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Symmetries along the N§Z line - AGATA Experiment @ Padova

Symmetries along the N§Z line - AGATA Experiment @ Padova

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International Workshop on Physics with <strong>AGATA</strong><br />

22-24 March 2004 Orsay<br />

<strong>Symmetries</strong> <strong>along</strong> <strong>the</strong> <strong>N§Z</strong> <strong>line</strong><br />

Silvia M. Lenzi - 8QLYHUVLWj GL 3DGRYD DQG ,1)1<br />

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Possible Signatures of Isospin Symmetry Breaking<br />

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WUDQVLWLRQV LQ PLUURU QXFOHL<br />

T = 1<br />

S.M. Lenzi - International Workshop on Physics with <strong>AGATA</strong> 2


Energy differences in <strong>the</strong> f 7/2 shell: MED and TED<br />

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T = 1<br />

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LQWHUDFWLRQ<br />

S.M. Lenzi - International Workshop on Physics with <strong>AGATA</strong> 3


Excitation energy differences: MED and TED<br />

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0(' - ( - ( = ! 1 ) ( - ( = 1 )<br />

7(' - ( - ( = ! 1 ) ( - ( = 1 ) 2(<br />

- ( 1 = )<br />

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EHWZHHQ WKH &RXORPE SRWHQWLDO 9& DQG WKH LVRVSLQ EUHDNLQJ QXFOHDU LQWHUDFWLRQ 9%<br />

S.M. Lenzi - International Workshop on Physics with <strong>AGATA</strong> 4


MED and TED in <strong>the</strong> shell model framework<br />

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S.M. Lenzi - International Workshop on Physics with <strong>AGATA</strong> 5


Coulomb effects in rotational bands: The Multipole Coulomb (CM) contribution<br />

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Its contribution is significant in rotational nuclei. CM “sees” to <strong>the</strong> alignment of nucleons.<br />

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S.M. Lenzi - International Workshop on Physics with <strong>AGATA</strong> 6<br />

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Monopole Coulomb and <strong>the</strong> drift in radii<br />

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S.M. Lenzi - International Workshop on Physics with <strong>AGATA</strong> 7


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KLJK VSLQ VWDWHV Æ larger radius and less Coulomb energy<br />

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The value of D U is obtained from <strong>the</strong> experimental data of A=41<br />

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/'0 0 $ %HQWOH\ HW DO 3K\V /HWW % S.M. Lenzi - International Workshop on Physics with <strong>AGATA</strong> 8


ISB component of <strong>the</strong> nuclear interaction in A=42<br />

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TED J = E J( 42 Ti) + E J( 42 Ca)<br />

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estimate V Bf7/2 (1) (Isovector)<br />

estimate V Bf7/2 (2) (Isotensor)<br />

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S.M. Lenzi - International Workshop on Physics with <strong>AGATA</strong> 9


MED and TED in <strong>the</strong> full fp shell model calculation<br />

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The isospin non-conserving nuclear contributions are deduced from <strong>the</strong> MED and TED<br />

in <strong>the</strong> T = 1, A = 42 triplet data.<br />

To construct an interaction in <strong>the</strong> whole pf shell we use a multiplicative prescription:<br />

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S.M. Lenzi - International Workshop on Physics with <strong>AGATA</strong> 10<br />

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Mirror Energy Differences in A=49<br />

Mn)<br />

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S.M. Lenzi - International Workshop on Physics with <strong>AGATA</strong> 11


([SHULPHQWDO GDWD<br />

MED <strong>along</strong> rotational bands in I 7/2 -shell nuclei<br />

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6 0 /HQ]L HW DO 3K\V 5HY /HWW S.M. Lenzi - International Workshop on Physics with <strong>AGATA</strong> 12


7('<br />

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TED <strong>along</strong> rotational bands in I 7/2 -shell nuclei<br />

T=1 triplets A=46, 50 in <strong>the</strong> f 7/2 shell have been recently observed at high spin<br />

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S.M. Lenzi - International Workshop on Physics with <strong>AGATA</strong> 13<br />

-


Mirror Energy Differences in <strong>the</strong> cross-conjugate A=42 and A=54 I shell nuclei<br />

6 3071<br />

451<br />

4 2620<br />

1227<br />

2 1392<br />

1392<br />

0 0<br />

54Ni<br />

First observation of<br />

excited states in 54 Ni<br />

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54Ni 54Co<br />

54Fe<br />

6 3043<br />

367<br />

4 2676<br />

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2 1556<br />

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0 0<br />

A=54<br />

A=42<br />

4 2815<br />

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MED (KeV)<br />

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A=42 MED = E J ( 42 Ti) - E J ( 42 Ca)<br />

A=54 -MED = E J ( 54 Fe) - E J ( 54 Ni)<br />

(-MED to keep <strong>the</strong> particle-hole symmetry)<br />

0 1 2 3 4 5 6<br />

A=42<br />

A=54<br />

0 1 2 3 4 5 6<br />

A rigorous treatment, calling upon state-of-<strong>the</strong>-art CSB potentials,<br />

is necessary to confirm <strong>the</strong>se phenomenological findings.<br />

S.M. Lenzi - International Workshop on Physics with <strong>AGATA</strong> 14<br />

