中間子ー原子核束縛系の物理 - a brief summary of current interests -...
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中間子ー原子核束縛系の物理中間子ー原子核束縛系の物理- A brief summary of current interests -- A brief summary of current interests -
奈良女子大学奈良女子大学比連崎 悟比連崎 悟
Pionic Atom, Kaonic Atoms(Pionic Atom, Kaonic Atoms( 代表的・歴史的なも代表的・歴史的なものの ))
Meson ( Yukawa Particle )
Large !!
Small !!
Electromagnetic
Strong
B.E.
Radius
Interactions
A(Z,N)
-
m ~ 300 me
Strong Interacting Particle System!
Observation of Pionic AtomObservation of Pionic Atom= Traditional Way : Slow Pion Trap =
X-ray DetectorX-ray
Slow
Nucleus
Absorption to Nucleus by Strong Interaction
4He 16O 40Ca
In-Medium Dispersion RelationIn-Medium Dispersion Relation
Pion – Nucleus Optical PotentialPion – Nucleus Optical Potential
with
Ericson-Ericson, Ann. Phys. 36 (66) 323Seki-Masutani, Phys. Rev. C27(83)2799
Medium Effects
Medium Effects
Nucleus Densities
Potential Parameters
Observed by Observed by
X-ray SpectroscopyX-ray Spectroscopy
Toki, Hirenzaki, Yamazaki, Hayano (1989)
Toki, Hirenzaki,
Yamazaki, Hayano (1989)
Energy
and
Width
Information on
pion-nucleus interactions
Do you believe this ?
の限界
Missing mass spectroscopyMissing mass spectroscopy
emitted particleemitted particle
Incident particleIncident particle
targettargetmesonmeson
-hole-holeprotonproton
Distortion effectDistortion effect
distortion Factor reduction of the flux due to absorption
[Eikonal approx.]
These two reactions haveThese two reactions havedifferent sensitivitiesdifferent sensitivities to systems. to systems.
Missing mass spectroscopyMissing mass spectroscopyIncident particleIncident particle
targettargetmesonmeson
-hole-holeprotonproton
emitted particleemitted particle
Deeply bound Deeply bound -- states in the states in the 208208Pb(d,3He) reactionPb(d,3He) reaction
PRC62(00)025202PRC62(00)025202
K. Itahashi et al.
Hirenzaki, Toki, Yamazaki PRC(1991)
PRL88(02)122301PRL88(02)122301
Deeply bound 1s and 2p Pionic States in the Deeply bound 1s and 2p Pionic States in the 206206Pb(d,Pb(d,33He) reactionHe) reaction
Hirenzaki, Toki PRC55(97)2791
Pionic 1s states of Sn nucleiPionic 1s states of Sn nuclei
Umemoto, Hirenzaki, Kume, Toki PRC62(00)024606Umemoto, Hirenzaki, Kume, Toki PRC62(00)024606
K. Suzuki et al. Phys. Rev. Lett. 92(2004) 072302 GOR relation + Tomozawa-Weinberg RelationGOR relation + Tomozawa-Weinberg Relation
New method – Observation of Meson-Nucleus states
( 数年間の試行錯誤があった ) Information on at finite ~ 0
Eigen state observation Invariant Mass Method
Quantum number fixed Selective information
Umemoto et al., PRC62 (2000)
Further ProgressesFurther Progresses
Exotic few body systems. (core, fermion, boson)
1. Exotic Many Body Physics
2. Hadron Physics at finite density Fundamental theory (QCD)
Effective theory
Hadron property at finite 有限系 無限系 観測量計算、 データ
• Higgs mechanism
•UA(1) Anomaly Effect
Meson Mass SpectrumMeson Mass Spectrum T.Kunihiro, T.Hatsuda, PLB206(88)385 T. Kunihiro, PLB219(89)363 R.D.Pisarski, R.Wilczek, PRD29(84)338 K.Fukushima, K.Onishi, K.Ohta, PRC63(01)045203 P. Costa et al.,PLB560(03)171, hep-ph/0408177etc…
: Jp = 0-
• Spontaneous Chiral Symmetry Breaking
Junko YamagataJunko Yamagata (Nara Women’s Univ.) H. Nagahiro (RCNP, Osaka Univ.) S. Hirenzaki (Nara Women’s Univ.)
