Albert, A.; Andre, M.; Anghinolfi, M.; Ardid Ramírez, Miguel; Aubert, J-J.; Aublin, J.; Baret, B.; Basa, S.; Belhorma, B.; Bertin, V.; Biagi, S.; Bissinger, M.; Boumaaza, J.; Bouta, M.; Bouwheis, M. C.; Martínez Mora, Juan Antonio; Poirè, Chiara(American Physical Society, 2020-10-27)
[EN] We present the results of the first combined dark matter search targeting the Galactic Center using the ANTARES and IceCube neutrino telescopes. For dark matter particles with masses from 50 to 1000 GeV, the sensitivities ...
Aiello, S.; Albert, A.; Alshamsi, M.; Alves Garre, S.; Aly, Z.; Ambrosone, A.; Ameli, F.; Andre, M.; Androulakis, G.; Anghinolfi, M.; Anguita, M.; Ardid Ramírez, Miguel; Ardid-Ramírez, Joan Salvador; Aublin, J.; Bagatelas, C.; Bou Cabo, M.; Diego-Tortosa, D.; Espinosa Roselló, Víctor; García-Méndez, J.; Llorens Álvarez, Carlos David; Martínez Mora, Juan Antonio; Poirè, Chiara(Springer-Verlag, 2022-03-09)
[EN] This article presents the potential of a combined analysis of the JUNO and KM3NeT/ORCA experiments to determine the neutrino mass ordering. This combination is particularly interesting as it significantly boosts the ...
Aiello, S.; Albert, A.; Alves Garre, S.; Aly, Z.; Ameli, F.; Anassontzis, E. G.; Andre, M.; Androulakis, G.; Anghinolfi, M.; Anguita, M.; Anton, G.; Ardid Ramírez, Miguel; Aublin, J.; Bagatelas, C.; Bakker, R.; Diego-Tortosa, D.; Espinosa Roselló, Víctor; Martínez Mora, Juan Antonio; Poirè, Chiara(IOP Publishing, 2020-11)
[EN] KM3NeT is a research infrastructure being installed in the deep Mediterranean Sea. It will house a neutrino telescope comprising hundreds of networked moorings ¿ detection units or strings ¿ equipped with optical ...
Ageron, M.; Aiello, S.; Ameli, F.; Andre, M.; Androulakis, G.; Anghinolfi, M.; Anton, G.; Ardid Ramírez, Miguel; Aublin, J.; Bagatelas, C.; Barbarino, G.; Baret, B.; du Pree, S. Basegmez; Belias, A.; Berbee, E.; Tortosa, Dídac D.; Llorens Alvarez, Carlos David; Martínez Mora, Juan Antonio; Poirè, Chiara(Springer-Verlag, 2020-02-06)
[EN] KM3NeT is a research infrastructure located in the Mediterranean Sea, that will consist of two deep-sea Cherenkov neutrino detectors. With one detector (ARCA), the KM3NeT Collaboration aims at identifying and studying ...
Aiello, S.; Albert, A.; Alves Garre, S.; Aly, Z.; Ameli, F.; Andre, M.; Androulakis, G.; Anghinolfi, M.; Anguita, M.; Anton, G.; Ardid Ramírez, Miguel; Aublin, J.; Bagatelas, C.; Barbarino, G.; Baret, B.; Diego-Tortosa, D.; Espinosa Roselló, Víctor; Martínez Mora, Juan Antonio; Poirè, Chiara(Elsevier, 2020-11)
[EN] The gSeaGen code is a GENIE-based application developed to efficiently generate high statistics samples of events, induced by neutrino interactions, detectable in a neutrino telescope. The gSeaGen code is able to ...
Albert, A; Alves, S; Andre, M.; Ardid, M.; Ardid, S.; Aubert, J.J.; Aublin, J.; Baret, B.; Basa, S.; Becherini, P.; Belhorma, B.; Bendahman, M.; Benfenati, F.; Bertin, V.; Biagi, S.; García-Méndez, Juan; Martínez Mora, Juan Antonio; Poirè, Chiara(Elsevier, 2023-06-10)
[EN] Interactions of cosmic ray protons, atomic nuclei, and electrons in the interstellar medium in the inner part of the Milky Way produce gamma-ray flux from the Galactic Ridge. If the gamma-ray emission is dominated by ...
