1 Fulvio TESSAROTTO GDD meeting, CERN, 01/10/2008 Trieste THGEM news First indications from...

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Fulvio TESSAROTTO GDD meeting, CERN, 01/10/2008 GDD meeting, CERN, 01/10/2008 Trieste THGEM news Trieste THGEM news 1 First indications from First indications from electrostatic simulation exercise electrostatic simulation exercise Goals of the simulation Parameters of simulated THGEM Values of E z Simulated trajectories News about UV light source work done by Gabriele Giacomini

Transcript of 1 Fulvio TESSAROTTO GDD meeting, CERN, 01/10/2008 Trieste THGEM news First indications from...

Fulvio TESSAROTTO GDD meeting, CERN, 01/10/2008 Trieste THGEM newsGDD meeting, CERN, 01/10/2008 Trieste THGEM news 11

First indications from electrostatic First indications from electrostatic simulation exercisesimulation exercise

Goals of the simulation

Parameters of simulated THGEM

Values of Ez

Simulated trajectories

News about UV light source

work done by Gabriele Giacomini

Fulvio TESSAROTTO GDD meeting, CERN, 01/10/2008 Trieste THGEM newsGDD meeting, CERN, 01/10/2008 Trieste THGEM news 22

Electrostatic calculations are Electrostatic calculations are essential to optimize our essential to optimize our

THGEMsTHGEMs

We decided to start from simple simulation exercises with ANSYS (and Garfield) in order to estimate the optimal geometrical and electrical configuration for the THGEM

Critical points:

- Effective CsI Q.E. depends on the electric field at the CsI surface

- The backscattering effect depends on the gas and on the field too

-The collection of photoelectrons in the holes for multiplication is

difficult to measure and critically depends on geometry and fields

The optimization of the THGEM geometry and operating parameters

will need some understanding, which can be achieved only

combining measurements and simulations

Fulvio TESSAROTTO GDD meeting, CERN, 01/10/2008 Trieste THGEM newsGDD meeting, CERN, 01/10/2008 Trieste THGEM news 33

Focusing is done by hole dipole field.• Maximum efficiency at Edrift =0 (like in GEM).• Slightly reversed Edrift (50-100V/cm) good photoelectron collection & low sensitivity to MIPS (~5-10%) !

-0.6 -0.4 -0.2 0.0 0.2 0.4 0.60.0

0.5

1.0

1.5

2.0

0

Gain~103

1 Atm. Ar/CH4(95:5)

40

20

80

60

100

e- tr

ansf

er e

ffici

ency

[%]

Edrift [kv/cm]

Re

lativ

e

Reverse drift studies at Weizmann

eRef. PC

Edrift

E

EE=0

MIP

Attention: gas and field dependent!

Fulvio TESSAROTTO GDD meeting, CERN, 01/10/2008 Trieste THGEM newsGDD meeting, CERN, 01/10/2008 Trieste THGEM news 44

High field on the PC surface (high effective QE)Also at low THGEM voltages (e.g. in Ne mixtures!)

eRef PC

0.4mm thick0.3mm holes0.7mm pitch

>3kV/cm

Electric field on photocathode surfacecreated by the hole dipole field

VTHGEM=2200V

VTHGEM=1200V

VTHGEM=800V

VTHGEM=2200V

VTHGEM=1200V

VTHGEM=800V

C. Shalem et al. NIM A558 (2006) 468

FIELD AT THE THGEM CsI SURFACE

Attention: varies with hole-pitch & hole-voltage

Fulvio TESSAROTTO GDD meeting, CERN, 01/10/2008 Trieste THGEM newsGDD meeting, CERN, 01/10/2008 Trieste THGEM news 55

Recent measurement by ElenaRecent measurement by ElenaSingle THGEM, diam. 0.4 mm, th. 0.4 mm, pitch: 0.8 mm

Fulvio TESSAROTTO GDD meeting, CERN, 01/10/2008 Trieste THGEM newsGDD meeting, CERN, 01/10/2008 Trieste THGEM news 66

Photocurrent vs field on CsIPhotocurrent vs field on CsI

not acceptable

acceptable good

Fulvio TESSAROTTO GDD meeting, CERN, 01/10/2008 Trieste THGEM newsGDD meeting, CERN, 01/10/2008 Trieste THGEM news 77

The operational The operational ΔΔVV of THGEMs depends of THGEMs depends on gason gas

Simulation performed using tools provided by RD51 Colleagues:

based on “ANSYS” and “GARFIELD”

Fulvio TESSAROTTO GDD meeting, CERN, 01/10/2008 Trieste THGEM newsGDD meeting, CERN, 01/10/2008 Trieste THGEM news 88

Geometrical parameters of simulated Geometrical parameters of simulated THGEMTHGEM

DEFAULT VALUES

Thickness: 0.6 mm,

Hole diameter: 0.4 mm,

Pitch 0.8 mm,

Rim: 0.0 mm,

Cu thickness: 0.035 mm,

Drift distance:4.0 mm, (cont. plane)

Induction dist.: 3.0 mm, (cont. plane)