In-Flight (K-,p) Reactions for the formation of Kaon-Nucleus bound systems
* J. Yamagata, H. Nagahiro, Y. Okumura, S. Hirenzaki, Prog. Theor. Phys. 114 (2005) 301; Errata 114 (2005) 905Prog. Theor. Phys. 114 (2005) 301; Errata 114 (2005) 905
* J. Yamagata, H. Nagahiro, S. Hirenzaki, arXive:nucl-th/0602021arXive:nucl-th/0602021
Kaonic Nuclei K-Nucleus bound system strong interaction Binding Energy : 10 – 100 MeV100 MeV
Formation ReactionFormation Reaction (In-flight K,N) reaction – Kishimoto Group ((In-flight K,N) reaction – Kishimoto Group (Exp.Exp.)) (Stopped K,N) reaction – Iwasaki, Suzuki Group ((Stopped K,N) reaction – Iwasaki, Suzuki Group (Exp.Exp.))
(K– light nuclei) system structure – Akaishi, Yamazaki, Dote (K– light nuclei) system structure – Akaishi, Yamazaki, Dote ((Theor.Theor.))
Critical analysis – E. Oset, H. Toki (Theor.)
Introduction for kaon KK
Very deep!!Very deep!!
We theoretically study the formation spectra of In-flight (K-,p) reactions.
• quasi-stable K-Nuclear State
• Ultra high density state Really Exist or not ?Really Exist or not ?
Cf. Kaonic Atoms
Introduction for kaon
Kaonic Nuclei case large widths
Green Function Method
Cf. Effective Number Approach (previous work)
Good for small width casesJ. Yamagata et. al., Prog. Theor. Phys. 114(05)301J. Yamagata et. al., Prog. Theor. Phys. 114(05)301
Our Study Structure of Kaonic Atoms and Kaonic Nuclei (two different K-Nucleus optical potentials) Formation spectra of In-flight (K-,p) reactions
Green Function Method
The energy dependence of the optical potential The Quasi-Free Kaon production processes
Formulation -- Structure Klein-Gordon Equation
Chiral Unitary Model
Phenomenological Model[Batty, Friedman, Gal, Phys. Rep. 287(97)385]
[A. Ramos, E. Oset, NPA671(00)481][Hirenzaki, Okumura, Toki, Oset, Ramos, PRC61(00)055205]
Phase Space Factor (for the phenomenological potential)
threshold ・・・
threshold ・・・
Pha
se S
pace
Fac
tor
Formulation -- Structure Klein-Gordon Equation
Chiral Unitary ModelChiral Unitary Model
Phenomenological ModelPhenomenological Model[Batty, Friedman, Gal, Phys. Rep. 287(97)385]
[A. Ramos, E. Oset, NPA671(00)481][Hirenzaki, Okumura, Toki, Oset, Ramos, PRC61(00)055205]
Energy level (examples by the potential at E=0)
Atomic StateAtomic StateSimilar
Nuclear StateNuclear StateDifferent
Formulation – Reaction
Green Function Method O. Morimatsu, K. Yazaki NPO. Morimatsu, K. Yazaki NPA435A435 (85)727 (85)727
O. Morimatsu, K. Yazaki NPO. Morimatsu, K. Yazaki NPA483A483 (88)493 (88)493
: Green function for K interacting with the nucleus
: Elementary cross section (Exp. data)
Previous work: Effective Number ApproachPrevious work: Effective Number Approach(J. Yamagata et. al., PTP114(05)301)
12C is interesting !
B.E. = 150 MeV
B.E. = 100 MeV
B.E. = 50 MeV
B.E. = 0 MeV
Kaon BindingEnergy
Momentum Transfer – =0°
Green vs. Effective (Energy Spectrum)
Nuclear States• Phenomenological
potential
• At E=0TK = 600 MeV
Target : 12C
Quasi-free regionBound regionBound region
Green vs. Effective (Energy Spectrum)
Nuclear States
• Phenomenological
potential
• At E=0
TK = 600 MeV
Target : 12C
Bound regionBound region
Energy Spectrum ( E=0 potential )
12C (K-,p) reactions – TK = 600 MeVGreenEffective Number
Atomic State
1s 2p 2s
Atomic State
1s 2p 2s
Energy Spectrum ( Energy dependence )
12C (K-,p) reactions – TK = 600 MeV
Smooth Structure?Structure?
