christian buck, mpik heidelberg
DESCRIPTION
Liquid scintillators. Christian Buck, MPIK Heidelberg. LowNu Reims, October 2009. Overview. Introduction Scintillator components Energy transfers Metal loaded scintillators Summary. Liquid scintillator past. Metal loaded: Reines Bugey Chooz Palo Verde. Unloaded: KamLand - PowerPoint PPT PresentationTRANSCRIPT
Christian Buck, MPIK Heidelberg
LowNu
Reims, October 2009
Liquid scintillators
Christian BuckMPIK Heidelberg
Reims, Neutrino Champagne 2009
Overview
Introduction
Scintillator components
Energy transfers
Metal loaded scintillators
Summary
Christian BuckMPIK Heidelberg
Reims, Neutrino Champagne 2009
Liquid scintillator past
Metal loaded:
Reines
Bugey
Chooz
Palo Verde
Unloaded:
KamLand
Borexino
Christian BuckMPIK Heidelberg
Reims, Neutrino Champagne 2009
Challenges: Stability and purity
Palo Verde:
A.G.Piepke, S.W.Moser, V.M.Novikov; NIM A 342 (1999) 392-398
Chooz:
τ ~ 240 days
Gd(NO3)3
Chooz Coll.; Eur.Phys.C27, 331-374 (2003)
KamLand Background:
Christian BuckMPIK Heidelberg
Reims, Neutrino Champagne 2009
Liquid scintillator properties
High energy resolution
Low energy detection threshold
high purity (Borexino)
fast signals (better understanding of timing properties)
moderate cost
Improved stability of metal loaded scintillators
Christian BuckMPIK Heidelberg
Reims, Neutrino Champagne 2009
Liquid scintillator future
Double Chooz, Daya Bay, Reno
SNO+
LENA,…
Christian BuckMPIK Heidelberg
Reims, Neutrino Champagne 2009
Liquid scintillator components
Solvent– pseudocumene, toluene, anisole– „Safe scintillators“: PXE, LAB, DIN– Admixtures: alkanes, mineral oil
Primary fluor– PPO– BPO– Butyl-PBD,…
Secondary fluor– Bis-MSB– POPOP
α, β, γ
*
PMT
Christian BuckMPIK Heidelberg
Reims, Neutrino Champagne 2009
Comparison solvents: Light yield
Solvent Yield (6 g/l PPO)
PC 1.00
Anisole 0.81
PXE 0.88
LAB 0.74
Dodecan 0.40
Oil 0.33
MPIK measurements M.Chen, INT Workshop 2005
Christian BuckMPIK Heidelberg
Reims, Neutrino Champagne 2009
Comparison solvents: Attenuation length
360 380 400 420 440 460 480 500 520 540 560
1
10
100
1000
atte
nuat
ion
leng
th [m
]
wavelength [nm]
n-Dodecan LAB o-PXE Anisole
MPIK measurements (UV/Vis, 10 cm cell)
M.Wurm (TUM), ANT 2009
Christian BuckMPIK Heidelberg
Reims, Neutrino Champagne 2009
Purification methods
Column purification – Radioimpurities– Optics
N2 purging
– Radon, 85Kr– Light yield (oxygen)
Water extraction– Radioimpurities (e.g. 40K)
Distillation– Radioimpurities– Optics
350 400 450 500 550 600-0,0020,0000,0020,0040,0060,0080,0100,0120,0140,016
ab
sorb
an
ce
wavelength [nm]
unpurified b1 unpurified b2 purified
10 m
320 360 400 440 480 520 560 600
0,0
0,1
0,2
0,3
0,4
0,5
abso
rban
cewavelength [nm]
not purified column purification
Christian BuckMPIK Heidelberg
Reims, Neutrino Champagne 2009
Purification methods
Column purification – Radioimpurities– Optics
N2 purging
– Radon, 85Kr– Light yield (oxygen)
Water extraction– Radioimpurities
Distillation– Radioimpurities– Optics
Borexino
KamLand
CTF
LAK
Solar neutrino phase
Christian BuckMPIK Heidelberg
Reims, Neutrino Champagne 2009
Borexino Background
PRL 101, 091302 (2008)
40K < 3 ∙10-18 g/g238U: 1.6 ± 0.1∙10-17 g/g232Th: 6.8 ± 1.5∙10-18 g/g
Christian BuckMPIK Heidelberg
Reims, Neutrino Champagne 2009
LAB
LAB is proposed in SNO+, Daya Bay, RENO New high light yield, transparent solvent?
