hideki yukawa and nuclear physics akito arima japan science foundation musashi gakuen

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Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

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Page 1: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

Hideki Yukawa and Nuclear Physics

Akito Arima

Japan Science Foundation

Musashi Gakuen

Page 2: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen
Page 3: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

1 Professor Hideki Yukawa has encouraged Japanese, especially young Japanese,  

   just after the Second World War.

2 Professor Hideki Yukawa’s creation of a new academic system for research in fundamental science: The inter-university research institutes.

3 Pions, nuclear interaction and nuclear structure.

Page 4: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

1 Professor Hideki Yukawa has

encouraged Japanese, and

especially young Japanese,

just after the Second World War.

Page 5: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

毎日新聞社提供

Page 6: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen
Page 7: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

毎日新聞社提供

Page 8: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

出典: TIME アーカイヴス

Page 9: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

出典:毎日新聞の好意による

Page 10: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

毎日新聞社提供

Page 11: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

2 Professor H. Yukawa’s creation of a new academic system to research fundamental sciences; inter-university research institutes

Page 12: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

Institute of Fundamental Physics

in Kyoto University

The first inter-university research institute

Page 13: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

Examples of inter-university research institutes

Cosmic ray laboratory (super Kamiokande)

Institute of Nuclear Study

KEK

etc.

The most important driving forces to develop research of fundamental sciences and technologies in Japan

Page 14: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

Workshops, Winter and summer schools

have been organized in Institute of

Fundamental Physics.

Page 15: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

3 Pions, nuclear interaction and nuclear structure

3-1   Nuclear magnetic moments

A difficult problem in 1950 was

the magnetic moment of 209Bi.

Page 16: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

Ⅰ Nuclear Shell Model

1 Magic Number

Z=2(He), 10(Ne), 18(Ar), 36(Kr), 54(Xe), 86(Rn)

They are rare gases.

Nuclear magic numbers

Z=2,8,20,50,82

N=2,8,20,28,50,82,126

Page 17: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

Nuclear radius(10-15m)

Har

tree

-Fo

ckp

ote

nti

al

(MeV

)

2g9/2

3p3/2

1i13/2

2d3/2

2s1/2

1f7/2

1d6/2

1d3/2

1p3/2

1p1/2

1s1/2

126

0

-10

82

50

20

2

8

-20

-30

-40

-50

0 102 84 6

1f5/2

2p3/2

2p1/2

1g9/2

1g7/2

2d6/2

1h11/2

2f7/2

3s1/2

1h9/2

2f5/2

3p1/2

1i11/2

-60

2g9/2

3p3/2

1i13/2

2d3/2

2s1/2

1f7/2

1d6/2

1d3/2

1p3/2

1p1/2

1s1/2

126

0

-10

82

50

20

2

8

-20

-30

-40

-50

0 102 84 6

1f5/2

2p3/2

2p1/2

1g9/2

1g7/2

2d6/2

1h11/2

2f7/2

3s1/2

1h9/2

2f5/2

3p1/2

1i11/2

-60

Page 18: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

208Pb is very stable, because Z=82 and

N=126 which are magic numbers.

Page 19: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

Pb20882 126 Very stable

Pb208

Pb+b208Bi209

This proton in h9/2 -shell is expected to rotatefreely about the center of 208Pb.

Page 20: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

The operator of magnetic moment

s +gsg

The Schmidt value

( ) ( )2 1s

sg g

j j g

12

j

1

0

g

g

5.585 for protonsg - 3.826 for neutronsg

unit n.m.

Page 21: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

μs ( h9/2 )=2.62  n.m.

( 209Bi )=4.11 n.m.

δμ = μobs - μs

   =1.5  n.m. Very large.

A   serious problem in 1950.

μobs

Page 22: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

Pi-meson exchange currentPi-meson(π)was Predicted byYukawa in 1935.π meson was discovered experimentallyby C.F.Powell.π +, π 0,and π -Pi-meson exchange currents H.Miyagawa 1951 Villars1952

Page 23: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

2 Nuclear Shell ModelMean field theory with strong spin-orbit force

Mayer and Jensen 1949 Shell model level scheme

(mean field approximation)

s

Page 24: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

A strong spin-orbit interaction

is necessary to explain the magic numbers

the jj-coupling shell model of Jensen and Mayer!

l

Page 25: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

magic number

× × j<=ℓ -12

× × × ×

16O   ,   40Ca

j>=ℓ +12

Page 26: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

× ×

× × × ○

Impossiblebecausej<-orbit is closed.