Effect of Branching Ratio of Decay Channel Phenomenological Potential
80%80%
20%20%
Pha
se S
pace
Fac
tor
80%
20%
90%90%
10%10%
Energy Spectrum : Phenomenological Model (Energy Dependent)
80%80% 90%90%
20%20% 10%10%
Energy Spectrum : Energy Dependent
PhenomenologyChiral Unitary
Green
Effective
Number
Green
Effective
Number
J. Yamagata, H. Nagahiro, S. Hirenzaki, arXive:nucl-th/0602021J. Yamagata, H. Nagahiro, S. Hirenzaki, arXive:nucl-th/0602021
Comparison with
Kishimoto group’s data
Energy SpectrumEnergy dependent
Green
Effective Number
Chiral Unitary
Phenomenology
Please ask
Kishimoto san group.
Nuclear State : Just a tiny bump.
**Exist!!Exist!! But, it is very difficult to see. (large decay width)
*Need *Need more accurate experimental datamore accurate experimental data..
Summary for kaon
( not simple peaks )
Atomic State :
**Exist Exist as quasi-stable state.as quasi-stable state.
We studied the formation spectra of In-flight (K-,p) reactions. Target : 12C, 16O ; TK = 600 MeV Green Function Method (cf. Effective number approach)
Interesting spectrum shape.
No peak structure is expected in spectra for all cases considered here.
Nuclear structure change was not considered.
Formation of Formation of -mesic nuclei-mesic nuclei› Optical potential ~ N*(1535) dominance model ~Optical potential ~ N*(1535) dominance model ~
» Chiral Doublet modelChiral Doublet model» Chiral Unitary modelChiral Unitary model
› Numerical Results of (d,Numerical Results of (d,33He) & (He) & (,p) reactions,p) reactions
Formation of Formation of ’(958)-mesic nuclei’(958)-mesic nuclei› NJL modelNJL model
» UUAA(1) anomaly in finite density(1) anomaly in finite density
› Numerical Results of (Numerical Results of (,p) reactions,p) reactions
Hideko NgahiroHideko Ngahiro, D.Jido and S.Hirenzaki, NPA761(05)92, D.Jido and S.Hirenzaki, NPA761(05)92Hideko NagahiroHideko Nagahiro, D.Jido and S.Hirenzaki, PRC68(03)035205, D.Jido and S.Hirenzaki, PRC68(03)035205D.Jido, D.Jido, Hideko NagahiroHideko Nagahiro and S.Hirenzaki, PRC66(02)045202 and S.Hirenzaki, PRC66(02)045202
Hideko NagahiroHideko Nagahiro, S. Hirenzaki, PRL94(05)232503, S. Hirenzaki, PRL94(05)232503Hideko NagahiroHideko Nagahiro, M.Takizawa and S. Hirenzaki, in preparation., M.Takizawa and S. Hirenzaki, in preparation.
’’(958)-Nucleus system(958)-Nucleus system
’’(958) meson …(958) meson …close connections with close connections with UUAA(1) anomaly(1) anomaly
› some theoretical workssome theoretical works» the effects of the Uthe effects of the UAA(1) anomaly on (1) anomaly on ’’ properties properties
» at finite temperature/densityat finite temperature/density T. Kunihiro, PLB219(89)363T. Kunihiro, PLB219(89)363 R.D.Pisarski, R.Wilczek, PRD29(84)338R.D.Pisarski, R.Wilczek, PRD29(84)338 Y. Kohyama, K.Kubodera and M.Takizawa, PLB208(1988)165Y. Kohyama, K.Kubodera and M.Takizawa, PLB208(1988)165 K.Fukushima, K.Onishi, K.Ohta, PRC63(01)045203K.Fukushima, K.Onishi, K.Ohta, PRC63(01)045203 P. Costa P. Costa et al.et al.,PLB560(03)171, hep-ph/0408177 etc…,PLB560(03)171, hep-ph/0408177 etc…
» the possiblethe possible character changes of character changes of ’’
› a a poor experimental informationpoor experimental information on on the Uthe UAA(1) anomaly at finite density(1) anomaly at finite density
proposal for the formation reaction proposal for the formation reaction of theof the ’’-mesic nuclei-mesic nuclei› UUAA(1) anomaly in medium from the viewpoint of “mesic nuclei”(1) anomaly in medium from the viewpoint of “mesic nuclei”
› the the ’’ properties, especially properties, especially mass shiftmass shift, at finite density, at finite density
Hideko Nagahiro, S. H, Phys.Rev.Lett.Hideko Nagahiro, S. H, Phys.Rev.Lett.9494, 232503 (2005), 232503 (2005)Hideko Nagahiro, M.Takizawa and S. H, in preparation.Hideko Nagahiro, M.Takizawa and S. H, in preparation.
