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CREDO: a citizen science initiative for astroparticle physics P - - PowerPoint PPT Presentation

Introduction and motivation Cosmic Ray Ensembles (CRE) CREDO app Other applications Summary CREDO: a citizen science initiative for astroparticle physics P eter Kov acs Wigner Research Centre for Physics kovacs.peter@wigner.mta.hu


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Introduction and motivation Cosmic Ray Ensembles (CRE) CREDO app Other applications Summary

CREDO: a citizen science initiative for astroparticle physics

P´ eter Kov´ acs

Wigner Research Centre for Physics kovacs.peter@wigner.mta.hu supported by:

7 September 2018 ELFT Summer School, M´ atrah´ aza

Many slides were borrowed from Piotr Homola (with his permission)

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Introduction and motivation Cosmic Ray Ensembles (CRE) CREDO app Other applications Summary

Overview

1

Introduction and motivation Pierre Auger Observatory

2

Cosmic Ray Ensembles (CRE)

3

CREDO app

4

Other applications Earthquake prediction

5

Summary

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Introduction and motivation Cosmic Ray Ensembles (CRE) CREDO app Other applications Summary

Cosmic rays, discovery

P a r t i c l e s c

  • m

i n g t

  • E

a r t h f r

  • m

S p a c e 1 9 1 2 . E l e c t r

  • s

c

  • p

e s d i s c h a r g e f a s t e r w i t h i n c r e a s i n g a l t i t u d e → r a y s

  • f

e x t r a t e r r e s t r i a l

  • r

i g i n : V . H e s s ( N

  • b

e l p r i z e 1 9 3 6 ) . 1 9 3 2 . D i s c

  • v

e r y

  • f

a n t i m a t t e r ( p

  • s

i t r

  • n

) : C . A n d e r s

  • n

( N

  • b

e l p r i z e 1 9 3 6 ) . 1 9 3 7 . D i s c

  • v

e r y

  • f

m u

  • n

s : S . N e d d e r m e y e r a n d C . A n d e r s

  • n

→ p a r t i c l e p h y s i c s b e g i n s . 1 9 3 8 . E x t e n s i v e a i r s h

  • w

e r s ( E A S ) → E > 1

1 5

e V : P . A u g e r 1 9 6 2 . F i r s t E A S a t 1

2

e V : J . L i n s l e y → w h a t a n d w h y c a n h a v e s

  • h

u g e e n e r g i e s ? ? ? . . . . h i g h t i m e f

  • r

a n e x t b r e a k t h r

  • u

g h ?

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Introduction and motivation Cosmic Ray Ensembles (CRE) CREDO app Other applications Summary

Cosmic rays, flux vs. energy

R a n g e s : e n e r g y : > 1

  • r

d e r s

  • f

m a g n i t u d e fm u x : >

  • r

d e r s

  • f

m a g n i t u d e → d i v e r s e p h y s i c s ( s

  • u

r c e s ) → d i v e r s e d e t e c t i

  • n

t e c h n i q u e s F l u x r a p i d l y d e c r e a s e s w i t h e n e r g y ( ~ 1

  • )

, H i g h e s t e n e r g i e s → t h e mo s t d e ma n d i n g c h a l l e n g e s : → t e c h n i c a l : e x t r e m e l y l

  • w

fm u x ( a t E = 1

2

e V 1 p a r t i c l e / ( k m

2

mi l l e n i u m) ) , b u t n

  • w

: t h e P i e r r e A u g e r O b s e r v a t

  • r

y ( ~ k m

2

) ( → p a r t i c l e / y e a r ) → s c i e n t i f c : Wh a t a r e U l t r a

  • H

i g h E n e r g y C

  • s

mi c R a y s ( U H E C R ) ? Wh e r e t h e y c

  • me

f r

  • m?

H

  • w

d

  • t

h e y p r

  • p

a g a t e ?

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Introduction and motivation Cosmic Ray Ensembles (CRE) CREDO app Other applications Summary Pierre Auger Observatory

State of the art detection by Pierre Auger Observatory

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Introduction and motivation Cosmic Ray Ensembles (CRE) CREDO app Other applications Summary Pierre Auger Observatory

Pierre Auger Observatory array

from arXiv:1307.3956

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Introduction and motivation Cosmic Ray Ensembles (CRE) CREDO app Other applications Summary Pierre Auger Observatory

Pierre Auger Observatory spectrum

from arXiv:1307.3956

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Introduction and motivation Cosmic Ray Ensembles (CRE) CREDO app Other applications Summary

Preshower effect

contains typically 100 particles, created at around 1000 km a.s.l. However: super preshower (SPS), 1000 particles at 10000 km a.s.l.

