Presentation of Activities Dr. Ji A. Mare Institute of Physics - - PowerPoint PPT Presentation

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Presentation of Activities Dr. Ji A. Mare Institute of Physics - - PowerPoint PPT Presentation

Presentation of Activities Dr. Ji A. Mare Institute of Physics Academy of Sciences of the Czech Republic Prague 6, Cukrovarnicka 10 Czech Republic amares@fzu.cz Experimental set-up for scintillation response studies using HPMT


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SLIDE 1

Presentation of Activities

  • Dr. Jiří
  • A. Mareš

Institute of Physics Academy of Sciences of the Czech Republic Prague 6, Cukrovarnicka 10 Czech Republic amares@fzu.cz

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SLIDE 2

Experimental set-up for scintillation response studies using HPMT

5 10 15 20 25 30 200 300 400 500 600 700 800 Quantum efficiency of the HPMT DEP Q.E. [%] Wavelength [nm]

ORTEC model 672 MCA ORTEC Model 927 MCB

Pulsed height spectra

241Am (59.6 keV) excited lines of

Cu, Rb, Mo, Ag, Ba, and Tb,

57Co, 22Na, 137Cs and 60Co

Here, we use α-ray sources instead of γ-rays

α-ray sources –

241Am, 239Pu

and 244Cm

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SLIDE 3

1 10 100 1000 104 105 106 107 108 100 200 300 400 500 no bias -no voltage 20 V bias - 6 kV 40 V bias - 6 kV 40 V bias - 10 kV 40 V bias - 12 kV long Counts Channel number n = 1 n = 2 n = 3 n = 4

Photoelectron response of the HPMT ➣ Bias – voltage at the Si PIN diode anode ➣ High voltage – between the photocathode focusing electrodes and the anode SIGNAL

  • no bias –

no voltage dark current, light

  • bias –

HV voltage – signal appear

  • nominal bias –

voltage photoelectrons appear calibration is possible

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SLIDE 4

1000 2000 3000 4000 5000 6000 1 mm 2 mm 5 mm 10 mm Counts Channel number 600 500 400 300 200 100 Sample thickness Arrows - 662 keV peak position

Gamma-ray pulse spectra of 662 keV line of the 137Cs source with YAG:Ce measured for different sample thickness

These gamma-ray spektra show that

  • YAG:Ce

has lower photo-peak efficiency compared with LuAG:Ce (photo- peak/Compton edge ~ 0.26 for 10 mm thickness) due to lower density (4.55 g/cm3) it is necessary to use longer crystals (lower attenuation than has LuAG:Ce)

  • YAG:Ce could be efficient for detection with the avalanche photodiodes
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SLIDE 5

HPMT se-up at CERN developed during late nineties

  • f past century for

scintillation characteristics

  • f large PWO crystals
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SLIDE 6

Carmelo D’ Ambrosio shows the HPMT set-up Carmelo Jiri

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SLIDE 7

Measurements at CERN –

  • Ing. A. Beitlerová
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SLIDE 8

HPMT scintillation set-up at the Laboratory

  • f

Luminescence and Scintillation Materials in Prague

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SLIDE 9

PHOS – photon calorimeter

Gamma a alfa spektroskopie scintilátorů

FZÚ – Department of Optical Materials – study of scintillation crystals RD-18 project – “Search for new radiation hard scintillators for new generation of electromagnetic calorimeters at LHC” Crystals: Ce-, Pr-doped garnets, perovskites, silicates. PbWO4 and other ones

Projects are supported by the Czech Committee for cooperation with CERN (from Ministry of Trade and Industry or later by Ministry of education, Youth and Sport

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SLIDE 10

All-Russian Science Research Institute of the Experimental Physics - VNIIEF

MECHANICAL DESIGN of the PHOS CRADLE MECHANICAL DESIGN of the PHOS CRADLE

General information General information

The overall dimensions

  • f the PHOS Cradle.

The total weight is around 3,5 t

PHOS CRADLE Project - schema

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SLIDE 11

End of 2004 year – CRADLE produced at TENEZ factory in Chotebor, Czech Republic

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SLIDE 12

JUNE 2005 - PHOS CRADLE assembled at CERN Point 2 by people from TENEZ factory

TENEZ people

MARES

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SLIDE 13

PHOS CRADLE is moving down into experimental position – CERN, Point 2, St. Genis

Rollers CRADLE

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SLIDE 14

PHOS CRADLE in the final position below the collision space of ALICE LHC experiment

PHOS CRADLE

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SLIDE 15

PHOS CRADLE position – November 2008 – Point 2 ALICE LHC

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SLIDE 16

Detail of PHOS CRADLE – November 2008 – ALICE LHC

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SLIDE 17

Works on or around PHOS CRADLE are not easy

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SLIDE 18

CERN – Point 2 – ALICE LHC space – with Martin Faltys Jiri Martin

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SLIDE 19

One PWO module is in the centre of PHOS CRADLE holder module

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SLIDE 20

Dmitry Budnikov from Sarov Jiri from Praha With Dmitry Budnikov from VNIIEF in Sarov at PHOS assembling hall at CERN

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SLIDE 21

With Karel Polak at the read side of one PHOS PWO module at the assembling hall at CERN Karel Polak Jiri Mares

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SLIDE 22

Front side of one of the PHOS PWO modules

  • individual PWO crystals are clearly seen
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SLIDE 23

CERN - November 2009 – control screen of PHOS detector at the ALICE CONTROL ROOM at Point 2

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SLIDE 24

CERN - Point 2– November 2009 – ALICE CONTROL ROOM - PHOS CONTROL Petr Zavada Jiri Mares

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SLIDE 25

CERN – Point 2 – November 2009 - PHOS control New start of LHC and first collisions

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SLIDE 26

CERN – Point 2 – ALICE CONTROL ROOM – first collision November 23, 2009

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SLIDE 27

CERN – Point 2 – ALICE CONTROL ROOM – people see first ciollisions

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SLIDE 28

CERN – picture of inner part of LHC, especially Of magnets