– Used since decades
– Average light yield
– Average transparency It is a high flash point, low toxicity solvent at moderate
cost and reasonable optics, …but:
– Mixture
– Biphenyls (absorption/emission!)
– Timing properties
CC
CC
CC
CC
CC
CC
CC
CC
C
360 380 400 420 440 460 480 500 520 540 560
1
10
100
1000
atte
nuat
ion
leng
th [m
]
wavelength [nm]
n-Dodecan LAB o-PXE Anisole
LAB (6 g/l PPO)
PXE (6 g/l PPO)
Christian BuckMPIK Heidelberg
Reims, Neutrino Champagne 2009
Solvent mixtures
Advantage: Parameters tuneable optimize material compatibility change timing properties match density adjust light yield
6 g/l PPO
Light production in alkanes Radiation creates e-- - hole pairs Recombination, fragmentation, radicals, reactions excited molecules energy transfer to fluors
M.Wurm, diploma thesis, TUM(2005)
Lig
ht
yie
ld [
% s
tan
da
rd]
C.Aberle, diploma thesis, MPIK (2008)
PXE (mass fraction)
0,0 0,2 0,4 0,6 0,8 1,00
10
20
30
40
50
60
70
80
90
100
Ligh
t Yie
ld [%
of s
tand
ard
]
PXE [volume fraction]
Christian BuckMPIK Heidelberg
Reims, Neutrino Champagne 2009
Comparison fluors
• transparent• well established• high quantum yield
BPO
(Butyl-)PBD pTP
PPO• high(est) light yield• emission around 400 nm
• absorption properties• limited availibility
• low solubility • poor quantum yield
• fast• overlap with bis-MSB
• high light yield
• poor quantum yield• costs
Christian BuckMPIK Heidelberg
Reims, Neutrino Champagne 2009
Energy transfer (non-radiative)
Jk RR
FRET 6
0
LRexchange eJk /2
dJ DA f 4
)()(
Christian BuckMPIK Heidelberg
Reims, Neutrino Champagne 2009
Critical concentration
30
10 Rc
Critical distance R0:
Critical conc.:
50 %50 %
Energy transferPhoton emission, decay
For PPO < 1g/l in PXE, PC,…
For PPO ~ 2.1 g/l in dodecane
Donor * Acceptor
0 2 4 6 8 100
10
20
30
40
50
60
70
80
90
100
110
PXE Dodecane
Lig
ht Y
ield
[% s
tan
da
rd]
PPO concentration [g/l]
Christian BuckMPIK Heidelberg
Reims, Neutrino Champagne 2009
Light yield model
C.Buck, F.X. Hartmann, D.Motta. S.Schönert, CPL, 435 (2007) 252 - 256
C.Aberle, diploma thesis, MPIK Heidelberg (2008)
A
A
e
e
sq
sq
d
1
q
a
'
a
'
q
i
D*
2 D2
A
Q
Q
D1
D*
1
'
i
See poster by C.Aberle!
