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First search for dark-trident processes using the MicroBooNE detector

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First search for dark-trident processes using the MicroBooNE detector. / MicroBooNE Collaboration ; Blake, A.; Devitt, A. et al.
In: Physical review letters, Vol. 132, No. 24, 14.06.2024.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

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MicroBooNE Collaboration, Blake A, Devitt A, Gu L, Mawby I, Nowak J et al. First search for dark-trident processes using the MicroBooNE detector. Physical review letters. 2024 Jun 14;132(24). Epub 2024 Jun 11. doi: 10.1103/PhysRevLett.132.241801

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MicroBooNE Collaboration ; Blake, A. ; Devitt, A. et al. / First search for dark-trident processes using the MicroBooNE detector. In: Physical review letters. 2024 ; Vol. 132, No. 24.

Bibtex

@article{1cdaf8415bb740458bb177053a95f4fb,
title = "First search for dark-trident processes using the MicroBooNE detector",
abstract = " We present a first search for dark-trident scattering in a neutrino beam using a data set corresponding to $7.2 \times 10^{20}$ protons on target taken with the MicroBooNE detector at Fermilab. Proton interactions in the neutrino target at the Main Injector produce $\pi^0$ and $\eta$ mesons, which could decay into dark-matter (DM) particles mediated via a dark photon $A^\prime$. A convolutional neural network is trained to identify interactions of the DM particles in the liquid-argon time projection chamber (LArTPC) exploiting its image-like reconstruction capability. In the absence of a DM signal, we provide limits at the $90\%$ confidence level on the squared kinematic mixing parameter $\varepsilon^2$ as a function of the dark-photon mass in the range $10\le M_{A^\prime}\le 400$ MeV. The limits cover previously unconstrained parameter space for the production of fermion or scalar DM particles $\chi$ for two benchmark models with mass ratios $M_{\chi}/M_{A^\prime}=0.6$ and $2$ and for dark fine-structure constants $0.1\le\alpha_D\le 1$. ",
keywords = "hep-ex",
author = "{MicroBooNE Collaboration} and P. Abratenko and O. Alterkait and Aldana, {D. Andrade} and L. Arellano and J. Asaadi and A. Ashkenazi and S. Balasubramanian and B. Baller and G. Barr and D. Barrow and J. Barrow and V. Basque and Rodrigues, {O. Benevides} and S. Berkman and A. Bhanderi and A. Bhat and M. Bhattacharya and M. Bishai and A. Blake and B. Bogart and T. Bolton and Book, {J. Y.} and Brunetti, {M. B.} and L. Camilleri and Y. Cao and D. Caratelli and F. Cavanna and G. Cerati and A. Chappell and Y. Chen and Conrad, {J. M.} and M. Convery and L. Cooper-Troendle and Crespo-Anadon, {J. I.} and R. Cross and Tutto, {M. Del} and Dennis, {S. R.} and P. Detje and A. Devitt and R. Diurba and Z. Djurcic and R. Dorrill and K. Duffy and S. Dytman and L. Gu and I. Mawby and J. Nowak and N. Patel and I. Pophale",
year = "2024",
month = jun,
day = "14",
doi = "10.1103/PhysRevLett.132.241801",
language = "English",
volume = "132",
journal = "Physical review letters",
issn = "1079-7114",
publisher = "American Physical Society",
number = "24",

}

RIS

TY - JOUR

T1 - First search for dark-trident processes using the MicroBooNE detector

AU - MicroBooNE Collaboration

AU - Abratenko, P.

AU - Alterkait, O.

AU - Aldana, D. Andrade

AU - Arellano, L.

AU - Asaadi, J.

AU - Ashkenazi, A.

AU - Balasubramanian, S.

AU - Baller, B.

AU - Barr, G.

AU - Barrow, D.

AU - Barrow, J.

AU - Basque, V.

AU - Rodrigues, O. Benevides

AU - Berkman, S.

AU - Bhanderi, A.

AU - Bhat, A.

AU - Bhattacharya, M.

AU - Bishai, M.

AU - Blake, A.

AU - Bogart, B.

AU - Bolton, T.

AU - Book, J. Y.

AU - Brunetti, M. B.

AU - Camilleri, L.

AU - Cao, Y.

AU - Caratelli, D.

AU - Cavanna, F.

AU - Cerati, G.

AU - Chappell, A.

AU - Chen, Y.

AU - Conrad, J. M.

AU - Convery, M.

AU - Cooper-Troendle, L.

AU - Crespo-Anadon, J. I.

AU - Cross, R.

AU - Tutto, M. Del

AU - Dennis, S. R.

AU - Detje, P.

AU - Devitt, A.

AU - Diurba, R.

AU - Djurcic, Z.

AU - Dorrill, R.

AU - Duffy, K.

AU - Dytman, S.

AU - Gu, L.

AU - Mawby, I.

AU - Nowak, J.

AU - Patel, N.

AU - Pophale, I.

PY - 2024/6/14

Y1 - 2024/6/14

N2 - We present a first search for dark-trident scattering in a neutrino beam using a data set corresponding to $7.2 \times 10^{20}$ protons on target taken with the MicroBooNE detector at Fermilab. Proton interactions in the neutrino target at the Main Injector produce $\pi^0$ and $\eta$ mesons, which could decay into dark-matter (DM) particles mediated via a dark photon $A^\prime$. A convolutional neural network is trained to identify interactions of the DM particles in the liquid-argon time projection chamber (LArTPC) exploiting its image-like reconstruction capability. In the absence of a DM signal, we provide limits at the $90\%$ confidence level on the squared kinematic mixing parameter $\varepsilon^2$ as a function of the dark-photon mass in the range $10\le M_{A^\prime}\le 400$ MeV. The limits cover previously unconstrained parameter space for the production of fermion or scalar DM particles $\chi$ for two benchmark models with mass ratios $M_{\chi}/M_{A^\prime}=0.6$ and $2$ and for dark fine-structure constants $0.1\le\alpha_D\le 1$.

AB - We present a first search for dark-trident scattering in a neutrino beam using a data set corresponding to $7.2 \times 10^{20}$ protons on target taken with the MicroBooNE detector at Fermilab. Proton interactions in the neutrino target at the Main Injector produce $\pi^0$ and $\eta$ mesons, which could decay into dark-matter (DM) particles mediated via a dark photon $A^\prime$. A convolutional neural network is trained to identify interactions of the DM particles in the liquid-argon time projection chamber (LArTPC) exploiting its image-like reconstruction capability. In the absence of a DM signal, we provide limits at the $90\%$ confidence level on the squared kinematic mixing parameter $\varepsilon^2$ as a function of the dark-photon mass in the range $10\le M_{A^\prime}\le 400$ MeV. The limits cover previously unconstrained parameter space for the production of fermion or scalar DM particles $\chi$ for two benchmark models with mass ratios $M_{\chi}/M_{A^\prime}=0.6$ and $2$ and for dark fine-structure constants $0.1\le\alpha_D\le 1$.

KW - hep-ex

U2 - 10.1103/PhysRevLett.132.241801

DO - 10.1103/PhysRevLett.132.241801

M3 - Journal article

VL - 132

JO - Physical review letters

JF - Physical review letters

SN - 1079-7114

IS - 24

ER -