Constraining non-standard neutrino interactions with neutral current events at long-baseline oscillation experiments

A bstract We explore, for the first time, neutral-current events at long-baseline experiments to constrain vector and axial-vector neutrino non-standard interactions (NSI) with quarks. We leverage the flavor dependence of NSIs to perform an oscillation analysis in the neutral- current channel. We first introduce a framework to parametrize the effect of NSI on the cross section. Then, as an example, we analyze NOvA neutral-current data which provides significantly improved constraints on the axial-vector NSI parameters $$ {\varepsilon}_{\mu \mu}^A $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msubsup> <mml:mi>ε</mml:mi> <mml:mi>μμ</mml:mi> <mml:mi>A</mml:mi> </mml:msubsup> </mml:math> , $$ {\varepsilon}_{\tau \tau}^A $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msubsup> <mml:mi>ε</mml:mi> <mml:mi>ττ</mml:mi> <mml:mi>A</mml:mi> </mml:msubsup> </mml:math> and $$ {\varepsilon}_{e\mu}^A $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msubsup> <mml:mi>ε</mml:mi> <mml:mi>eμ</mml:mi> <mml:mi>A</mml:mi> </mml:msubsup> </mml:math> . This is highly complementary to constraints from SNO data, which, differently from long-baseline neutral current data, is not sensitive to isospin conserving NSIs $$ {\varepsilon}_u^A $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msubsup> <mml:mi>ε</mml:mi> <mml:mi>u</mml:mi> <mml:mi>A</mml:mi> </mml:msubsup> </mml:math> = $$ {\varepsilon}_d^A $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msubsup> <mml:mi>ε</mml:mi> <mml:mi>d</mml:mi> <mml:mi>A</mml:mi> </mml:msubsup> </mml:math> . Additionally, we disfavor large values of the diagonal vectorial NSI $$ {\varepsilon}_{\mu \mu}^{VV} $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msubsup> <mml:mi>ε</mml:mi> <mml:mi>μμ</mml:mi> <mml:mi>VV</mml:mi> </mml:msubsup> </mml:math> and $$ {\varepsilon}_{\tau \tau}^V $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msubsup> <mml:mi>ε</mml:mi> <mml:mi>ττ</mml:mi> <mml:mi>V</mml:mi> </mml:msubsup> </mml:math> which originate from the LMA-Dark solution. We also highlight the complementarity between NSI searches at oscillation experiments using charged current and neutral current channels.

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Publication Details

Journal
Journal of High Energy Physics
Published
2025-05-07
DOI
https://doi.org/10.1007/jhep05(2025)065
Citations
6
Primary Topic
Neutrino Physics Research
Type
article
Field-Weighted Citation Impact
11.22

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article

Constraining non-standard neutrino interactions with neutral current events at long-baseline oscillation experiments

João Paulo Pinheiro, Julia Gehrlein, P. Machado
6 citations
Journal of High Energy Physics
Neutrino Physics Research
11.22
article

Constraining non-standard neutrino interactions with neutral current events at long-baseline oscillation experiments

João Paulo Pinheiro, Julia Gehrlein, P. Machado
article en
6 citations

Abstract

A bstract We explore, for the first time, neutral-current events at long-baseline experiments to constrain vector and axial-vector neutrino non-standard interactions (NSI) with quarks. We leverage the flavor dependence of NSIs to perform an oscillation analysis in the neutral- current channel. We first introduce a framework to parametrize the effect of NSI on the cross section. Then, as an example, we analyze NOvA neutral-current data which provides significantly improved constraints on the axial-vector NSI parameters $$ {\varepsilon}_{\mu \mu}^A $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msubsup> <mml:mi>ε</mml:mi> <mml:mi>μμ</mml:mi> <mml:mi>A</mml:mi> </mml:msubsup> </mml:math> , $$ {\varepsilon}_{\tau \tau}^A $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msubsup> <mml:mi>ε</mml:mi> <mml:mi>ττ</mml:mi> <mml:mi>A</mml:mi> </mml:msubsup> </mml:math> and $$ {\varepsilon}_{e\mu}^A $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msubsup> <mml:mi>ε</mml:mi> <mml:mi>eμ</mml:mi> <mml:mi>A</mml:mi> </mml:msubsup> </mml:math> . This is highly complementary to constraints from SNO data, which, differently from long-baseline neutral current data, is not sensitive to isospin conserving NSIs $$ {\varepsilon}_u^A $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msubsup> <mml:mi>ε</mml:mi> <mml:mi>u</mml:mi> <mml:mi>A</mml:mi> </mml:msubsup> </mml:math> = $$ {\varepsilon}_d^A $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msubsup> <mml:mi>ε</mml:mi> <mml:mi>d</mml:mi> <mml:mi>A</mml:mi> </mml:msubsup> </mml:math> . Additionally, we disfavor large values of the diagonal vectorial NSI $$ {\varepsilon}_{\mu \mu}^{VV} $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msubsup> <mml:mi>ε</mml:mi> <mml:mi>μμ</mml:mi> <mml:mi>VV</mml:mi> </mml:msubsup> </mml:math> and $$ {\varepsilon}_{\tau \tau}^V $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msubsup> <mml:mi>ε</mml:mi> <mml:mi>ττ</mml:mi> <mml:mi>V</mml:mi> </mml:msubsup> </mml:math> which originate from the LMA-Dark solution. We also highlight the complementarity between NSI searches at oscillation experiments using charged current and neutral current channels.

Journal of High Energy PhysicsVol. 2025(5)
Fermi National Accelerator Laboratory (US), Universitat de Barcelona (ES), Colorado State University (US)
U.S. Department of Energy, European Commission, Generalitat de Catalunya, Office of Science, HORIZON EUROPE Framework Programme, Agencia Estatal de Investigación, Fermilab
Openalex Percentile: Top 2%
Neutrino Physics Research
11.22
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