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INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids and shell evolutions in exotic nuclei Takaharu Otsuka University of Tokyo / MSU HPCI Strategic Programs for Innovative Research (SPIRE)
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INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

Dec 18, 2015

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Page 1: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS36th Course

Nuclei in the Laboratory and in the CosmosErice, Sicily

September 21 (16-24), 2014

Dual quantum liquids and

shell evolutions in exotic

nuclei

Takaharu Otsuka University of Tokyo / MSU

HPCI Strategic Programs for Innovative Research (SPIRE)

Field 5 “The origin of matter and the universe”

Page 2: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

Outline

1. Introduction

2. (Type I) Shell Evolution

3. Computational aspect

4. Type II Shell Evolution and Dual Quantum Liquids

5. Summary

Page 3: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

Difference between stable and exotic nuclei

life time infinite or long short

number ~300 7000 ~ 10000

propertiesconstant inside (density saturation)

density low-density surface (halo, skin)

shell same magic numbers(2,8,20,28, … (1949))

shell evolution

shapeshape phase transition (?)shape coexistence

?

stable nuclei exotic nuclei

Page 4: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

Schematic picture of shape evolution (sphere to ellipsoid)

- monotonic pattern throughout the nuclear chart –

Distance from the nearest closed shell in N or Z

exc

itati

on

en

erg

y

From Nuclear Structure from a Simple Perspective, R.F. Casten (2001)

Page 5: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

Quantum (Fermi) liquid (of Landau)

e1

e2

e5

e4e3

e8

e7e6

interplay between single-particle energies and interaction - in a way like free particles -

e1

e2

e5

e4e3

e8

e7e6

proton

neutron

For shape evolution, there may have been Ansatz that

Spherical singleparticle energiesremain basicallyunchanged. -> spherical part of Nilsson modelCorrelations, particularly due to proton-neutron interaction, produce shape evolutions.

Similar argument to Shape coexistence

Page 6: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

shape coexistence

186Pb A.N. Andreyev et al., Nature 405, 430 (2000)

16O H. Morinaga(1956)

Island of Inversion (Z=10~12, N=20)

Page 7: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

Outline

1. Introduction

2. (Type I) Shell Evolution

3. Computational aspect

4. Type II Shell Evolution and Dual Quantum Liquids

5. Summary

Page 8: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

Spin-orbit splitting

Eigenvalues of HO potential

Magic numbers

Mayer and Jensen (1949)126

8

20

28

50

82

2

5hw

4hw

3hw

2hw

1hw

Page 9: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

TO, Suzuki, et al.PRL 95, 232502 (2005)

One of the primary origins :

change of spin-orbit splitting due to the tensor

force

Type I Shell Evolution :

change of nuclear shell as a function of N or Z

due to nuclear forces

Page 10: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

f7/2

p 3/2

p 1/2

f5/2

Normalshell structurefor neutrons

in Ni isotopes(proton f7/2

fully occupied)

28

N=34 (and 32) magic number appears, if

neutron f5/2 becomes

less bound in Ca.

f7/2

p 3/2

p 1/2

f5/2

28

34

32byproduct

Example : N=34 and 32 (sub-) magic numbers

TO et al., PRL 87, 82501 (2001)

Page 11: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

Shell evolution from Fe down to Ca due to proton-neutron interaction

neutron f5/2 – p1/2 spacing increases by ~0.5 MeV per one-proton removal from f7/2, where tensor and central forces works coherently and almost equally.

note : f5/2 = j < f7/2 = j > Steppenbeck et al. Nature, 502, 207 (2013)

Page 12: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

Steppenbeck et al. Nature, 502, 207 (2013)

Experiment @ RIBF Finally confirmed

newRIBFdata

Page 13: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

Exotic Ca Isotopes : N = 32 and 34 magic numbers ?

52Ca 54Ca

51Ca 53Ca GXPF1B int.: p3/2-p1/2 part refined from GXPF1 int. (G-matrix problem)

2+ 2+

Some exp.levels : priv. com.

From my talk at Erice 2006

Page 14: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

Shell evolutionin two dimensions

Ca

Evolution along isotopesdriven by three-body force

Evolution along isotonesdriven by tensor force

Ni

Page 15: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

Island of Inversion (N~20 shell structure) : model independence

20

16

16

20

cvcvcv cv

16

20

Strasbourg SDPF-NR Tokyo sdpf-M

Color code of lines is different from the left figure.

