ISOSPIN MIXING PHENOMENA IN THE VICINITY OF N=Z LINE

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ISOSPIN MIXING PHENOMENA IN THE VICINITY OF N=Z LINE Wojciech Satuła + NNN + .... tens of MeV ab initio ntro: effective low-energy theory for medium mass and heavy nuclei mean-field (or nuclear DFT) beyond mean-field (projection) Summary Symmetry (isospin) violation and restoration: unphysical symmetry violation isospin projection Coulomb rediagonalization (explicit symmetry violation) collaboration with J. Dobaczewski, W. Nazarewicz, M. Rafalski & M. Borucki structural effects SD bands in 56 Ni superallowed beta decay isospin impurities in ground-states of e-e nuclei symmetry energy – new opportunities of studying with the isospin proje

description

ISOSPIN MIXING PHENOMENA IN THE VICINITY OF N=Z LINE. Wojciech Satuła. in collaboration with J. Dobaczewski , W. Nazarewicz, M. Rafalski & M. Borucki. Intro : effective low-energy theory for medium mass and heavy nuclei  - PowerPoint PPT Presentation

Transcript of ISOSPIN MIXING PHENOMENA IN THE VICINITY OF N=Z LINE

Page 1: ISOSPIN  MIXING PHENOMENA IN THE VICINITY OF  N=Z  LINE

ISOSPIN MIXING PHENOMENA IN THE VICINITY OF N=Z LINEWojciech Satuła

+ NNN + .... tens of MeV

ab initio

Intro: effective low-energy theory for medium mass and heavy nuclei mean-field (or nuclear DFT) beyond mean-field (projection)

Summary

Symmetry (isospin) violation and restoration: unphysical symmetry violation isospin projection Coulomb rediagonalization (explicit symmetry violation)

in collaboration with J. Dobaczewski, W. Nazarewicz, M. Rafalski & M. Borucki

structural effects SD bands in 56Ni superallowed beta decay

isospin impurities in ground-states of e-e nuclei

symmetry energy – new opportunities of studying with the isospin projection

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Effective theories for low-energy (low-resolution) nuclear physics (I):

Low-resolution separation of scales which isa cornerstone of all effective theories

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Fourierlocal

correctingpotential

hierarchy of scales:2roA1/3

ro~ 2A1/3

is based on a simple and very intuitive assumption that low-energy

nuclear theory is independent on high-energy dynamics

~ 10

The nuclear effective theory

Long-range part of the NN interaction(must be treated exactly!!!)

where

regularizationCoulomb

ultravioletcut-off

denotes an arbitrary Dirac-delta model

Gogny interaction

przykład

There exist an „infinite” number

of equivalent realizationsof effective theories

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lim daa 0

Skyrme interaction - specific (local) realization of the nuclear effective interaction:

spin-orbitdensity dependence10(11)

parameters

Y | v(1,2) | YSlater determinant

(s.p. HF states are equivalent to the Kohn-Sham states)

Skyrme-force-inspired local energy density functional

local energy density functional

relative momenta spin exchange

LO

NLO

SV

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Elongation (q)

Tota

l ene

rgy

(a.u

.)

Symmetry-conserving

configuration

Symmetry-breaking

configurations

Skyrme (nuclear) interaction conserves such symmetries like: rotational (spherical) symmetry isospin symmetry: Vnn = Vpp = Vnp (in reality approximate) parity…

LS LS LS

Mean-field solutions (Slater determinants) break (spontaneously) these symmetries

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Euler angles gauge angle

Restoration of broken symmetry

rotated Slater determinantsare equivalent

solutions

where

Beyond mean-field multi-reference density functional theory

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There are two sources of the isospin symmetry breaking:- unphysical, caused solely by the HF approximation- physical, caused mostly by Coulomb interaction (also, but to much lesser extent, by the strong force isospin non-invariance)

Find self-consistent HF solution (including Coulomb) deformed Slater determinant |HF>:

