Constraints on non-thermal Dark Matter from Planck lensing extraction
L. A. Popa, A. Vasile (Institute for Space Sciences, Bucharest,, Romania)

TL;DR
This paper demonstrates that gravitational lensing of the CMB can be used to constrain the mass of sterile neutrino dark matter, providing an alternative to traditional methods with certain advantages.
Contribution
It introduces a novel analysis of Planck CMB lensing data to set limits on sterile neutrino mass, accounting for cosmological parameter biases and non-linear effects.
Findings
Lower limit on sterile neutrino mass m_s > 2.08 keV at 95% CL
Lensing constraints are consistent with previous combined analyses
Weak lensing of CMB offers a valuable alternative for dark matter studies
Abstract
Distortions of CMB temperature and polarization anisotropy maps caused by gravitational lensing, observable with high angular resolution and sensitivity, can be used to constrain the sterile neutrino mass, offering several advantages against the analysis based on the combination of CMB, LSS and Ly\alpha forest power spectra. As the gravitational lensing effect depends on the matter distribution, no assumption on light-to-mass bias is required. In addition, unlike the galaxy clustering and Ly\alpha forest power spectra, the projected gravitational potential power spectrum probes a larger range of angular scales, the non-linear corrections being required only at very small scales. Taking into account the changes in the time-temperature relation of the primordial plasma and the modification of the neutrino thermal potential, we compute the projected gravitational potential power spectrum…
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