M1-Giant Resonance

Page 27: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

208Pb  ( The Ground state O+ )

××××××××××××

magic number

j<=ℓ -12

j>=ℓ +12

Page 28: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

××× ○××××××××

× Possiblej< is vacunt

208Pb  ( M1-Giant 1+ ) h11/2 →   h9/2 protons i13/2 →   h11/2neutrons

Page 29: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

209 208

83 126 9 / 2

+ ;9 9( Bi ) ( Pb(0 ) )2 2h

208

9 / 2

+ ; 9( Pb(1 ) )2h

( ) 0

Configuration Mixing

= Core-Polarization (Bohr and Mottelson)

Page 30: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

2099 / 2 9 / 2

9 9( Bi) ( Bi) 0 , 0 ,2 2h h

29 / 2 9 / 2

9 92 0 , 1 , ( )2 2 sh h

9 / 2 9 / 29 92 0 , 1 , 02 2h h

CM 0.8 n.m.

Page 31: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

17O 0 0.0217F 0 -0.08

41Ca 0 0.3241Sc 0 -0.37209Bi 0.8 1.5

cm obsNucleus

Page 32: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

Chemtob in 1967 found that the pi-meson exchange current modifies .g

g 0.10 for proton

g 0.10 for neutron

MEC 9/ 2( ) 0.5 n.m.h

theory CM MECBi)

0.8 0.5

1.3 n.m.

209obs ( Bi) 1.5 n.m.

Page 33: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

0

0.5

1

1.5

1st orderC.P.

MEC2nd order

C.P.

CrossingC.P. × MEC

OBS

Magnetic moment of Bi12620983

0.79

1.37

1.49

1.05

Ref. : A.Arima, K.Shimizu, W.Bentz, H.HyugaAdv. Nucl.Phys. 18 (1987) 1.

δ

Page 34: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

Most important contributions to the magnetic moment of 209Bi :

(1) first order configuration mixing=first order core-polarization CP CM

(2) one pi-meson exchange current

Page 35: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

Yamazaki, Nagamiya, Nomura and Katou in 1970confirmed experimentally

g 0.1 for protons

and

g 0.09 for neutrons

The contribution of pi-meson current is experimentally confirmed.

Page 36: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

17O, 17F, 41Ca and 41Sc

obs are small, and CM 0

But are not zero.obs

Therefore higher order corrections, such as secondorder configuration mixings, must be considered:Shimizu, Ichimura and Arima in 1974,Towner and Khanna in 1979.

GT transition rates deviate from theirshell model values.

Page 37: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

ISOSCALAR MOMENT

ISOVECTOR MOMENT

17 39 41-11/2p 5/2d

-13/2d 7/2

f

2ndCROSSMEC

-hole

Ref. : I.S.Towner, F.C.Khanna, Nucl.Phys. A339 (1983) 334.

δδ

Page 38: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

GAMOW - TELLER

17 39 41-11/2p 5/2d

-13/2d 7/2f

2ndCROSSMEC

0.2

-0 .2

0

REL

-hole

Ref. : I.S.Towner, F.C.Khanna, Nucl.Phys. A399 (1983) 334.

δ

Page 39: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

GT transition rates2s

2

obs2

shell model

12

s

s

2

obss are observed by using the (p,n) reaction.

(Goodman et al (1980))

This quenching has been explained by hole effect.

is the isobar of nucleon. ( )300MeV excitationenergy

The effect of the second order configuration mixing(= 2 particle -2 hole mixing) was not believed.

Page 40: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

Why is quenched ?

Simple shell model

2p-2h or2p-1h mixings(second order configuration mixing)

hole mixing

h states( 300MeV)2p-2h

or2p-1h states

strength spread 50%of

over 20 50 MeV

50%of

strength

1p-1h or 1p statesBertsch, HamamotoShimizu et alTowner, Khanna

100%of

strength

1p-1hor

1p states

0p-0hor 1p

0p-0hor 1p

0p-0hor 1p

1p-1hor

1p states

Page 41: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

Dang,Arima et al .

Rijsdijk,Dickhoff et al .

exp (K.Yoko,      H.Sakai et al.)

Zr(p,n)90

Zr(n,p)90

IVSM

Ref. : K.Yoko, H.Sakai et al, Phys.Lett.B615 (2005) 193.

Page 42: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

Comparison between experimental and theoretical results for GT strength

distributions

IVSM should be subtracted to evaluate GT quenching Q

IVSMIVSM

IVSM

• (p,n) Calc. with 2p2h• Bertsch,Hamamoto PRC 26 1323 (1982)

• Dang, Arima et al. PRL 79, 1638 (1997)

– Fairly good agreement with experimental results in contituum

– Exp. > Theory → IVSM

• (p,n) and (n,p) Calculations• DRPA by Rijssijk et al.PRC 48, 1752 (1993)

