Cosmic-Ray Extremely Distributed Observatory: Difference between revisions

Revision as of 06:01, 5 October 2018

Latest revision as of 18:37, 24 December 2023

(36 intermediate revisions by 12 users not shown)

Line 1:

[[File:CredoCREDO Detector 2018-zdjecie10-czasteczki17 06.38.34.040 local time.png|thumb|Particle registered by telephoneCREDO detector|alt=]]

{{tone|date=March 2018}}

'''Cosmic-Ray Extremely Distributed Observatory (CREDO)''' –is a scientific project initiated at the end of August 2016 by Polish scientists from the [[InstytutInstitute Fizykiof JądrowejNuclear im.Physics HenrykaPolish NiewodniczańskiegoAcademy of PANSciences|Institute of Nuclear Physics PAN]] in [[Kraków]] (Researchersresearchers 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>{{Cite web |url=https://credo.science/testnowy/credo-read-more/ |title=Cosmic Ray Extremely Distributed Observatory}}</ref> Its aim is to involve as many people as possible in the construction of a global system of cosmic ray detectors, thanks tofrom which it will be possible to examine the essence of dark matter. Thanks toHaving a [[photosensitive sensor]]camera and a [[GPS]] module]], a [[smartphone]] works perfectlywell as a detector that reachesof particles from space.<ref name="aasp">https://{{Cite journal |arxiv.org/abs/ = 1709.05230|doi = 10.17721/2227-1481.7.23-29|title = Cosmic-Ray Extremely Distributed Observatory: a global cosmic ray detection framework|journal = Advances in Astronomy and Space Physics|volume = 7|issue = 1–2|pages = 23–29|year = 2017|last1 = Sushchov|first1 = O.|last2 = Homola|first2 = P.|last3 = Dhital|first3 = N.|last4 = Bratek|first4 = Ł.|last5 = Poznański|first5 = P.|last6 = Wibig|first6 = T.|last7 = Zamora-Saa|first7 = J.|last8 = Almeida Cheminant|first8 = K.|last9 = Alvarez Castillo|first9 = D.|last10 = Góra|first10 = D.|last11 = Jagoda|first11 = P.|last12 = Jałocha|first12 = J.|last13 = Jarvis|first13 = J. F.|last14 = Kasztelan|first14 = M.|last15 = Kopański|first15 = K.|last16 = Krupiński|first16 = M.|last17 = Michałek|first17 = M.|last18 = Nazari|first18 = V.|last19 = Smelcerz|first19 = K.|last20 = Smolek|first20 = K.|last21 = Stasielak|first21 = J.|last22 = Sułek|first22 = M.|bibcode = 2017AASP....7...23S|s2cid = 119402212}}</ref><ref>{{Cite web | url=https://indico.ifj.edu.pl/event/182/overview |title = Cosmic-Ray Extremely Distributed Observatory 2017: The Anniversary Symposium (Aug 30) and Collaboration Meeting (Aug 31) (30-31 August 2017) · Institute of Nuclear Physics Polish Academy of Sciences (Indico)}}</ref><ref>{{Cite web | url=https://www.ncbj.gov.pl/seminaria/cosmic-ray-extremely-distributed-observatory-novel-astrophysical-potential-and-beyond |title = Cosmic-Ray Extremely Distributed Observatory: Novel astrophysical potential and beyond}}</ref>

