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NNN05 Next Generation of Nucleon Decay and Neutrino Detectors 7-9 April 2005, Aussois, Savoie, France detector considerations for neutrino physics Tony Wright, Electron Tubes Limited
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NNN05 Next Generation of Nucleon Decay and Neutrino Detectors 7-9 April 2005, Aussois, Savoie, France detector considerations for neutrino physics Tony.

Jan 04, 2016

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Page 1: NNN05 Next Generation of Nucleon Decay and Neutrino Detectors 7-9 April 2005, Aussois, Savoie, France detector considerations for neutrino physics Tony.

NNN05 Next Generation of Nucleon Decay and Neutrino Detectors7-9 April 2005, Aussois, Savoie, France

detector considerations for neutrino physics

Tony Wright, Electron Tubes Limited

Page 2: NNN05 Next Generation of Nucleon Decay and Neutrino Detectors 7-9 April 2005, Aussois, Savoie, France detector considerations for neutrino physics Tony.

detector considerations for neutrino physics

light detection: large solid angle large cathode area long operating life high gain well-resolved SER fast timing and freedom from artefacts pressure resistant chemically inert glass – free from radioisotopes low temperature operation

power considerations high voltage supplies and control voltage dividers

Page 3: NNN05 Next Generation of Nucleon Decay and Neutrino Detectors 7-9 April 2005, Aussois, Savoie, France detector considerations for neutrino physics Tony.

range of hemispherical photomultipliers

Type d(mm) dynodes σ(τ) ns comments

 

9116 25 6 1.0 high light levels

9114 25 10 1.2

9117 38 6 1.1 high light levels

9372 130 12 2.7

9350 200 14 8

9352 200 6 6 high light levels

9353 200 12 2.7 chemically inert

9354 200 12 2.7 ultra low background 5 Atm

9357 200 12 2.7 -200 0C operation

D737 230 12 2.7

D738 250 12 2.8

9360 280 12 3.0

Page 4: NNN05 Next Generation of Nucleon Decay and Neutrino Detectors 7-9 April 2005, Aussois, Savoie, France detector considerations for neutrino physics Tony.

glass characteristics

thickness: ranges from 2 to 4 mm

 

pressure: 2 to 5 atmospheres

 

radionuclides:

 

type K(ppm) Th(ppb) U(ppb)

 

8246 30 30 30

 

B53 60 30 30

 

B47.2 300 250 100

 

8245 1400 900 1100

Page 5: NNN05 Next Generation of Nucleon Decay and Neutrino Detectors 7-9 April 2005, Aussois, Savoie, France detector considerations for neutrino physics Tony.

0

0.5

1

1.5

2

2.5

3

0 0.5 1 1.5 2 2.5 3 3.5 4 4.5 5

photoelectrons equivalent, h

p(h

)dh

single electron response SER

Page 6: NNN05 Next Generation of Nucleon Decay and Neutrino Detectors 7-9 April 2005, Aussois, Savoie, France detector considerations for neutrino physics Tony.

timing distribution

Page 7: NNN05 Next Generation of Nucleon Decay and Neutrino Detectors 7-9 April 2005, Aussois, Savoie, France detector considerations for neutrino physics Tony.

0.003 0.004 0.005 0.006 0.007 0.008 0.00910

-2

10-1

100

101

102

103

104

105

106

107

-160

-150

-140

-130

-120

-110

-100

-90

-80

-70

-60

-50

-40

-30

-20

-10

+0

+10

+20

S20

Low temperature bialkali

Bialkali

Temperature / deg. C

A ### ### ###

Re

sist

an

ce /

M.s

q-1

1/T / K-1

Page 8: NNN05 Next Generation of Nucleon Decay and Neutrino Detectors 7-9 April 2005, Aussois, Savoie, France detector considerations for neutrino physics Tony.

lifetime

Page 9: NNN05 Next Generation of Nucleon Decay and Neutrino Detectors 7-9 April 2005, Aussois, Savoie, France detector considerations for neutrino physics Tony.

