Implementation and first results of the KM3NeT real-time core-collapse supernova neutrino search

被引：12

作者：

Aiello, S. ^{[1
]}

Albert, A. ^{[2
,55
]}

Alshamsi, M. ^{[3
]}

Alves Garre, S. ^{[4
]}

Aly, Z. ^{[5
]}

Ambrosone, A. ^{[6
,7
]}

Ameli, F. ^{[8
]}

Andre, M. ^{[9
]}

Androulakis, G. ^{[10
]}

Anghinolfi, M. ^{[11
]}

Anguita, M. ^{[12
]}

Ardid, M. ^{[13
]}

Ardid, S. ^{[13
]}

Aublin, J. ^{[3
]}

Bagatelas, C. ^{[10
]}

Baret, B. ^{[3
]}

du Pree, S. Basegmez ^{[14
]}

Bendahman, M. ^{[3
,15
]}

Benfenati, F. ^{[16
,17
]}

Berbee, E. ^{[14
]}

van den Berg, A. M. ^{[18
]}

Bertin, V ^{[5
]}

Biagi, S. ^{[19
]}

Boettcher, M. ^{[20
]}

Cabo, M. Bou ^{[21
]}

Boumaaza, J. ^{[15
]}

Bouta, M. ^{[22
]}

Bouwhuis, M. ^{[14
]}

Bozza, C. ^{[23
,24
]}

Branzass, H. ^{[25
]}

Bruijn, R. ^{[14
,26
]}

Brunner, J. ^{[5
]}

Bruno, R. ^{[1
]}

Buis, E. ^{[27
]}

Buompane, R. ^{[6
,28
]}

Busto, J. ^{[5
]}

Caiffi, B. ^{[11
]}

Calvo, D. ^{[4
]}

Campion, S. ^{[8
,29
]}

Capone, A. ^{[8
,29
]}

Carretero, V ^{[4
]}

Castaldi, P. ^{[16
,30
]}

Celli, S. ^{[8
,29
]}

Chabab, M. ^{[31
]}

Chau, N. ^{[3
]}

Chen, A. ^{[32
]}

Cherubini, S. ^{[19
,33
]}

Chiarella, V ^{[34
]}

Chiarusi, T. ^{[16
]}

Circella, M. ^{[35
]}

机构：

[1] Ist Nazl Fis Nucl, Sez Catania, Via Santa Sofia 64, I-95123 Catania, Italy

[2] Univ Strasbourg, CNRS, IPHC UMR 7178, F-67000 Strasbourg, France

[3] Univ Paris, Astroparticule & Cosmol, CNRS, F-75013 Paris, France

[4] Univ Valencia, IFIC Inst Fis Corpuscular, CSIC, C Catedrat Jose Beltran 2, Valencia 46980, Spain

[5] Aix Marseille Univ, CPPM, CNRS IN2P3, Marseille, France

[6] Complesso Univ Monte S Angelo, Sez Napoli, Ist Nazl Fis Nucl, Via Cintia G, I-80126 Naples, Italy

[7] Univ Napoli Federico II, Complesso Univ Monte S Angelo, Dip Sci Fis E Pancini, Via Cintia G, I-80126 Naples, Italy

[8] Ist Nazl Fis Nucl, Sez Roma, Piazzale Aldo Moro 2, I-00185 Rome, Italy

[9] Univ Politecn Cataluna, Ctr Tecnol Vilanova & Geltru, Lab Aplicac Bioacust, Avda Rambla Exposicio S-N, Vilanova I La Geltru 08800, Spain

[10] NCSR Demokritos, Inst Nucl & Particle Phys, Athens 15310, Greece

[11] Ist Nazl Fis Nucl, Sez Genova, Via Dodecaneso 33, I-16146 Genoa, Italy

[12] Univ Granada, Dept Comp Architecture & Technol, CITIC, Granada 18071, Spain

[13] Univ Politecn Valencia, Inst Invest Gest Integrada Zonas Costeras, C Paranimf 1, Gandia 46730, Spain

[14] Natl Inst Subatom Phys, Nikhef, POB 41882, NL-1009 DB Amsterdam, Netherlands

[15] Univ Mohammed V Rabat, Fac Sci, 4 Av Ibn Battouta,BP 1014, Rabat 10000, Morocco

[16] Ist Nazl Fis Nucl, Sez Bologna, Vle C Berti Pichat 6-2, I-40127 Bologna, Italy

[17] Univ Bologna, Dipartimento Fis & Astron, Vle C Berti Pichat 6-2, I-40127 Bologna, Italy

[18] KVI CART Univ Groningen, Groningen, Netherlands

[19] Ist Nazl Fis Nucl, Lab Nazl Sud, Via S Sofia 62, I-95123 Catania, Italy

[20] North West Univ, Ctr Space Res, Private Bag X6001, ZA-2520 Potchefstroom, South Africa

[21] Inst Espanol Oceanog, Unidad Mixta IEO UPV, C Paranimf 1, Gandia 46730, Spain

