Extensive air showers event reconstruction using spatial and temporary particle distribution at Horizon-T experiment

Beznosko, D.; Yelshibekov, K; Beisembaev, R. U.; Beisembaeva, Elena; Beremkulov, T.; Iakovlev, Alexander; Jakupov, S.; Sheverdin, Arsen; Tagay, Z; Uakhitov, Tileubek; Vildanova, Marina; Zhukov, V. V.

doi:10.1088/1742-6596/1342/1/012136

Cited by 4 publications

(3 citation statements)

References 3 publications

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“…However, there is an unused piece of information here. As the EAS disk passes the detection level, the detectors can measure not only the integral number of detected particles but their distribution over time as well, getting an effective width of the disk [161]. This technique was first developed and used at the Horizon-T [162] experiment that holds close ties with the CREDO collaboration.…”

Section: Cosmic-ray Detection Techniquesmentioning

confidence: 99%

Cosmic-Ray Extremely Distributed Observatory

et al. 2020

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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.

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Section: Cosmic-ray Detection Techniquesmentioning

confidence: 99%

Cosmic-Ray Extremely Distributed Observatory

et al. 2020

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show abstract

“…However, there is an unused piece of information here. As the EAS disk passes the detection level, the detectors can measure not only the integral number of detected particles but their distribution over time as well, getting an effective width of the disk [164]. This technique was first developed and used at the Horizon-T [165] experiment that holds close ties with the CREDO collaboration.…”

Section: Cosmic Ray Detection Techniquesmentioning

confidence: 99%

Cosmic Ray Extremely Distributed Observatory

Homola¹,

Beznosko²,

Bhatta³

et al. 2020

Preprint

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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 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. CRE are expected to be partially observable on Earth even if the initiating interaction or process occurs as far as ~1 Gpc away. They would have a footprint composed of at least two extensive air showers with correlated arrival directions and arrival times. Since CRE are mostly expected to be spread over large areas and, because of the expected wide energy range of the contributing particles, CRE detection might only be feasible when using 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 share any cosmic ray data useful for the specific CRE detection strategies.

show abstract

“…However, there is an unused piece of information here. As the EAS disk passes the detection level, the detectors can measure not only the integral number of detected particles but their distribution over time as well, getting an effective width of the disk [164]. This technique was first developed and used at the Horizon-T [165] experiment that holds close ties with the CREDO collaboration.…”

Section: Cosmic Ray Detection Techniquesmentioning

confidence: 99%

Cosmic Ray Extremely Distributed Observatory

Homola,

Beznosko,

Bhatta

et al. 2020

Preprint

View full text Add to dashboard Cite

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 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. Since CRE are mostly expected to be spread over large areas and, because of the expected wide energy range of the contributing particles, CRE detection might only be feasible when using 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 share any cosmic ray data useful for the specific CRE detection strategies.

show abstract

Extensive air showers event reconstruction using spatial and temporary particle distribution at Horizon-T experiment

Cited by 4 publications

References 3 publications

Cosmic-Ray Extremely Distributed Observatory

Cosmic-Ray Extremely Distributed Observatory

Cosmic Ray Extremely Distributed Observatory

Cosmic Ray Extremely Distributed Observatory

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