experimental and theoretical status of neutrino-nucleus...
TRANSCRIPT
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Nu HoRIzons VII, 2018
Experimental and Theoretical status ofneutrino-nucleus cross section
Mohammad Sajjad Athar
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Nu HoRIzons VII, 2018
Outline
1 Introduction
2 Quasielastic Scattering
3 Single Pion Production
4 Deep Inelastic Scattering
5 Quasielastic Hyperon Production
6 Conclusions
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Nu HoRIzons VII, 2018
Introduction
Good understanding of neutrino interactions is important for:
neutrino detection, energy reconstruction, neutrino flux calibration
determination of backgrounds
reduction of systematic errors
needed in the quest for CP violation and mass hierarchy
Precision of 1-5% in cross sections is required
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Nu HoRIzons VII, 2018
Introduction
Good understanding of neutrino interactions is important for:
neutrino detection, energy reconstruction, neutrino flux calibration
determination of backgrounds
reduction of systematic errors
needed in the quest for CP violation and mass hierarchy
Precision of 1-5% in cross sections is required
Near detectors help to reduce systematic errors, still there arelimitations:
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Nu HoRIzons VII, 2018
Introduction
Good understanding of neutrino interactions is important for:
neutrino detection, energy reconstruction, neutrino flux calibration
determination of backgrounds
reduction of systematic errors
needed in the quest for CP violation and mass hierarchy
Precision of 1-5% in cross sections is required
Near detectors help to reduce systematic errors, still there arelimitations:
ND vs FD: These detectors are exposed to the
different fluxes with different flavor composition
different geometry, acceptance and targets
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Nu HoRIzons VII, 2018
Introduction
Neutrino Antineutrino
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Nu HoRIzons VII, 2018
Quasielastic Scattering
Theory of QE ν−Nucleus scattering
Inclusive CCQE Process
N
N ′
W+
νl
l−
X
A
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Nu HoRIzons VII, 2018
Quasielastic Scattering
Theory of QE ν−Nucleus scattering
Inclusive CCQE Process
N
N ′
W+
νl
l−
X
A
Nuclear medium effects
Fermi motion & bindingenergy
Pauli blocking
Multinucleon effects
Final stateinteraction(FSI)effect
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Nu HoRIzons VII, 2018
Quasielastic Scattering
Theory of QE ν−Nucleus scattering
Inclusive CCQE Process
N
N ′
W+
νl
l−
X
A
Nuclear medium effects
Fermi motion & bindingenergy
Pauli blocking
Multinucleon effects
Final stateinteraction(FSI)effect
1p-1h Excitation
W+(q)
W+(q)
n(p) p(p+ q)
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Nu HoRIzons VII, 2018
Quasielastic Scattering
Theory of QE ν−Nucleus scattering
Inclusive CCQE Process
N
N ′
W+
νl
l−
X
A
Nuclear medium effects
Fermi motion & bindingenergy
Pauli blocking
Multinucleon effects
Final stateinteraction(FSI)effect
1p-1h Excitation
W+(q)
W+(q)
n(p) p(p+ q)
RPA
+ + +.............. +..............
