Scintillation R.L. Cooper
What is Scintillation? • In particle physics, particles deposit energy into a detector medium • The medium is “excited” • How do we extract this information? • Last week we heard of a number of ways • Utilize the EM interaction in some way
• Scintillation is the conversion of the excitation energy to photons • Depending on timescale, also referred to luminescence, phosphorescence, fluorescence, etc
Some Scintillators I Have Used 128
Inorganic BGO Crystals (RDK)
Organic Liquids (SciBath) Liquid Noble Gas (COHERENT) !-"#$%:+*(*(>:'%&'(')(*+ =>,&8+1'(16(,&*?34;(,
●*9'%)/:* ;* 1 ms • Impurities or defects can create “energy” traps or metastable states • BGO (among others) tend to have low afterglow out to 3 ms • Many Tl-doped scintillators can be quite high à order-% after 3 ms • COHERENT experiment uses CsI[Na] instead of more traditional CsI[Tl] for this reason
A Table of the Most Common Inorganic Scintillators NaI(Tl)
CsI(Tl)
CsI(Na)
CsI(pure)
BGO
CaF2 (Eu)
Light Yield (photons / keV) 300 K
38
54
41
2
8-10
19
Light Yield at 77 K relative to 300 K
< 1∗
< 1∗
< 1∗
10
3
n/a
Emission wavelength (nm)
415
550
420
315
480
435
Primary Decay Time (ns) 300 K
250
1000
630
16
300
940
Density (g/cm3)
3.67
4.51
4.51
4.51
7.13
3.18
Index of Refraction
1.85
1.79
1.84
1.95
2.15
1.47
Hygroscopic
yes
slightly
yes
slightly
no
no
A more extensive HTML table is available at: http://scintillator.lbl.gov
Scintillation Mechanism for Most Inorganic Crystal Band Structure Inorganic Crystals
excitation
electron
hole
from S.E. Derenzo
Organic Liquid Scintillators
Minimum Amount of Chemistry • Carbon bonds hybridize • sp2 hybridization forms s bonds that are in plane and bond carbons together • The remaining 6p orbitals form p bonds are out of plane and delocalized • Electrons in p bonds “orbit” with both spins in both directions
ersystem crossing can Competing Effects populating the triplet
• Excited state waveT1 and T 1-S0 cannot occur function has some ctly due to angular overlap with ground mentumstate à and parity non-radiative ection rules decay
s a long lifetime since • Intersystem excitation longto theof triplet state à S0 is forbidden
lived phosphorescence is phosphorescence
• T1 ßà S0 forbidden by ed fluorescence from spin / parity (slow)
plet can also occur
+ T1 → S1 + S0 + phonons
http://micro.magnet.fsu.edu/primer/techniques/fl uorescence/fluorescenceintro.html
from http://micro.magnet.fsu.edu/primer/techniques/fluorescence/fluorescenceintro
Making a Liquid Scintillator 1. Start with inexpensive benzene derivative
pseudocumene
xylene
2. Add high-efficiency fluor to non-radiatively transfer energy: tend to be more expensive butyl-PBD
PPO
p-terphenyl
3. Add additional wavelength shifters: bis-MSB, POPOP 4. Dilute for attenuation length (e.g., mineral oil)
Other Popular Solvents • Other issues with benzene derived solvents • Flammability, flash point, carcinogenic, etc • DIN
• LAB
Pulse Shape Discrimination • Some scintillators have different pulse shape due to different ionization / excitation methods (e-, nuclear-recoil)
Quenching from Ionization Recombination • A photon strikes an atomic electronic • Electron carries tremendous energy and creates ionization and excitation in a long track • Ionization and excitation decay back to ground state emitting photons
Quenching from Ionization Recombination • Neutron strikes an atomic nucleus • Recoiling nucleus deposits more energy in a given path length (higher dE/dx than electrons) • Ionization and excitation density higher • More non-radiative recombination may be possible in shortened region
Ionization Quenching: Birks’ Law Ionization Quenching – Birks’ Rule • Assume linear light output to start with linearity at low ionization dE density dL =A energy deposit at low dx dx ionization density let the density of excited molecules be proportional to the dL/dx = A dE/dx ionization density dE B • Also, density of excitation is dx let k be the fraction that is proportional to energy quenched dE A density dL = dx B dE/dX dx 1 + kB dE dx for small dE/dx, approaches • k is the fraction of excitation linearity that get quenched for large dE/dx, approaches saturation dL dE AA dL