== Objective ==

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

The main objective of CREDO is the detection and analysis of extended cosmic ray phenomena, so-called super-preshowers (SPS), using existing as well as new infrastructure (cosmic-ray observatories, educational detectors, single detectors etc.). The search for ensembles of cosmic ray events initiated by SPS is yet an untouched topic, 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 astronomy|high energy astrophysics]] and [[cosmology]]. The ensembles of cosmic rays can be classified based on the spatial and temporal extent of particles constituting the ensemble. Some classes of SPS are predicted to have huge spatial distribution, a unique signature detectable only with a facility of global size. Since development and commissioning of a completely new facility with such requirements is economically unwarranted and time-consuming, the global 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 isolated stations clustered in a small time window. On the other hand, CREDO's strategy is also aimed at an active engagement 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 manpower necessary for a more efficient crowd-sourced pattern recognition scheme to identify and classify SPS. A worldwide network 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 can list the potential to predict [[earthquakes]] by monitoring the rate of low energy cosmic-ray events. This diversity of potential applications has motivated the researchers to advertise the concept across the astroparticle physics community.<ref name="aasp"/><ref>{{cite web |url=https://icd.desy.de/e49245/ |title=Global Cosmic Ray Studies |website=DESY Deutsches Elektronen-Synchrotron |access-date=2018-03-22 |archive-date=2018-02-03 |archive-url=https://web.archive.org/web/20180203212718/https://icd.desy.de/e49245/ |url-status=dead }}</ref><ref>{{Cite web | url=http://www.intibs.pl/en/seminars/current-seminars/seminar/1002.html |title = Cosmic-Ray Extremely Distributed Observatory: New research possibilities in astroparticle physics &#124; Seminar of the Institute of Theoretical Physics of University of Wrocław &#124; INTiBS}}</ref><ref>{{cite web |url=http://www.oa.uj.edu.pl/2017czastki/homola.pdf |title=CosmicRay Extremely Distributed Observatory |author=Piotr Homola |date=20 September 2017 |website=oa.uj.edu.pl}}</ref>

Is the detection and analysis of extended cosmic ray phenomena, so-called super-preshowers (SPS), using existing as well as new infrastructure (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><ref>http://www.oa.uj.edu.pl/2017czastki/homola.pdf</ref>

== Application credoImplementation ==

The user must install an [[Application software|application]] that turns histheir phone into a cosmic ray detector, connect it to the charger and arrange it horizontally,; for example, put it on a table or bedside cabinet. It is also important that the cameras of thisthe device are well covered, for example with a piece of black adhesive tape, and notifications indicated by the blinking of thelights diodesare areturned off. If a radiation particle passes through a photosensitive matrix in the phone, it will stimulate several pixels, which will be noticed by the program that sends information to the server. Thanks to the GPS module, youthe will also know wheretime and whenplace of the event tookis placealso known.

All data from smartphones will then be analyzed together in the [http://www.cyfronet.krakow.pl/en/ Academic Computer Center Cyfronet AGH], which will keep youparticipants informed about the progress of the search for signs of high-energy particles.

By 2020 the application is still under testing and may not produce the expected results on some mobile devices.<ref>{{cite web |url=https://indico.cern.ch/event/596002/contributions/2447178/attachments/1412820/2161711/credo-highlight-hq.pdf |title=Cosmic-Ray Extremely Distributed Observatory (CREDO) |website=[[CERN]]}}</ref><ref>{{cite journal |url=http://aasp.kiev.ua/volume7/23-29-Sushchov.pdf |doi=10.17721/2227-1481.7.23-29 |via=[[ResearchGate]]|title=Cosmic-Ray Extremely Distributed Observatory: A global cosmic ray detection framework |year=2017 |last1=Sushchov |first1=O. |last2=Homola |first2=P. |last3=Dhital |first3=N. |last4=Bratek |first4=Ł. |last5=Poznański |first5=P. |last6=Wibig |first6=T. |last7=Zamora-Saa |first7=J. |last8=Almeida Cheminant |first8=K. |last9=Alvarez Castillo |first9=D. |last10=Góra |first10=D. |last11=Jagoda |first11=P. |last12=Jałocha |first12=J. |last13=Jarvis |first13=J. F. |last14=Kasztelan |first14=M. |last15=Kopański |first15=K. |last16=Krupiński |first16=M. |last17=Michałek |first17=M. |last18=Nazari |first18=V. |last19=Smelcerz |first19=K. |last20=Smolek |first20=K. |last21=Stasielak |first21=J. |last22=Sułek |first22=M. |journal=Advances in Astronomy and Space Physics |volume=7 |issue=1–2 |pages=23–29 |arxiv=1709.05230 |bibcode=2017AASP....7...23S |s2cid=119402212 }}</ref><ref>{{cite journal |url=https://www.researchgate.net/publication/319875663 |arxiv=1709.05230 |via=[[ResearchGate]]|doi=10.17721/2227-1481.7.23-29 |title=Cosmic-Ray Extremely Distributed Observatory: A global cosmic ray detection framework |year=2017 |last1=Sushchov |first1=O. |last2=Homola |first2=P. |last3=Dhital |first3=N. |last4=Bratek |first4=Ł. |last5=Poznański |first5=P. |last6=Wibig |first6=T. |last7=Zamora-Saa |first7=J. |last8=Almeida Cheminant |first8=K. |last9=Alvarez Castillo |first9=D. |last10=Góra |first10=D. |last11=Jagoda |first11=P. |last12=Jałocha |first12=J. |last13=Jarvis |first13=J. F. |last14=Kasztelan |first14=M. |last15=Kopański |first15=K. |last16=Krupiński |first16=M. |last17=Michałek |first17=M. |last18=Nazari |first18=V. |last19=Smelcerz |first19=K. |last20=Smolek |first20=K. |last21=Stasielak |first21=J. |last22=Sułek |first22=M. |journal=Advances in Astronomy and Space Physics |volume=7 |issue=1–2 |pages=23–29 |bibcode=2017AASP....7...23S |s2cid=119402212 }}