Model for Model for and and ’’ meson in medium meson in medium
Nambu-Jona-Lasinio modelNambu-Jona-Lasinio model with the with the KMT interaction KMT interaction › unified treatment of the unified treatment of the and and ’’ meson meson
du s
u d s
One can reproduce the heavy One can reproduce the heavy ’’ mass mass
Kunihiro, Hatsuda, PLB206(88)385, Fig.3Kunihiro, Hatsuda, PLB206(88)385, Fig.3
Anomaly effect in vacuumAnomaly effect in vacuum
explicit breaking the Uexplicit breaking the UAA(1) sym.(1) sym.
Kobayashi, Maskawa Prog.Theor.Phys.44, 1422 (70)Kobayashi, Maskawa Prog.Theor.Phys.44, 1422 (70)G. ’t Hooft, Phys.Rev.D14,3432 (76)G. ’t Hooft, Phys.Rev.D14,3432 (76)
Masses in finite Masses in finite with with NJLNJL
==== …………
quark-anti-quark scatteringquark-anti-quark scattering
++++
Bethe-Salpeter equationBethe-Salpeter equation
==== ++++
condensate in finite condensate in finite
Fermi distribution functionFermi distribution function
== ++ ++
Gap equations for quarksGap equations for quarks
meson properties (mass)meson properties (mass)
mesonmesonmesonmeson
T. Kunihiro, PLB219(89)363,T. Kunihiro, PLB219(89)363,P. Costa P. Costa et al.et al.,PLB560(03)171. etc…,PLB560(03)171. etc…
flavor mixing termsflavor mixing terms
partial restoration in mediumpartial restoration in medium[MeV
] [MeV
]
SU(2) sym. matterSU(2) sym. matter
SU(3)SU(3)
SU(2) symmetric matterSU(2) symmetric matter
we consider the SU(2) sym. matter as the sym. nuclear matter.we consider the SU(2) sym. matter as the sym. nuclear matter.
’’
mm’’ ~ ~ -150-150 MeV @ MeV @ 00
mm ~ ~ +20+20 MeV @ MeV @ 00
and and ’’ mass shifts @ mass shifts @ 00
P. Rehberg, et al., PRC53(96)410.P. Rehberg, et al., PRC53(96)410.
parameters (in vacuum)parameters (in vacuum)
= 602.3 = 602.3 [MeV][MeV]
ggS S 22 = 3.67 = 3.67
ggDD55 = -12.36 = -12.36
mmu,du,d = 5.5 = 5.5 [MeV][MeV]
mmss = 140.7 = 140.7 [MeV][MeV]
MMu,du,d = 367.6 = 367.6 [MeV][MeV]
MMss = 549.5 = 549.5 [MeV][MeV]
〈〈 uuuu 〉〉 1/3 1/3 = -241.9 = -241.9 [MeV][MeV]
〈〈 ssss 〉〉 1/31/3 = -257.7 = -257.7 [MeV][MeV]
mm’’ = 958 = 958 [MeV][MeV]
mm = 514 = 514 [MeV][MeV]
mm = 135 = 135 [MeV][MeV]
We can see the large medium effect even We can see the large medium effect even at normal nuclear densityat normal nuclear density..
anomaly term anomaly term effecteffect
anomaly effect in the finite densityanomaly effect in the finite density
We simulate an extreme case.We simulate an extreme case.
