Very High QE bialkali PMTs

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1 Very High QE bialkali PMTs Mª Victoria Fonseca University Complutense, Madrid, Spain

2 How a classical PMT is operating photons

3 Quantum Efficiency Quantum efficiency (QE) of a sensor QE = N(ph.e.) / N(photons) Conversion of a photon into ph.e. is a purely binomial process (and not poisson!) Assume N photons are impinging onto a photocathode and every photon has the same probability P to kick out one ph.e. Then the mean number of ph.e.s is N x P and the Variance is equal to N x P x (1 P)

4 Signal to noise ratio The signal-to noise ratio (SNR) of a given photocathode with QE=P can be calculated as SNR = [N x P/(1 - P)] For example, for N = 1 (single impinging photon): P SNR

5 Short Historical Excursion 1889: Elster and Geitel discovered that in alkali metals a photo-electric effect can be induced by visible light (the existence of the e- was yet unknown) 1905: Einstein put forward the concept that photoemission is the conversion of a photon into a free e- Until ~1930 QE of available materials was < : discovered Ag-O-Cs photo-emitter (Koller; Campbell) improved the QE to the level of ~ st important application: reproduce sound for film

6 Short Historical Excursion Improved materials discovered later as a combination of good luck with intelligent guessing A very important step was to realize that the photocathode materials are SEMICONDUCTORS Metallic versus Nonmetallic materials: yield of metallic photocathodes is very low because of very high reflectivity semiconductors have less reflection losses The main loss process in metals is the e-e scattering; => e-e escape depth of only few atomic layers is possible

7 Short Historical Excursion 1910: Photoelectric effect on K-Sb K compound was found (Pohl & Pringsheim). 1923: found that thermionic emission of W is greatly enhanced when exposed to Cs vapour (Kingdon & Langmuir). It was found that the work function in the above case was lower than of Cs metal in bulk. 1936: discovered high efficiency of Cs-Sb (Görlich).

8 QE of Metals For photon energies > 12 ev QE of % were reported for Ni, Cu,, Pt, Au,, W, Mo, Ag and Pd (1953, Wainfan). 7% for 15 ev 2% for 17 ev

9 QE: Short Historical Excursion Sommers found the multialkali effect: combination of Cs-K-Na Na-Sb has high QE in the visible spectrum. Also were discovered Cs 3 Sb on MnO (S11, QE ~ 20%) (Cs)Na 2 KSb (S20, QE ~ 30%) K 2 CsSb ( QE ~ 30%) K 2 CsSb(O) ( ( QE ~ 35%)

10 Typical Quantum Efficiencies

11 Boost of the QE of Bialkali PMTs In recent years we were intensively working with the well-known PMT manufacturers trying to boost QE of bialkali PMTs. Over past 40 years there was no progress. After several iterations there was success. Already 2 years ago PMTs with peak QE values in the range of % became available. These new high QE PMTs are used in the imaging camera of the MAGIC-II II telescope

12 How is it possible to boost the QE and who is interested in it? Use of highly purified materials for the photo cathode (change from or even of higher purity; will provide less scattering length for e - (low recombination probability) Optimal tuning of the photo cathode thickness Optimal tuning of the material composition Optimal tuning of the anti-reflective layer Optimal tuning of the Cs layer thickness

13 QE of our old champion 2 PMT from Hamamatsu Mirzoyan, et al., NIM A (proc. Beaune 05)

14 PMTs of MAGIC-I WLS milky layer effect QE by a diffuse scattering coating, +WLS (D. Paneque, et al., 2002) Effective QE ~ 15 %

15 Recent PMTs Electron Tubes Different Different batches show different behaviour QE QE is high (~30%!!) Peak ~ 350 nm Low Low QE at long (> 450 nm)

16 QE of 3 PMTs (2 Hamamatsu + 1 ET) before and after coating with milky layer

17 Charge collection efficiency QE alone is not a very meaningful parameter for a PMT. The charge collection efficiency (CE) is an equally important parameter. The convolution of the QE with the CE is the real important parameter, the photon detection efficiency, PDE. This is what one needs to measure While an absolute measurement is not easy, a comparative, relative measurement can be easily performed.

18 PDE measurements 0.6 m 2.1 m laser Optical axis is adjusted 0.6 m PMTs were observing a piece of white wall of 2.1 m size. The full observing angle was set to 120.

19 PDE measurements We performed Photon Detection Efficiency (PDE) measurements for Hamamatsu and ET PMTs. 80 ps flashes from a 400 nm were illuminating a white wall in a storage room.

20 PDE measurements Single photoelectrons ET v v v v Hamamatsu3352

21 Final PMT selection Our measurements show that Hamamatsu PMT have on average 20 % higher photon detection efficiency (PDE) than ET PMTs(this essentially reflects the existing differences between the QE s). The QE of a not coated PMT from Hamamatsu is comparable to the QE of a milky coated ET. The coating of Hamamatsu PMT is increasing its effective QE by ~10 %. => select Hamamatsu PMTs for the M-II camera. Short before we were making the order for the selected PMTs for the M-II camera to Hamamatsu, they released news on their very recent developments, Ultrabialkali PMTs:

22 Recent Surprises All the 3 PMT manufacturers could report enhanced QE values, the best being Hamamatsu, who gave it the name Super-bialkali (QE~ %). One year ago Hamamatsu claimed to produce PMTs with peak QE of %! (once the djinn comes out of the lamp you cannot control it anymore) ;-) Recently also Photonis joined club of Ultra-bialkali. Moreover, it pushed the QE values even higher up!

