%0 Generic %1 Hu1995 %A Hu, Wayne %A Sugiyama, Naoshi %D 1995 %K Anisotropies CMB %T Small Scale Cosmological Perturbations: An Analytic Approach %U http://arxiv.org/abs/astro-ph/9510117 %X Through analytic techniques verified by numerical calculations, we establish general relations between the matter and cosmic microwave background (CMB) power spectra and their dependence on cosmological parameters on small scales. Fluctuations in the CMB, baryons, cold dark matter (CDM), and neutrinos receive a boost at horizon crossing. Baryon drag on the photons causes alternating acoustic peak heights in the CMB and is uncovered in its bare form under the photon diffusion scale. Decoupling of the photons at last scattering and of the baryons at the end of the Compton drag epoch, freezes the diffusion-damped acoustic oscillations into the CMB and matter power spectra at different scales. We determine the dependence of the respective acoustic amplitudes and damping lengths on fundamental cosmological parameters. The baryonic oscillations, enhanced by the velocity overshoot effect, compete with CDM fluctuations in the present matter power spectrum. We present new exact analytic solutions for the cold dark matter fluctuations in the presence of a growth- inhibiting radiation and baryon background. Combined with the acoustic contributions and baryonic infall into CDM potential wells, this provides a highly accurate analytic form of the small-scale transfer function in the general case.

@misc{Hu1995, abstract = { Through analytic techniques verified by numerical calculations, we establish general relations between the matter and cosmic microwave background (CMB) power spectra and their dependence on cosmological parameters on small scales. Fluctuations in the CMB, baryons, cold dark matter (CDM), and neutrinos receive a boost at horizon crossing. Baryon drag on the photons causes alternating acoustic peak heights in the CMB and is uncovered in its bare form under the photon diffusion scale. Decoupling of the photons at last scattering and of the baryons at the end of the Compton drag epoch, freezes the diffusion-damped acoustic oscillations into the CMB and matter power spectra at different scales. We determine the dependence of the respective acoustic amplitudes and damping lengths on fundamental cosmological parameters. The baryonic oscillations, enhanced by the velocity overshoot effect, compete with CDM fluctuations in the present matter power spectrum. We present new exact analytic solutions for the cold dark matter fluctuations in the presence of a growth- inhibiting radiation {\it and} baryon background. Combined with the acoustic contributions and baryonic infall into CDM potential wells, this provides a highly accurate analytic form of the small-scale transfer function in the general case. }, added-at = {2011-04-27T18:10:31.000+0200}, author = {Hu, Wayne and Sugiyama, Naoshi}, biburl = {https://www.bibsonomy.org/bibtex/23ed7e44013967b967cf4197a91f77a01/ad4}, description = {Small Scale Cosmological Perturbations: An Analytic Approach}, interhash = {374920a42da392ab4e671a8c89daa898}, intrahash = {3ed7e44013967b967cf4197a91f77a01}, keywords = {Anisotropies CMB}, note = {cite arxiv:astro-ph/9510117 Comment: Revised accepted version; no changed results but several minor typos corrected; index & other roadmaps added. TeX + 20 Figs}, timestamp = {2011-04-27T18:10:31.000+0200}, title = {Small Scale Cosmological Perturbations: An Analytic Approach}, url = {http://arxiv.org/abs/astro-ph/9510117}, year = 1995 }