Induction field: 0.0 V/cm

Drift field: 0.0 V/cm

ΔV: 1500 V

Basic cell structure

Simulation performed by Gabriele Giacomini, using tools provided by Matteo Alfonsi and Gabriele Croci, based on ANSYS and GARFIELD

Fulvio TESSAROTTO GDD meeting, CERN, 01/10/2008 Trieste THGEM newsGDD meeting, CERN, 01/10/2008 Trieste THGEM news 99

Values of Ez along the “z” axis, for different diameters

diameter scan

0

5000

10000

15000

20000

25000

30000

-0.1 -0.08 -0.06 -0.04 -0.02 0 0.02 0.04 0.06 0.08 0.1

z (cm)

Ez

(V/c

m)

0.1 mm

0.2

0.3

0.4

0.5

0.6

holescan along the

“z” axis (hole axis)

Thickness: 0.6 mm,

Pitch: 0.8 mm,

Induction field: 0.0 V/cm

Drift field: 0.0 V/cm

Fulvio TESSAROTTO GDD meeting, CERN, 01/10/2008 Trieste THGEM newsGDD meeting, CERN, 01/10/2008 Trieste THGEM news 1010

diameter scan

-10000

-7500

-5000

-2500

0

2500

5000

7500

10000

0 0.01 0.02 0.03 0.04 0.05 0.06 0.07

y (cm)

Ez

(V/c

m)

0.1 mm

0.2

0.3

0.4

0.5

0.6

Values of Ez along the “y” axis, for different diameters

0.4 mm diam. hole

Thickness: 0.6 mm,

Pitch: 0.8 mm,

Induction field: 0.0 V/cm

Drift field: 0.0 V/cm

diameter:

Fulvio TESSAROTTO GDD meeting, CERN, 01/10/2008 Trieste THGEM newsGDD meeting, CERN, 01/10/2008 Trieste THGEM news 1111

Values of Ez along the “y” axis, for different pitches

-8000

-6000

-4000

-2000

0

2000

4000

6000

8000

10000

0 0.01 0.02 0.03 0.04 0.05 0.06 0.07

y (cm)

Ez

(V/c

m)

0.6 mm

0.7

0.8

1

1.2

pitch:

hole

Thickness: 0.6 mm,

Diameter: 0.4 mm,

Induction field: 0.0 V/cm

Drift field: 0.0 V/cm

Fulvio TESSAROTTO GDD meeting, CERN, 01/10/2008 Trieste THGEM newsGDD meeting, CERN, 01/10/2008 Trieste THGEM news 1212

field values depend on: field values depend on:

Thickness: Ez = Ez0 × (th0 / th)

Hole diameter: non trivial (see slides)

Pitch: non trivial (see slides)

Rim: unknown

Drift field: Ez = Ez0 + ED

ΔV: Ez = Ez0 × ΔV / ΔV0

Max. V attained with th. = 0.2 mm ~ 900 V

Max. V attained with th. = 0.4 mm: ~1400 V

Max. V attained with th. = 0.6 mm: ~1700 V

Fulvio TESSAROTTO GDD meeting, CERN, 01/10/2008 Trieste THGEM newsGDD meeting, CERN, 01/10/2008 Trieste THGEM news 1313

Values of Ez on the CsI surface for various diameters and pitches, compared with active area

0

500

1000

1500

2000

2500

3000

0 0.2 0.4 0.6 0.8 1 1.2 1.4pitch(mm)

Ez

on

TO

P s

urf

ace

0.4

0.5

0.6

0.7

0.8

0.9

1

acti

ve a

rea

diam. = 0.2 mm

0.3

0.4

0.5

0.6

Ez ~ 1/ (pitch)4

Fulvio TESSAROTTO GDD meeting, CERN, 01/10/2008 Trieste THGEM newsGDD meeting, CERN, 01/10/2008 Trieste THGEM news 1414

Values of Ez on the CsI surface for various pitches and diameters, compared with active area

0

500

1000

1500

2000

2500

3000

0 0.1 0.2 0.3 0.4 0.5 0.6 0.7

diameter (mm)

Ez

on

TO

P s

urf

ace

0.4

0.5

0.6

0.7

0.8

0.9

1

ac

tiv

e a

rea

pitch = 0.6 mm

0.7

0.8

1

1.2 Ez ~ exp(diam.)

Fulvio TESSAROTTO GDD meeting, CERN, 01/10/2008 Trieste THGEM newsGDD meeting, CERN, 01/10/2008 Trieste THGEM news 1515

Photoelectron collectionPhotoelectron collection

hole

efficient collection area

dead area

x

y

Fulvio TESSAROTTO GDD meeting, CERN, 01/10/2008 Trieste THGEM newsGDD meeting, CERN, 01/10/2008 Trieste THGEM news 1616

trajectories for drift = 0 V/cm

x

y scan along the “y” axis

scan along the “x” axis

x

y

Collection efficiency is o.k.

