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Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

Feb 14, 2022

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Page 1: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

Cosmic ray physics with the GAMMA-400

experiment

P. Cumani (University of Trieste - INFN Sez. di Trieste)

on the behalf of the GAMMA-400 collaboration

Page 2: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

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Page 3: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

Mission approved by ROSCOSMOS (launch currently schedule

by November 2018)

GAMMA-400 will be installed onboard the platform

"Navigator" manufactured by Lavochkin

Scienti�c payload mass: 2600 kg

Power budget: 2000 W

Telemetry downlink capability: 100 GB/day

Lifetime: 10 years

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Page 4: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

Space mission GAMMA-400

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Page 5: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

Acceptance of the Calorimeter (Side view)

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Page 6: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

Acceptance of the Calorimeter

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Page 7: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

Original Russian design focused on:

High energy gamma-rays (10 GeV - 3 TeV)

High energy electrons (e− and e+) up to TeV energies

Scienti�c objectives (from Russian proposal):

"To study the nature and features of weakly interacting

massive particles, from which the dark matter consists"

"To study the nature and features of variable gamma-ray

activity of astrophysical objects from stars to galactic clusters"

"To study the mechanisms of generation, acceleration,

propagation and interaction of cosmic rays in galactic and

intergalactic spaces"

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Page 8: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

GAMMA-400 baseline

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Page 9: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

GAMMA-400 present con�guration

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Page 10: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

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Page 11: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

Electrons spectrum

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Page 12: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

Cosmic ray acceleration and propagation

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Page 13: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

Nuclei

Knee structure

Structures in the

GeV-TeV region recently

discovered for p and He

Spectral measurements in

the knee region up to

now are only indirect

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Page 14: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

Physics Goal

e− up to the TeV region to

search for structures in the

spectrum and to study

close-by sources

High energy proton and

nuclei to study the knee

region

Requirements

Very large geometrical factor

Good electron and hadron

energy resolution

Excellent electron/hadron

separation

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Page 15: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

GAMMA-400 detectors

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Page 16: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

GAMMA-400: Silicon Array

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Page 17: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

GAMMA-400: Silicon Array

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Page 18: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

GAMMA-400: Silicon Array

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Page 19: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

GAMMA-400: Tracker

4 towers

10 planes (each plane 2 array of

the Si tiles)

Si: microstrip along x-axis

Honeycomb Al support

First 8 planes: W (0.1 X0)

Si: microstrip along y-axis

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Page 20: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

Simulated performance: e�ective area (Preliminary)

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Page 21: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

Simulated performance: angular resolution (Preliminary)

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Page 22: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

Simulated performance: energy resolution for γ

(Preliminary)

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Page 23: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

GAMMA-400: CalorimeterCalorimeter CC1 (Si-CsI(Tl))

N layers 2

Si pitch 0.5 mm

Size 1x1x0.04 m3

X0 2

λI 0.1

Calorimeter CC2 (CsI(Tl))

NxNxN 28x28x12

L 3.6 cm

Size 1x1x0.47 m3

X0 54.6x54.6x23.4

λI 2.5x2.5x1.1

Mass 1683 kg22

Page 24: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

Calorimeter CC2: readout

At least 2 photo diodes per crystals to cover the huge dynamical

range (1-107 MIP)23

Page 25: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

Calorimeter CC2: test beam

October 2012 @ CERN SPS (e−, p, muons): small, so called

"pre-prototype" (4 layers, 3 crystals each)

February 2013 @ CERN SPS (Ions): bigger, properly called

"prototype" (14 layers, 9 crystals each)

October 2013 @ INFN Frascati: 700 MeV e−

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Page 26: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

"Pre-prototype" results

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Page 27: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

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Page 28: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

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Page 29: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

Pulse height spectrum in a crystal

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Page 30: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

Energy deposit

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Page 31: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

Energy resolution

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Page 32: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

Test beam results

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Page 33: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

Electron count estimation

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Page 34: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

p and He count estimation

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Page 35: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

Nuclei count estimation

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Page 36: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

Conclusions

Important for the multiwavelength/multimessenger approach

Pointing strategy without Earth occultation / Big FOV

The GAMMA-400 Tracker is an evolution of AGILE and

Fermi-LAT

The GAMMA-400 calorimeter design of novel concept gives

unique energy resolution and depth for electrons and nuclei

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Page 37: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

Conclusions

The GAMMA-400 mission represents a unique opportunity to

perform simultaneous measurements of photons, electrons and

nuclei with unprecedented accuracy.

GAMMA-400 can provide in-depth investigations on some of

the most challenging physics items, such as DM searches, CR

origin, production and acceleration to the highest energies...

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Page 38: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

GAMMA-400 website

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Page 39: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern
Page 40: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

SPARE SLIDES

Page 41: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

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Page 42: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

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Page 43: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

Cygnus region above 30 MeV

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Page 44: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

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Page 45: Cosmic ray physics with the GAMMA-400 experiment - Indico - Cern

GAMMA-400 Physics Geometry Conclusions

Topology

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