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Extending <strong>the</strong>se investigations to o<strong>the</strong>r regions<br />

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S.M. Lenzi - International Workshop on Physics with <strong>AGATA</strong> 16


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f 7/2<br />

d 3/2<br />

Large MED in <strong>the</strong> sd shell: <strong>the</strong> electromagnetic spin-orbit term<br />

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It is important when a nucleon is promoted from a j=l-s level to a j=l+s<br />

level. The effect on a proton is opposite to <strong>the</strong> effect on a neutron orbit<br />

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S.M. Lenzi - International Workshop on Physics with <strong>AGATA</strong> 17<br />

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MED between negative parity states in T Z =1/2 sd-shell nuclei<br />

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Its contribution to MED becomes significant for configurations with<br />

SXUH single-nucleon excitations: a proton excitation in one nucleus<br />

and a neutron excitation in its mirror<br />

S.M. Lenzi - International Workshop on Physics with <strong>AGATA</strong> 18


Loosely-bound nuclei: The Thomas-Ehrman shift<br />

(Coulomb and nuclear effect in mirror nuclei)<br />

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The effect is large for small- orbits and light nuclei<br />

TES<br />

large MED<br />

3 * %L]]HWL DQG $ 0 %L]]HWL 6RQD<br />

Different E1 strengths: isospin mixing<br />

due to coupling with <strong>the</strong> continuum<br />

for weakly-bound or unbound states<br />

3.9 10 -2 W.u.<br />

10 -1 W.u.<br />

S.M. Lenzi - International Workshop on Physics with <strong>AGATA</strong> 19


Forbidden and Irregular E1 transitions<br />

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N=Z<br />

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S.M. Lenzi - International Workshop on Physics with <strong>AGATA</strong> 20


Isospin symmetry and E1 transitions <strong>along</strong> <strong>the</strong> N~Z <strong>line</strong><br />

In <strong>the</strong> validity of<br />

isospin symmetry<br />

1) &KDUJH LQYDULDQFH of <strong>the</strong> QXFOHDU LQWHUDFWLRQ<br />

Possible origin:<br />

E1 ( T=0) transitions are forbidden in N=Z nuclei<br />

E1 transitions in mirror nuclei have identical strength<br />

2) /RQJ ZDYHOHQJWK DSSUR[LPDWLRQ (first term in M 1 (NU) in <strong>the</strong> expansion of <strong>the</strong> E1 operator)<br />

Signatures of symmetry breaking:<br />

forbidden E1’s in N=Z nuclei,<br />

irregular E1 transitions in mirror nuclei<br />

isospin breaking of <strong>the</strong> QXFOHDU LQWHUDFWLRQ<br />

KLJKHU RUGHU WHUPV in <strong>the</strong> series expansion in M1 (NU<br />

- Isospin mixing due to <strong>the</strong> coupling to <strong>the</strong> continuum for nuclei close to <strong>the</strong> proton drip <strong>line</strong><br />

- Isospin mixing of quasi degenerate levels of equal J and different T<br />

- Isospin mixing with <strong>the</strong> IVGMR<br />

S.M. Lenzi - International Workshop on Physics with <strong>AGATA</strong> 21


Isospin mixing due to <strong>the</strong> coupling to <strong>the</strong> IVGMR<br />

even-even nuclei<br />

Hartree Fock spherical<br />

H-F unrestricted<br />

EWSR + IVGMR<br />

Isospin impurity of <strong>the</strong> g.s. due to mixing with <strong>the</strong> Isovector Giant Monopole Resonance.<br />

The calculated mixing increases significantly with A and, for a given A, is maximum for N=Z<br />

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, +DPDPRWR DQG + 6DJDZD 35& 5 S.M. Lenzi - International Workshop on Physics with <strong>AGATA</strong> 22<br />