Christian BuckMPIK Heidelberg
Reims, Neutrino Champagne 2009
Timing properties
C.Aberle, Diploma thesis, MPIK Heidelberg (2008)
D.Motta (CEA Saclay): pulse shape to tag events in different detector regions
Target
Gamma Catcher candidates
Eve
nts
Time [ns]
Christian BuckMPIK Heidelberg
Reims, Neutrino Champagne 2009
Metal loaded scintillators
Solar neutrinos (LENS, SIREN):– Metal: Ytterbium, Indium, Gadolinium– Challenge: High loadings
Reactor (Double Chooz, Daya Bay, RENO) – Metal: Gadolinium – Challenge: Stability
ββ-decay (SNO+)– Metal: Neodymium– Challenges:
transparency; purity
Christian BuckMPIK Heidelberg
Reims, Neutrino Champagne 2009
Indium
Indium-loaded scintillators at LLBF > 1 year (2003/04) MPIK: In(acac)3 (F.X.Hartmann et al.)
INR/LNGS: Carboxylic acid version
> 50 g/l Indium
D. Motta, C. Buck, F. Hartmann, T. Lasserre, S. Schönert, U.Schwan, NIM A 547 (2005) 368.N.A. Danilov, C.Cattadori, A..di Vacri et al., Radiochemistry 47 (2005) 487-493.
Christian BuckMPIK Heidelberg
Reims, Neutrino Champagne 2009
Gadolinium (Carboxylates)
400 420 440 460 480 500 520 540 560 580 6000,000
0,005
0,010
0,015
0,020
0,025
0,030
0,035
0,040
0,045
0,050Target
5 m
Ab
sorb
an
ce
wavelength [nm]
Dec 05 Jan 06 Feb 06 Mar 06 Apr 06
0 1 2 3 4 50,0
0,1
0,2
0,3
0,4
0,5
0,6
0,7
0,8
0,9
1,0Target
Gd-
conc
. [g/
l]
months
Double Chooz mockup (TMHA, MPIK 2003):
INR/LNGS: 2 x 1.2 t Gd-LS (0.1%) in frame of LVD
Now used in Daya Bay and RENO• Y.Ding et al., NIM A 584 (2008) 238-243.• M.Yeh et al., NIM A 578 (2007) 329-339.
arXiv:0803.1577v1 [physics.ins-det] 11
Mar 2008
Christian BuckMPIK Heidelberg
Reims, Neutrino Champagne 2009
Gadolinium (β-diketones)
Purified by sublimation
stability/compatibility tests > 4 y
att. length (1 g/l) > 50 m in ROI
100 kg produced
0 300 600 900 1200 1500 1800 2100 2400 2700
0,1
1
coun
ts
Energy [keV]
before sublimation after sublimation
Ge spectrum Gd(BDK)3
400 420 440 460 480 500 520 540 560 580 6000,000
0,005
0,010
0,015
0,020
0,025
0,030
2.5m
5mA
bs (
10 c
m c
ell)
wavelength [nm]
02Aug2006 30Aug2006 04Feb2009
10m
Christian BuckMPIK Heidelberg
Reims, Neutrino Champagne 2009
Scintillator production for Double Chooz
Scintillator production has started
Poster by F.X.Hartmann on DC scintillator chemistry
Christian BuckMPIK Heidelberg
Reims, Neutrino Champagne 2009
Neodymium
400 425 450 475 500 525 550 575 600 625 6500
5
10
15
20
25
mo
l.ext
.[l/(
mo
l*cm
)]
wavelength [nm]
Nd(acac)3nH
2O
NdCl3
MPIK (2003): Tests on BDK and CBX versions (F.X.Hartmann et al.)
Light yield measurements at LNGS
C.Cattadori et al., submitted to NIM A (2009)arXiv:0909.2152v1 [physics.ins-det] 11 Sep 2009
Christian BuckMPIK Heidelberg
Reims, Neutrino Champagne 2009
Summary
Liquid scintillators key technology for upcoming large scale neutrino detectors
Many solvent and fluor candidates
- Choice depends on application and detector characteristics
- Requirement for „safe“ scintillators (PXE, LAB,…)
Energy transfer models allow light yield predictions
Several applications for metal loaded scintillators
significant improvement in last years (stability etc.)