Calculate the projected energy andthe Coulomb mixingBefore Rediagonalization:

BR

aC = 1 - |bT=|Tz||2

BR

in order to create good isospin„basis”:

Apply the isospin projector:

Isospin symmetry restoration

Engelbrecht & Lemmer, PRL24, (1970) 607

See: Caurier, Poves & Zucker, PL 96B, (1980) 11; 15

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Diagonalize total Hamiltonian in„good isospin basis” |a,T,Tz> takes physical isospin mixing

Isospin invariant

Isospin breaking: isoscalar, isovector & isotensor

aC = 1 - |aT=Tz

|2AR n=1

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0

0.2

0.4

0.6

0.8

1.0

aC

[%]

40 44 48 52 56 60Mass number A

0.01

0.1

1

44 48 52 5640 60

0

0.2

0.4 BRARSLy4

Ca isotopes:

eMF = 0

eMF = e

Numerical results:(I) Isospin impurities in ground states of e-e nuclei

Here the HF is solved without Coulomb |HF;eMF=0>.

Here the HF is solved with Coulomb |HF;eMF=e>.

In both cases rediagonalizationis performed for the total Hamiltonian including Coulomb

W.Satuła, J.Dobaczewski, W.Nazarewicz, M.Rafalski, PRL103 (2009) 012502

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0123456

00.20.40.60.81.0

20 28 36 44 52 60 68 76 84 92A

ARBR

SLy4

aC [%

]E

-EH

F [M

eV]

N=Z nuclei

100

This is not a single Slater determinatThere are no constraints on mixing coefficients

AR

AR

BR

BR

(II) Isospin mixing & energy in the ground states of e-e N=Z nuclei:

~30%DaC

HF tries to reduce the isospin mixing by:

in order to minimize the total energy

Projection increases the ground state energy(the Coulomb and symmetryenergies are repulsive)

Rediagonalization (GCM)

lowers the ground state energy but only slightlybelow the HF

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3.0

3.5

4.0

4.5

29.5 30.0 30.5 31.0 31.5

aC

[%]

aCaC

(AR)

(BR)

80Zr

ET=1 [MeV](AR)

MSk

1M

Sk1

SkO

’Sk

O’

SkP

SLy5

SLy4

SLy7

SkM

*Sk

Xc

SkP

SLy5

SLy4 Sk

M*

SLy7 Sk

Xc

SIII

SIII

Isospin mixing in 80Zr from GDR gamma decay studies

communicated byFranco Camera

at the Zakopane’10meeting

doorway state energy

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D. Rudolph et al. PRL82, 3763 (1999)

f7/2

f5/2p3/2

neutrons protons

4p-4h

[303]7/2

[321]1/2

Nilsson

1

space-spin symmetric

2

f7/2

f5/2p3/2

neutrons protons

g9/2 pp-h

two isospin asymmetricdegenerate solutions

Isospin symmetry violation insuperdeformed bands in 56Ni

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4

8

12

16

20

5 10 15 5 10 15

Exp. band 1Exp. band 2Th. band 1Th. band 2

Angular momentum Angular momentum

Exc

itatio

n en

ergy

[MeV

] Hartree-Fock Isospin-projection

aC [%

]

band 12468 band 2

56Ni

Mean-field

pph

nph

T=0

T=1centroiddET

dET

Isospin projection

W.Satuła, J.Dobaczewski, W.Nazarewicz, M.Rafalski, PRC81 (2010) 054310

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Primary motivation of the project isospin corrections

for superallowed beta decay

s1/2

p3/2

p1/2

p2

8

n p2

8

n

d5/2

14O 14NHartree-Fock

Experiment:Fermi beta decay:

f statistical rate function f (Z,Qb)t partial half-life f (t1/2,BR)

GV vector (Fermi) coupling constant <t+/-> Fermi (vector) matrix element

|<t+/->|2=2(1-dC)

Tz=-/+1 J=0+,T=1

J=0+,T=1t+/-

BR

(N-Z=-/+2)

(N-Z=0)Tz=0Qb

t1/2

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Experiment world data survey’08

10 cases measured with accuracy ft ~0.1% 3 cases measured with accuracy ft ~0.3%

nucleus-independent

~2.4%Marciano & Sirlin, PRL96 032002 (2006)

~1.5% 0.3% - 1.5%

PRC77, 025501 (2008)

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What can we learn out of it?From a single transiton we can determine experimentally:

GV2(1+DR) GV=const.