dx = dx = kB dx 1 + kB dE dx
from Birks
• for any given scintillator composition, must fit the quenching data to get kB • A is the absolute scintillation efficiency
Light Output vs. Recoiling Species for Typical Organic Liquid ELJEN TECHNOLOGY SWEETWATER, TEXAS
RESPONSE OF EJ-301 LIQUID SCINTILLATOR SCINTILLATION LIGHT PRODUCED VS. PARTICLE ENERGY 6
NUMBER OF SCINTILLATION PHOTONS PRODUCED
10
105
ELECTRONS
104 PROTONS
103 ALPHAS
CARBONS
102
10
Data Source: V.V. Verbinski et al, Nucl. Instrum. & Meth. 65 (1968) 8-25
0.1
1
10 PARTICLE ENERGY (MeV)
100
Comparing Inorganic vs. Organic Scintillators • Best crystals have 40,000 photons / MeV energy deposit: Best organics produce just over 10,000 • Inorganic crystals have high density (5 g/cm3) whereas organics are similar to water • Inorganic crystals have variable Z for excellent photoelectric effect response vs. organics have Z ~ 6 • Organic scintillators have fast timing on ns timescales vs. 0.1-1 microsecond timing for inorganic scintillators • Radiation damaging a big issue crystals
Liquid Noble Gas Scintillators
The Basics:
The Basic Properties •
Light yield ~ few 10,000’s of photons per MeV (dependences on E field, LNG has high scintillation light yield particle type and purity)
E. Morikawa et al., J Chem
J Chem Phys vol 91 (1989) Phys 91 (1989) 1469. 1469 E Morikawa et al
(10s photons per keV)
•Wavelength Up to 40 for LAr, 25 for LXe of emission is 128nm
• “Fast” and “slow” components in Light with two characteristic time pulse shape •
constants: • 6 ns: 1600 ns for LAr, 3 ns: 27 ns for LXe - fast component, 6 ns VUV light production - slow component,1500 ns
• 128 nm for LAr, 178 nm for LXe Argon is highly transparent to its • Long photon attenuation lengths and own scintillation light. electron transport lengths (> 10 m)
• For Ar, scalable to > 10 kTon detectors
l (nm) = (1240 eV·nm) / E (eV)
Liquid Noble Gas Scintillation Path Self-Trapped Exciton Luminescence
Ar+
Ar+ Ar e-
e-
µAr Particle Collision
Thermal e- & Recombination
Ionization
Ar*
Excitation Recombination Luminescence
Ar*
Ar
Exciton Formation
Ar
g
Ar
Radiative Decay
Adapted from slides by Ben Jones talk on LArTPC Workshop
Exciton Formation and Light
http://www.e15.ph.tum.de/research_and_projects/liquified_rare_gases/
Exciton Formation and Light Calculations of the excimer state energies of xenon, as a function of nuclear separation J. Chem Phys 52, 5170 (1970)
eAr2+
http://www.e15.ph.tum.de/research_and_projects/liquified_rare_gases/
Excitons: Singlets and Triplets Ar*
Ar*
Ar
Exciton Formation
Ar
Singlet Exciton
Ar*
Singlet Scintillation Time Constants of LAr Scintillat Decay Time ~6 ns
An example from: 2010 JINST 5 P06003 (WArP collaboration)
Ar
Triplet Exciton
Triplet Scintillation Decay Time ~1600 ns
Pulse Shape Discrimination: Exciton Formation Path Matters Self-Trapped Exciton Luminescence
Ar
35% Singlet
Exciton Formation
65% Triplet
Ar*
Ar
50% Singlet
Exciton Formation
50% Triplet
Ar* Recombination Luminescence
Ar
g
Ar
Radiative Decay
Adapted from slides by Ben Jones talk on LArTPC Workshop
Quenching Results in Argon: Results from DEAP Collaboration
Mechanisms for Quenching Quenching by Nitrog • Because triplet is long, strongest effect on slow lifetime • 2 ppm N2 concentrations • What about Xenon dimers? • Nitrogen also absorbs photon Competing Excimer Dissociation Process
Ar*
Ar
Ar
Ar
N
N
N
N*
• First measured by WArP:
Acciarri et al 2010 JINST 5 P06003
Additional Thoughts About Purity: O2 & H2O Is NOT Your Friend • Oxygen highly electronegative à readily absorbs ionization electrons and stunts recombination scintillation pathway • Diatomic excimer competition too? • 21% of air and generally in all cryogenic liquids • 10 ppb levels of oxygen affect scintillation • For TPCs, oxygen will absorb the traveling electrons • Argon can be too pure and leads to high voltage standoff issues à track down more than anecdotal evidence