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Observable Consequences of a Scalar Boson Coupled only to Neutrinos

1993/09/21 by G. J. Stephenson Jr., G. J. Stephenson, T. Goldman +2 · 1 citation
Physics and Astronomy · #Astrophysics (astro-ph) #Dark Matter and Cosmic Phenomena #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #Neutrino Physics Research #Nuclear Theory (nucl-th) #Particle physics theoretical and experimental studies #astro-ph #hep-ph #nucl-th

paper · pdf · doi:10.48550/arxiv.hep-ph/9309308

15 pages, LaTeX, 2 figures in uuencoded, compressed format, Los Alamos preprint LA-UR-93-3348

arxiv created 1993/09/21 · openalex publication_date 1993/09/21 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

We have examined the consequences of assuming the existence of a light scalar boson, weakly coupled to neutrinos, and not coupled to any other light fermions. For a range of parameters, we find that this hypothesis leads to the development of neutrino clusters which form in the early Universe and which provide gravitational fluctuations on scales small compared to a parsec (i.e., the scale of solar systems). The existence of such clustering produces an effect which would appear as a negative mass squared for the electron neutrino in Tritium beta decay, without conflicting with other experiments. The neutrino masses arising in unified gauge theories would then be very much larger than the masses extracted from experiments within the solar system.

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