Astronomy potential of KM3NeT/ARCA

被引：2

作者：

Aiello, S. ^{[1
]}

Albert, A. ^{[2
,57
]}

Alshamsi, M. ^{[3
,4
]}

Garre, S. Alves ^{[5
]}

Aly, Z. ^{[3
]}

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

Ameli, F. ^{[8
]}

Andre, M. ^{[9
]}

Androutsou, E. ^{[10
]}

Anguita, M. ^{[11
]}

Aphecetche, L. ^{[12
]}

Ardid, M. ^{[13
]}

Ardid, S. ^{[13
]}

Atmani, H. ^{[14
]}

Aublin, J. ^{[15
]}

Badaracco, F. ^{[16
]}

Bailly-Salins, L. ^{[17
]}

Bardacova, Z. ^{[18
,19
]}

Baret, B. ^{[15
]}

Bariego-Quintana, A. ^{[5
]}

Baruzzi, A. ^{[16
]}

du Pree, S. Basegmez ^{[20
]}

Becherini, Y. ^{[15
]}

Bendahman, M. ^{[14
,15
]}

Benfenati, F. ^{[21
,22
]}

Benhassi, M. ^{[6
,23
]}

Benoit, D. M. ^{[24
]}

Berbee, E. ^{[20
]}

Bertin, V ^{[3
]}

Biagi, S. ^{[25
]}

Boettcher, M. ^{[26
]}

Bonanno, D. ^{[25
]}

Boumaaza, J. ^{[14
]}

Bouta, M. ^{[27
]}

Bouwhuis, M. ^{[20
]}

Bozza, C. ^{[6
,28
,29
]}

Bozza, R. M. ^{[6
,7
]}

Branzas, H. ^{[30
]}

Bretaudeau, F. ^{[12
]}

Breuhaus, M. ^{[3
]}

Bruijn, R. ^{[20
,31
]}

Brunner, J. ^{[3
]}

Bruno, R. ^{[1
]}

Buis, E. ^{[20
,32
]}

Buompane, R. ^{[6
,23
]}

Busto, J. ^{[3
]}

Caiffi, B. ^{[16
]}

Calvo, D. ^{[5
]}

Campion, S. ^{[8
,33
]}

Capone, A. ^{[8
,33
]}

机构：

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

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

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

[4] Univ Sharjah, Sharjah Acad Astron Space Sci & Technol, Univ Campus,POB 27272, Sharjah, U Arab Emirates

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

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

[7] Univ Napoli Federico II, Complesso Univ Monte S Angelo, Dip Sci Fis E Pancini, Via Cintia Ed 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] Univ Granada, Dept Comp Architecture & Technol, CITIC, Granada 18071, Spain

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

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

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

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

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

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

[18] Czech Tech Univ, Inst Expt & Appl Phys, Husova 240-5, Prague 11000, Czech Republic

[19] Comenius Univ, Dept Nucl Phys & Biophys, Mlynska Dolina F1, Bratislava 84248, Slovakia

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

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

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

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

[24] Univ Hull, EA Milne Ctr Astrophys, Kingston Upon Hull HU6 7RX, N Humberside, England

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

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

[27] Univ Mohammed 1, Fac Sci, BV Mohammed 6,BP 717, Oujda 60000, Morocco

[28] Univ Salerno, Via Giovanni Paolo II 132, I-84084 Fisciano, Italy

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

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

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

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

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

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

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

[36] Friedrich Alexander Univ Erlangen Nurnberg FAU, Erlangen Ctr Astroparticle Phys, Nikolaus Fiebiger Str 2, D-91058 Erlangen, Germany

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

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

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

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

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

[42] IN2P3, LPC, Campus Cezeaux 24,Ave Landais,BP 80026, F-63171 Aubiere, France

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

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

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

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

[50] Univ Georgia, Inst Phys, Kostava Str 77, GE-0171 Tbilisi, Georgia

来源：

EUROPEAN PHYSICAL JOURNAL C | 2024年 / 84卷 / 09期

基金：

欧盟地平线“2020”; 美国国家科学基金会;

关键词：

33;

D O I：

10.1140/epjc/s10052-024-13137-2

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/ARCA neutrino detector is currently under construction at 3500 m depth offshore Capo Passero, Sicily, in the Mediterranean Sea. The main science objectives are the detection of high-energy cosmic neutrinos and the discovery of their sources. Simulations were conducted for the full KM3NeT/ARCA detector, instrumenting a volume of 1 km(3), to estimate the sensitivity and discovery potential to point-like neutrino sources. This paper covers the reconstruction of track- and shower-like signatures, as well as the criteria employed for neutrino event selection. With an angular resolution below 0.1 degrees for tracks and under 2 degrees for showers, the sensitivity to point-like neutrino sources surpasses existing observed limits across the entire sky.

引用

页数：17

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