The application is still under testing and may not produce the expected results on some mobile devices.<ref>https://indico.cern.ch/event/596002/contributions/2447178/attachments/1412820/2161711/credo-highlight-hq.pdf</ref><ref>http://aasp.kiev.ua/volume7/23-29-Sushchov.pdf</ref><ref>https://www.researchgate.net/publication/319875663_Cosmic-Ray_Extremely_Distributed_Observatory_a_global_cosmic_ray_detection_framework</ref><ref>https://www.utef.cvut.cz/seminars/2017-02-21/cosmic-ray-extremely-distributed-observatory:-new-research--possibilities-in-astroparticle-physics</ref>

</ref><ref>{{Cite web|url=http://www.utef.cvut.cz/seminars/2017-02-21/cosmic-ray-extremely-distributed-observatory:-new-research--possibilities-in-astroparticle-physics|title = IEAP - Piotr Homola: Cosmic-Ray Extremely Distributed Observatory: New research possibilities in astroparticle physics}}</ref>

== Preview of collected data ==

All traces of particles registered by smartphones can be viewed on a dedicated [https://api.credo.science dedicated/web/ website]. Their size and shape depends on the type and energy of the captured particle and the direction from which it came.

{| class="wikitable sortable"

Line 31 ⟶ 27:

!Date

|-

|10,695,152

|548,298

|13831

|975

|11096

|107

|20182021 - 0305

|}

== External links ==

* [http://credo.science Project page]

* [https://api.credo.science PreviewDetected detectionevents]

*[https://credo.science/credodetektor/ Polish board] {{Webarchive|url=https://web.archive.org/web/20180317035853/https://credo.science/credodetektor/ |date=2018-03-17 }}

* [https://www.zooniverse.org/projects/credo/dark-universe-welcome Dark Universe]

* [https://credo.science/credodetector/ English board] {{Webarchive|url=https://web.archive.org/web/20180317035720/https://credo.science/credodetector/ |date=2018-03-17 }}

* [https://www.zooniverse.org/projects/credo/private-particle-detective zooniverse]

* [https://www.youtube.com/watch?v=6rHnW--PZQk&t=1s Video about credoCREDO]

* [https://credo.science/credodetektor/ Polish board]

* [https://credo.science/credodetector#/science/publications EnglishCREDO board]Scientific publications]

* [https://credo.science/credodetector/viewtopic.php?t=5&f=3#p5 Mini tutorial]

* [https://www.youtube.com/watch?v=6rHnW--PZQk&t=1s Video about credo]

== References ==

Line 52 ⟶ 45:

[[Category:Astronomy in Poland]]

[[Category:Astronomy projects]]

[[Category:Citizen science]]