Aiello, S.; Albert, A.; Alshamsi, M.; Alves Garre, S.; Aly, Z.; Ambrosone, A.; Ameli, F.; Andre, M.; Androulakis, G.; Anghinolfi, M.; Anguita, M.; Ardid Ramírez, Miguel; Ardid-Ramírez, Joan Salvador; Aublin, J.; Bagatelas, C.; Bou Cabo, Manuel; Diego-Tortosa, Dídac; Espinosa Roselló, Víctor; Llorens Alvarez, Carlos David; Martínez Mora, Juan Antonio; Poirè, Chiara(Springer-Verlag, 2022-04-11)
[EN] The KM3NeT research infrastructure is uncon-
struction in the Mediterranean Sea. KM3NeT will study atmospheric and astrophysical neutrinos with two multi- purpose neutrino detectors, ARCA and ORCA, primar-ily aimed ...
Albert, A.; Alves, S.; Andre, M.; Ardid, M.; Ardid, S.; Aubert, J.J.; Aublin, J.; Baret, B.; Basa, S.; Belhorma, B.; Bendahman, M.; Benfenati, F.; Bertin, V.; Biagi, S.; Bissinger, M.; García, J.; Martínez Mora, Juan Antonio; Poirè, Chiara(IOP Publishing, 2023-01)
[EN] In this work, a search for nuclearites of strange quark matter by using nine years of ANTARES data taken in the period 2009-2017 is presented. The passage through matter of these particles is simulated taking into ...
Albert, A.; Alves, S.; Andre, M.; Anghinolfi, M.; Anton, G.; Ardid Ramírez, Miguel; Aubert, J-J.; Aublin, J.; Baret, B.; Basa, S.; Belhorma, B.; Bendahman, M.; Bertin, V.; Biagi, S.; Bissinger, M.; J. A. Martínez Mora; Poirè, Chiara(Elsevier, 2021-05-10)
[EN] This letter presents a combined measurement of the energy spectra of atmospheric nu(e) and nu(mu) in the energy range between similar to 100 GeV and similar to 50 TeV with the ANTARES neutrino telescope. The analysis ...
Albert, A.; Andre, M.; Anghinolfi, M.; Anton, G.; Ardid Ramírez, Miguel; Aubert, J.J.; Aublin, J.; Baret, B.; Basa, S.; Belhorma, B.; Bertin, V.; Biagi, S.; Bissinger, M.; Boumaaza, J.; Bouta, M.; Martínez Mora, Juan Antonio; Poirè, Chiara(IOP Publishing, 2021-01-29)
[EN] Monte Carlo simulations are a unique tool to check the response of a detector
and to monitor its performance. For a deep-sea neutrino telescope, the variability of the
environmental conditions that can a ect the ...
Albert, A.; Andre, M.; Anghinolfi, M.; Anton, G.; Ardid Ramírez, Miguel; Aubert, J-J; Aublin, J.; Baret, B.; Basa, S.; Belhorma, B.; Bertin, V.; Biagi, S.; Bissinger, M.; Boumaaza, J.; Bouta, M.; Martínez Mora, Juan Antonio; Poirè, Chiara(American Physical Society, 2020-12-28)
[EN] The ANTARES detector is an undersea neutrino telescope in the Mediterranean Sea. The search for pointlike neutrino sources is one of the main goals of the ANTARES telescope, requiring a reliable method to evaluate the ...
Aiello, S.; Albert, A.; Alves Garre, S.; Aly, Z.; Ambrosone, A.; Ameli, F.; Andre, M.; Anghinolfi, M.; Anguita, M.; Ardid, M.; Ardid, S.; Aublin, J.; Bagatelas, C.; Bailly-Salins, L.; Baret, B.; Di Palma, I.; García-Méndez, Juan(Springer-Verlag, 2023-04-19)
[EN] In the era of precision measurements of the neutrino oscillation parameters, upcoming neutrino experiments will also be sensitive to physics beyond the Standard Model. KM3NeT/ORCA is a neutrino detector optimised for ...
