation on ({simeq}10mbox100mbox { Mpc}) scales.
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