d. lo presti, s. aiello e. leonora, g.v. russo, r. leanza infn, … · 2018. 11. 21. · d. lo...

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D. Lo Presti, S. Aiello, E. Leonora , G.V. Russo, R. Leanza INFN, section of Catania And Department of Physics, Catania VLVNT11, Erlangen 12-14 October 2011 1

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Page 1: D. Lo Presti, S. Aiello E. Leonora, G.V. Russo, R. Leanza INFN, … · 2018. 11. 21. · D. Lo Presti, S. Aiello, E. Leonora, G.V. Russo, R. Leanza INFN, section of Catania And Department

D. Lo Presti, S. Aiello, E. Leonora, G.V. Russo, R. Leanza

INFN, section of Catania

And Department of Physics, Catania

VLVNT11, Erlangen 12-14 October 2011 1

Page 2: D. Lo Presti, S. Aiello E. Leonora, G.V. Russo, R. Leanza INFN, … · 2018. 11. 21. · D. Lo Presti, S. Aiello, E. Leonora, G.V. Russo, R. Leanza INFN, section of Catania And Department

Measurement motivation

Characterization of the photomultiplier

stability over long term operation

Gain

TT

TTS

Spurious pulses

Modelling of the ageing mechanism

VLVNT11, Erlangen 12-14 October 2011 2

Page 3: D. Lo Presti, S. Aiello E. Leonora, G.V. Russo, R. Leanza INFN, … · 2018. 11. 21. · D. Lo Presti, S. Aiello, E. Leonora, G.V. Russo, R. Leanza INFN, section of Catania And Department

Ageing definition for this study

Ageing: operative parameters variations of a

photomultiplier with operating time

drift : instability over short time

life : instability over time longer than 1000 hours

Photocathode fatigue is negligible

Ageing mainly depends on variations of

secondary emission ratio

VLVNT11, Erlangen 12-14 October 2011 3

Page 4: D. Lo Presti, S. Aiello E. Leonora, G.V. Russo, R. Leanza INFN, … · 2018. 11. 21. · D. Lo Presti, S. Aiello, E. Leonora, G.V. Russo, R. Leanza INFN, section of Catania And Department

Ageing model supposed Ageing is due to the progressive sputtering of caesium layer in

dynodes due to secondary electrons hitting, followed by sputtering on dynode surface

Caesium layer on dynode surfaces: Reduce thermo-electrons emission ( reduce noise)

Reduce secondary-electron emission (reduce noise)

Presence of excess layer of caesium is confirmed by Hamamatsu

Caesium layer thickness dispersion is due to technology process (different behaviour on different PMTs)

Ageing depends on the total accumulated charge

VLVNT11, Erlangen 12-14 October 2011 4

Page 5: D. Lo Presti, S. Aiello E. Leonora, G.V. Russo, R. Leanza INFN, … · 2018. 11. 21. · D. Lo Presti, S. Aiello, E. Leonora, G.V. Russo, R. Leanza INFN, section of Catania And Department

Ageing model : Up-drift and down-drift

Up-drift

Down-drift

Progressive sputtering by secondary

electrons of the excess caesium layer :

• Gain increase ( decreasing the layer

of Cs in excess)

• Evaporation of caesium ions in

vacuum

Once the excess caesium layer is

removed, sputtering continues on the

essential layer of Cs and on the dynode

surface:

• Gain decrease

• Evaporation of caesium ions in

vacuum

VLVNT11, Erlangen 12-14 October 2011 5

Page 6: D. Lo Presti, S. Aiello E. Leonora, G.V. Russo, R. Leanza INFN, … · 2018. 11. 21. · D. Lo Presti, S. Aiello, E. Leonora, G.V. Russo, R. Leanza INFN, section of Catania And Department

Up-drift and down-drift model

VLVNT11, Erlangen 12-14 October 2011 6

Typical time stability of photomultipliers tube

( from Hamamatsu Hand book. “ PMT, principle and application ”

≡ 3600 C≡ 360 C

Page 7: D. Lo Presti, S. Aiello E. Leonora, G.V. Russo, R. Leanza INFN, … · 2018. 11. 21. · D. Lo Presti, S. Aiello, E. Leonora, G.V. Russo, R. Leanza INFN, section of Catania And Department

Devices Under Test

2 Hamamatsu R7081 10” photomultiplier:

Standard Bi-alkali photocathode (STD)

Super-bialkali photocathode (SBA)