’’
ggDD : constant : constant
mm’’ ~ ~ -150-150 MeV @ MeV @ 00
mm ~ ~ +20+20 MeV @ MeV @ 00
’’
mm’’ ~ ~ -250 -250 MeV @ MeV @ 00
mm ~ ~ -100 -100 MeV @ MeV @ 00
ggDD = g = gDD(() ??) ??ggDD = g = gDD((=0) exp(-(=0) exp(-(//00))22))
- & - & ’’-Nucleus optical potential-Nucleus optical potential
Real Part VReal Part V00
› evaluated by possible evaluated by possible ’’ mass shift mass shift at at 00
~ potential description~ potential description
ggDD : constant : constant
VV’’(r)(r)
VV(r)(r)
: : repulsiverepulsive’’ : : attractiveattractive
ggDD = g = gDD((=0) e=0) e-(-(//0)0) 22
VV’’(r)(r)
VV(r)(r)
: : attractiveattractive’’ : : attractiveattractive
- & - & ’’-Nucleus optical potential-Nucleus optical potential
Real Part VReal Part V00
› evaluated by possible evaluated by possible ’’ mass shift mass shift at at 00
Imaginary Part WImaginary Part W0 0 for for ’’› estimated from AIP Conf.Proc.717 (04)837(A.Sibirtsev,Ch.Elster, S.Krewald, J.Speth)estimated from AIP Conf.Proc.717 (04)837(A.Sibirtsev,Ch.Elster, S.Krewald, J.Speth)
analysis of analysis of p p ’’p datap datafix a coupling gfix a coupling g
N N*(1535)
’
gg
(only one resonance included)
› in analogy with in analogy with -hole model for the -hole model for the -nucleus system-nucleus system
’
’
~ phenomenological estimation~ phenomenological estimation
Imaginary Part for Imaginary Part for WW00 = - 40 MeV = - 40 MeV D.Jido,H.N.,S.Hirenzaki, PRC66(02)045202, D.Jido,H.N.,S.Hirenzaki, PRC66(02)045202,
H.N.,D.Jido,S.Hirenzaki, PRC68(03)035205,H.N.,D.Jido,S.Hirenzaki, PRC68(03)035205,
~ potential description~ potential description
((,p) reaction : Parameters,p) reaction : Parameters
((,p) reaction @ E,p) reaction @ E=2.7 GeV=2.7 GeV
target … target … 1212CC
Forward (Forward ( ~ 0 deg.) ~ 0 deg.)
Elementary cross section for Elementary cross section for p p ’’pp
-mesic nuclei-mesic nuclei› mm ~ 547 MeV ~ 547 MeV mm ~ 783 MeV ~ 783 MeV m m’’ ~ 958 MeV ~ 958 MeV
› plan of experiment for the formation of plan of experiment for the formation of -mesic nuclei @ SPring-8, 2005-mesic nuclei @ SPring-8, 2005› two different predictions for optical potentialstwo different predictions for optical potentials
» 【【 attractiveattractive 】】 V= - (156 + 29 i) V= - (156 + 29 i) //00 MeV MeV [Klingl, Waas, Weise NPA650(99)299][Klingl, Waas, Weise NPA650(99)299]
» 【【 repulsiverepulsive 】 】 V= - ( - 42.8 + 19.5i) V= - ( - 42.8 + 19.5i) //00 MeV MeV [Lutz, Wolf, Friman NPA706(02)4[Lutz, Wolf, Friman NPA706(02)4
31] 31]
› elementary cross section ~ 150 nb/srelementary cross section ~ 150 nb/sr» event # [event # [] ~ [] ~ [] ~ [] ~ [’’]]@ test experiment at SPring-8 @ test experiment at SPring-8
[N.Muramatsu, private communication] [N.Muramatsu, private communication]
-mesic nuclei-mesic nuclei› elementary cross section ~ 150 nb/srelementary cross section ~ 150 nb/sr
Data:SAPHIR collaboration, PLB444(98)555-562
Chiang, Yang, PRC68(03)045202
Numerical results : Numerical results : 1212C(C(,p),p)1111BB,,,,’’
quasi-freequasi-free
quasi-freequasi-free
’’
We only We only observe the observe the quasi-free quasi-free ’’
peakpeak
no medium effectno medium effect
Numerical results : Numerical results : 1212C(C(,p),p)1111BB,,,,’’
quasi-freequasi-free
quasi-freequasi-free
’’VV00= - (- 42.8 + 19.5i) [MeV]= - (- 42.8 + 19.5i) [MeV]
(NPA706(02)431)(NPA706(02)431)
