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Radio telescopes as high-energy particle detectors Justin Bray, University of Manchester On behalf of groups: SKA-lunar: Justin Bray, Jaime Alvarez-Mu˜ niz, Stijn Buitink, Rustam Dagkesamanskii, Ron Ekers, Heino Falcke, Ken Gayley, Tim Huege, Clancy James, Maaijke Mevius, Robert Mutel, Ray Protheroe, Olaf Scholten, Ralph Spencer, Sander ter Veen SKA-EAS: Tim Huege, Justin Bray, Stijn Buitink, Richard Dallier, Ron Ekers, Heino Falcke, Clancy James, Lilian Martin, Benoit Revenu, Olaf Scholten, Frank Schroder
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Justin Bray, University of Manchestersjs/ras2015/6-justin_bray.pdf · Justin Bray, University of Manchester On behalf of groups: SKA-lunar: Justin Bray, Jaime Alvarez-Muniz,~ Stijn

Jun 28, 2020

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Page 1: Justin Bray, University of Manchestersjs/ras2015/6-justin_bray.pdf · Justin Bray, University of Manchester On behalf of groups: SKA-lunar: Justin Bray, Jaime Alvarez-Muniz,~ Stijn

Radio telescopes as high-energy particle detectors

Justin Bray, University of Manchester

On behalf of groups:

SKA-lunar: Justin Bray, Jaime Alvarez-Muniz, Stijn Buitink, Rustam Dagkesamanskii, Ron Ekers, Heino Falcke, Ken Gayley,

Tim Huege, Clancy James, Maaijke Mevius, Robert Mutel, Ray Protheroe, Olaf Scholten, Ralph Spencer, Sander ter Veen

SKA-EAS: Tim Huege, Justin Bray, Stijn Buitink, Richard Dallier, Ron Ekers, Heino Falcke, Clancy James, Lilian Martin,

Benoit Revenu, Olaf Scholten, Frank Schroder

Page 2: Justin Bray, University of Manchestersjs/ras2015/6-justin_bray.pdf · Justin Bray, University of Manchester On behalf of groups: SKA-lunar: Justin Bray, Jaime Alvarez-Muniz,~ Stijn

Cosmic rays

Very highenergies

Very low flux

Sources notwell-understood

Magneticdeflection

(compiled by R. Engel)

Justin Bray Radio telescopes as particle detectors February 13, 2015 2 / 14

Page 3: Justin Bray, University of Manchestersjs/ras2015/6-justin_bray.pdf · Justin Bray, University of Manchester On behalf of groups: SKA-lunar: Justin Bray, Jaime Alvarez-Muniz,~ Stijn

Extensive air showers

Detection:ns-µs transients

nitrogen fluorescence

scintillators/Cherenkov

geomagnetic radio

Largest current detector:Pierre Auger Observatory

Justin Bray Radio telescopes as particle detectors February 13, 2015 3 / 14

Page 4: Justin Bray, University of Manchestersjs/ras2015/6-justin_bray.pdf · Justin Bray, University of Manchester On behalf of groups: SKA-lunar: Justin Bray, Jaime Alvarez-Muniz,~ Stijn

Energy & composition

proton iron

Shower simulations, T. Huege et al., ARENA 2012

Justin Bray Radio telescopes as particle detectors February 13, 2015 4 / 14

Page 5: Justin Bray, University of Manchestersjs/ras2015/6-justin_bray.pdf · Justin Bray, University of Manchester On behalf of groups: SKA-lunar: Justin Bray, Jaime Alvarez-Muniz,~ Stijn

Penetration depth: Xmax

Justin Bray Radio telescopes as particle detectors February 13, 2015 5 / 14

Page 6: Justin Bray, University of Manchestersjs/ras2015/6-justin_bray.pdf · Justin Bray, University of Manchester On behalf of groups: SKA-lunar: Justin Bray, Jaime Alvarez-Muniz,~ Stijn

Ground coverage

1000 500 0 500 1000West-East (m)

1000

500

0

500

1000

South

-Nort

h (

m)

LOFAR

3000 2000 1000 0 1000 2000 3000West-East (m)

3000

2000

1000

0

1000

2000

3000

South

-Nort

h (

m)

AERA

2000 1500 1000 500 0 500 1000 1500 2000West-East (m)

2000

1500

1000

500

0

500

1000

1500

2000

South

-Nort

h (

m)

SKA

Typical resolution with fluorescence detectors: ∼ 20 g/cm2

Current resolution with LOFAR: 20 g/cm2 (S. Buitink, ICRC 2013)

Resolution with SKA: 10 g/cm2 looks feasible

Justin Bray Radio telescopes as particle detectors February 13, 2015 6 / 14

Page 7: Justin Bray, University of Manchestersjs/ras2015/6-justin_bray.pdf · Justin Bray, University of Manchester On behalf of groups: SKA-lunar: Justin Bray, Jaime Alvarez-Muniz,~ Stijn

