Transcript
Page 1: Symmetries of the Cranked Mean Field

Symmetries of the Cranked Mean Field

S. Frauendorf

Department of Physics

University of Notre Dame

USA

IKH, Forschungszentrum

Rossendorf, Dresden

Germany

Page 2: Symmetries of the Cranked Mean Field

In collaboration withA. Afanasjev, UND, USAB. V. Dimitrov, ISU, USAF. Doenau, FZR, GermanyJ. Dudek, CRNS, FranceJ. Meng, PKU, China N. Schunck, US, GB Y.-ye Zhang, UTK, USAS. Zhu, ANL, USA

Page 3: Symmetries of the Cranked Mean Field

Rotating mean field: Tilted Axis Cranking model

Seek a mean field state |> carrying finite angular momentum,where |> is a Slater determinant (HFB vacuum state)

.0|| zJ

Use the variational principle

with the auxiliary condition

0|| HEi

0||' zJHEi

The state |> is the stationary mean field solution in the frame that rotates uniformly with the angular velocity about the z axis.

TAC: The principal axes of the density distribution need not coincide with the rotational axis (z).

Page 4: Symmetries of the Cranked Mean Field

functions) (wave states particle single

)(routhians frame rotating in energies particle single '

ial)(potentent field mean

energy kinetic

(routhian) frame rotating thein nhamiltonia field mean '

|'' -'

i

i

mf

iiizmf

e

V

t

h

ehJVth

tency selfconsis mfi V

Variational principle : Hartree-Fock effective interactionDensity functionals (Skyrme, Gogny, …)Relativistic mean field

Micro-Macro (Strutinsky method) …….

(Pairing+QQ)

X

S. Frauendorf Nuclear Physics A557, 259c (1993)

Page 5: Symmetries of the Cranked Mean Field

Spontaneous symmetry breaking

Symmetry operation S

.|'|'|'

energy same the withsolutions field mean are states All

1||| and ,''but ''

HHE

hhHH

|SS

|S

|SSSSS

Page 6: Symmetries of the Cranked Mean Field

Which symmetries

Combinations of discrete operations

rotation withreversal time- )(

inversion space-

2 angleby axis-zabout rotation - )

2(

y

z nn

TR

P

R

leave zJHH ' invariant?

axis-zabout rotation - )(zRBroken by m.f. rotational

bands

Obeyed by m.f.spinparitysequence

Page 7: Symmetries of the Cranked Mean Field

Common bands

by axis-zabout rotation - )(

rotation withreversal time- 1 )(

inversion space - 1

z

y

R

TR

P

Principal Axis CrankingPAC solutions

nI

e iz

2

signature ||)(

R

TAC or planar tilted solutionsMany cases of strongly brokensymmetry, i.e. no signature splitting

Page 8: Symmetries of the Cranked Mean Field

ChiralityChiral or aplanar solutions: The rotational axis is out of all principal planes.

rotation withreversal time- 1 )(

by axis-zabout rotation - 1 )(

inversion space - 1

y

z

TR

R

P

Page 9: Symmetries of the Cranked Mean Field

Consequence of chirality: Two identical rotational bands.

Page 10: Symmetries of the Cranked Mean Field

band 2 band 1134Pr

h11/2 h11/2

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The prototype of a chiral rotor

Frauendorf, Meng, Frauendorf, Meng, Nucl. Phys. A617, 131 (1997Nucl. Phys. A617, 131 (1997) )

Page 12: Symmetries of the Cranked Mean Field

10 12 14 16 18 20 220

100

200

300

400

500

600

700

800

900

1000

backbend

134Prexperiment

E2-

E1

I

E2E1 omega1

There is substantial tunneling between the left- and right-handed configurations

chiralregime

Rotational frequency

Energy difference Between the chiral sisters

chiral regime

rotEE 3.012

Page 13: Symmetries of the Cranked Mean Field

Chiral sister bands

Representativenucleus I

observed13 0.21 145910445 Rh 2/11

12/9 hg

13 0.21 4011118877 Ir

2/912/9 gg

447935 Br

12/132/13

ii

13 0.21 14

predicted

predicted

9316269 Tm 1

2/112/13ii predicted45 0.32 26

12/112/11

hh observed13 0.18 267513459 Pr

31/37

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Composite chiral bands Demonstration of the symmetry concept:It does not matter how the three components of angular momentum are generated.

7513560 Nd 1

2/112

2/11hh observed23 0.20 29

6010545 Rh 2

2/1112/9 hg

observed20 0.22 29

I

Is it possible to couple 3 quasiparticles to a chiral configuration?

Page 15: Symmetries of the Cranked Mean Field

Reflection asymmetric shapes

Two mirror planes

Combinations of discrete operations

rotation withreversal time- )(

inversion space-1

by axis-zabout rotation - )(

PTR

P

R

y

z

Page 16: Symmetries of the Cranked Mean Field

Good simplex

Several examples in mass 230 region

Other regions? Substantial tunneling

I

i

z

e

)(parity

simplex ||

1)(

S

PRS

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Th225

Parity doubling

Only good case.Must be better studied!