Shell-model interactions

Based on Fig 41, Caurier et al. RMP 77, 427 (2005)

VMU interaction central + tensorTO et al., PRL, 104, 012501 (2010)

Page 16: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

thFranchoo et al., PRC 64, 054308 (2001) “level scheme … newly established for 71,73Cu” “… unexpected and sharp lowering of the pf5/2 orbital” “… ascribed to the monopole term of the residual int. ..”

a clean example of tensor-force driven shell evolution

TO, Suzuki, et al.PRL 104, 012501 (2010)

Flanagan et al., PRL 103, 142501 (2009) ISOLDE exp.k1

k2

k1k2

g9/2

Proton f5/2 - p3/2 inversion in Cu due to neutron occupancy of g9/2

Page 17: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

Outline

1. Introduction

2. (Type I) Shell Evolution

3. Computational aspect

4. Type II Shell Evolution and Dual Quantum Liquids

5. Summary

Page 18: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

BN

n

nJi DPcD

1

)(, )()(

)()()( DHDDE Minimize E(D) as a function of D utilizing qMC and conjugate gradient methods

p spN N

i

nii

n DcD1 1

)()( )(

Step 1 : quantum Monte Carlo type method candidates of n-th basis vector (s : set of random numbers)

“ s ” can be represented by matrix D Select the one with the lowest E(D)        

)0()()(

eh

Step 2 : polish D by means of the conjugate gradient method “variationally”.       

Advanced Monte Carlo Shell Model

steepestdescentmethod

conjugategradient method

NB : number of basis vectors (dimension)

Projection op.

Nsp : number of single-particle states

Np : number of (active) particles

Deformed single-particle state

N-th basis vector(Slater determinant)

amplitude a

Page 19: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

MCSM (Monte Carlo Shell Model -Advanced version-)1. Selection of important many-body basis vectors by quantum Monte-Carlo + diagonalization methods basis vectors : about 100 selected Slater determinants

composed of deformed single-particle states

2. Variational refinement of basis vectors conjugate gradient method 3. Variance extrapolation method -> exact eigenvalues K computer (in Kobe) 10 peta flops machine

Projection of basis vectors

Rotation with three Euler angles with about 50,000 mesh points

Example : 8+ 68Ni 7680 core x 14 h

+ innovations in algorithm and code (=> now moving to GPU)

Page 20: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

Outline

1. Introduction

2. (Type I) Shell Evolution

3. Computational aspect

4. Type II Shell Evolution and Dual Quantum Liquids

5. Summary

Page 21: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

Effective interaction : based on A3DA interaction by Honma

• Two-body matrix elements (TBME) consist of microscopic and empirical ints.– GXPF1A (pf-shell)– JUN45 (some of f5pg9)– G-matrix (others)

• Revision for single particle energy (SPE) and monopole part of TBME

Example : Ni and neighboring nuclei

• pfg9d5-shell (f7/2, p3/2, f5/2, p1/2, g9/2, d5/2) large Hilbert space (5 x 1015 dim. for 68Ni) accessible by MCSM

Configuration space

Page 22: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

Yrast and Yrare levels of Ni isotopes

fixed Hamiltonian-> all variations

exp th

Y. Tsunoda et al. PRC89, 030301 (R) (2014)

Page 23: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

Level scheme of 68Ni

Colors are determined from the calculation

R. Broda et al., PRC 86, 064312 (2012)

Recchia et al., PRC 88, 041302 (2013)

Page 24: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

R. Broda et al., PRC 86, 064312 (2012)

Broad lines correspond to large B(E2)

Band structure of 68Ni

Taken from Suchyta, Y. Tsunoda et al., Phys. Rev. C89, 021301 (R) (2014) ;Y. Tsunoda et al., Phys. Rev. C89, 031301 (R) (2014)

Page 25: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

MCSM basis vectors on Potential Energy Surface

• PES is calculated by CHF

• Location of circle : quadrupole deformation of unprojected MCSM basis vectors

• Area of circle : overlap probability between each projected basis and eigen wave function

0+1 state of 68Ni

oblate

prolatespherical

triaxial

eigenstate Slater determinant -> intrinsic deformation

Page 26: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

68Ni 0+ wave functions different shapes⇔

• 68Ni 0+1 - 0+

3 states are comprised mainly of basis vectors generated in

0+1 : spherical

0+2 : oblate

0+3 : prolate

0+1 state of 68Ni 0+

3 state of 68Ni

0+2 state of 68Ni

Page 27: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

Shell Evolution within a nucleus : Type II

Neutron particle-hole excitation changes proton spin-orbitsplittings, particularly f7/2 – f5/2 , crucial for deformation

  →  shell deformation interconnected

Z=28 closed shell

attraction

repulsion

stronger excitationi.e., more mixing

( prolate superdef. )

f5/2

f7/2

g9/2

f5/2

N=40

normal Type II Shell Evolution

Page 28: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

Type I Shell Evolution : different isotopes

Type II Shell Evolution : within the same nucleus

: holes

Page 29: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

Shell evolutions in the “3D nuclear chart”

C C : configuration (particle-hole excitation)

Type I Shell Evolution

Type II Shell Evolution

C=0 : naïve filling configuration -> 2D nuclear chart

Page 30: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

Effective single-particle energy

effect oftensor force

Page 31: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

Stability of local minimum and the tensor force

Green line : proton-neutron monopole interactions

f5/2 – g9/2

f7/2 – g9/2

so that proton f7/2 – f5/2 splitting is

NOT changed due to the g9/2

occupation.

