Zobrazeno 1 - 10
of 97
pro vyhledávání: '"Stasielak, Jaroslaw"'
Autor:
Alvarez-Castillo, David, Homola, Piotr, Sushchov, Oleksandr, Stasielak, Jarosław, Stuglik, Sławomir, Góra, Dariusz, Nazari, Vahab, Oancea, Cristina, Granja, Carlos, Beznosko, Dmitriy, Zabari, Noemi, Gupta, Alok C., Hnatyk, Bohdan, Mozgova, Alona, Kasztelan, Marcin, Bielewicz, Marcin, Kovacs, Peter, Łozowski, Bartosz, Medvedev, Mikhail V., Miszczyk, Justyna, Bibrzycki, Łukasz, Niedźwiecki, Michał, Smelcerz, Katarzyna, Piekarczyk, Tomasz Hachaj Marcin, Pawlik, Maciej, Rzecki, Krzysztof, Rosas, Matías, Smolek, Karel, Svanidze, Manana, Beradze, Revaz, Tursunov, Arman, Wibig, Tadeusz, Zamora-Saa, Jilberto, Poncyljusz, Bożena, Mędrala, Justyna, Opiła, Gabriela, Pryga, Jerzy, Ruimi, Ophir, Cahuantzi, Mario Rodriguez
Publikováno v:
Rev. Mex. Fis. 4(2) 021123 1-8 (2023)
This contribution presents the recent research developments within the Cosmic Ray Extremely Distributed Observatory (CREDO) in the search for resolution of various scientific puzzles, ranging from fundamental physical questions to applications like t
Externí odkaz:
http://arxiv.org/abs/2403.03916
Autor:
Alvarez-Castillo, David, Homola, Piotr, Poncyljusz, Bożena, Gora, Dariusz, Dhital, Niraj, Sushchov, Oleksandr, Stasielak, Jarosław, Stuglik, Sławomir, Nazari, Vahab, Oancea, Cristina, Beznosko, Dmitriy, Zabari, Noemi, Gupta, Alok C., Hnatyk, Bohdan, Mozgova, Alona, Kasztelan, Marcin, Bielewicz, Marcin, Kovacs, Peter, Łozowski, Bartosz, Medvedev, Mikhail V., Miszczyk, Justyna, Bibrzycki, Łukasz, Niedźwiecki, Michał, Smelcerz, Katarzyna, Hachaj, Tomasz, Piekarczyk, Marcin, Pawlik, Maciej, Rzecki, Krzysztof, Rosas, Matías, Smolek, Karel, Svanidze, Manana, Beradze, Revaz, Tursunov, Arman, Wibig, Tadeusz, Zamora-Saa, Jilberto, Mędrala, Justyna, Opiła, Gabriela, Pryga, Jerzy, Ruimi, Ophir, Cahuantzi, Mario Rodriguez
Publikováno v:
PoS(ICRC2023)446
In this contribution we study the possibility of the formation of cosmic ray ensembles (CRE) created by the interaction of ultra-high energy (UHE) photons with the magnetic field of the Sun. The lack of observation of those UHE and the difficulties f
Externí odkaz:
http://arxiv.org/abs/2309.15256
Autor:
Cheminant, Kevin Almeida, Gora, Dariusz, Borodai, Nataliia, Engel, Ralph, Pierog, Tanguy, Pekala, Jan, Roth, Markus, Stasielak, Jarosław, Unger, Michael, Veberic, Darko, Wilczynski, Henryk
The number of muons in an air shower is a strong indicator of the mass of the primary particle and increases with a small power of the cosmic ray mass by the $\beta$-exponent, $N_{\mu} \sim A^{(1-\beta)}$. This behaviour can be explained in terms of
Externí odkaz:
http://arxiv.org/abs/2308.16525
Autor:
Cheminant, Kevin Almeida, Góra, Dariusz, Borodai, Nataliia, Engel, Ralph, Pierog, Tanguy, Pękala, Jan, Roth, Markus, Stasielak, Jarosław, Unger, Michael, Veberič, Darko, Wilczyński, Henryk
Simulations of extensive air showers using current hadronic interaction models predict too small numbers of muons compared to events observed in the air-shower experiments, which is known as the muon-deficit problem. In this work, we present a new me
Externí odkaz:
http://arxiv.org/abs/2302.07932
Autor:
Poncyljusz, Bożena, Bulik, Tomasz, Dhital, Niraj, Sushchov, Oleksandr, Stuglik, Sławomir, Homola, Piotr, Alvarez-Castillo, David, Piekarczyk, Marcin, Wibig, Tadeusz, Stasielak, Jaroslaw, Kovács, Péter, Smelcerz, Katarzyna, Frias, M D Rodriguez, Niedźwiecki, Michał, Miszczyk, Justyna, Sośnicki, Tomasz, Bibrzycki, Łukasz, Tursunov, Arman, Del Peral, Luis, Rzecki, Krzysztof
Publikováno v:
Universe 8 (2022) 498
Both the lack of observation of ultra-high energy (UHE) photons and the limitations of the state-of-the-art methodology being applied for their identification motivate studies on alternative approaches to the relevant simulations and the related obse
