Precision branching-ratio measurement for the superallowed ...
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Precision branching-ratio measurement for thesuperallowed Fermi β emitter 18Ne
Precision branching-ratio measurement for thesuperallowed Fermi β emitter 18Ne
Kushal Kapoor University of ReginaPrecision branching-ratio measurement for the superallowed Fermi β emitter 18Ne
Kushal Kapoor
University of Regina
February 10, 2021
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Kushal Kapoor University of ReginaPrecision branching-ratio measurement for the superallowed Fermi β emitter 18Ne
● IntroductionI.Nuclear β decay
II.Why 18Ne?● Experimental Setup
I. GANIL Lab
II. Detector system● Results● Future plan
Overview
Introduction Experimental Setup Results
Kushal Kapoor University of ReginaPrecision branching-ratio measurement for the superallowed Fermi β emitter 18Ne
Nuclear β decay● Nuclear β decay occurs when an unstable nucleus of an atom, with atomic number (Z) and neutron
number (N), transforms into a more stable nucleus, with Z±1 and N±1
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Introduction Experimental Setup Results
Kushal Kapoor University of ReginaPrecision branching-ratio measurement for the superallowed Fermi β emitter 18Ne
Nuclear β decay● Nuclear β decay occurs when an unstable nucleus of an atom, with atomic number (Z) and neutron
number (N), transforms into a more stable nucleus, with Z±1 and N±1
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● β decays can be characterized by: ● Q value (energy released) ● Half life T1/2 (parent nucleus)● Branching ratio (BR) (to a
particular state of interest in the daughter)
Introduction Experimental Setup Results
Kushal Kapoor University of ReginaPrecision branching-ratio measurement for the superallowed Fermi β emitter 18Ne
Nuclear β decay● Nuclear β decay occurs when an unstable nucleus of an atom, with atomic number (Z) and neutron
number (N), transforms into a more stable nucleus, with Z±1 and N±1
•◦◦◦ ◦◦◦◦◦ ◦◦◦◦
● β decays can be characterized by:● Q value (energy released) ● Half life T1/2 (parent nucleus)● Branching ratio (BR) (to a
particular state of interest in the daughter)
BR≅N γ(x )
NβTot
state x
Kushal Kapoor University of ReginaPrecision branching-ratio measurement for the superallowed Fermi β emitter 18Ne
Nuclear β decay – selection rules◦•◦◦ ◦◦◦◦◦ ◦◦◦◦
IAS
Isobaric Analogue State (IAS)
Angular momentum (L): Allowed decays (L=0), Forbidden decays (L=1,2,3,…)
Introduction Experimental Setup Results
Spin angular momentum (S) = Sβ +SSν:
Fermi decays (S=0), Gamow-Teller decays (S=1)
Kushal Kapoor University of ReginaPrecision branching-ratio measurement for the superallowed Fermi β emitter 18Ne
Nuclear β decay – selection rules ◦•◦◦ ◦◦◦◦◦ ◦◦◦◦
IAS
Isobaric Analogue State (IAS)
Angular momentum (L): Allowed decays (L=0), Forbidden decays (L=1,2,3,…)
Introduction Experimental Setup Results
Spin angular momentum (S) = Sβ +SSν:
Fermi decays (S=0), Gamow-Teller decays (S=1)
Total Isospin (T), projection (tz= +S1/2 (Neutron), -1/2(Proton))
Super (δT=0, transition to IAS)
Super (δT=0, IAS) Allowed (L=0) Fermi (S=0) decays,
Kushal Kapoor University of ReginaPrecision branching-ratio measurement for the superallowed Fermi β emitter 18Ne
Nuclear β decay – ft values
● All nuclear β decays to any daughter state can be characterized in terms of a single quantity known as the ft value
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IAS
Isobaric Analogue State (IAS)
Introduction Experimental Setup Results
Super (δT=0, IAS) Allowed (L=0) Fermi(S=0) decays,
For the special case of superallowed Fermi beta decay between isospin T=1 states
= Constant
Kushal Kapoor University of ReginaPrecision branching-ratio measurement for the superallowed Fermi β emitter 18Ne
Nuclear β decay – ft values
● All nuclear β decays to any daughter state can be characterized in terms of a single quantity known as the ft value
◦•◦◦ ◦◦◦◦◦ ◦◦◦◦
IAS
Isobaric Analogue State (IAS)
Introduction Experimental Setup Results
Super (δT=0, IAS) Allowed (L=0) Fermi(S=0) decays,
For the special case of superallowed Fermi beta decay between isospin T=1 states
= Constant
This can be test experimentally!
