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arXiv · 1108.0639

The magnitude of the non-adiabatic pressure in the cosmic fluid

Iain A. Brown·Adam J. Christopherson·Karim A. Malik
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Abstract

Understanding the non-adiabatic pressure, or relative entropy, perturbation is crucial for studies of early-universe vorticity and Cosmic Microwave Background observations. We calculate the evolution of the linear non-adiabatic pressure perturbation from radiation domination to late times, numerically solving the linear governing equations for a wide range of wavenumbers. Using adiabatic initial conditions consistent with WMAP seven year data, we find nevertheless that the non-adiabatic pressure perturbation is non-zero and grows at early times, peaking around the epoch of matter/radiation equality and decaying in matter domination. At early times or large redshifts (z=10,000) its power spectrum peaks at a comoving wavenumber k~0.2h/Mpc, while at late times (z=500) it peaks at k~0.02 h/Mpc.

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Iain A. Brown, Adam J. Christopherson, Karim A. Malik. 2012-07-09. The magnitude of the non-adiabatic pressure in the cosmic fluid. https://doi.org/10.1111/j.1365-2966.2012.20966.x

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