Curtailing the dark side in non-standard neutrino interactions

Coloma, Pilar; Denton, Peter B.; Gonzalez-Garcia, Maria C.; Maltoni, Michele; Schwetz, Thomas

doi:10.1007/JHEP04(2017)116

Title: Curtailing the dark side in non-standard neutrino interactions

Journal Article · 20 April 2017 · Journal of High Energy Physics (Online)

DOI: https://doi.org/10.1007/JHEP04(2017)116 · OSTI ID:1345608

^[1];

^[2]; Gonzalez-Garcia, Maria C. ^[3];

^[4];

^[5]

Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Univ. of Copenhagen, Copenhagen (Denmark)
Univ. de Barcelona, Barcelona (Spain); Institucio Catalana de Recerca i Estudis Avancats (ICREA), Barcelona (Spain); Stony Brook Univ., Stony Brook, NY (United States)
Univ. of Autonoma de Madrid, Madrid (Spain)
Karlsruher Institut fur Technologie (KIT), Karlsruhe (Germany)

In presence of non-standard neutrino interactions the neutrino flavor evolution equation is affected by a degeneracy which leads to the so-called LMA-Dark solution. It requires a solar mixing angle in the second octant and implies an ambiguity in the neutrino mass ordering. Non-oscillation experiments are required to break this degeneracy. We perform a combined analysis of data from oscillation experiments with the neutrino scattering experiments CHARM and NuTeV. We find that the degeneracy can be lifted if the non-standard neutrino interactions take place with down quarks, but it remains for up quarks. However, CHARM and NuTeV constraints apply only if the new interactions take place through mediators not much lighter than the electroweak scale. For light mediators we consider the possibility to resolve the degeneracy by using data from future coherent neutrino-nucleus scattering experiments. Here we find that, for an experiment using a stopped-pion neutrino source, the LMA-Dark degeneracy will either be resolved, or the presence of new interactions in the neutrino sector will be established with high significance.

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Research Organization:: Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)

Sponsoring Organization:: USDOE Office of Science (SC), High Energy Physics (HEP)

Grant/Contract Number:: AC02-07CH11359

OSTI ID:: 1345608

Report Number(s):: FERMILAB-PUB-17-016-T; YITP-SB-17-4; IFT-UAM-CSIC-17-004; arXiv:1701.04828; 1509503

Journal Information:: Journal of High Energy Physics (Online), Vol. 2017, Issue 4; ISSN 1029-8479

Publisher:: Springer BerlinCopyright Statement

Country of Publication:: United States

Language:: English

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