Searcharxiv⌕ Search

arXiv subjects

D. J. Buettner

Publications and source records attributed to D. J. Buettner.

4 recordsLinked to original sources

Why not Neutrinos as the Dark Matter? A Critical Review, KATRIN and New Research Directions

We challenge the traditional wisdom that cosmological (big bang relic) neutrinos can only be hot Dark Matter. We provide a critical review of the concepts, derivations and arguments in foundational books and recent publications that led respected researchers to proclaim that "[Dark Matter] cannot be neutrinos". We then provide the physics resulting in relic neutrino's significant power loss from the interaction of its anomalous magnetic moment with a high-intensity primordial magnetic fields, resulting in subsequent condensation into Condensed Neutrino Objects (CNOs). Finally, the experimental degenerate mass bounds that would rule out condensed cosmological neutrinos as the Dark Matter (unless there is new physics that would require a modification to the CNO Equation of State) are provided. We conclude with a discussion on new directions for research.

hep-ph↗

Neutrinos: the Real Nature of Dark Matter After All?

What exactly is Dark Matter? New theories for what really constitutes Dark Matter appear to make the news headlines every week. At a slower pace, these theories are slowly being eliminated. We revisit this scientific thriller and make the case that condensed neutrino matter is a leading suspect. We provide a forensic discussion of some subtle evidence and show that independent experimental results due out in 2019 from the KATRIN experiment will either be the definitive result or eliminate condensed neutrinos as a Dark Matter candidate.

physics.gen-ph↗

Dark Matter in the Local Group of Galaxies

We describe the neutrino flavor (e = electron, u = muon, t = tau) masses as m(i=e;u;t)= m + [Delta]mi with |[Delta]mij|/m < 1 and probably |[Delta]mij|/m << 1. The quantity m is the degenerate neutrino mass. Because neutrino flavor is not a quantum number, this degenerate mass appears in the neutrino equation of state. We apply a Monte Carlo computational physics technique to the Local Group (LG) of galaxies to determine an approximate location for a Dark Matter embedding condensed neutrino object(CNO). The calculation is based on the rotational properties of the only spiral galaxies within the LG: M31, M33 and the Milky Way. CNOs could be the Dark Matter everyone is looking for and we estimate the CNO embedding the LG to have a mass 5.17x10^15 Mo and a radius 1.316 Mpc, with the estimated value of m ~= 0.8 eV/c2. The up-coming KATRIN experiment will either be the definitive result or eliminate condensed neutrinos as a Dark Matter candidate.

physics.gen-ph↗

A Dark Matter Signature for Condensed Neutrinos

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.

astro-ph.HE↗