quasi-freequasi-free
no medium effectno medium effect
quasi-freequasi-free
quasi-freequasi-free
’’
Numerical results : Numerical results : 1212C(C(,p),p)1111BB,,,,’’
no medium effectno medium effect
quasi-freequasi-free
VV00= - (156+29i) [MeV]= - (156+29i) [MeV](NPA650(99)299)(NPA650(99)299)
Numerical results : Numerical results : 1212C(C(,p),p)1111BB,,,,’’
quasi-freequasi-free
quasi-freequasi-free
’’
quasi-freequasi-free
VV00= - (156+29i) [MeV]= - (156+29i) [MeV](NPA650(99)299)(NPA650(99)299)
ggDD = -12.36/ = -12.36/55
Numerical results : Numerical results : 1212C(C(,p),p)1111BB,,,,’’
quasi-freequasi-free
quasi-freequasi-free
’’
quasi-freequasi-free
VV00= - (156+29i) [MeV]= - (156+29i) [MeV](NPA650(99)299)(NPA650(99)299)
mass reductionmass reductiondue to the medium due to the medium
effect througheffect throughanomaly termanomaly term
ggDD = -12.36/ = -12.36/55
quasi-freequasi-free
quasi-freequasi-free
’’
Numerical results : Numerical results : 1212C(C(,p),p)1111BB,,,,’’
ggDD = -12.36/ = -12.36/55 quasi-freequasi-free
VV00= - (- 42.8 + 19.5i) [MeV]= - (- 42.8 + 19.5i) [MeV](NPA706(02)431)(NPA706(02)431)
Quasi-free Quasi-free overlap with bound overlap with bound
’’
Quasi-free Quasi-free overlap with bound overlap with bound
’’
Numerical results : Numerical results : 1212C(C(,p),p)1111BB,,,,’’
quasi-freequasi-free
quasi-freequasi-free
’’ and and ’’ mass reductions mass reductions
quasi-freequasi-free
VV00= - (- 42.8 + 19.5i) [MeV]= - (- 42.8 + 19.5i) [MeV](NPA706(02)431)(NPA706(02)431)
density dependent gdensity dependent gDD
Numerical results : Numerical results : 1212C(C(,p),p)1111BB,,,,’’
quasi-freequasi-free
VV00= - (156+29i) [MeV]= - (156+29i) [MeV](NPA650(99)299)(NPA650(99)299)
density dependent gdensity dependent gDD
quasi-freequasi-free
quasi-freequasi-free
’’
Summary for Summary for and and ’ : ’ : mesic nuclei … hadron properties in finite mesic nuclei … hadron properties in finite
-mesic nuclei by (d,-mesic nuclei by (d,33He) and (He) and (,p) reactions,p) reactions» Chiral doublet modelChiral doublet model» Chiral unitary modelChiral unitary model
Different pictures for the N*(1535) in mediumDifferent pictures for the N*(1535) in medium
’’-mesic nuclei by (-mesic nuclei by (,p) reactions,p) reactions» NJL modelNJL model
UUAA(1) anomaly in finite density(1) anomaly in finite density
Future worksFuture works› -mesic nuclei-mesic nuclei
» (d,(d,33He) experiment for He) experiment for -mesic nuclei formation @ GSI -mesic nuclei formation @ GSI
› ’’-mesic nuclei -mesic nuclei » ((,p) experiment for ,p) experiment for -mesic nuclei @ SPring-8 -mesic nuclei @ SPring-8 Coming soon ?Coming soon ?
» What is the density dependence of gWhat is the density dependence of gDD ?? ??
» Other treatment ?Other treatment ?» relation with other models for relation with other models for & & ’’
chiral doublet model & chiral unitary approach for the chiral doublet model & chiral unitary approach for the -mesic nuclei-mesic nuclei
SummarySummary Mesic Atoms and Mesic Nuclei A finite density Laboratory 観測量の物理的意味をキッチリ抑えたい 微視的な理解から実際のハドロン反応の計算まで、
統一的にやりたい
by (d,3He) Hayano (Tokyo group) @GSI (,’) by (,p) Muramatsu (LEPS group) @SPring8 k by In-Flight (K,p) Kishimoto (Osaka group)
+Many Others
いろいろな事が、まだまだ不十分でわからない
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