y0- 0.2 0.2 0.5- 0.5

Ez = - 543 V/cm

th. 0.6 mm, diam. 0.4 mm, pitch: 0.8 mm, ΔV = 1500 V

Fulvio TESSAROTTO GDD meeting, CERN, 01/10/2008 Trieste THGEM newsGDD meeting, CERN, 01/10/2008 Trieste THGEM news 1717

trajectories for drift = -50 V/cm

x

y scan along the “y” axis

scan along the “x” axis

x

y

partial collection efficiency

y0- 0.2 0.2 0.5- 0.5

Ez = - 593 V/cm

“full collection radius” = 0.42 mm

th. 0.6 mm, diam. 0.4 mm, pitch: 0.8 mm, ΔV = 1500 V

Fulvio TESSAROTTO GDD meeting, CERN, 01/10/2008 Trieste THGEM newsGDD meeting, CERN, 01/10/2008 Trieste THGEM news 1818

trajectories for drift = -500 V/cm

scan along the “y” axis

scan along the “x” axis

low collection efficiency

y0- 0.2 0.2 0.5- 0.5

Ez = - 1043 V/cm“full collection radius” = 0.33 mm

th. 0.6 mm, diam. 0.4 mm, pitch: 0.8 mm, ΔV = 1500 V

Fulvio TESSAROTTO GDD meeting, CERN, 01/10/2008 Trieste THGEM newsGDD meeting, CERN, 01/10/2008 Trieste THGEM news 1919

trajectories for drift = +500 V/cm

scan along the “y” axis

scan along the “x” axis

Ez by far too low

y0- 0.2 0.2 0.5- 0.5

Ez = - 43 V/cm x

yy

x

th. 0.6 mm, diam. 0.4 mm, pitch: 0.8 mm, ΔV = 1500 V

Fulvio TESSAROTTO GDD meeting, CERN, 01/10/2008 Trieste THGEM newsGDD meeting, CERN, 01/10/2008 Trieste THGEM news 2020

trajectories for drift = +500 V/cm

scan along the “y” axis

scan along the “x” axis

y0- 0.2 0.2 0.5- 0.5

Ez = + 57 V/cmx

yy

x Loss of e-

th. 0.6 mm, diam. 0.4 mm, pitch: 0.8 mm, ΔV = 1500 V

Fulvio TESSAROTTO GDD meeting, CERN, 01/10/2008 Trieste THGEM newsGDD meeting, CERN, 01/10/2008 Trieste THGEM news 2121

Consistency check with other Consistency check with other simulation programssimulation programs

lattice spacing:

50 μm, 30 μm, 20 μm

Fulvio TESSAROTTO GDD meeting, CERN, 01/10/2008 Trieste THGEM newsGDD meeting, CERN, 01/10/2008 Trieste THGEM news 2222

Consistency check with other Consistency check with other simulation programssimulation programs

diameter scan

-10000

-7500

-5000

-2500

0

2500

5000

7500

10000

0 0.01 0.02 0.03 0.04 0.05 0.06 0.07

y (cm)

Ez

(V/c

m)

0.1 mm0.20.30.40.50.6

Fulvio TESSAROTTO GDD meeting, CERN, 01/10/2008 Trieste THGEM newsGDD meeting, CERN, 01/10/2008 Trieste THGEM news 2323

Main uses of UV lightMain uses of UV light

UVA light (315 nm – 400 nm) is also called photochemical ray because many kinds of adhesives, fluorescence, and other chemistries react to UVA light. For the reason, its potential uses are uncountable, including UV curing/printing/coating, skin therapy, bank note detector, bio-weapon detector, air purification, etc Applications: 1) UV curing systems, UV coating/printing assemblies for PVC, film, glass materials, and etc. 2) Security products such as Bank note detectors, Bio-weapon Detectors, Crime scene inspection, etc. 3) Phototheraphy devices to treat skin diseases including psoriasis, rickets, eczema, jaundice, and atopic dermatitis. 4) Automotive leak detector, Food checking.  UVB light (280 nm – 315 nm) is well known that UVB light exposures can be hazardous to human eyes and skin, but also UVB, often called as a dorno ray or a health ray, is assumed to be a beneficial to human health, UVB produces vitamin D in the skin, and prevent skin cancer caused by inefficient UVB exposure.Also in combinations of UVA (or by it self) UVB has become an increasingly popular and effective treatment for psoriasis, vitiligo, eczema, and other skin conditions. Most effective in case of psoriasis is UV light with wavelength of 311 nmApplications: 1) Sterilization systems to purify water, surface, and air 2) Analysis of Minerals 3) EPROM Erasure 4) High Security UV marks  UVC light (200 nm – 280 nm) is also called germicidal ray. are the highest energy, most dangerous type of ultraviolet light. With that energy, it destroys DNA & PNA in microorganisms such as bacteria, viruses & mold, Thus, it generates Ozone.Especially 254.7nm is most effective wavelength for disinfectionsApplications: 1) Water/Surface purification system 2) Laboratory testing devices

Fulvio TESSAROTTO GDD meeting, CERN, 01/10/2008 Trieste THGEM newsGDD meeting, CERN, 01/10/2008 Trieste THGEM news 2424

LED at 255 nmLED at 255 nm