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Cosmic neutrino background: a minireview

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Abstract

The standard model of cosmology, i.e., the big bang theory, along with cosmic microwave background (CMB), also predicts the existence of a cosmic neutrino background (C\(\nu \)B). This C\(\nu \)B is comprised of ultra low energy neutrinos. Their detection can provide us the information about the Universe at a stage earlier than the CMB can provide. In this short review, we present basic theoretical properties and constraints on C\(\nu \)B and subsequently present a quick review of the experimental proposals for its detection. In addition to this, we also discuss the effect of generalized neutrino interactions on the C\(\nu \)B detection via the neutrino capture process at PTOLEMY.

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This manuscript has no associated data or the data will not be deposited. [Authors’ comment: This is a theoretical study and no experimental data has been used.]

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Acknowledgements

UKD thanks I K Banerjee for useful discussions. A clarifying comment from the anonymous referee is also acknowledged.

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  1. Department of Physical Sciences, Indian Institute of Science Education and Research Berhampur, Transit Campus, Govt. ITI, Engg. School Junction, Berhampur, Odisha, 760010, India

    Ujjal Kumar Dey

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Dey, U.K. Cosmic neutrino background: a minireview. Eur. Phys. J. Spec. Top. (2024). https://doi.org/10.1140/epjs/s11734-024-01101-w

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