10 stages

The two PMTs differ only for the photocathode

PMTs at the same start gain condition

G ≈ 5 E 7

The PMT bases for voltage supply wereidentical, passive

VLVNT11, Erlangen 12-14 October 2011 7

Page 8: D. Lo Presti, S. Aiello E. Leonora, G.V. Russo, R. Leanza INFN, … · 2018. 11. 21. · D. Lo Presti, S. Aiello, E. Leonora, G.V. Russo, R. Leanza INFN, section of Catania And Department

Characterizationprocedure

Two alternate phases:

Ageing (continuosly pulsed light)

○ LED ON (about 3pe @ 1 MHz. High frequency to accelerate

the aging process)

○ PicoLog recording of the anode DC current for each PMT

Measurements of PMT parameters ( once a week)

○ LED OFF

○ Pulsed Laser at s.p.e. condition

○ s.p.e. charge spectrum

○ s.p.e. Transit Time spectrum

○ Spurious pulses

Measurements time : from 28/5/2008 to 8/10/2011

≈ 3 years (considering Holidays)

VLVNT11, Erlangen 12-14 October 2011 8

Page 9: D. Lo Presti, S. Aiello E. Leonora, G.V. Russo, R. Leanza INFN, … · 2018. 11. 21. · D. Lo Presti, S. Aiello, E. Leonora, G.V. Russo, R. Leanza INFN, section of Catania And Department

Experimental set-up• A light-tight dark box ( 65 x 65 x 110 ) cm. Thickness 2 cm

• A 400 nm LED ( switched 50/50) to illuminate the PMTs uniformily

• A pulsed LASER set in s.p.e. condition ( Picoquant PDL-800)

( 410 nm, 60 ps width, 10 KHz )

• NIM electronics for timing and charge acquisition

• A bolometer as monitor for the LED light stability

• A PicoScope logger to record ( simultaneously, Tc = 1 sec)

• the anodes current

• internal and external temperature in the box

• the bolometer output

VLVNT11, Erlangen 12-14 October 2011 9

Page 10: D. Lo Presti, S. Aiello E. Leonora, G.V. Russo, R. Leanza INFN, … · 2018. 11. 21. · D. Lo Presti, S. Aiello, E. Leonora, G.V. Russo, R. Leanza INFN, section of Catania And Department

Results : premises

• In the following plots, the x-axes is the anodic charge

measured by the PicoLog.

• The plots refers to the same operating time

• The SBA anodic current collected during the ageing phase

is higher than the STD one (higher detection efficiency)

• The ageing process was stopped when the total charge

arrived up to about 1800 C for the STD PMT and

2600 C for the SBA PMT

• LED light of about 3pe @ 1 MHz is equivalent to 15 times a

source of 1 pe @ 200 KHz

the ageing operating time of 3 years is equivalent to

about 45 years of operative life of 1 pe @ 200 KHz

VLVNT11, Erlangen 12-14 October 2011 10

Page 11: D. Lo Presti, S. Aiello E. Leonora, G.V. Russo, R. Leanza INFN, … · 2018. 11. 21. · D. Lo Presti, S. Aiello, E. Leonora, G.V. Russo, R. Leanza INFN, section of Catania And Department

Results: Gain

VLVNT11, Erlangen 12-14 October 2011 11

Measured studying the peak position of the Charge spectrum acquired

in s.p.e. condition

• the up and down drift model was confirmed by measurements

• a first phase of up-drift with an increase of about 20 %

• a final phase of down drift with a diminuition up to 40% from the max value

Page 12: D. Lo Presti, S. Aiello E. Leonora, G.V. Russo, R. Leanza INFN, … · 2018. 11. 21. · D. Lo Presti, S. Aiello, E. Leonora, G.V. Russo, R. Leanza INFN, section of Catania And Department

Results : Transit Time (relative)

VLVNT11, Erlangen 12-14 October 2011 12

Not considerable variations in Transit Time during operating time

Page 13: D. Lo Presti, S. Aiello E. Leonora, G.V. Russo, R. Leanza INFN, … · 2018. 11. 21. · D. Lo Presti, S. Aiello, E. Leonora, G.V. Russo, R. Leanza INFN, section of Catania And Department

Results: Transit Time Spread (FWHM)

