Radiation Detection
description
Transcript of Radiation Detection
Radiation Detection
• ionization chambers (dosimeters, pulse chambers, particle track chambers)
• scintillation detectors
• semiconductor detectors
• photographic emulsions
interaction with atoms
E = h
12
1. EXCITATION
(Energy of the radiation used for increasing the internal energy of the atom)
2. IONIZATION
(Radiation separates the atom into an electron and an ion.)
ionization level
Particles of different radiation carry different amounts of energy.
typical ionization energy range: 10 - 25 eV
-radiation - 100
number of primary ions:
-, -radiation - 100 000
recombination
+
-
+
-
+-
Ions may collide inelastically to form a neutral atom.
The probability of recombination:
2nnndt
dn
n - number of pairs of ions - recombination coefficient
Excess energy is released in the form of electromagnetic radiation.
ionization chamber dose meters
+ +
+ +
+ +
++
pocket ion chamber electroscope
condenser-R-meter
V
electrometer
V
charge collection
+- -+
+ -
• With no field the ions eventually recombine leaving no record of radiation.
+- -+
+ -
+- -+
+ -
• With a weak field some ions recombine and some are discharged by the electrodes.
• With a sufficiently strong (but limited) field all the ions are discharged by the electrodes (saturation).
• Further increase of the field results in an avalanche discharge.
gas-amplification factor
The collected charge is proportional to the charge of the primary ions. The proportionality coefficient is called the gas-amplification factor.
recombination region: ions remain in the chamber for an extended time; some ions recombine and are not collected
(factor < 1)
saturation region: no time for recombination; no energy for secondary ionization
(factor = 1)
avalanche ionization: ions achieve sufficient energy to ionize neutron atoms
(factor > 1)
Geiger – Müller (G-M) tube
+
ab
concentric electric field:
r
1
ln
VE
b/a
ionization potential:
V2510V
required field:
V
E
where is the mean free path of the ions.
a ~ 0.08 mm
The strongest field is at the anode.
G-M tube operation regimes
0 250 500 7501
102
104
106
108
1010
tube voltage
puls
e si
ze
A
A – recombination region
B
B – saturation region (dependent on energy)
CC – proportional region
D D – limited proportionality
E
E – Geiger region (independent of energy)
F
F – continuous discharge
electric pulse in the Geiger region
space charge
r0
E1 E2
From Gauss’s law
rl
1
2
qE
0
1
rl
1
2
qQE
0
2
,
With a relatively small signal V const and the charge on the central wire is
tr
bln
2
tQV
ln
2tq
00
0
lb/a
l
Typically the space charge reaches the cathode and gets neutralized in 100 s.
quenching the discharge
Neutralization of ion results in photoelectric effect. The electrons liberated from the cathode often trigger self-perpetuating series of discharge at a frequency determined by the circuit time constant.
Quenching circuits or quenching gases are used to prevent secondary discharge.
Properties of a quenching gas:
• ionization energy lower than that of the main gas and the work function of the cathode material
• absorb UV
• dissociate rather than radiate UV
pulse shape
1.0
0.5
1.0
time (10-4 s)
puls
e vo
ltag
e
0 2 4 6 8
0.89
V
The discharge (slightly) lowers the anode potential.
After the discharge the potential of the anode is restored by the high voltage power supply.
G-M counter
HV- +
counting circuit
amplifier/discriminator
The proportional region:
gas amplification factor ~ 103
moderately strong pulses;dispersive pulse size;
G-M region:
gas amplification factor ~ 106 - 107
very sensitive to radiation;
resolving time
1.0
0.5
1.0
time (10-4 s)
puls
e vo
ltag
e
0 2 4 6 8
0.89
V
0.2
V
The dead time and the recovery time depend on the threshold voltage of the circuit.
counting rate
600 800 1000 12000
100
200
300
tube voltage
coun
ts p
er m
inut
e
A
A – threshold voltage
B
B – fraction of primary events countedC D
C-D – all primary events counted (plateau)
E
E – continuous discharge(a single event results in repetitive spontaneous discharge)