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    Rights statement: This is an author-created, un-copyedited version of an article accepted for publication/published in Journal of Cosmology and Astroparticle Physics. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at doi:10.1088/1475-7516/2021/03/043

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Sensitivity of future liquid argon dark matter search experiments to core-collapse supernova neutrinos

Research output: Contribution to Journal/Magazine › Journal article › peer-review

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Sensitivity of future liquid argon dark matter search experiments to core-collapse supernova neutrinos. / The Darkside Collaboration ; Nowak, J.
In: Journal of Cosmology and Astroparticle Physics, Vol. 2021, No. 3, 043, 15.03.2021.

Research output: Contribution to Journal/Magazine › Journal article › peer-review

Harvard

The Darkside Collaboration & Nowak, J 2021, 'Sensitivity of future liquid argon dark matter search experiments to core-collapse supernova neutrinos', Journal of Cosmology and Astroparticle Physics, vol. 2021, no. 3, 043. https://doi.org/10.1088/1475-7516/2021/03/043

APA

The Darkside Collaboration, & Nowak, J. (2021). Sensitivity of future liquid argon dark matter search experiments to core-collapse supernova neutrinos. Journal of Cosmology and Astroparticle Physics, 2021(3), Article 043. https://doi.org/10.1088/1475-7516/2021/03/043

Vancouver

The Darkside Collaboration, Nowak J. Sensitivity of future liquid argon dark matter search experiments to core-collapse supernova neutrinos. Journal of Cosmology and Astroparticle Physics. 2021 Mar 15;2021(3):043. doi: 10.1088/1475-7516/2021/03/043

Author

The Darkside Collaboration ; Nowak, J. / Sensitivity of future liquid argon dark matter search experiments to core-collapse supernova neutrinos. In: Journal of Cosmology and Astroparticle Physics. 2021 ; Vol. 2021, No. 3.

Bibtex

@article{cd2bf9f2bd0f47619e5e76f9319b6ea3,
title = "Sensitivity of future liquid argon dark matter search experiments to core-collapse supernova neutrinos",
abstract = " Future liquid-argon DarkSide-20k and ARGO detectors, designed for direct dark matter search, will be sensitive also to core-collapse supernova neutrinos, via coherent elastic neutrino-nucleus scattering. This interaction channel is flavor-insensitive with a high-cross section, enabling for a high-statistics neutrino detection with target masses of $\sim$50~t and $\sim$360~t for DarkSide-20k and ARGO, respectively. Thanks to the low-energy threshold of $\sim$0.5~keV$_{nr}$ achievable by exploiting the ionization channel, DarkSide-20k and ARGO have the potential to discover supernova bursts throughout our galaxy and up to the Small Magellanic Cloud, respectively, assuming a 11-M$_{\odot}$ progenitor star. We report also on the sensitivity to the neutronization burst, whose electron neutrino flux is suppressed by oscillations when detected via charged current and elastic scattering. Finally, the accuracies in the reconstruction of the average and total neutrino energy in the different phases of the supernova burst, as well as its time profile, are also discussed, taking into account the expected background and the detector response. ",
keywords = "astro-ph.HE, astro-ph.IM, physics.ins-det",
author = "{The Darkside Collaboration} and P. Agnes and S. Albergo and Albuquerque, {I. F. M.} and T. Alexander and A. Alici and Alton, {A. K.} and P. Amaudruz and S. Arcelli and M. Ave and Avetissov, {I. Ch} and Avetisov, {R. I.} and O. Azzolini and Back, {H. O.} and Z. Balmforth and V. Barbarian and Olmedo, {A. Barrado} and P. Barrillon and A. Basco and G. Batignani and A. Bondar and Bonivento, {W. M.} and E. Borisova and B. Bottino and Boulay, {M. G.} and G. Buccino and S. Bussino and J. Busto and A. Buzulutskov and M. Cadeddu and M. Cadoni and A. Caminata and N. Canci and G. Cappello and M. Caravati and M. C{\'a}rdenas-Montes and M. Carlini and F. Carnesecchi and P. Castello and S. Catalanotti and V. Cataudella and P. Cavalcante and S. Cavuoti and S. Cebrian and Ruiz, {J. M. Cela} and B. Celano and S. Chashin and A. Chepurnov and C. Cical{\`o} and L. Cifarelli and J. Nowak",
note = "This is an author-created, un-copyedited version of an article accepted for publication/published in Journal of Cosmology and Astroparticle Physics. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at doi:10.1088/1475-7516/2021/03/043",
year = "2021",
month = mar,
day = "15",
doi = "10.1088/1475-7516/2021/03/043",
language = "English",
volume = "2021",
journal = "Journal of Cosmology and Astroparticle Physics",
issn = "1475-7516",
publisher = "IOP Publishing",
number = "3",

}

RIS

TY - JOUR

T1 - Sensitivity of future liquid argon dark matter search experiments to core-collapse supernova neutrinos

AU - The Darkside Collaboration

AU - Agnes, P.