Substantial tunneling

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Tetrahedral shapes

J. Dudek et al. PRL 88 (2002) 25250232a

5.032 a

15.032 a

Page 19: Symmetries of the Cranked Mean Field

Which orientation has the rotational axis?

minimum

maximum

Classical no preference

Page 20: Symmetries of the Cranked Mean Field

)2/(

zR

P

2/)(parity

12

,2

doublex |

1)2/(

2

signature 1)(

I

i

z

z

e

nI

|D

PRD

R

0

2

4E3

3

5

7E3

Page 21: Symmetries of the Cranked Mean Field

509040 Zr

Prolate ground state

Tetrahedral isomer at 2 MeV

132 MeVp

18 MeVt

Page 22: Symmetries of the Cranked Mean Field

Isospatial analogy

Which symmetries leave

ATHZNHH zpn ' invariant?

axis-zabout nisorotatio - )( zTiz e R

Broken by m.f. isorotationalbands

Proton-neutron pairing: symmetries of the pair-fieldAnalogy between angular momentum J and isospin T

space gauge in rotation- 1D - )( Aig e R

Broken by m.f. Pair-rotationalbands

Page 23: Symmetries of the Cranked Mean Field

1t

0t

Isovectorpair fieldbreaks isorotationalinvariance.

Isoscalarpair fieldkeeps isorotationalinvariance.

Page 24: Symmetries of the Cranked Mean Field

The isovector scenario

02

ˆ

np

ppnn

y

Calculate without np-pair field.

Add isorotational energy.

ionsconfigurat possible restricts for 0

2

)1()0 field, mean( np

ZNT

TTEE

y

iso

preferred axis

Page 25: Symmetries of the Cranked Mean Field

The isovector scenario works well(see poster 161).

Page 26: Symmetries of the Cranked Mean Field

Isorotational energy gives the Wigner term in the binding energies mWigner terenergysymmetry

)(75

2

)1( 2

TTA

MeVTT

iso

Structure of rotational bands in 377437 Rb

nrestrictio ionconfigurat 0yT

reproduced

For the lowest states in odd-odd nuclei with ZN

isoisoTETE

TETE

2/122/1)1(2)0(

)1()0(

No evidence for the presence of an isoscalar pair field

See poster 161

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Isoscalar pairing at high spin?

Isoscalar pairs carry finite angular momentum

iJ z 2

total angular momentum

•A. L. GoodmanPhys. Rev. C 63, 044325 (2001)

Predicted by

Which evidence?

Page 28: Symmetries of the Cranked Mean Field

Adding nn pairs to the condensate does not change the structure.

Pair rotational bands are an evidence for the presence of a pair field.

Ordinary nn pair field

Page 29: Symmetries of the Cranked Mean Field

which symmetries leave ATHH z ' invariant?

1 )( Aig e R Either even or odd A belong to the band.

1 )( Nin e R Even and odd N belong to the band.

1 )( zJiz e R Both signatures belong to the band.

nNI

e ig

nzg

2

gaugeplex ||

1)()(

S

RRS

iJ z 2

total angular momentum

If an isoscalar pair field is present,

Page 30: Symmetries of the Cranked Mean Field

Pair rotational bands for an isoscalar neutron-proton pair field

ZNA 22

2/))()2(( AEAE

Even-even, even I Odd-odd, odd I

Not enough data yet.

Page 31: Symmetries of the Cranked Mean Field

Summary

Symmetries of the mean field are very useful to characterizenuclear rotational bands.

Nuclei can rotate about a tilted axis: New discrete symmetries manifest by the spin and parity sequence in the rotational band:-New type of chirality in nuclei: Time reversal changes left-handed into right handed system.

-Spin-parity sequence for reflection asymmetric (tetrahedral) shapes

The presence of an isovector pair field and isospin conservation explain the binding energies and rotational spectra of N=Z nuclei.

Page 32: Symmetries of the Cranked Mean Field

Out of any plane: parity doubling + chiral doubling

,,,10

,,,9

,,,8

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Banana shapes

Z=70, N=86,88J. Dudek, priv. comm.

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Doublex quantum number

2/)2/(

1

2

)(

)2/(

12

,2

2,2)(

2

||)(||

)2/(

IIi

z

z

iz

i

z

eparity

nI

ee

DRP

RD

RD

PRD

Page 37: Symmetries of the Cranked Mean Field

Restrictions due to the symmetry yT

States with good N, Z –parity are in general no eigenstates of .yT

If they are (T=0) the symmetry restricts the possible configurations, if not (T=1/2) the symmetry does not lead to anything new.

0|:0 yTT

00|)(2

1

00|)(2

1

00|)(2

1

00|)(2

1

00|

00|

jnipjpiny

jnipjpiny

jpipjniny

jpipjniny

inipy

y

T

T

T

T

T

T

Page 38: Symmetries of the Cranked Mean Field

)(yTR

Page 39: Symmetries of the Cranked Mean Field

Rotationalbands in

Er163

1 1’ 2 3 4 7

PAC TAC


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