CMB at 2 × 2 order: the dissipation of primordial acoustic waves and the observable part of the associated energy release

By J. Chluba, R. Khatri, R. Sunyaev. 2012

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Silk damping of primordial small scale perturbations in the photon-baryon fluid due to di ffusion of photons inevitably creates spectral distortions in the CMB. With the proposed CMB experiment PIXIE it might become possible to measure these distortions and thereby constrain the primordial power spectrum at comoving wavenumbers 50 Mpc −1 . k. 10 4 Mpc −1 . Since primordial fluctuations on these scales are completel y erased by Silk damping, these distortions may provide the only way to shed light on otherwise unobservable aspects of inflationary physics. A consistent treatment of the primordial dissipation problem requires going to second order in perturbation theory, while thermalizati on of these distortions necessitates consideration of second order in Compton scattering energy transfer. Here we give a full 2x2 treatment for creation and evolution of spectral distortio ns due to the acoustic dissipation process, consistently including the effect of polarization and photon mixing in the free streaming regime. We show that 1/3 of the total energy (9/4 larger than previous estimate) stored in small scale temperature perturbations imprints observable spectral distortions, while the remaining 2/3 only raise the average CMB temperature, an effect that is unobservable. At high redshift dissipation is mainly mediated through the quadrupole anisotropies, while after recombination peculiar motions are most important. During recombination the damping of the higher multipoles is also significant. We compute the average disto rtion for several examples using CosmoTherm, analyzing their dependence on parameters of the primordial power spectrum. For one of the best fit WMAP7 cosmologies, with nS = 1.027 and nrun =−0.034, the cooling of baryonic matter practically compensates the heating from acoustic dissipation in the µ-era. We also derive the evolution equations in first order pe rturbation theory for the spectral distortions. These first order anisotropies of spectral dis tortions may dominate over the corresponding second order contributions from recombination if an average fractional distortion of ∼ 10 −5 is already present before recombination.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/0886b17da61f703fbb0408db8a710305d6197c29

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Citations in the corpus

PRISM (Polarized Radiation Imaging and Spectroscopy Mission): an extended white paper (2013, background): “of the photon ﬂuid gives rise to CMB distortions [5,55,97,203] that depend directly on the shape and amplitude of the primordial power spectrum at scales 0:6kpc . . 1Mpc (or multipoles 105 . ‘. 108) [40,114] (see Fig.17and18for illustration). This allows constraining the trajectory of the inﬂaton at”
PROBING THE INFLATON: SMALL-SCALE POWER SPECTRUM CONSTRAINTS FROM MEASUREMENTS OF THE COSMIC MICROWAVE BACKGROUND ENERGY SPECTRUM (2012, methodology): “(4), were discussed in detail by Chluba et al. (2012), with simple analytic approximations given for different values ofnS and nrun.”