power supplies

CW type with n individual socket outputs

active divider with n individual outputs

low power dc-dc converter with single output

industrial dc-dc converter with single output

Page 10: NNN05 Next Generation of Nucleon Decay and Neutrino Detectors 7-9 April 2005, Aussois, Savoie, France detector considerations for neutrino physics Tony.

power supply outlines

PS1800/PS1806 PS2010

PS2001

Page 11: NNN05 Next Generation of Nucleon Decay and Neutrino Detectors 7-9 April 2005, Aussois, Savoie, France detector considerations for neutrino physics Tony.

optimising photomultiplier performance with low power consumption

battery operated solar powered (Auger, satellites) underwater, under ice, in liquid argon

 

two considerations:-

  consuming power (voltage divider) providing power (HV supply)

Page 12: NNN05 Next Generation of Nucleon Decay and Neutrino Detectors 7-9 April 2005, Aussois, Savoie, France detector considerations for neutrino physics Tony.

voltage divider considerations

Requirement:  establish and maintain set of fixed dynode potentials there are two generic types available:  traditional resistor configuration active type (FET) The all-resistor divider always fails the requirement if the mean anode current varies

significantly. Active dividers fix the dynode potentials regardless of mean anode current.

Page 13: NNN05 Next Generation of Nucleon Decay and Neutrino Detectors 7-9 April 2005, Aussois, Savoie, France detector considerations for neutrino physics Tony.

active divider networks

Page 14: NNN05 Next Generation of Nucleon Decay and Neutrino Detectors 7-9 April 2005, Aussois, Savoie, France detector considerations for neutrino physics Tony.
Page 15: NNN05 Next Generation of Nucleon Decay and Neutrino Detectors 7-9 April 2005, Aussois, Savoie, France detector considerations for neutrino physics Tony.
Page 16: NNN05 Next Generation of Nucleon Decay and Neutrino Detectors 7-9 April 2005, Aussois, Savoie, France detector considerations for neutrino physics Tony.

power supplies

Type Input power (mW) Efficiency Output current

PS1800 120 - Ia = 200 A

PS1806 400 - Ia = 200 A

PS2010 340 60% ID0 = 100 A

PS2001 4800 40%ID0 = 1000 A

Page 17: NNN05 Next Generation of Nucleon Decay and Neutrino Detectors 7-9 April 2005, Aussois, Savoie, France detector considerations for neutrino physics Tony.

high voltage supply and control system – HVSys

multichannel power supply system individual channel control and monitoring RS485 interface requires only single +12V supply

Page 18: NNN05 Next Generation of Nucleon Decay and Neutrino Detectors 7-9 April 2005, Aussois, Savoie, France detector considerations for neutrino physics Tony.

functional diagram of 1 channel. The hardware shown is integrated within each power base enclosure

Page 19: NNN05 Next Generation of Nucleon Decay and Neutrino Detectors 7-9 April 2005, Aussois, Savoie, France detector considerations for neutrino physics Tony.

0

20

40

60

80

100

0 100 200 300 400 500

anode current, microamps

dg

/g %

R = 680 kΩID0 = 80 μA

R = 100 kΩID0 = 500 μA

R = 20 kΩID0 = 2.5 mA

active divider

Page 20: NNN05 Next Generation of Nucleon Decay and Neutrino Detectors 7-9 April 2005, Aussois, Savoie, France detector considerations for neutrino physics Tony.

-20

-15

-10

-5

0

5

0.1 1 10 100

Ipeak, mA

devia

tio

n f

rom

lin

eari

ty %

HV = 700 V HV = 900 V

Page 21: NNN05 Next Generation of Nucleon Decay and Neutrino Detectors 7-9 April 2005, Aussois, Savoie, France detector considerations for neutrino physics Tony.

detector considerations for neutrino physics

Ron Stubberfield

[email protected]

Tony Wright

[email protected]

available to discuss your particular

requirements