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Probing hidden leptonic scalar portals using the NA64 experiment at CERN
Indexado
WoS WOS:001329377000007
Scopus SCOPUS_ID:85206250613
DOI 10.1140/EPJC/S10052-024-13421-1
Año 2024
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



In this study, we demonstrate the potential of the NA64 experiment at CERN SPS to search for New Physics processes involving e ->mu\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$e\rightarrow \mu $$\end{document} transitions after the collision of 100 GeV electrons with target nuclei. A new Dark Sector leptonic portal in which a scalar boson phi\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\varphi $$\end{document} could be produced in the lepton-flavor-changing bremsstrahlung-like reaction, eN ->mu N phi\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$eN\rightarrow \mu N\varphi $$\end{document}, is used as benchmark process. In this work, we develop a realistic Monte Carlo simulation of the NA64 experimental setup implementing the differential and total production cross-section computed at exact tree-level and applying the Weisz & auml;cker-Williams phase space approximation. Using this framework, we investigate the main background sources and calculate the expected sensitivity of the experiment. The results indicate that with minor setup optimization, NA64 can probe a large fraction of the available parameter space compatible with the muon g-2\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$g-2$$\end{document} anomaly and the Dark Matter relic predictions in the context of a new Dark Sector leptonic portal with 1011\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$10<^>{11}$$\end{document} EOT. This result paves the way to the exploration of lepton-flavour-changing transitions in NA64.

Revista



Revista ISSN
European Physical Journal C 1434-6044

Métricas Externas



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Disciplinas de Investigación



WOS
Physics, Particles & Fields
Scopus
Sin Disciplinas
SciELO
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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



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Autores - Afiliación



Ord. Autor Género Institución - País
1 Ponten, A. - UPPSALA UNIV - Suecia
Uppsala Universitet - Suecia
2 Sieber, H. - ETH - Suiza
ETH Zurich - Suiza
3 Banto Oberhauser, B. - ETH - Suiza
ETH Zurich - Suiza
4 Crivelli, P. - ETH - Suiza
ETH Zurich - Suiza
5 Kirpichnikov, D. - Russian Acad Sci - Rusia
Institute for Nuclear Research of the Russian Academy of Sciences - Rusia
6 Gninenko, S. N. - Russian Acad Sci - Rusia
Universidad Nacional Andrés Bello - Chile
Institute for Nuclear Research of the Russian Academy of Sciences - Rusia
7 Hösgen, M. - UNIV BONN - Alemania
Universität Bonn - Alemania
8 Bueno, L. Molina - UV - España
CSIC-UV - Instituto de Física Corpuscular (IFIC) - España
9 Mongillo, M. - ETH - Suiza
ETH Zurich - Suiza
10 Zhevlakov, Alexey S. Hombre JINR - Rusia
Matrosov Inst Syst Dynam & Control Theory SB RAS - Rusia
Bogoliubov Laboratory of Theoretical Physics, Joint Institute for Nuclear Research - Rusia
Matrosov Institute for System Dynamics and Control Theory of Siberian Branch of Russian Academy of Sciences - Rusia

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Financiamiento



Fuente
Ministerio de Ciencia e Innovación
SNSF
Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung
Agencia Estatal de Investigación
Eidgenossische Technische Hochschule Zurich
ETH
Ministerio de Ciencia e Innovacin
UE (Spain)

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Agradecimientos



Agradecimiento
We acknowledge the members of the NA64 collaboration for fruitful discussions. In particular, we thank N. V. Krasnikov for his helpful suggestions and correspondence. The work of P. Crivelli, B. Banto Oberhauser, M. Mongillo, and H. Sieber is supported by the SNSF Grants No. 186158, and No. 197346 No. 216602, No. 219485 (Switzerland) and by ETH Grant No. 22-2 ETH-031. The work of L. Molina-Bueno is supported by SNSF Grant No. 186158 (Switzerland), RyC-030551-I, PID2021-123955NA-100 and CNS2022-135850 funded by MCIN/AEI/ 10.13039/501100011033/FEDER, UE (Spain).
We acknowledge the members of the NA64 collaboration for fruitful discussions. In particular, we thank N. V. Krasnikov for his helpful suggestions and correspondence. The work of P. Crivelli, B. Banto Oberhauser, M. Mongillo, and H. Sieber is supported by the SNSF Grants No. 186158, and No. 197346 No. 216602, No. 219485 (Switzerland) and by ETH Grant No. 22-2 ETH-031. The work of L. Molina-Bueno is supported by SNSF Grant No. 186158 (Switzerland), RyC-030551-I, PID2021-123955NA-100 and CNS2022-135850 funded by MCIN/AEI/ 10.13039/501100011033/FEDER, UE (Spain).

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