Cosmic-Ray Extremely Distributed Observatory

被引：38

作者：

Homola, Piotr ^{[1
]}

Beznosko, Dmitriy ^{[2
]}

Bhatta, Gopal ^{[3
]}

Bibrzycki, Lukasz ^{[4
]}

Borczynska, Michalina ^{[5
]}

Bratek, Lukasz ^{[6
]}

Budnev, Nikolay ^{[7
]}

Burakowski, Dariusz ^{[8
]}

Alvarez-Castillo, David E. ^{[1
,9
]}

Almeida Cheminant, Kevin ^{[1
]}

Cwikla, Aleksander ^{[10
]}

Dam-o, Punsiri ^{[11
]}

Dhital, Niraj ^{[12
]}

Duffy, Alan R. ^{[13
]}

Glownia, Piotr ^{[6
]}

Gorzkiewicz, Krzysztof ^{[1
]}

Gora, Dariusz ^{[1
]}

Gupta, Alok C. ^{[14
]}

Hlavkova, Zuzana ^{[15
]}

Homola, Martin ^{[15
]}

Jalocha, Joanna ^{[6
]}

Kaminski, Robert ^{[1
]}

Karbowiak, Michal ^{[16
]}

Kasztelan, Marcin ^{[17
]}

Kierepko, Renata ^{[1
]}

Knap, Marek ^{[18
]}

Kovacs, Peter ^{[19
]}

Kulinski, Szymon ^{[6
]}

Lozowski, Bartosz ^{[20
]}

Magrys, Marek ^{[21
]}

Medvedev, Mikhail V. ^{[22
,23
]}

Medrala, Justyna ^{[24
]}

Mietelski, Jerzy W. ^{[1
]}

Miszczyk, Justyna ^{[1
]}

Mozgova, Alona ^{[25
]}

Napolitano, Antonio ^{[26
]}

Nazari, Vahab ^{[1
,9
]}

Ng, Y. Jack ^{[27
]}

Niedzwiecki, Michal ^{[10
]}

Oancea, Cristina ^{[28
,29
]}

Ogan, Boguslaw ^{[30
]}

Opila, Gabriela ^{[24
]}

Oziomek, Krzysztof ^{[21
]}

Pawlik, Maciej ^{[21
,24
]}

Piekarczyk, Marcin ^{[4
]}

Poncyljusz, Boezna ^{[5
]}

Pryga, Jerzy ^{[31
]}

Rosas, Matias ^{[32
]}

Rzecki, Krzysztof ^{[24
]}

Zamora-Saa, Jilberto ^{[33
]}

机构：

[1] Polish Acad Sci, Inst Nucl Phys, PL-31342 Krakow, Poland

[2] Clayton State Univ, Dept Chem & Phys, Morrow, GA 30260 USA

[3] Jagiellonian Univ, Astron Observ, PL-30244 Krakow, Poland

[4] Pedag Univ Krakow, Inst Comp Sci, PL-30084 Krakow, Poland

[5] Univ Warsaw, Fac Phys, PL-02093 Warsaw, Poland

[6] Cracow Univ Technol, Inst Phys, PL-30084 Krakow, Poland

[7] Irkutsk State Univ, Irkutsk 664003, Russia

[8] Astroparticle Phys Amateur, PL-30322 Krakow, Poland

[9] Joint Inst Nucl Res, Joliot Curie St 6, Dubna 141980, Russia

[10] Cracow Univ Technol, Fac Comp Sci & Telecommun, Dept Comp Sci, PL-31155 Krakow, Poland

[11] Walailak Univ, Sch Sci, Thasala 80160, Thailand

[12] St Xaviers Coll, Dept Phys, Kathmandu 44600, Nepal

[13] Swinburne Univ Technol, Ctr Astrophys & Supercomp, Melbourne, Vic 3122, Australia

[14] Aryabhatta Res Inst Observat Sci ARIES, Manora Peak 263001, Nainital, India

[15] Comenius Univ, Fac Math Phys & Informat, Bratislava 84248, Slovakia

[16] Univ Lodz, Fac Phys & Appl Informat, 149-153 Pomorska, PL-90236 Lodz, Poland

