A Dark Matter Signature for Condensed Neutrinos

TL;DR

This paper proposes that condensed neutrino objects could be the primary source of dark matter, and suggests a potential weak signature detectable through weak lensing and Sunyaev-Zel'dovich data.

Contribution

It introduces the concept of CNOs as dark matter candidates and demonstrates a method to detect their weak signature using specific observational data.

Findings

Potential weak CNO signature detected

Weak lensing and SZ data can be used for detection

Supports neutrino-based dark matter models

Abstract

We derive the signature for condensed neutrino objects (CNOs) as the primary source of Dark Matter. Restricting our source data to minimize systematic errors, we find that by just using weak lensing data and Sunyaev-Zel'dovich data, that there may be a weak CNO signature.