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Introduction and motivation Cosmic Ray Ensembles (CRE) CREDO app Other applications Summary

Super preshower calculations

S U N E A R T H

A T M O S P H E R E

γU

H E ( e . g . 1

2

e V )

N

A T M

> 1

6

γ ? B

S U N

→ F i r s t c a l c u l a t i

  • n

s : W. B e d n a r e k 1 9 9 9 l

  • w

e n e r g i e s n

  • t

t r e a t e d : e x t e n t ~ t e n s

  • f

k m → N . D h i t a l , 2 1 7 c

  • m

p l e t e e n e r g y s p e c t r u m : e x t e n t ~ t h

  • u

s a n d s

  • f

k m

[ O U T O F S C A L E : ]

N

A T M

> 1 →

  • b

s e r v a b l e ( l i n e e v e n 1 k m w i d e ) , n

  • t

y e t t r i e d

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Introduction and motivation Cosmic Ray Ensembles (CRE) CREDO app Other applications Summary

Cosmic Ray Ensembles

N

A T M

= 1 → N

A T M

> 1

p r i ma r y C

  • s

mi c R a y ( p , F e , . . . )

A T M O S P H E R E

a n y t h i n g + i n t e r a c t i

  • n

N

A T M

= 1 N

A T M

> 1

G R O U N D

: a c

  • s

m i c

  • r

a y d e t e c t

  • r

S T A T I S T I C S → S I G N A T U R E S C H A N C E F O R A U N I Q U E S I G N A T U R E ! R E Q U I R E S A G L O B A L R E S E A R C H ! C

  • s

mi c

  • R

a y E n s e mb l e

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Introduction and motivation Cosmic Ray Ensembles (CRE) CREDO app Other applications Summary

Possible CRE observation (1)

C

  • r

r e l a t e d c

  • s

m i c r a y s ?

N

A T M

> 1 ?

Δt ~ 5 mi n . Δx > = s ma l l Y e a r = 1 9 8 1 N

  • b

s

= 3 2 N

e x p

= 1 E = 3 x 1

1 5

e V

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Introduction and motivation Cosmic Ray Ensembles (CRE) CREDO app Other applications Summary

Possible CRE observation (2)

C

  • r

r e l a t e d c

  • s

m i c r a y s ?

N

A T M

> 1 ?

Δx > = 2 5 k m Y e a r = 1 9 7 5 E > 7 x 1

1 3

e V Δt ~ 2 s

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Introduction and motivation Cosmic Ray Ensembles (CRE) CREDO app Other applications Summary

Cosmic Ray Ensemble’s untested scenario (1)

? E A R T H

A T M O S P H E R E

γU

H E ( e . g . 1

2

e V ) Δx : ~ f e w k m E A R T H

A T M O S P H E R E

γU

H E ( e . g . 1

2

e V ) Δx > E a r t h s i z e ?

  • b

v i

  • u

s u n d e t e c t i

  • n
  • b

v i

  • u

s d e t e c t i

  • n

E A R T H

A T M O S P H E R E

γU

H E ( e . g . 1

2

e V ) ? Δx < E a r t h s i z e

„ i n b e t w e e n ” ( u n c h e c k e d )

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Introduction and motivation Cosmic Ray Ensembles (CRE) CREDO app Other applications Summary

Cosmic Ray Ensemble’s untested scenario (2)

There is no wordwide dedicated CR detector array yet  

  • Let’s use what we have + add some new ones

 

  • Existing detectors (observatories, educational detectors, single

detectors) + GPS synchronized array of smartphones  

  • Covered cameras – to filter small energy photons – of smartphones

can act as cosmic particle detectors ֒ → Software development for Android platform at IFJ PAN (Poland, 2016)

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Introduction and motivation Cosmic Ray Ensembles (CRE) CREDO app Other applications Summary

Lunch of the application (end of beta test), 2018 May

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Introduction and motivation Cosmic Ray Ensembles (CRE) CREDO app Other applications Summary

CREDO network

C

  • s

m i c

  • R

a y E x t r e m e l y D i s t r i b u t e d O b s e r v a t

  • r

y

C e n t r a l d a t a b a s e / i n t e r f a c e : a c c e s s t

  • e

v e r y t h i n g f

  • r

e v e r y b

  • d

y

D A T A B A S E / I N T E R F A C E

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Introduction and motivation Cosmic Ray Ensembles (CRE) CREDO app Other applications Summary

Mainframe (AGH Univ., Krakow)

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Introduction and motivation Cosmic Ray Ensembles (CRE) CREDO app Other applications Summary

Usual camera snapshots

2 3

U s e r : „ s m p h

  • k

i t k a t ” , h t t p s : / / a p i . c r e d

  • .

s c i e n c e / w e b / u s e r / s m p h

  • k

i t k a t / D e v i c e : S m a s u n g S M

  • G

3 5 7 F Z , A n d r

  • i

d 4 . 4 . 4 ( K i t K a t ) A v e r a g e d e t e c t i

  • n

r a t e : ~ 1 / h r ( fm i g h t t

  • K

yj i v

  • n

9 . 5 : 6 / h r : )i E x a m p l e i m a g e s :

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Introduction and motivation Cosmic Ray Ensembles (CRE) CREDO app Other applications Summary

User contributions (1), webcam

→ P C a p p l i c a t i

  • n

t

  • c

a t c h p a r t i c l e s w i t h a n i n t e r n e t c a me r a , b y M a r e k K n a p s c i e n c e e n t h u s i a s t !