Externí odkaz:
http://arxiv.org/abs/2205.14266
Autor:
Alvarez-Castillo, David E., Sushchov, Oleksandr, Homola, Piotr, Beznosko, Dmitriy, Budnev, Nikolai, Góra, Dariusz, Gupta, Alok C., Hnatyk, Bohdan, Kasztelan, Marcin, Kovacs, Peter, Łozowski, Bartosz, Medvedev, Mikhail V., Miszczyk, Justyna, Mozgova, Alona, Nazari, Vahab, Niedźwiecki, Michał, Pawlik, Maciej, Rosas, Matías, Rzecki, Krzysztof, Smelcerz, Katarzyna, Smolek, Karel, Stasielak, Jarosław, Stuglik, Sławomir, Svanidze, Manana, Tursunov, Arman, Verbetsky, Yuri, Wibig, Tadeusz, Zamora-Saa, Jilberto, Poncyljusz, Bożena, Mędrala, Justyna, Opiła, Gabriela, Bibrzyck, Łukasz, Piekarczyk, Marcin
Cosmic Ray Ensembles (CRE) are yet not observed groups of cosmic rays with a common primary interaction vertex or the same parent particle. One of the processes capable of initiating identifiable CRE is an interaction of an ultra-high energy (UHE) ph
Externí odkaz:
http://arxiv.org/abs/2112.11421
Autor:
Stasielak, Jaroslaw
Ultra-high-energy cosmic rays (UHECRs) are studied with giant ground-based detector systems recording extensive air showers, induced by cosmic ray particles in the atmosphere. Research at the Pierre Auger Observatory - the largest of such detectors e
Externí odkaz:
http://arxiv.org/abs/2110.09487
Autor:
Bibrzycki, Łukasz, Alvarez-Castillo, David, Bar, Olaf, Gora, Dariusz, Homola, Piotr, Kovács, Péter, Niedźwiecki, Michał, Piekarczyk, Marcin, Rzecki, Krzysztof, Stasielak, Jaroslaw, Stuglik, Sławomir, Sushchov, Oleksandr, Tursunov, Arman
The wealth of smartphone data collected by the Cosmic Ray Extremely Distributed Observatory(CREDO) greatly surpasses the capabilities of manual analysis. So, efficient means of rejectingthe non-cosmic-ray noise and identification of signals attributa
Externí odkaz:
http://arxiv.org/abs/2110.00297
Autor:
Góra, Dariusz, Borodai, Nataliia, Engel, Ralph, Pierog, Tanguy, Pękala, Jan, Roth, Markus, Stasielak, Jaroslaw, Unger, Michael, Veberic, Darko, Wilczyński, Henryk
Publikováno v:
PoS(ICRC2021)207
The number of muons in extensive air showers predicted using LHC-tuned hadronic interaction models, such as EPOS-LHC and QGSJetII-04, is smaller than observed in showers recorded by leading cosmic ray experiments. In this paper, we present a new meth
Externí odkaz:
http://arxiv.org/abs/2108.07527
Autor:
Homola, Piotr, Beznosko, Dmitriy, Bhatta, Gopal, Bibrzycki, Lukasz, Borczynska, Michalina, Bratek, Lukasz, Budnev, Nikolai, Burakowski, Dariusz, Alvarez-Castillo, David E., Cheminant, Kevin Almeida, Cwikla, Aleksander, Dam-o, Punsiri, Dhital, Niraj, Duffy, Alan R., Glownia, Piotr, Gorzkiewicz, Krzysztof, Gora, Dariusz, Gupta, Alok C., Hlavkova, Zuzana, Homola, Martin, Jalocha, Joanna, Kaminski, Robert, Karbowiak, Michal, Kasztelan, Marcin, Kierepko, Renata, Knap, Marek, Kovacs, Peter, Kulinski, Szymon, Lozowski, Bartosz, Magrys, Marek, Medvedev, Mikhail V., Medrala, Justyna, Mietelski, Jerzy W., Miszczyk, Justyna, Mozgova, Alona, Napolitano, Antonio, Nazari, Vahab, Ng, Y. Jack, Niedzwiecki, Michal, Oancea, Cristina, Ogan, Boguslaw, Opila, Gabriela, Oziomek, Krzysztof, Pawlik, Maciej, Piekarczyk, Marcin, Poncyliusz, Bozena, Pryga, Jerzy, Rosas, Matias, Rzecki, Krzysztof, Zamora-Saa, Jilberto, Smelcerz, Katarzyna, Smolek, Karel, Stanek, Weronika, Stasielak, Jaroslaw, Stuglik, Slawomir, Sulma, Jolanta, Sushchov, Oleksandr, Svanidze, Manana, Tam, Kyle, Tursunov, Arman, Vaquero, Jose M., Wibig, Tadeusz, Wozniak, Krzysztof W.
Publikováno v:
Symmetry 2020, 12(11), 1835
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 a minimum of two CR with a common primary interaction vert
Externí odkaz:
http://arxiv.org/abs/2010.08351