W+
W+ W+
W+
W+
W+
W+
W+
W+
W+
V V
V
V
V
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Nu HoRIzons VII, 2018
Quasielastic Scattering
Dytman et al., Nucl.Phys.Proc.Suppl. 229-232 (2012) 167-173
Cross Section
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Nu HoRIzons VII, 2018
Quasielastic Scattering
Dytman et al., Nucl.Phys.Proc.Suppl. 229-232 (2012) 167-173
Cross Section
2p-2h Excitations
W+(q)
W+(q)
W+(q)
W+(q)
W+(q)
W+(q)
Marco MartiniJuan Nieves
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Nu HoRIzons VII, 2018
Quasielastic Scattering
GENIE 2.8.0
Rel. FGM (Smith & Moniz):MA = 1 GeV
Bodek-Richie model thatsimulates short range nucleon
correlations
2p-2h (Valencia)
GENIE 2.8.4
Rel. FGM (Smith & Moniz):MA = 1 GeV
RPA (Valencia)2p-2h (Valencia)
Tuned to inclusive MINERvA
CCQE data
NuWro
Local FGM+RPA+2p-2h: MA = 1.16 GeV
SF+2p-2h (MA = 1.2 GeV )
RFG+TEM (MA = 1.14 GeV )
NEUT
Local FGM+RPA+2p-2hSF+2p-2h with a raised value of
MA
Local FGM+RPA+2p-2h(Martini)
SuSA
NEUT 5.3.2
RFGM+RPA+2p-2h:MA = 1.15 GeV
2p-2h is normalised to 27%
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Nu HoRIzons VII, 2018
Quasielastic Scattering
Wilkinson et al., Phys. Rev. D 93, 072010 (2016)
RFG (Smith & Moniz) + relativistic RPA + 2p2h (Valencia model)MA=1.01GeV
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Nu HoRIzons VII, 2018
Quasielastic Scattering
Wilkinson et al., Phys. Rev. D 93, 072010 (2016)
RFG (Smith & Moniz) + relativistic RPA + 2p2h (Valencia model)MA=1.01GeV
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Nu HoRIzons VII, 2018
Quasielastic Scattering
Wilkinson et al., Phys. Rev. D 93, 072010 (2016)
Simultaneously fitted MINERvA and MiniBooNE data
Fit type MA (GeV) 2p2h norm. (%)
RFG+rel.RPA+2p2h 1.15±0.03 27±12RFG+non-rel.RPA+2p2h 1.07±0.03 34±12
SF+2p2h 1.33±0.02 0 (at limit)
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Nu HoRIzons VII, 2018
Quasielastic Scattering
Ankowski et al., Phys. Rev. D93, 113004 (2016)
1st approach: SF + MA=1.2 GeV (simulates 2p-2h reaction mechanism in aphenomenological manner).2nd approach: GENIE (SF + empirical procedure developed by Dytman et al.to take into account 2p2h) MA =1.03 GeV.
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Nu HoRIzons VII, 2018
Quasielastic Scattering
M. Betancourt et al., (MINERvA Collab); PRL 119, 082001 (2017)
GENIE: RFGM with MA= 1 GeV (No FSI) and with RPA and 2p2h (FSI) (Va-lencia model) contribution tuned to MINERvA inclusive scattering data.NuWro: A local Fermi gas model with MA= 1 GeV, (with 2p2h (No FSI) and withRPA and 2p2h (FSI) (Valencia model)).
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Nu HoRIzons VII, 2018
Quasielastic Scattering
M. Betancourt et al. (MINERvA Collab); PRL 119, 082001(2017)
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Nu HoRIzons VII, 2018
Quasielastic Scattering
d2σdcosθ dp
vs pµ
K. Abe et al.(T2K Collab) PRD 97, 012001 (2018)
Water target without pions in the final state
Comparison with NEUT and GENIE MC
In NEUT
RFGM+Rel RPA+2p2h
tuned to external MINERvA and MiniBooNE data
MA=1.15GeV, 2p2h norm=27%
GENIE 2.8.0 is used
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Nu HoRIzons VII, 2018
Quasielastic Scattering
d2σdcosθ dp
vs pµ