I n f

  • &

d

  • w

n l

  • a

d [ a u t h

  • r

: M a r e k K n a p ] : h t t p s : / / c r e d

  • .

s c i e n c e / c r e d

  • d

e t e k t

  • r

/ v i e w t

  • p

i c . p h p ? f = 3 & t = 4 5

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Introduction and motivation Cosmic Ray Ensembles (CRE) CREDO app Other applications Summary

User contributions (2), telescope

c

  • s

mi c r a y t r a c k

E x a mp l e „ d a r k f r a me ” t a k e n b y a n a s t r

  • n
  • mi

c a l C C D c a me r a w i t h c

  • v

e r

  • n

C r e d i t & i d e a b y M a s s i m

  • R

a m e l l a ( I N A F )

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Introduction and motivation Cosmic Ray Ensembles (CRE) CREDO app Other applications Summary

User contributions (3), raspberry pi

→ P C a p p l i c a t i

  • n

: l i n u x v e r s i

  • n

w

  • r

k i n g w i t h R a s p b e r r y P i ! B y u s e r „ T r u e T

  • m”

I n f

  • [

a u t h

  • r

: T

  • me

k / T r u e T

  • m]

: h t t p s : / / g i t h u b . c

  • m

/ c r e d

  • s

c i e n c e / C r e d

  • d

e t e c t

  • r
  • f
  • r
  • l

i n u x

  • d

e s k t

  • p
  • a

n d

  • R

a s p b e r r y

  • P

i

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Introduction and motivation Cosmic Ray Ensembles (CRE) CREDO app Other applications Summary

Different applications of CREDO network

quantum gravity previewer

  • b

s e r v e d e x p e c t e d f r

  • m

r a n d

  • m

[ p

  • i

n t s h e r e f

  • r

i l l u s t r a t i

  • n
  • n

l y , c

  • m

p l e t e c a l c u l a t i

  • n

s i n p r

  • g

r e s s ] C u mu l a t i v e n u mb e r

  • f

h i t p a i r s ( „ d

  • u

b l e t s ” ) w i t h i n 5 mi n , i n a s i n g l e d e v i c e b y K e v i n A l m e i d a C h e m i n a n t , f

  • r

t h e C R E D O C

  • l

l a b

  • r

a t i

  • n

earthquake prediction bilogical effects caused by CR Is there a correlation between higher CR rate and known diseases? space weather, e.g. correlation between the changes of Schumann resonances and incoming muon flux

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Introduction and motivation Cosmic Ray Ensembles (CRE) CREDO app Other applications Summary Earthquake prediction

Experimental indication (one case)

Figure: Increase in the low energy signal rate at least six hours before a 8.8ML earthquake in 27.02.2010, 06:34:14 UTC at Chile [by A. Saleh]

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Introduction and motivation Cosmic Ray Ensembles (CRE) CREDO app Other applications Summary Earthquake prediction

Papers from the literature

  • A. L. Morozova et al.,“Variations of the Cosmic Ray Fluxes as a

Possible Earthquake Precursor” , Phys. Chem. Earth (A), Vol. 25,

  • No. 3, pp. 321-324, 2000: Correlations between the annual number
  • f earthquakes and air pressure, cosmic ray fluxes, interplanetary B

are investigated. Some correlation was found.

  • S. M. Korotaeva et al., “The Effect and Forerunners of the

Earthquake of August 28, 2008, in the Vertical Component of the Electric Field in Lake Baikal”, ISSN 1028334X, Doklady Earth Sciences, 2011, Vol. 438, Part 2, pp. 842–845: Changes of EZ electric field component hours before an earthquake of 5.9 − 6.4ML Romanova, N. V. et al., “On the magnetic precursor of the Chilean earthquake of February 27, 2010”, Geomagnetism and Aeronomy, Volume 55, Issue 2, pp.219-222, 2014: Anomalous geomagnetic disturbance (three days before the event) was a mid - size substorm that was not related to seismic activity.

Basically no physical explanation

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Introduction and motivation Cosmic Ray Ensembles (CRE) CREDO app Other applications Summary Earthquake prediction

Change of magnetic field due to EQ

geomagnetism:

(https://commons.wikimedia.org/w/index.php?curid=1712490)

Earthquake − → stress wave in earth − → perturbing the geodynamo and/or deformation of magnetostrictive materials − → changes of magnetic field − → incoming particle flux changes perturbation of geodynamo: MHD equtions + seismic waves the Villari or inverse magnetostrictive effect: change of magnetization of a magnetostrictive material due to mechanical stress.

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Introduction and motivation Cosmic Ray Ensembles (CRE) CREDO app Other applications Summary

To sum up (1)

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

  • bservatories, 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. 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 the global size. 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.

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Introduction and motivation Cosmic Ray Ensembles (CRE) CREDO app Other applications Summary

To sum up (2)

The idea to use the instruments in operation is based on a novel trigger algorithm: in parallel to looking for neighbor surface detectors receiving the signal simultaneously, one should also look for spatially isolated stations clustered in a small time window. CREDO 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 has to list the potential to predict earthquakes by monitoring the rate of low energy cosmic-ray events.

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Introduction and motivation Cosmic Ray Ensembles (CRE) CREDO app Other applications Summary

Thank you for your attention!