Albert, A.; Alves, S.; Andre, M.; Ardid, M.; Ardid, S.; Aubert, J.J.; Aublin, J.; Baret, B.; Basa, S.; Belhorma, B.; Bendahman, M.; Benfenati, F.; Bertin, V.; Biagi, S.; Bissinger, M.; Capone, A.; García-Méndez, Juan(IOP Publishing, 2023-08)
[EN] By constantly monitoring a very large portion of the sky, neutrino telescopes are well-designed to detect neutrinos emitted by transient astrophysical events. Real-time searches with the ANTARES telescope have been ...
Albert, A.; Andre, M.; Anghinolfi, M.; Anton, G.; Ardid Ramírez, Miguel; Aubert, J-J.; Aublin, J.; Baret, B.; Basa, S.; Belhorma, B.; Bertin, V.; Biagi, S.; Bissinger, M.; Boumaaza, J.; Bourret, S.; Martínez Mora, Juan Antonio; Poirè, Chiara(Elsevier, 2020-06-10)
[EN] Neutrino detectors participate in the indirect search for the fundamental constituents of dark matter (DM) in form of weakly interacting massive particles (WIMPs). In WIMP scenarios, candidate DM particles can ...
Albert, A.; Alves, S.; Andre, M.; Anghinolfi, M.; Anton, G.; Ardid Ramírez, Miguel; Aubert, J.J.; Aublin, J.; Baret, B.; Basa, S.; Belhorma, B.; Bendahman, M.; Benfenati, F.; Bertin, V.; Biagi, S.; Martínez Mora, Juan Antonio; Poirè, Chiara(American Astronomical Society, 2021-10)
[EN] On 2019 October 1, the IceCube Collaboration detected a muon track neutrino with a high probability of being of astrophysical origin, IC191001A. After a few hours, the tidal disruption event (TDE) AT2019dsg, observed ...
Albert, A.; Alves, S.; Andre, M.; Anghinolfi, M.; Anton, G.; Ardid Ramírez, Miguel; Ardid-Ramírez, Joan Salvador; Aubert, J. J.; Aublin, J.; Baret, B.; Basa, S.; Belhorma, B.; Bendahman, M.; Benfenati, F.; Bertin, V.; Martínez Mora, Juan Antonio; Poirè, Chiara(IOP Publishing, 2022-06)
[EN] Searches for dark matter (DM) have not provided any solid evidence for the
existence of weakly interacting massive particles in the GeV-TeV mass range. Coincidentally,
the scale of new physics is being pushed by ...
Albert, A.; Alves, S.; Andre, M.; Anghinolfi, M.; Anton, G.; Ardid Ramírez, Miguel; Ardid-Ramírez, Joan Salvador; Aubert, J. J.; Aublin, J.; Baret, B.; Basa, S.; Belhorma, B.; Bendahman, M.; Benfenati, F.; Bertin, V.; Biagi, S.; Martínez Mora, Juan Antonio; Poirè, Chiara(IOP Publishing, 2022-06-15)
[EN] Solar Atmospheric Neutrinos (SA nu s) are produced by the interaction of cosmic rays with the solar medium. The detection of SA nu s would provide useful information on the composition of primary cosmic rays as well ...
Aiello, S.; Albert, A.; Alshamsi, M.; Alves Garre, S.; Aly, Z.; Ambrosone, A.; Ameli, F.; Andre, M.; Androulakis, G.; Anghinolfi, M.; Anguita, M.; Ardid Ramírez, Miguel; Ardid-Ramírez, Joan Salvador; Aublin, J.; Avgitas, T.; Bou Cabo, M.; Diego-Tortosa, D.; Espinosa Roselló, Víctor; Llorens Alvarez, Carlos David; Martínez Mora, Juan Antonio; Poirè, Chiara(IOP Publishing, 2022-07)
[EN] The optical module of the KM3NeT neutrino telescope is an innovative multi-faceted
large area photodetection module. It contains 31 three-inch photomultiplier tubes in a single 0.44
m diameter pressure-resistant glass ...