[17] Natl Ctr Nucl Res, Andrzeja Soltana 7, PL-05400 Otwock, Poland

[18] Astroparticle Phys Amateur, PL-58170 Dobromierz, Poland

[19] Wigner Res Ctr Phys, Inst Particle & Nucl Phys, Konkoly ThegeMiklos Ut 29-33, H-1121 Budapest, Hungary

[20] Univ Silesia Katowice, Fac Nat Sci, Bankowa 9, PL-40007 Katowice, Poland

[21] ACC Cyfronet AGH UST, PL-30950 Krakow, Poland

[22] Univ Kansas, Dept Phys & Astron, Lawrence, KS 66045 USA

[23] MIT, Nucl Sci Lab, Cambridge, MA 02139 USA

[24] AGH Univ Sci & Technol, PL-30059 Krakow, Poland

[25] Natl Univ Kyiv, Astron Observ Taras Shevchenko, UA-04053 Kiev, Ukraine

[26] Univ Napoli Parthenope, I-80143 Naples, Italy

[27] Univ N Carolina, Dept Phys & Astron, Chapel Hill, NC 27599 USA

[28] ADVACAM, Prague 17000, Czech Republic

[29] Univ Bucharest, Bucharest 077125, Romania

[30] Astroparticle Phys Amateur, PL-86170 Nowe, Poland

[31] Jagiellonian Univ, PL-31007 Krakow, Poland

[32] Inst Secondary Educ, Highsch 65, Montevideo 12000, Uruguay

[33] Univ Andres Bello, Dept Ciencias Fisicas, Piso 7,Sazie 2212, Santiago, Chile

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

[35] Publ Szkola Podstawowa Sw Jadwigi Krolowej Rzezaw, PL-32765 Rzezawa, Poland

[36] Tbilisi State Univ, E Andronikashvili Inst Phys, Tbilisi 0177, Georgia

[37] Univ Waterloo, Waterloo Rocketry, Waterloo, ON N2L 3G1, Canada

[38] Silesian Univ Opava, Inst Phys, Res Ctr Theoret Phys & Astrophys, Bezrucovo Nam 13, CZ-74601 Opava, Czech Republic

[39] Univ Extremadura, Dept Phys, Merida 06800, Spain

来源：

SYMMETRY-BASEL | 2020年 / 12卷 / 11期

关键词：

cosmic rays; cosmic-ray ensembles; extensive air showers; large scale cosmic-ray correlations; CREDO Collaboration; ENERGY PHOTON PROPAGATION; CP CONSERVATION; MAGNETIC-FIELDS; PENROSE PROCESS; BLACK-HOLES; RADIATION; SPECTRUM; EARTHQUAKE; SEARCH; EXTRACTION;

D O I：

10.3390/sym12111835

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

The Cosmic-Ray Extremely Distributed Observatory (CREDO) is a newly formed, global collaboration dedicated to observing and studying cosmic rays (CR) and cosmic-ray ensembles (CRE): groups of at least two CR with a common primary interaction vertex or the same parent particle. The CREDO program embraces testing known CR and CRE scenarios, and preparing to observe unexpected physics, it is also suitable for multi-messenger and multi-mission applications. Perfectly matched to CREDO capabilities, CRE could be formed both within classical models (e.g., as products of photon-photon interactions), and exotic scenarios (e.g., as results of decay of Super-Heavy Dark Matter particles). Their fronts might be significantly extended in space and time, and they might include cosmic rays of energies spanning the whole cosmic-ray energy spectrum, with a footprint composed of at least two extensive air showers with correlated arrival directions and arrival times. As the CRE are predominantly expected to be spread over large areas and, due to the expected wide energy range of the contributing particles, such a CRE detection might only be feasible when using all available cosmic-ray infrastructure collectively, i.e., as a globally extended network of detectors. Thus, with this review article, the CREDO Collaboration invites the astroparticle physics community to actively join or to contribute to the research dedicated to CRE and, in particular, to pool together cosmic-ray data to support specific CRE detection strategies.

引用

页码：1 / 55

页数：55

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