[22] Univ Mohammed 1, Fac Sci, BV Mohammed VI,BP 717, Oujda 60000, Morocco

[23] Univ Salerno, Dipartimento Matemat, Via Giovanni Paolo II 132, I-84084 Fisciano, Italy

[24] Ist Nazl Fis Nucl, Grp Collegato Salerno, Via Giovanni Paolo II 132, I-84084 Fisciano, Italy

[25] ISS, Atomistilor 409, Magurele 077125, Romania

[26] Univ Amsterdam, Inst Phys, IHEF, POB 94216, NL-1090 GE Amsterdam, Netherlands

[27] TNO, Tech Sci, POB 155, NL-2600 Delft, Netherlands

[28] Univ Campania Luigi Vanvitelli, Dipartimento Matemat & Fis, Viale Lincoln 5, I-81100 Caserta, Italy

[29] Univ Roma La Sapienza, Dipartimento Fis, Piazzale Aldo Moro 2, I-00185 Rome, Italy

[30] Univ Bologna, Dipartimento Ingn Energia Elettr & Informaz Gugli, Via Univ 50, I-47521 Cesena, Italy

[31] Cadi Ayyad Univ, Fac Sci Semlalia, Phys Dept, Av My Abdellah,POB 2390, Marrakech 40000, Morocco

[32] Univ Witwatersrand, Sch Phys, Private Bag 3, ZA-2050 Johannesburg, South Africa

[33] Univ Catania, Dipartimento Fis & Astron Ettore Majorana, Via Santa Sofia 64, I-95123 Catania, Italy

[34] Ist Nazl Fis Nucl, LNF, Via Enrico Fermi 40, I-00044 Frascati, Italy

[35] Ist Nazl Fis Nucl, Sez Bari, Via Orabona 4, I-70125 Bari, Italy

[36] Curtin Univ, Int Ctr Radio Astron Res, Bentley, WA 6102, Australia

[37] Univ Nantes, IMT Atlantique, Subatech, IN2P3 CNRS, 4 Rue Alfred Kastler La Chantrerie,BP 20722, F-44307 Nantes, France

[38] Univ Wurzburg, Emil Fischer Str 31, D-97074 Wurzburg, Germany

[39] Friedrich Alexander Univ Erlangen Nurnberg, Erlangen Ctr Astroparticle Phys, Erwin Rommel Str 1, D-91058 Erlangen, Germany

[40] Western Sydney Univ, Sch Comp Engn & Math, Locked Bag 1797, Penrith, NSW 2751, Australia

[41] Univ Salerno, Dipartimento Fis, Via Giovanni Paolo II 132, I-84084 Fisciano, Italy

[42] Univ Genoa, Via Dodecaneso 33, I-16146 Genoa, Italy

[43] Normandie Univ, ENSICAEN, UNICAEN, CNRS IN2P3,LPC Caen,LPCCAEN, 6 Blvd Marechal Juin, F-14050 Caen, France

[44] Univ Granada, Dept Fis Teor & Cosmos, Granada 18071, Spain

[45] Univ Granada, CAFPE, Granada 18071, Spain

[46] NIOZ Royal Netherlands Inst Sea Res, POB 59, NL-1790 AB Den Burg, Texel, Netherlands

[47] Tbilisi State Univ, Dept Phys 3, Chavchavadze Ave, GE-0179 Tbilisi, Georgia

[48] Leiden Univ, Leiden Inst Phys, POB 9504, NL-2300 Leiden, Netherlands

[49] Natl Ctr Nucl Res, PL-02093 Warsaw, Poland

[50] Inst Univ France, 1 Rue Descartes, F-75005 Paris, France

来源：

EUROPEAN PHYSICAL JOURNAL C | 2022年 / 82卷 / 04期

基金：

美国国家科学基金会;

关键词：

DATA-ACQUISITION SYSTEM;

D O I：

10.1140/epjc/s10052-022-10137-y

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

The KM3NeT research infrastructure is unconstruction in the Mediterranean Sea. KM3NeT will study atmospheric and astrophysical neutrinos with two multi-purpose neutrino detectors, ARCA and ORCA, primarily aimed at GeV-PeV neutrinos. Thanks to the multi-photomultiplier tube design of the digital optical modules, KM3NeT is capable of detecting the neutrino burst from a Galactic or near-Galactic core-collapse supernova. This potential is already exploitable with the first detection units deployed in the sea. This paper describes the real-time implementation of the supernova neutrino search, operating on the two KM3NeT detectors since the first months of 2019. A quasi-online astronomy analysis is introduced to study the time profile of the detected neutrinos for especially significant events. The mechanism of generation and distribution of alerts, as well as the integration into the SNEWS and SNEWS 2.0 global alert systems, are described. The approach for the follow-up of external alerts with a search for a neutrino excess in the archival data is defined. Finally, an overview of the current detector capabilities and a report after the first two years of operation are given.

引用

页数：16

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