Absolute Measurement of Air Fluorescence Yield for Ultra-High Energy Cosmic Rays Paolo Privitera...

12
Absolute Measurement of Air Fluorescence Yield for Ultra-High Energy Cosmic Rays Paolo Privitera Carlos Hojvat Fermilab, June 27 2008 FD SD

Transcript of Absolute Measurement of Air Fluorescence Yield for Ultra-High Energy Cosmic Rays Paolo Privitera...

Page 1: Absolute Measurement of Air Fluorescence Yield for Ultra-High Energy Cosmic Rays Paolo Privitera Carlos Hojvat Fermilab, June 27 2008 FD SD.

Absolute Measurement of Air Fluorescence Yield for Ultra-

High Energy Cosmic Rays

Paolo Privitera

Carlos Hojvat

Fermilab, June 27 2008

FD

SD

Page 2: Absolute Measurement of Air Fluorescence Yield for Ultra-High Energy Cosmic Rays Paolo Privitera Carlos Hojvat Fermilab, June 27 2008 FD SD.

Auger results

Flux suppression

Anisotropy < 75 Mpc

Astrophysical interpretation GZK horizon

Page 3: Absolute Measurement of Air Fluorescence Yield for Ultra-High Energy Cosmic Rays Paolo Privitera Carlos Hojvat Fermilab, June 27 2008 FD SD.

Auger Energy Calibration

Lateral density distribution

Fluorescence Detector

Surface Detector

The largest systematic uncertainty is the air fluorescence yield (15%)

The Auger energy scale is based on the FD calorimetric energy.

10 km

Page 4: Absolute Measurement of Air Fluorescence Yield for Ultra-High Energy Cosmic Rays Paolo Privitera Carlos Hojvat Fermilab, June 27 2008 FD SD.

The Auger hybrid detector concept

300-400 nm light from de-excitation of atmospheric nitrogen (fluorescence light)

≈ 4 γ’s / m /electron

1019 eV 1010 e

Light attenuation in the atmosphere; showers develop in 15 km

• Fluorescence spectrum

• Dependence on pressure, temperature and humidity

• Absolute yield 20

FD

SD

Page 5: Absolute Measurement of Air Fluorescence Yield for Ultra-High Energy Cosmic Rays Paolo Privitera Carlos Hojvat Fermilab, June 27 2008 FD SD.

AIRFLY measurements

391.4 nm337.1 nm

353.7 nmrelative band intensities

Temperature and humidity dependence

Pressure dependence

Page 6: Absolute Measurement of Air Fluorescence Yield for Ultra-High Energy Cosmic Rays Paolo Privitera Carlos Hojvat Fermilab, June 27 2008 FD SD.

Chemistry Division Van de Graaf (0.6-3 MeV)

Advanced Photon Source (6-30 KeV)

HEP Division Advanced Wakefield Accelerator

(3 MeV-15 MeV)

AIRFLY beams

Beam Test Facility at DANE INFN FRASCATI (50-750 MeV)

ARGONNEANL

Collaboration: Cezch Republic, Germany, Italy, US

Page 7: Absolute Measurement of Air Fluorescence Yield for Ultra-High Energy Cosmic Rays Paolo Privitera Carlos Hojvat Fermilab, June 27 2008 FD SD.

Chamber

Gas system

Vacuum pump

Lead shielding support

BTF (Frascati)

Argonne Chemistry VdG

Page 8: Absolute Measurement of Air Fluorescence Yield for Ultra-High Energy Cosmic Rays Paolo Privitera Carlos Hojvat Fermilab, June 27 2008 FD SD.

Absolute Fluorescence Yield at the Fermilab Meson Test Beam

Goal: ≤ 5% uncertainty with the fluorescence/Cherenkov ratio method

Photon Detector

Particle beam

Fluorescence photons

Cherenkov photons

Photon Detector

Particle beam

45° mirror

(a) (b)

337 nm filter

Q.E uncertainty >10% Normalize to known yield: Q.E cancels

Tested at Frascati and Argonne

Page 9: Absolute Measurement of Air Fluorescence Yield for Ultra-High Energy Cosmic Rays Paolo Privitera Carlos Hojvat Fermilab, June 27 2008 FD SD.

Absolute Fluorescence Yield at the Fermilab Meson Test Beam

Fluorescence/Cherenkov ratio method + independent laser calibration

• Low intensity: Integrating sphere, Ultra Bialkali PMTs (43% QE)

Particle beam

Photon Detector

Integrating sphere

Diffuser to be placed for Cherenkov run

Cherenkovdump

Acceptance counter

Veto counter

• High energy (reduce multiple scattering, air as Cherenkov Radiatior)

• Well defined beam: single particle trigger and geometry

• Wide range of particles type and intensity

Page 10: Absolute Measurement of Air Fluorescence Yield for Ultra-High Energy Cosmic Rays Paolo Privitera Carlos Hojvat Fermilab, June 27 2008 FD SD.

Collaborative Initiative Grant

• Crucial measurement for Auger (South and North); will have a strong impact in the Auger scientific results and in the UHECR field

• Use of Fermilab facility: Meson Test Beam• University of Chicago and Fermilab have a long history of collaboration in Auger; Auger design Workshop

held at Fermilab in 1995• Collaboration well matched for the success of the initiative• P. Privitera (Chicago), C. Hojvat (Fermilab), H. Spinka (Argonne), AIRFLY collaborators • Some hardware from AIRFLY• Funds: 1 postdoc (100% FTE), hardware for new chamber • 2 years proposal

Tank n. 1600

Page 11: Absolute Measurement of Air Fluorescence Yield for Ultra-High Energy Cosmic Rays Paolo Privitera Carlos Hojvat Fermilab, June 27 2008 FD SD.

Air fluorescence spectrum

• Argonne 3 MeV electron VdG, DC beam, 10 μA• Spectrograph instead of monochromator:Insensitive to changes of beam intensity or position

VdG Beam

Sphericalmirror

Optical fiber

L.O.T. Oriel MS257 = 0.1 nm

Andor CCD DV 420

Page 12: Absolute Measurement of Air Fluorescence Yield for Ultra-High Energy Cosmic Rays Paolo Privitera Carlos Hojvat Fermilab, June 27 2008 FD SD.

Chamber

Gas system

Vacuum pump

Lead shielding support

BTF (Frascati)

HPD