Lunar approach

Page 8: Justin Bray, University of Manchestersjs/ras2015/6-justin_bray.pdf · Justin Bray, University of Manchester On behalf of groups: SKA-lunar: Justin Bray, Jaime Alvarez-Muniz,~ Stijn

Aperture

1018 1019 1020 1021

ECR (eV)

101

102

103

104

105

106

107

Aef

f (km

2 sr)

Band Frequency(MHz)

SKA-LOW 100-350SKA-MID 1 350-1050SKA-MID 2 950-1760

cosmic rays1019 1020 1021 1022 1023 1024

Eν (eV)

neutrinos

Sensitive to the top end of the cosmic-ray spectrum.Detection rate up to 1 per 100 hr with SKA1.

Justin Bray Radio telescopes as particle detectors February 13, 2015 8 / 14

Page 9: Justin Bray, University of Manchestersjs/ras2015/6-justin_bray.pdf · Justin Bray, University of Manchester On behalf of groups: SKA-lunar: Justin Bray, Jaime Alvarez-Muniz,~ Stijn

Arrival directions (Galactic coords)

-120 ◦0 ◦+120 ◦

-60 ◦

-30 ◦

0 ◦

+30 ◦

+60 ◦

Pierre Auger Collaboration 2010, Astropart. Phys., 34, 314;Telescope Array Collaboration 2014, ApJ, 790, 21

Justin Bray Radio telescopes as particle detectors February 13, 2015 9 / 14

Page 10: Justin Bray, University of Manchestersjs/ras2015/6-justin_bray.pdf · Justin Bray, University of Manchester On behalf of groups: SKA-lunar: Justin Bray, Jaime Alvarez-Muniz,~ Stijn

Arrival directions (Galactic coords)

-120 ◦0 ◦+120 ◦

-60 ◦

-30 ◦

0 ◦

+30 ◦

+60 ◦

CenA

?

Pierre Auger Collaboration 2010, Astropart. Phys., 34, 314;Telescope Array Collaboration 2014, ApJ, 790, 21

Justin Bray Radio telescopes as particle detectors February 13, 2015 10 / 14

Page 11: Justin Bray, University of Manchestersjs/ras2015/6-justin_bray.pdf · Justin Bray, University of Manchester On behalf of groups: SKA-lunar: Justin Bray, Jaime Alvarez-Muniz,~ Stijn

Field of view

Moon

-60 ◦ -30 ◦ 0 ◦ +30 ◦+60 ◦-60 ◦

-30 ◦

0 ◦

+30 ◦

+60 ◦

0

4

8

12

16

20

24

28

32

Dire

ctiona

l ape

rture (1

03 km

2 )

Moon

-60 ◦ -30 ◦ 0 ◦ +30 ◦ +60 ◦-60 ◦

-30 ◦

0 ◦

+30 ◦

+60 ◦

0

1

2

3

4

5

6

7

8

Dire

ctiona

l ape

rture (1

02 km

2 arcmin−2

)

Justin Bray Radio telescopes as particle detectors February 13, 2015 11 / 14

Page 12: Justin Bray, University of Manchestersjs/ras2015/6-justin_bray.pdf · Justin Bray, University of Manchester On behalf of groups: SKA-lunar: Justin Bray, Jaime Alvarez-Muniz,~ Stijn

Angular resolution

1019 1020 1021

Energy (eV)

0

5

10

15

20

Res

olut

ion

(◦)

SKA1-LOWSKA1-MID 1

SKA1-MID 2

magnetic deflection

radialtangential

Sufficient to test anisotropy.

Justin Bray Radio telescopes as particle detectors February 13, 2015 12 / 14

Page 13: Justin Bray, University of Manchestersjs/ras2015/6-justin_bray.pdf · Justin Bray, University of Manchester On behalf of groups: SKA-lunar: Justin Bray, Jaime Alvarez-Muniz,~ Stijn

Summary

Radio telescopes can detect cosmic rays.

Atmospheric detection:

works now

commensal operation

emission mechanisms understood

ready to start doing astrophysics

Lunar detection:

not yet, but soon

prospect of source detection

neutrinos?

Justin Bray Radio telescopes as particle detectors February 13, 2015 13 / 14

Page 14: Justin Bray, University of Manchestersjs/ras2015/6-justin_bray.pdf · Justin Bray, University of Manchester On behalf of groups: SKA-lunar: Justin Bray, Jaime Alvarez-Muniz,~ Stijn

Thanks for listening!

“Towards the radio-detection of cosmic particles with the SKA”

Jodrell Bank, 5–7 May 2015

http://www.jb.man.ac.uk/meetings/cosmic2015/

Justin Bray Radio telescopes as particle detectors February 13, 2015 14 / 14