VLVNT11, Erlangen 12-14 October 2011 13

Not considerable variations in Transit Time Spread

Page 14: D. Lo Presti, S. Aiello E. Leonora, G.V. Russo, R. Leanza INFN, … · 2018. 11. 21. · D. Lo Presti, S. Aiello, E. Leonora, G.V. Russo, R. Leanza INFN, section of Catania And Department

Spurious pulses

VLVNT11, Erlangen 12-14 October 2011 14

For each group the ratio of spurious events on main pulses events were

calculated

After pulse 1 After pulse 2

Page 15: D. Lo Presti, S. Aiello E. Leonora, G.V. Russo, R. Leanza INFN, … · 2018. 11. 21. · D. Lo Presti, S. Aiello, E. Leonora, G.V. Russo, R. Leanza INFN, section of Catania And Department

Results: fraction of pre-pulses

VLVNT11, Erlangen 12-14 October 2011 15

Not considerable variations during operating time

Anodic charge [C]

Page 16: D. Lo Presti, S. Aiello E. Leonora, G.V. Russo, R. Leanza INFN, … · 2018. 11. 21. · D. Lo Presti, S. Aiello, E. Leonora, G.V. Russo, R. Leanza INFN, section of Catania And Department

Results: fraction of delayed pulses

VLVNT11, Erlangen 12-14 October 2011 16

Not significative variations during operating time

Anodic charge [C]

Page 17: D. Lo Presti, S. Aiello E. Leonora, G.V. Russo, R. Leanza INFN, … · 2018. 11. 21. · D. Lo Presti, S. Aiello, E. Leonora, G.V. Russo, R. Leanza INFN, section of Catania And Department

Results: Type 1 after pulse

VLVNT11, Erlangen 12-14 October 2011 17

Not considerable variations during operating time

Anodic charge [C]

Page 18: D. Lo Presti, S. Aiello E. Leonora, G.V. Russo, R. Leanza INFN, … · 2018. 11. 21. · D. Lo Presti, S. Aiello, E. Leonora, G.V. Russo, R. Leanza INFN, section of Catania And Department

Results: type 2 after pulse

VLVNT11, Erlangen 12-14 October 2011 18

• Not considerable variations for a lot of the operating time

• Significative decrease for SBA PMT, from the 8% to 5% , after 1700 C

• Study of the effects of ions Cs evaporated on fraction of after pulses 2

Anodic charge [C]

Page 19: D. Lo Presti, S. Aiello E. Leonora, G.V. Russo, R. Leanza INFN, … · 2018. 11. 21. · D. Lo Presti, S. Aiello, E. Leonora, G.V. Russo, R. Leanza INFN, section of Catania And Department

Conclusions• Apart the Gain, all the measured parameter of the two PMTs

are stable during ageing

• A first phase of Up-drift with a gain increase of about 20 %

followed by a final phase of down-drift with an gain decrease

of about the 40% from max value

• The ageing model of Up- and Down- drift has been

demonstrated by the results

• The ageing process was stopped when the total charge

arrived up to about 1800 C for STD PMT and 2600 C for SBA

PMT

• The measuring time ( 3 years) is equivalent to an operating

time of about 45 years @ 1 pe @ 200 KHz

• The final values of the Gain for both PMTs is still suitable for

their use

VLVNT11, Erlangen 12-14 October 2011 19

Page 20: D. Lo Presti, S. Aiello E. Leonora, G.V. Russo, R. Leanza INFN, … · 2018. 11. 21. · D. Lo Presti, S. Aiello, E. Leonora, G.V. Russo, R. Leanza INFN, section of Catania And Department

Work in progress

• An accurate study of the dynode surfaces after ageing

by microscope is being carried in the next months

VLVNT11, Erlangen 12-14 October 2011 20

Page 21: D. Lo Presti, S. Aiello E. Leonora, G.V. Russo, R. Leanza INFN, … · 2018. 11. 21. · D. Lo Presti, S. Aiello, E. Leonora, G.V. Russo, R. Leanza INFN, section of Catania And Department

Thanks for the attention

VLVNT11, Erlangen 12-14 October 2011 21

Further information:

[email protected]

[email protected]

Page 22: D. Lo Presti, S. Aiello E. Leonora, G.V. Russo, R. Leanza INFN, … · 2018. 11. 21. · D. Lo Presti, S. Aiello, E. Leonora, G.V. Russo, R. Leanza INFN, section of Catania And Department

VLVNT11, Erlangen 12-14 October 2011 22

Pictures of sputtered dynodes

First Dynode

Last Dynode