Kushal Kapoor University of ReginaPrecision branching-ratio measurement for the superallowed Fermi β emitter 18Ne
Why 18Ne?
Har
dy a
nd I
. S. T
owne
r, P
hys.
Rev
. C 1
02, 0
4550
1 (2
020)
*Har
dy e
t. al
., N
ucl.
Phys
. A 2
46, 6
1 (1
975)
.
◦◦◦• ◦◦◦◦◦ ◦◦◦◦ Introduction Experimental Setup Results
|M fi|2=2(1−δc)
● ∆VR- nucleus independent- radiative correction, δ′R – radiative
correction -transition-dependent (Z-dependent), δC – isospin symmetry breaking correction and δNS -nuclear-structure-dependent part of radiative correction
● In the recent years, our group has been investigating low Z superallowed emitters (10C, 14O, 18Ne)
● ft value for 18Ne is 2912 ± 79 (s)
● 18Ne is not on the plot because of the large uncertainty in the BR for this decay.
● 18Ne ft-value is also one of the most interesting cases to better constrain isospin symmetry breaking
Matrix Elements
~2%
Before Corrections
AfterCorrections
Kushal Kapoor University of ReginaPrecision branching-ratio measurement for the superallowed Fermi β emitter 18Ne
Why 18Ne?
Har
dy a
nd I
. S. T
owne
r, P
hys.
Rev
. C 1
02, 0
4550
1 (2
020)
*Har
dy e
t. al
., N
ucl.
Phys
. A 2
46, 6
1 (1
975)
.
◦◦◦• ◦◦◦◦◦ ◦◦◦◦ Introduction Experimental Setup Results
~2%
Before Corrections
AfterCorrections
● Uncertainties dominated by BR● Hardy et. al., 18Ne Branching Ratio = 7.66 (0.27)%*. ● Only one previous measurement, so our goal is to reduce
the uncertainties in the BR of 18Ne.
Frac
tion
al u
ncer
tain
ity
in ft (%
)
Kushal Kapoor University of ReginaPrecision branching-ratio measurement for the superallowed Fermi β emitter 18Ne
Experimental Setup - GANIL facility in Caen, France
Gri
nyer
et.
al.,
Nuc
l.Ins
trum
.Met
h.A
741
(20
14)
18-2
5
◦◦◦◦ •◦◦◦◦ ◦◦◦◦ Introduction Experimental Setup Results
Cyclotron building
SPIRAL Target
Experimental Hall
20Ne
18Ne
Kushal Kapoor University of ReginaPrecision branching-ratio measurement for the superallowed Fermi β emitter 18Ne
Collection chamber
Experimental Setup
Gri
nyer
et.
al.,
Nuc
l.Ins
trum
.Met
h.A
741
(20
14)
18-2
5
◦◦◦◦ ◦◦•◦◦ ◦◦◦◦
● Beams of radioactive isotopes enter the collection chamber from the right and are implanted into an aluminized-mylar tape
● The beam is then interrupted and the samples are moved to the decay counting chamber (bottom)
Introduction Experimental Setup Results
Bordeaux Group
● Absolute HPGe efficiency calibration
● Detailed source work● X-ray imaging● Source scanning table ● Detailed simulations● 10 yrs of calibration!
BeamEntrance
Frac
tion
al u
ncer
tain
ity
in ft (%
)
Kushal Kapoor University of ReginaPrecision branching-ratio measurement for the superallowed Fermi β emitter 18Ne
Collection chamber
Experimental Setup
Gri
nyer
et.
al.,
Nuc
l.Ins
trum
.Met
h.A
741
(20
14)
18-2
5
◦◦◦◦ ◦◦•◦◦ ◦◦◦◦ Introduction Experimental Setup Results
Bordeaux Group
BeamEntrance
● A total of 23 different radioactive sources were used.● Some of them are only available as a radioactive beam.● Efficiency = 0.231 (4)% at 1042 keV.
