Cosmic-Ray Extremely Distributed Observatory: Difference between revisions

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'''Cosmic-Ray Extremely Distributed Observatory (CREDO)''' – scientific project initiated at the end of August 2016 by Polish scientists from [[Instytut Fizyki Jądrowej im. Henryka Niewodniczańskiego PAN|Institute of Nuclear Physics PAN]] in [[Kraków]] (Researchers from the Czech Republic, Slovakia and Hungary also joined the project) whose purpose is the detection of [[cosmic ray]]s and the search for [[dark matter]].<ref>https://credo.science/credo-read-more/</ref> Its aim is to involve as many people as possible in the construction of a global system of cosmic ray detectors, thanks to which it will be possible to examine the essence of dark matter. Thanks to a [[photosensitive sensor]] and a [[GPS module]], a [[smartphone]] works perfectly as a detector that reaches particles from space.<ref>https://arxiv.org/abs/1709.05230</ref><ref>https://indico.ifj.edu.pl/event/182/overview</ref><ref>https://www.ncbj.gov.pl/seminaria/cosmic-ray-extremely-distributed-observatory-novel-astrophysical-potential-and-beyond</ref>

== The main objective of the Cosmic-Ray Extremely Distributed Observatory (CREDO) ==

Is the detection and analysis of extended cosmic ray phenomena, so-called super -preshowers (SPS), using existing as well as new in- frastructure (cosmic-ray observatories, educational detectors, single detectors etc.). The search for ensembles of cosmic ray events initiated by SPS is yet an untouched ground, in contrast to the current state-of-the-art analysis,which is focused on the detection of single cosmic ray events. Theoretical explanation of SPS could be given either within classical (e.g., photon-photon interaction) or exotic (e.g., Super Heavy Dark Matter decay or annihilation)

scenarios, thus detection of SPS would provide a better understanding of particle physics, high energy astrophysicsand cosmology. The ensembles of cosmic rays can be classifiedbased on the spatial and temporal extent of particlesconstituting the ensemble. Some classes of SPS are predicted to have huge spatial distribution, a unique signaturedetectable only with a facility of the global size. Since dev

elopment and commissioning of a completely new facilitywith such requirements is economically unwarranted and time-consuming, the global n analysis goals are achievable when all types of existing detectors are merged into a worldwide network. The idea to use the instruments in operation is based on a novel trigger algorithm: in parallel to looking for neighbour surface detectors receiving the signal simultaneously, one should also look for spatially i solated stations clustered in a small time window. On the other hand, CREDO strategy is also aimed at an active engagem ent of a large number of participants, who will contribute to the project by using common electronic devices (e.g., smartphones), capable of detecting cosmic rays. It will help not only in expanding the geographical spread of

CREDO, but also in managing a large manpowernecessary for a more efficient crowd-sourced pattern recognition scheme to identify and classify SPS. A worldwidenetwork of cosmic-ray detectors could not only become a unique tool to study fundamental physics, it will also

provide a number of other opportunities, including space-weather or geophysics studies. Among the latter one hasto list the potential to predict earthquakes by monitoring the rate of low energy cosmic-ray events. The diversity of goals motivates us to advertise this concept across the astroparticle physics community. <ref>https://arxiv.org/pdf/1709.05230.pdf</ref><ref>http://inspirehep.net/record/1623988/plots</ref><ref>https://icd.desy.de/e49245/</ref><ref>http://www.intibs.pl/en/seminars/current-seminars/seminar/1002.html</ref>

== Application credo ==