AU - Albergo, S.

AU - Albuquerque, I. F. M.

AU - Alexander, T.

AU - Alici, A.

AU - Alton, A. K.

AU - Amaudruz, P.

AU - Arcelli, S.

AU - Ave, M.

AU - Avetissov, I. Ch

AU - Avetisov, R. I.

AU - Azzolini, O.

AU - Back, H. O.

AU - Balmforth, Z.

AU - Barbarian, V.

AU - Olmedo, A. Barrado

AU - Barrillon, P.

AU - Basco, A.

AU - Batignani, G.

AU - Bondar, A.

AU - Bonivento, W. M.

AU - Borisova, E.

AU - Bottino, B.

AU - Boulay, M. G.

AU - Buccino, G.

AU - Bussino, S.

AU - Busto, J.

AU - Buzulutskov, A.

AU - Cadeddu, M.

AU - Cadoni, M.

AU - Caminata, A.

AU - Canci, N.

AU - Cappello, G.

AU - Caravati, M.

AU - Cárdenas-Montes, M.

AU - Carlini, M.

AU - Carnesecchi, F.

AU - Castello, P.

AU - Catalanotti, S.

AU - Cataudella, V.

AU - Cavalcante, P.

AU - Cavuoti, S.

AU - Cebrian, S.

AU - Ruiz, J. M. Cela

AU - Celano, B.

AU - Chashin, S.

AU - Chepurnov, A.

AU - Cicalò, C.

AU - Cifarelli, L.

AU - Nowak, J.

N1 - This is an author-created, un-copyedited version of an article accepted for publication/published in Journal of Cosmology and Astroparticle Physics. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at doi:10.1088/1475-7516/2021/03/043

PY - 2021/3/15

Y1 - 2021/3/15

N2 - Future liquid-argon DarkSide-20k and ARGO detectors, designed for direct dark matter search, will be sensitive also to core-collapse supernova neutrinos, via coherent elastic neutrino-nucleus scattering. This interaction channel is flavor-insensitive with a high-cross section, enabling for a high-statistics neutrino detection with target masses of $\sim$50~t and $\sim$360~t for DarkSide-20k and ARGO, respectively. Thanks to the low-energy threshold of $\sim$0.5~keV$_{nr}$ achievable by exploiting the ionization channel, DarkSide-20k and ARGO have the potential to discover supernova bursts throughout our galaxy and up to the Small Magellanic Cloud, respectively, assuming a 11-M$_{\odot}$ progenitor star. We report also on the sensitivity to the neutronization burst, whose electron neutrino flux is suppressed by oscillations when detected via charged current and elastic scattering. Finally, the accuracies in the reconstruction of the average and total neutrino energy in the different phases of the supernova burst, as well as its time profile, are also discussed, taking into account the expected background and the detector response.

AB - Future liquid-argon DarkSide-20k and ARGO detectors, designed for direct dark matter search, will be sensitive also to core-collapse supernova neutrinos, via coherent elastic neutrino-nucleus scattering. This interaction channel is flavor-insensitive with a high-cross section, enabling for a high-statistics neutrino detection with target masses of $\sim$50~t and $\sim$360~t for DarkSide-20k and ARGO, respectively. Thanks to the low-energy threshold of $\sim$0.5~keV$_{nr}$ achievable by exploiting the ionization channel, DarkSide-20k and ARGO have the potential to discover supernova bursts throughout our galaxy and up to the Small Magellanic Cloud, respectively, assuming a 11-M$_{\odot}$ progenitor star. We report also on the sensitivity to the neutronization burst, whose electron neutrino flux is suppressed by oscillations when detected via charged current and elastic scattering. Finally, the accuracies in the reconstruction of the average and total neutrino energy in the different phases of the supernova burst, as well as its time profile, are also discussed, taking into account the expected background and the detector response.

KW - astro-ph.HE

KW - astro-ph.IM

KW - physics.ins-det

U2 - 10.1088/1475-7516/2021/03/043

DO - 10.1088/1475-7516/2021/03/043

M3 - Journal article

VL - 2021

JO - Journal of Cosmology and Astroparticle Physics

JF - Journal of Cosmology and Astroparticle Physics

SN - 1475-7516

IS - 3

M1 - 043

ER -