K. Abe et al.(T2K Collab) PRD 97, 012001 (2018)
Water target without pions in the final state
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Nu HoRIzons VII, 2018
Quasielastic Scattering
Comparison with Martini Model and SuSA model
K. Abe et al.(T2K Collab), PRD 97, 012001 (2018)
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Nu HoRIzons VII, 2018
Quasielastic Scattering
Patrick et al. (The MINERvA Collab), arXiv:1801.01197
MINERvA-tuned GENIE (includes RPA and MINERvA-tuned 2p2h), (red line)
GENIE without any modifications except the single non-resonant pion correction (blue line)
GENIE with the RPA weight but no 2p2h component (green line)
GENIE with MINERvA-tuned 2p2h but no RPA (violet line)
GENIE with RPA and untuned 2p2h (orange line)
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Nu HoRIzons VII, 2018
Quasielastic Scattering
Charged Kaon Decay at Rest (KDAR) Experiment
MiniBooNE Collab arXiv:1801.03848 [hep-ex]
First Measurement of Monoenergetic νµ Charged Current Interactions
At Eνµ=236 MeV σCC = 0.27 ± 0.09 ± 0.08 × 10−38 cm2/neutron
Akbar et al. J. Phys. G 44 (2017) 125108
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Nu HoRIzons VII, 2018
Quasielastic Scattering
Charged Kaon Decay at Rest (KDAR) Experiment
MiniBooNE Collab arXiv:1801.03848 [hep-ex]
First Measurement of Monoenergetic νµ Charged Current Interactions
At Eνµ=236 MeV σCC = 0.27 ± 0.09 ± 0.08 × 10−38 cm2/neutron
Akbar et al. J. Phys. G 44 (2017) 125108
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Nu HoRIzons VII, 2018
Single Pion Production
ν/ν induced single pion production(SPP)
Charged current(CC)
νl p → l−
pπ+ νl n → l+
nπ−
νl n → l−
nπ+ νl p → l+
pπ−
νl n → l−
pπ0 νl p → l+
nπ0l = e,µ
Neutral current(NC)
νl p → νl nπ+ νl p → νl pπ0
νl p → νl pπ0 νl p → νl nπ+
νl n → νl nπ0 νl n → νl nπ0
νl n → νl pπ− νl n → νl pπ−
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Nu HoRIzons VII, 2018
Single Pion Production
Higher Resonances
Resonances MR [GeV] Γtot0
πN branching
RIJ (GeV) ratio (%)
P33(1232) 1.232 0.117 100
P11(1440) 1.430 0.350 55 − 75
D13(1520) 1.515 0.115 55 − 65
S11(1535) 1.535 0.150 35 − 55
S31(1620) 1.630 0.140 20 − 30
S11(1650) 1.655 0.140 50 − 90
D15(1675) 1.675 0.150 35 − 45
F15(1680) 1.685 0.130 65 − 70
D33(1700) 1.700 0.150 12
P13(1720) 1.720 0.250 11
F35(1905) 1.880 0.330 9 − 15
P31(1910) 1.890 0.280 15 − 30
F37(1950) 1.930 0.285 35 − 45
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Nu HoRIzons VII, 2018
Single Pion Production
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Nu HoRIzons VII, 2018
Single Pion Production
cosθc
p
q
∆+
0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 2E
νµ(GeV)
0
0.5
1
1.5
2
σ(×
10
-39 c
m2)
Without Medium Effects(ME)With MEWith ME + π Abspn
No cut on W, MA
= 1.03 GeV
Eur. Phys. J. A 43, 209 (2010).
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Nu HoRIzons VII, 2018
Single Pion Production
cosθc
p
q
∆+
0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 2E
νµ(GeV)
0
0.5
1
1.5
2
σ(×
10
-39 c
m2)
Without Medium Effects(ME)With MEWith ME + π Abspn
No cut on W, MA
= 1.03 GeV
Eur. Phys. J. A 43, 209 (2010).
Eνµ(GeV) σ with ME σ with ME
+ π absorption(% reduction) (% reduction)
0.8 42 14
1.0 36 15
1.4 31 14
1.8 28 15