From many transitions we can: test of the CVC hypothesis

(Conserved Vector Current)

exotic decays Test for presence of a Scalar Current

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one can determine

mass eigenstates

CKMCabibbo-Kobayashi-Maskawaweak eigenstates

With the CVC being verified and knowing Gm (muon decay)

test unitarity of the CKM matrix

0.9491(4) 0.0504(6) <0.0001

|Vud|2+|Vus|2+|Vub|2=0.9996(7)

|Vud| = 0.97425 + 0.00023

test of three generation quark Standard Model of electroweak interactions

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Hardy &TownerPhys. Rev. C77, 025501 (2008)

Model dependence

Liang & Giai & MengPhys. Rev. C79, 064316 (2009)

spherical RPACoulomb exchange treated in the

Slater approxiamtion

dC=dC1+dC2shell

modelmeanfield

Miller & SchwenkPhys. Rev. C78 (2008) 035501;C80 (2009) 064319

radial mismatch of the wave functions

configuration mixing

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Isobaric symmetry violation in o-o N=Z nuclei

ground stateis beyond mean-field!

T=0n pT=0

T=1n p

Mean-field can differentiate between n p and n p

only through time-odd polarizations!

aligned configurationsn p

nn p p

n panti-aligned configurations

or n por n p

nn p pCORE CORE

Tz=-/+1 J=0+,T=1

J=0+,T=1t+/-

BR

(N-Z=-/+2)

(N-Z=0)Tz=0Qb

t1/2

ISOSPIN PROJECTION

MEAN FIELD

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0

10

20

30

40

1 3 5 7

aC

[%]

2K

isospin

isospin & angular momentum

0.586(2)%

42Sc – isospin mixing in nKpK antialigned configurations for

K=1/2,3/2,5/2, and 7/2

(

( (

(

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Hartree-Fock

ground statein N-Z=+/-2 (e-e) nucleus

antialigned statein N=Z (o-o) nucleus

Project on good isospin (T=1) and angular momentum (I=0)

(and perform Coulomb rediagonalization)

<T~1,Tz=+/-1,I=0| |I=0,T~1,Tz=0>t+/-

CPU~5h

~50000h

14O 14NH&T dC=0.330%

L&G&M dC=0.181%our: dC=0.303% (Skyrme-V; N=12)

~ ~

Project on good isospin (T=1) and angular momentum (I=0)

(and perform Coulomb rediagonalization)

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0

0.5

1.0

1.5

2.0

30 40 50 60 70

d C [

%]

Tz=0 Tz=1

A

00.20.40.60.81.01.2

10 15 20 25 30 35 40

d C [

%]

Tz=-1 Tz=0

A

our

Vud=0,97418(26)

Vud=0,97466

Ft=3071.4(8)+0.85(85)

Ft=3069.2(8)our (no A=38):

H&T:

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0

2

4

6

10 20 30 40 50

a’sy

m [

MeV

]

SV

SLy4LSkML*

SLy4

A (N=Z)

„NEW OPPORTUNITIES” IN STUDIES OF THE SYMMETRY ENERGY:

T=0

T=1n p

E’sym = a’symT(T+1)

12a’sym

asym=32.0MeV

asym=32.8MeV

SLy4:

In infinite nuclear matter we have:

SV:

asym=30.0MeVSkM*:

asym= eF + aintmm*

SLy4: 14.4MeV SV: 1.4MeV SkM*: 14.4MeV

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Summary and outlook Elementary excitations in binary systems may differ

from simple particle-hole (quasi-particle) exciatationsespecially when interaction among particles posseses additional

symmetry (like the isospin symmetry in nuclei)

Superallowed beta decay: encomapsses extremely rich physics: CVC, Vud, unitarity of the CKM matrix, scalar currents… connecting nuclear and particle physics … there is still something to do in dc business …

Projection techniques seem to be necessary to account for those excitations - how to construct non-singular EDFs?