– Good agreement in low (GT)– Exp. > Theory in high → IVSM

Page 43: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

• Final Values (Up to 50 MeV of 90Nb)– Total GT strengths

• •

– GT sum rule•

– Quenching Factor•

GT Quenching Factor Q after Subtraction of IVSM

)ˆ(7.1)IVSM(9.0)MDAstat(6.06.28 GT S

)ˆ(2.0)IVSM(3.0)MDAstat(5.08.2 GT S

)ˆ(5.1)IVSM(7.0)MDAstat(7.05.82 GT SS

)ˆ(05.0)IVSM(02.0)MDAstat(02.086.0 GTQ

)ˆ(15.0 .....)MDAstat(05.090.0 GTQPreviousInaccessible errors in TRIUMF data

07.086.0 Q (quadratic sum of uncertainties)Our final(latest) result

Page 44: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen
Page 45: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen
Page 46: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

One- + two- exchange potential

M. Taketani, S. Machida, and S. Onuma:Prog. Theor. Phys. 7 45 (1952)

Central

Tensor

One-exchange

Two-exchange

One-exchange

Two-exchange

Tensor Operator

Page 47: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

Summary:Most important parts of the nuclear force

ShortInter-mediate Long range

Tensor force

Spin-orbit force

Central force

Page 48: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

(2) (2)12 12 12

0

12 12( ) , ( )TV S Y f r r

where

2(2)12

(2)

12

1 2

12

, spherical harmonics

( ) a function of relative distance r

S s s

Y

f r

(0)(2) (2) 223( ) ( ) /S Y r 1 1 2s r s r s s

Page 49: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

The deuteron wave function has the form

(1)(0) (1) (2) (1)( ) ( ) ( ) ( )N u r Y r Y

where N is a normalization constant, u(r) andare radial wave functions , and    are the spin wave functions of the two nucleons:

(1)

1 2

1 2 1 2 / 2

1 2

(1)( )r

Page 50: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

The quadrupole moment of the deuteron confirms that the deuteron is not spherical.

This is the best evidence of the tensor force.

observed

OPEP

Page 51: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

Deuteron

z-axis

z-axis

+ 0.03×

Deformed rotor

z-axis

=

03 22)2( rzQ

3S1 state 3D1 state

03 22)2( rzQ

Tensor force mixes 3S1 and 3D1 states

Page 52: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

The first order effect of the tensor force is zero between a valence nucleon and the core16O or 40Ca, in which both j j and are closed.

This is because

magicnumber

1

0

0

ii

ii

S s

L

1 12 2

j j l lwhen both and are closed, and therefore

3( )( ) ( ) 0 .i ik k ik i ki

s r s r s s0 0

Page 53: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

The second order effect of the tensor force suggested by Wigner in 1950.

Arima and Terasawa calculated the second order effect of the tensor foce in OPEP.

in 17O

Page 54: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

-meson weakens the tensor force.

The second order effect of the tensor force could be 1/3 ~ 1/4 of the spin-orbit interaction.

Page 55: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

51Sb isotopes (Proton SPE)J. P. Schiffer et al., Phys. Rev. Lett. 92 162501 (2004)

1h11/2

1g7/2

64 70 82Neutron number

En

erg

y [

MeV

]

Page 56: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

The first order effect of tensor force on :sV s ( < 0 in shell model)

change of

1

2j

orbit is being occupied

0, 0S L

1

2j

orbit is being occupied

0, 0S L

j isclosed

after two orbitsj j and areclosed

0, 0S L

occupation

Page 57: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

Shell model requires 0, where is the strength

of the spin-orbit interaction :

sV s

The first order effect of the tensor force weakensthe spin-orbit interaction when valence nucleon levels are being occupied.

j

is being occupied

11/ 2his being occupied

9 / 2h

Single particleenergy of protons

j

jj

1h11/2

1g7/2

Page 58: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

1h9/21h11/2

Sb isotopes (Proton SPE)T. Otsuka, T. Matsuo, and D. Abe, Phys. Rev. Lett. 97 162501 (2006)J. P. Schiffer et al., Phys. Rev. Lett. 92 162501 (2004)

Page 59: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

Summary:Most important parts of the nuclear force

ShortInter-mediate Long range

Tensor force

Central force

Spin-orbit force

Page 60: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

In summary, I discussed the contributions of

Professor Hideki Yukawa in fostering and

encouraging young researchers and this

contributions to promote fundamental

sciences, especially by establishing inter-

university research institutes in Japan.

Page 61: Hideki Yukawa and Nuclear Physics Akito Arima Japan Science Foundation Musashi Gakuen

I then discussed nuclear magnetic moments where the one pi-meson exchange current plays a veryessential role together with the configuration-mixingeffect. The tensor force is of the most importantConsequences of the pion exchange potential. The best evidence is provided by the deuteron. The g7/2-h11/2 spacing of proton levels in the Sbistopes also provides an evidence of the tensorforce. Thus pions predicted by Professor H.Yukawa still plays important role in nuclear physicstoday.