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D J Buettner

USA

Title: Condensed neutrino object models and galaxy cluster data

Biography

Biography: D J Buettner

Abstract

In part-I of our talk, by Dr. Morley, relativistic magnetic dipole radiation loss was proposed as a potential mechanism for slowing down primordial “Big Bang” neutrinos. That talk outlined the CNO equation of state and the resulting equilibrium objects, revealing that the CNO would constitute the largest and most massive objects in the universe. The purpose of this talk is to bridge the previous theoretical discussion to the current status of CNO research, identifying the astrophysical evidence. The upcoming KATRIN experiment measuring the mass of the electron anti-neutrino down to 0.35 eV/c^2 can confirm the viability of CNOs as the Dark Matter.