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Nu HoRIzons VII, 2018
Single Pion Production
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Nu HoRIzons VII, 2018
Single Pion Production
Phys. Rev. D 94, 052005 (2016)
MINERvA Collaboration
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Nu HoRIzons VII, 2018
Single Pion Production
ArgoNeuT
Deborah Harris NuInt 2017 Talk
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Nu HoRIzons VII, 2018
Deep Inelastic Scattering
CC νl(νl)− N DIS
νl/νl(k) + N (p) → l−/l
+(k′) + X(p′)
νl/νll−/l+
W+/W−
NX
d2σνl (νl )
dx dy=
G2F MN Eν
π(1 + Q2/M2W
)2
(
[
y2
x +m2
l y
2Eν MN
]
F1N (x, Q2) + F2N (x, Q
2)
×
[
(1 −m2
l
4E2ν
) − (1 +MN x
2Eν
)y
]
±
[
xy(1 −y
2) −
m2l y
4Eν MN
]
F3N (x, Q2)
)
Fνp2
= 2x[d(x) + s(x) + u(x) + c(x)],
Fνp2
= 2x[u(x) + c(x) + d(x) + s(x)],
xFνp3
= 2x[d(x) + s(x) − u(x) − c(x)],
xFνp3
= 2x[u(x) + c(x) − d(x) − s(x)],
νl/νl(k) + N (p) → l−/l
+(k′) + X(p′)
νl/νll−/l+
W+/W−
NX
d2σνl (νl )
dx dy=
G2F MN Eν
π(1 + Q2/M2W
)2
(
[
y2
x +m2
l y
2Eν MN
]
F1N (x, Q2) + F2N (x, Q
2)
×
[
(1 −m2
l
4E2ν
) − (1 +MN x
2Eν
)y
]
±
[
xy(1 −y
2) −
m2l y
4Eν MN
]
F3N (x, Q2)
)
Fνp2
= 2x[d(x) + s(x) + u(x) + c(x)],
Fνp2
= 2x[u(x) + c(x) + d(x) + s(x)],
xFνp3
= 2x[d(x) + s(x) − u(x) − c(x)],
xFνp3
= 2x[u(x) + c(x) − d(x) − s(x)],
For a nuclear target
d2σνl (νl )
dx dy=
G2F MN Eν
π(1 + Q2/M2W
)2
(
[
y2
x +m2
l y
2Eν MN
]
F1A(x, Q2)
+
[
(1 −m2
l
4E2ν
) − (1 +MN x
2Eν
)y
]
F2A(x, Q2)
±
[
xy(1 −y
2) −
m2l y
4EνMN
]
F3A(x, Q2)
)
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Nu HoRIzons VII, 2018
Deep Inelastic Scattering
CC νl(νl)− N DIS
νl/νl(k) + N (p) → l−/l
+(k′) + X(p′)
νl/νll−/l+
W+/W−
NX
d2σνl (νl )
dx dy=
G2F MN Eν
π(1 + Q2/M2W
)2
(
[
y2
x +m2
l y
2Eν MN
]
F1N (x, Q2) + F2N (x, Q
2)
×
[
(1 −m2
l
4E2ν
) − (1 +MN x
2Eν
)y
]
±
[
xy(1 −y
2) −
m2l y
4Eν MN
]
F3N (x, Q2)
)
Fνp2
= 2x[d(x) + s(x) + u(x) + c(x)],
Fνp2
= 2x[u(x) + c(x) + d(x) + s(x)],
xFνp3
= 2x[d(x) + s(x) − u(x) − c(x)],
xFνp3
= 2x[u(x) + c(x) − d(x) − s(x)],
νl/νl(k) + N (p) → l−/l
+(k′) + X(p′)
νl/νll−/l+
W+/W−
NX
d2σνl (νl )
dx dy=
G2F MN Eν
π(1 + Q2/M2W
)2
(
[
y2
x +m2
l y
2Eν MN
]
F1N (x, Q2) + F2N (x, Q
2)
×
[
(1 −m2
l
4E2ν
) − (1 +MN x
2Eν
)y
]
±
[
xy(1 −y
2) −
m2l y
4Eν MN
]
F3N (x, Q2)
)
Fνp2
= 2x[d(x) + s(x) + u(x) + c(x)],
Fνp2
= 2x[u(x) + c(x) + d(x) + s(x)],
xFνp3
= 2x[d(x) + s(x) − u(x) − c(x)],
xFνp3
= 2x[u(x) + c(x) − d(x) − s(x)],
For a nuclear target
d2σνl (νl )
dx dy=
G2F MN Eν
π(1 + Q2/M2W
)2
(
[
y2
x +m2
l y
2Eν MN
]
F1A(x, Q2)
+
[
(1 −m2
l
4E2ν
) − (1 +MN x
2Eν
)y
]
F2A(x, Q2)
±
[
xy(1 −y
2) −
m2l y
4EνMN
]
F3A(x, Q2)
)
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Nu HoRIzons VII, 2018
Deep Inelastic Scattering
Only two theoretical groups have studied Nuclear MediumEffects
Kulagin & Petti Aligarh Group
Phenomenological Efforts
Phenomenological group data types used
EKS98 l+A DIS, p+A DYHKM l+A DISHKN04 l+A DIS, p+A DYnDS l+A DIS, p+A DYEKPS l+A DIS, p+A DYHKN07 l+A DIS, p+A DY
EPS08 l+A DIS, p+A DY, h±, π
0, π
± in d+Au
EPS09 l+A DIS, p+A DY, π0 in d+Au
nCTEQ l+A DIS, p+A DYnCTEQ l+A and ν+A DIS, p+A DYDSSZ l+A and ν+A DIS, p+A DY,
π0
, π± in d+Au
Paukkunen and Salgado:JHEP2010: “find no apparent disagreement with the nu-clear effects in neutrino DIS and those in charged lepton DIS.”