23 The very recent 3 Photonis PMTs: QE peak values in excess 50 %! Preliminary!

24 Afterpulse PMT Selection MAGIC-II photocathode Afterpulse Palma ~ 130 MHz time 1st dynode Phe. H 2 O H+ Ions fly back and hit the cathode then produce photoelectrons again. Secondary e-e 2ed dynode If Afterpulse rate is high > 1 %, the afterpulses will dominate MAGIC trigger.

25 PMT Selection MAGIC-II Afterpulse Timing Spectrum Main pulses The time between the main pulse and the afterpulse is about the transit time of the ion from the 1st dynode to the cathode. The ions may come from H 2 O, CH 4 and He Assume the electric field between cathode and 1st dynode is E q*e = m*a a = q*e/m S = 0.5*a*t²; t² = 2*S/a ns t = sqrt( 2*S*m/(q*E))

26 Afterpulse Rate PMT Selection MAGIC-II Most of the PMTs have afterpulse rate 0.2~0.8% even for SBA PMT from Hamamatsu NO correlation between QE and afterpulse rate!!

27 PMT Selection MAGIC-II Aging Test: PMT never die; they just fade away Due to long time illumination => the ynodes become tired (fatigue) => gain rops. The PMTs were run totally for inutes (7 days), under the constant llumination that induced an initial anode urrent of 150 µa.(the Palma is bout 1 µa). So we illuminate with tronger light intensity to speed up the easurement.

28 Aging Test H-xc-3348 H-xc-3344 ET-2325 ET Light intensity variations are taken into account by using a monitoring PIN diode. MAGIC PMTs are operated under moon observation. Assume average DC is 2 ua. 1 year operation : 2000 h * 3600 s * 2uA ~ 15 C. => For h-xc3348: gain drop to 90 % Total charge, C

29 PMT Selection MAGIC-II Pulse Width, Rising and falling time An fast oscilloscope (1.5 GHz bandwidth), 5 G/s sampling rate, followed by a 2 GHz bandwidth amplifier (gain x 100) is used. ET Single ph.e. Ham Single ph.e. Fast response : rising time ~ 700 ps, FWHM~ 1.1 ns

30 Requested budget 400 Hamamatsu UBA PMTs: 500 /unit Associated electronics Travel 3 years Oscilloscope Laser Others total euros total euros Tests using MAGIC I central inner camera

31 Conclusions In recent years on our request the main PMT manufacturers were working on boosting the QE of classical PMTs As a result bialkali PMTs of size with % peak QE became commercially available already in 2006 (~ 35% boost!)(they they got the name super-bialkali) In autumn 2006 we learned from Hamamatsu about the so-called ultra-bialkali PMTs with % peak QE Now also Photonis could demonstrate on the example of 3 PMT peak QE values scattered in the range %. Together with SiPM the new bialkali PMTs will dominate the market very soon!

32 THE END

33 Other strongly competing ultra-fast, LLL sensors with single ph.e. resolution In recent times two more types of ultra-fast response LLL sensors, providing good single ph.e. resolution, start to strongly compete with the classical PMTs. These are HPDs with GaAsP photocathode SiPM (and its variations)

34 Calibration with SiPM: <46> ph.e. are measured

35 HPD Output Signal <pulse shape> <pulse height distribution> Time [ns] FWHM~2.7 ns

36 Escape Depth Escape depth can be defined as the thickness above which the photoemission becomes independent on thickness (in reflective mode) The measured escape depth was atomic layers for K, Rb, Cs (1932).

37 QE boost with Wavelength Shifter WLS Butyl- PBD ( to nm) POPOP ( to nm) Paraloid B72 (n = 1.4) in Toluene On the Input window

38 Light conversion into a measurable Visible light can react and become measurable by: Eye Eye (human: QE ~ 3 % & animal), plants, paints,... Photoemulsion (QE ~ %) (photo-chemical) Photodiodes (photoelectrical, evacuated) Classical & hybrid photomultipliers (QE ~ 25 %) QE ~ 45 % (HPD with GaAsP photocathode) Photodiodes (QE ~ %) (photoelectrical) PIN PIN diodes, Avalanche diodes, SiPM,... photodiode arrays like CCD, CMOS cameras,...

39 Short Historical Excursion The losses in Semiconductors because of phonon scattering (interaction with lattice) are much less, i.e. e-e from deeper layers can reach the surface

40 Short Historical Excursion Metal Semiconductor Photon e- conversion e- motion High reflectivity Low efficiency Low efficiency: e- e- scattering Low reflectivity High efficency High efficiency low phonon loss Surface barrier Work function > 2 ev Determined by e-e affinity

41 PMT Selection MAGIC-II Single Photoelectron Spectrum p/v =1 p/v=3 DW 139 p/v=1.4 zl-7016 Keep 1 phe events < 5% P/V =1 ET117 P/V =1 xc-3353 Require P / V ratio > 1.3 in order to get better Single Photoelectron Resolution.

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