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Search for the sterile neutrino mixing with the ICAL detector at INO
Indexado
WoS WOS:000401336000002
Scopus SCOPUS_ID:85019203040
DOI 10.1140/EPJC/S10052-017-4851-4
Año 2017
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



The study has been carried out on the prospects of probing the sterile neutrino mixing with the magnetized iron calorimeter (ICAL) at the India-based Neutrino Observatory (INO), using atmospheric neutrinos as a source. The so-called 3 + 1 scenario is considered for active-sterile neutrino mixing and lead to projected exclusion curves in the sterile neutrino mass and mixing angle plane. The analysis is performed using the neutrino event generator NUANCE, modified for ICAL, and folded with the detector resolutions obtained by the INO collaboration from a full GEANT4-based detector simulation. A comparison has been made between the results obtained from the analysis considering only the energy and zenith angle of the muon and combined with the hadron energy due to the neutrino induced event. A small improvement has been observed with the addition of the hadron information to the muon. In the analysis we consider neutrinos coming from all zenith angles and the Earth matter effects are also included. The inclusion of events from all zenith angles improves the sensitivity to sterile neutrino mixing by about 35% over the result obtained using only down-going events. The improvement mainly stems from the impact of Earth matter effects on active-sterile mixing. The expected precision of ICAL on the active-sterile mixing is explored and the allowed confidence level (C.L.) contours presented. At the assumed true value of 10. for the sterile mixing angles and marginalization over Delta m(41)(2) and the sterile mixing angles, the upper bound at 90% C.L. (from two-parameter plots) is around 20 degrees for theta(14) and theta(34), and about 12 degrees for theta(24).

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
Sin Disciplinas

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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 Behera, S. P. - Bhabha Atom Res Ctr - India
Homi Bhabha Natl Inst - India
Bhabha Atomic Research Centre - India
Homi Bhabha National Institute - India
2 Ghosh, A. - Universidad Técnica Federico Santa María - Chile
3 Choubey, Sandhya Mujer Harish Chandra Res Inst - India
Harish Chandra Research Institute - India
4 Datar, V. M. - Tata Inst Fundamental Res - India
Tata Institute of Fundamental Research, Mumbai - India
5 Mishra, D. - Bhabha Atom Res Ctr - India
Bhabha Atomic Research Centre - India
6 Mohanty, A. K. - Bhabha Atom Res Ctr - India
Homi Bhabha Natl Inst - India
Saha Inst Nucl Phys - India
Bhabha Atomic Research Centre - India
Homi Bhabha National Institute - India
Saha Institute of Nuclear Physics - India

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Origen de Citas Identificadas



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Citas identificadas: Las citas provienen de documentos incluidos en la base de datos de DATACIENCIA

Citas Identificadas: 10.0 %
Citas No-identificadas: 90.0 %

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Citas identificadas: Las citas provienen de documentos incluidos en la base de datos de DATACIENCIA

Citas Identificadas: 10.0 %
Citas No-identificadas: 90.0 %

Financiamiento



Fuente
European Union
Seventh Framework Programme
Neutrino Project under the XII plan of Harish-Chandra Research Institute

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Agradecimientos



Agradecimiento
We thank the INO collaboration for useful suggestions and discussions. We also thank Vibhuti Duggal for her support while running the program at the BARC supper-computing facility. We would also like to thank S. Umasankar, A. Raychaudhuri, S. Goswami and Md. Naimuddin for their helpful suggestions and useful discussions. SC acknowledges support from the Neutrino Project under the XII plan of Harish-Chandra Research Institute and partial support from the European Union FP7 ITN INVISIBLES (Marie Curie Actions, PITN-GA-2011-289442).
We thank the INO collaboration for useful suggestions and discussions. We also thank Vibhuti Duggal for her support while running the program at the BARC supper-computing facility. We would also like to thank S. Umasankar, A. Raychaudhuri, S. Goswami and Md. Naimuddin for their helpful suggestions and useful discussions. SC acknowledges support from the Neutrino Project under the XII plan of Harish-Chandra Research Institute and partial support from the European Union FP7 ITN INVISIBLES (Marie Curie Actions, PITN-GA-2011-289442).

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