CTEQ-Grenoble-Karlsruhe collaboration “observed that the nuclear corrections inν-A DIS are indeed incompatible with the predictions derived from l±-A DIS andDY data”
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Nu HoRIzons VII, 2018
Deep Inelastic Scattering
Only two theoretical groups have studied Nuclear MediumEffects
Kulagin & Petti Aligarh Group
Phenomenological Efforts
Phenomenological group data types used
EKS98 l+A DIS, p+A DYHKM l+A DISHKN04 l+A DIS, p+A DYnDS l+A DIS, p+A DYEKPS l+A DIS, p+A DYHKN07 l+A DIS, p+A DY
EPS08 l+A DIS, p+A DY, h±, π
0, π
± in d+Au
EPS09 l+A DIS, p+A DY, π0 in d+Au
nCTEQ l+A DIS, p+A DYnCTEQ l+A and ν+A DIS, p+A DYDSSZ l+A and ν+A DIS, p+A DY,
π0
, π± in d+Au
Paukkunen and Salgado:JHEP2010: “find no apparent disagreement with the nu-clear effects in neutrino DIS and those in charged lepton DIS.”
CTEQ-Grenoble-Karlsruhe collaboration “observed that the nuclear corrections inν-A DIS are indeed incompatible with the predictions derived from l±-A DIS andDY data”
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Nu HoRIzons VII, 2018
Deep Inelastic Scattering
MINERvA at Fermilab: Phys.Rev. D93 (2016) 071101
Deep Inelastic Scattering
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Nu HoRIzons VII, 2018
Deep Inelastic Scattering
MINERvA at Fermilab: Phys.Rev. D93 (2016) 071101
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Nu HoRIzons VII, 2018
Quasielastic Hyperon Production
νl(k) + p(p) → l+(k′) + Λ(p′)
νl(k) + p(p) → l+(k′) + Σ0(p′)
νl(k) + n(p) → l+(k′) + Σ−(p′)
νl
l+
W−
N
Y
N
π
W−
N
Y
sinθc
|∆S | = 1 processes are Cabibbo suppressed as compared to |∆S | = 0 processes by
a factor of tan2θc = 0.054.
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Nu HoRIzons VII, 2018
Quasielastic Hyperon Production
Hyperon giving rise to pions
As the decay modes of hyperonsto pions are highly suppressed inthe nuclear medium, making themlive long enough to pass throughthe nucleus and decay outside thenuclear medium.
Therefore, the produced pions areless affected by the strong interac-tion of nuclear field, and their FSIhave not been taken into account.
Phys. Rev. D 88, 077301 (2013)
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Nu HoRIzons VII, 2018
Quasielastic Hyperon Production
scaled by a factor of 2.5 i.e ∼ 40% Phys. Rev. D 88, 077301 (2013)
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Nu HoRIzons VII, 2018
Quasielastic Hyperon Production
scaled by a factor of 1.3 i.e ∼ 30% Phys. Rev. D 88, 077301 (2013)
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Nu HoRIzons VII, 2018
Quasielastic Hyperon Production
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Nu HoRIzons VII, 2018
Quasielastic Hyperon Production
0 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 2
Eνµ (GeV)
0
5
10
15
20
σ (
10
-40 c
m2)
Andrepoulos
Present results
Our results are are multiplied bya factor of 7
Result from Andrepoulos talk
J. Phys. G 42 (2015) 055107Phys. Rev. D 94 (2016) 114031
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Nu HoRIzons VII, 2018
Conclusions
Conclusions
We have moved closer in the last one decade but still there aremany more unanswered questions than the solutions we havecome up with.
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Nu HoRIzons VII, 2018
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