Efficiency: 0.2177(4)% at 1173 keV 0.1996(3)% at 1332 keV
Blank et. al., Nucl. Instr and Meth in Phys Res A 776 (2015) 34-38
Kushal Kapoor University of ReginaPrecision branching-ratio measurement for the superallowed Fermi β emitter 18Ne
Experimental Setup
Decay scheme for 18Ne, the IAS is the 0+S excited state at 1042 keV, with a BR of approximately 7.66%
◦◦◦◦ ◦◦◦◦• ◦◦◦◦
Beam rate monitor
Plastic scintillator
CENBG HPGe
HPGemonitor
Introduction Experimental Setup Results
7.66 %
Kushal Kapoor University of ReginaPrecision branching-ratio measurement for the superallowed Fermi β emitter 18Ne
Results◦◦◦◦ ◦◦◦◦◦ •◦◦◦ Introduction Experimental Setup Results
18Ne decay--> T1/2 = 1664.22 (0.47) ms
Beta Decay-- plastic scintillator Gamma rays--
HPGe detectorPeak of interest
Kushal Kapoor University of ReginaPrecision branching-ratio measurement for the superallowed Fermi β emitter 18Ne
Results◦◦◦◦ ◦◦◦◦◦ ◦•◦◦
Gri
nyer
et a
l., N
ucl.
Inst
r. a
nd M
eth.
in P
hys
Res
A 5
79 (
2007
) 10
05–1
033
Introduction Experimental Setup Results
Rate dependent Corrections ~33 % (max) - correction (γ-counts)
Well known effects:
BR≅N γ(1042)
N βTot
Total 380 cycles for beam ON/OFF Single run:-->
Cycle threshold
= 7.57 (0.13) %
I. Pile-up and dead-time correctionsII.Background subtraction
Kushal Kapoor University of ReginaPrecision branching-ratio measurement for the superallowed Fermi β emitter 18Ne
Results◦◦◦◦ ◦◦◦◦◦ ◦◦•◦
Preliminary results for Branching Ratio = 7.52 (±0.043)%
This is in excellent agreement and ~5 times more precise than the previous reported value: 7.66 (±0.21)%
Introduction Experimental Setup Results
Kushal Kapoor University of ReginaPrecision branching-ratio measurement for the superallowed Fermi β emitter 18Ne
Summary & Future Plan◦◦◦◦ ◦◦◦◦◦ ◦◦◦•
● We deduced the branching ratio of 18Ne from an experiment perfomed at GANIL. ● Obtained the value 7.52 (±0.043)%, which is 5x more precise than the only previous measurments.● Results are preliminary, a detailed evaluation of systematic uncertainties is required.● In future, we plan on revisiting the simulations of the detector efficiency. Since the branching ratio
measurment is dominated by the uncertainitites in the efficiency, any improvement we can make will directly decrease the uncertainty in the final result.
Ha
rdy
et.
al.,
19
75
Pre
sen
t w
ork
Introduction Experimental Setup Results
Preliminary results for Branching Ratio = 7.52 (±0.043)%
This is in excellent agreement and ~5 times more precise than the previous reported value: 7.66 (±0.21)%
Kushal Kapoor University of ReginaPrecision branching-ratio measurement for the superallowed Fermi β emitter 18Ne
THANK YOU
G.F. Grinyer A.T.LaffoleyJ.C.ThomasB.BlankH.BouzomitaR.A.E.Austin G.C.Ball F.Bucaille P.Delahaye P.FinlayG.Fremont J.GibelinJ.Giovinazzo T.Kurtukian-NietoK.G.LeachA.LefevreF.LegruelG.LescalieD.Perez-Loureiro
Kushal Kapoor University of ReginaPrecision branching-ratio measurement for the superallowed Fermi β emitter 18Ne
ft=f xT 1 /2
BRx=
K
g2|M fi|
2=K
2Gv
Q-value
BranchingRatio Strength
Matrixelement
ConstantsHalf-life
18Ne
Kushal Kapoor University of ReginaPrecision branching-ratio measurement for the superallowed Fermi β emitter 18Ne
18Ne
Kushal Kapoor University of ReginaPrecision branching-ratio measurement for the superallowed Fermi β emitter 18Ne
Experimental Setup◦◦◦◦ ◦◦◦•◦ ◦◦◦◦
● Detector calibration table● Precise positioning of the source● Laser calibrated x,y positioning
Bla
nk e
t. al
., N
ucl.I
nstr
um.M
eth.
A 9
84,
1646
31 (
2020
)
Bordeaux Group
Introduction Experimental Setup Results