Isopin projection, unlike angular-momentum and particle-number projections, is practically non-singular !!!

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0.0001

0.001

0.01

0.1

1

0.0 0.5 1.0 1.5 2.0 2.5 3.0

|OV

ER

LA

P|

bT [rad]

only IP

IP+AMP

pr =S yi

* Oij jjij

-1

inverse of theoverlap matrix

space & isospin rotatedsp state

HF sp state

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-1

01

23

4

0 10 20 30 40 50 60

Qb –

Qb

[MeV

]th

exp

Atomic number

0,2%

0,8%

0,9%

1,5%

2,5%

3,7%

4,1%

time-even

Hartree-Fock

isospin projected

0 10 20 30 40 50 60Atomic number

0,9%

7,9%

15,1%10,1%

26,3%

29,9%

21,7%

time-odd

Qb values in super-allowed transitions

time-odd

T=1,Tz=-1 T=1,Tz=0 T=1,Tz=1e-e e-eo-o

Isospin symmetry violation due to time-odd fields in the intrinsic system

Isobaric analogue states:

isospin projected

Hartree-Fock

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4567

18 19 20 21 22asym(rNM/2) [MeV]

4567

29 30 31 32asym(rNM) [MeV]

0.70.80.91.01.1

aC [

%]

18 19 20 21 22asym(rNM/2) [MeV]

29 30 31 32asym(rNM) [MeV]

0.70.80.91.01.1

aC [

%]

40Ca

40Ca 100Sn

100Sn

SkO

SkO’SkM*

MSk1SkXc

SIIISLy

SkP

SIII

SkP MSk1

SkXcSkM*

SLy5SLy

SkO’SkO

SkO

SkO’SkM*

SIII

SIII SkO

SkP

SLySLySkXc

MSk1

SkPMSk1

SkXcSkM* SLy

SkO’SLy5

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0.20

0.25

0.30

0.35

6 8 10 12Number of shells

d C [

%]

Towner & Hardy 2008

Liang et al. (NL3)

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aligned configurationsn p

nn p p

n panti-aligned configurations

Isobaric symmetry breaking in odd-odd N=Z nucleiLet’s consider N=Z o-o nucleus disregarding, for a sake of simplicity,

time-odd polarization and Coulomb (isospin breaking) effects

or n por n p

T=0

After applying „naive” isospin projection we get:

T=0T=1

ground stateis beyond mean-field!

n p n p

Mean-field can differentiate between n p and n p

only through time-odd polarizations!

4-fold degeneracy

nn p pCORE CORE

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Position of the T=1 doorway state in N=Z nuclei

20

25

30

35

20 40 60 80 100A

SIII SLy4 SkP

E(T

=1)-

EH

F [M

eV]

meanvalues

Sliv & Khartionov PL16 (1965) 176

based on perturbation theoryDE ~ 2hw ~ 82/A1/3 MeV

Bohr, Damgard & Mottelsonhydrodynamical estimateDE ~ 169/A1/3 MeV

31.5 32.0 32.5 33.0 33.5 34.0 34.5

y = 24.193 – 0.54926x R= 0.91273

doorway state energy [MeV]

4567

aC [%

] 100Sn

SkO

SIIIMSk1

SkP SLy5

SLy4SkO’

SLySkPSkM*

SkXc

Dl=0, Dnr=1 DN=2