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arXiv:2104.03329·v2·Cosmology and Nongalactic Astrophysics

Non-thermal neutrino-like hot dark matter in light of the tension

Subinoy Das🇮🇳 · Anshuman Maharana🇮🇳 · Vivian Poulin🇫🇷 · Ravi Kumar Sharma🇮🇳

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Abstract

The CDM prediction of -- where is the root mean square of matter fluctuations on a 8 Mpc scale -- once calibrated on Planck CMB data is lower than its direct estimate by a number of weak lensing surveys. In this paper, we explore the possibility that the '-tension' is due to a non-thermal hot dark matter (HDM) fractional contribution to the universe energy density leading to a power suppression at small-scales in the matter power spectrum. Any HDM models can be characterized by its effective mass and its contribution to the relativistic degrees of freedom at CMB decoupling . Taking the specific example of a sterile particle produced from the decay of the inflaton during a matter dominated era, we find that from Planck only the tension can be reduced below , but Planck does not favor a non-zero . In combination with a measurement of from KIDS1000+BOSS+2dfLenS, the -tension would hint at the existence of a particle of mass with a contribution to . However, Pantheon and BOSS BAO/ data restricts the particle mass to and contribution to . We discuss implications of our results for other canonical non-thermal HDM models -- the Dodelson-Widrow model and a thermal sterile particle with a different temperature in the hidden sector. We report competitive results on such hidden sector temperature which might have interesting implications for particle physics model building, in particular connecting the -tension to the longstanding short baseline oscillation anomaly.

Comments: accepted Physical Review D, new figures, references and discussion added conclusion is same

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