Formation of cosmic structure by Doppler instability

Statistics – Computation

Scientific paper

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Cosmology, Doppler Effect, Evolution (Development), Gravitational Collapse, Interstellar Gas, Astronomical Spectroscopy, Atomic Recombination, Background Radiation, Computational Astrophysics

Scientific paper

A new mechanism is described which can create an instability in homogeneous gaseous matter at very low density. When an isotropic background radiation field has, near an electronic resonance, a spectral feature for which photon occupation number increases with frequency, moving atoms increase their speed by taking energy from the photon distribution. In a cosmological setting, a sufficiently intense spectral feature can interact with neutral atomic gas, after recombination, to generate protogalactic perturbations of the scale and magnitude needed to explain large-scale cosmic structure.

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