Same for f5/2 – f5/2 , f7/2 – f5/2

are reset to their average

attraction

repulsion

f5/2

f7/2

g9/2

f5/2

The pocket is lost.

Page 32: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

Effect of the tensor force

Present

Bohr-model calc. by HFB with Gogny force,Girod, Dessagne, Bernes, Langevin, Pougheon and Roussel, PRC 37,2600 (1988)

no (expicit) tensor force

Page 33: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

Dual quantum liquids in the same nucleus

Liquid 1 Liquid 2

neutron

core

proton

core

neutron

core

proton

core

leading to spherical state leading to prolate state

Certain different configurations produce different shell structures owing to (i) tensor force and (ii) proton-neutron

compositionsNote : Despite almost the same density, different single-particle energies

Page 34: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

ZrPb

Same type

h9/2

h11/2

i13/2

h9/2

proton neutron

g9/2

p1/2

g7/2

d5/2

proton neutron

Fermi energyof 186Pb

Variation

Page 35: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

critical phenomenon : two phases (dual quantum liquids) nearly degenerate

large fluctuation near critical point

Page 36: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

70Ni

2+22+

1

spherical prolate

0+1

0+2

spherical +prolate, but no oblate !

74Ni

2+22+

1 gamma unstable

0+1

0+2

Large fluctuation

weaker prolate by Pauli principle

Page 37: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

Different appearance of Double Magicity of 56,68,78Ni

2+ Ex. Energy

Ex(2

+ ) (M

eV)

0+1 state of 56Ni 0+

1 state of 68Ni

0+1 state of

78Ni

78Ni68Ni

sharper minimum

Page 38: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

Summary

1. Shell evolution occurs in two ways Type I Changes of N or Z (2D) -> occupation of specific orbits Type II Particle-hole excitation (3D) -> occupation and vacancy of specific orbits 2. Tensor force, at low momentum, remains unchanged after renormalizations (short-range and in-medium). (Tsunoda et al. PRC 2011) It can change the shape indirectly, through Jahn-Teller mechanism.

3. Dual quantum liquids appear owing also to proton-neutron composition

of nuclei, giving high barrier and low minimum for shape coexistence. Dual quantum liquids can be viewed as a critical phenomenon. The transition from dual to normal quantum liquids results in large (dynamical) fluctuation of the nuclear shape.

4. Many cases (Zr, Pb, etc.) of shape coexistence can be studied in this way, with certain perspectives to fission and island of stability.

Page 39: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

Collaborators in main slides

Y. Tsunoda Tokyo

Y. Utsuno JAEA N. Shimizu Tokyo M. Honma Aizu

54Ca magicity (RIKEN-Tokyo)

Ni calculation (an HPCI project)

Page 40: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

70Ni

0+1

0+2

2+22+

1

68Ni 0+3

2+2

0+1

0+2

72Ni

prolate

spherical

oblate

spherical prolate

0+1

0+2

spherical and prolate still coexist, but no oblate !

Page 41: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

74Ni

0+1 0+

2

2+22+

1

76Ni

gamma unstable

0+1

0+2

g-unstable and prolate w/o barrier

prolate byPauli principle

74Ni

The situation continues to

0+2

Page 42: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

78Ni

2+22+

1

0+1

weak oblate or

0+2 0+

3

stronger triaxial w/o pot. min.

gamma-unstable or E(5)-like

strong tendency towardsoblate, triaxiality, or E(5) - all “-like” -

Page 43: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

E N Dcollaborators in main slides

Page 44: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.
Page 45: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

also by Suchyta et al. (2013)

Very recent paper shows

Calc. by Strasbourgtheory group

Page 46: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.
Page 47: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

Yrast and Yrare levels of heavier Ni isotopes

g unstable

Page 48: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

78Ni

0+1

0+2

2+22+

1

76Ni

0+1

weak oblate or

0+2 0+

3

stronger triaxial w/o pot. min.

gamma-unstable or E(5)-like

strong tendency towardsoblate, triaxiality, or E(5)

Page 49: INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 36th Course Nuclei in the Laboratory and in the Cosmos Erice, Sicily September 21 (16-24), 2014 Dual quantum liquids.

critical point and large fluctuation - requirement for the phase transition -

neutron part :too rigid