N=Z<br />

B-M


Forbidden E1 transition in N=Z nuclei<br />

IS � �� G��� Pure E1 non<br />

stretched<br />

The minimum isospin mixing is<br />

( )DUQHD $ *DGHD 1 0 UJLQHDQ HW DO<br />

2 |<br />

α<br />

0.<br />

15%<br />

*H M2/E1<br />

Measured: lifetime, ang. distr. and polarization<br />

The PLQLPXP isospin mixing results<br />

2<br />

α<br />

( )DUQHD HW DO 3/%<br />

2.<br />

3(<br />

1.<br />

4)%<br />

(XUREDOO GDWD<br />

S.M. Lenzi - International Workshop on Physics with <strong>AGATA</strong> 23


Irregular E1 transitions in mirror nuclei<br />

E1: 7/2 - Æ5/2+<br />

7KH HOHFWURPDJQHWLF WUDQVLWLRQ RSHUDWRU FDQ EH H[SUHVVHG LQ WHUPV RI<br />

LVRVFDODU ,6 LW GRHV QRW GHSHQG RQ 7]<br />

LVRYHFWRU ,9 LV OLQHDU LQ 7] FKDQJHV VLJQ LQ HDFK PLUURU<br />

( DPSOLWXGHV LQ PLUURU QXFOHL WKH ,6 FRPSRQHQW YDQLVKHV N5 !!<br />

WKHUHIRUH ( WUDQVLWLRQV ,9 LQ PLUURU QXFOHL PXVW KDYH WKH VDPH VWUHQJWK<br />

+LJKHU RUGHU ,6 DPSOLWXGHV DQG LVRVSLQ PL[LQJ DUH UHVSRQVLEOH<br />

RI DV\PPHWULHV LQWHUIHUHQFH RI UHJXODU ,9 DQG LUUHJXODU DPSOLWXGHV<br />

Lifetime measurements are needed.<br />

- (NPDQ HW DO<br />

35/ LQ SUHVV<br />

4896 (21/2 + )<br />

1390<br />

3506 (17/2 + )<br />

1226<br />

2260 (13/2 + )<br />

915<br />

1365 (9/2 + )<br />

717<br />

648 (7/2 – )<br />

648<br />

0 (5/2 – ) 0 5/2 –<br />

67<br />

34Se33 4950 21/2 +<br />

1358<br />

3592 17/2 +<br />

1228<br />

2364 13/2 +<br />

942<br />

1422 9/2 +<br />

* GH $QJHOLV HW DO<br />

DQDO\VLV LQ SURJUHVV<br />

725<br />

697 7/2 –<br />

697<br />

67<br />

33As34 ,QGXFHG ,VRVFDODU DPSOLWXGH<br />

)LUVW RUGHU HIIHFW<br />

LQ PLUURU QXFOHL<br />

7KH\ FDQ EH PHDVXUHG<br />

S.M. Lenzi - International Workshop on Physics with <strong>AGATA</strong> 24


Conclusions<br />

7KH LVRVSLQ V\PPHWU\ LV VOLJKWO\ EURNHQ LQ LVREDULF PXOWLSOHWV GXH PDLQO\ WR WKH &RXORPE LQWHUDFWLRQ<br />

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(QHUJ\ GLIIHUHQFHV<br />

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¾ 0HFKDQLVP RI QXFOHRQ DOLJQPHQW DW WKH EDFNEHQGLQJ<br />

¾ (YROXWLRQ RI WKH UDGLL DORQJ D URWDWLRQDO EDQG<br />

¾ ,VRVSLQ QRQ FRQVHUYLQJ WHUPV LQ WKH QXFOHDU LQWHUDFWLRQ<br />

([WHQGLQJ WKHVH VWXGLHV WR FURVV VKHOO H[FLWDWLRQV ZH FDQ OHDUQ DERXW<br />

¾ )XUWKHU &RXORPE HIIHFWV<br />

¾ &RQILJXUDWLRQ RI VWDWHV<br />

( WUDQVLWLRQV<br />

6WXG\LQJ ( WUDQVLWLRQV LQ 1 = QXFOHL DQG PLUURUV ZH FDQ OHDUQ DERXW<br />

¾ ,VRVSLQ PL[LQJ<br />

¾ &RXSOLQJ WR *5<br />

¾ ,QGXFHG ,6 WHUPV<br />

¾ &RXSOLQJ WR WKH FRQWLQXXP<br />

with: good spectroscopy and<br />

good SM description<br />

need: good spectroscopy and<br />

good SM description<br />

S.M. Lenzi - International Workshop on Physics with <strong>AGATA</strong> 25


Perspectives with <strong>AGATA</strong><br />

7KHVH LQYHVWLJDWLRQV DUH DW WKH EHJLQQLQJ<br />

+LJK LQWHQVLW\ VWDEOH EHDPV<br />

:H QHHG WR NQRZ WKH OLPLWV RI YDOLGLW\ RI WKH LVRVSLQ V\PPHWU\<br />

¾ get a deeper understanding of nuclear INC term<br />

¾ identify <strong>the</strong> different Coulomb effects<br />

¾ identify <strong>the</strong> origin of isospin mixing<br />

/LJKW DQG PHGLXP OLJKW QXFOHL<br />

¾ N=Z nuclei up to high spin<br />

¾ MED for positive and negative parity states<br />

¾ MED for T > 1<br />

¾ TED measurements<br />

3RZHUIXO VKHOO PRGHO FRGHV<br />

5DGLRDFWLYH EHDPV<br />

$QFLOODU\ GHWHFWRUV WR VHOHFW WKH FKDQQHOV RI LQWHUHVW<br />

+LJK JUDQXODULW\ DQG VHQVLWLYLW\<br />

+LJK HIILFLHQF\ IRU K H -UD\V<br />

�LQHPDWLFDO UHFRQVWUXFWLRQ<br />

IRU 'RSSOHU FRUUHFWLRQ<br />

6RPH HIIHFWV DUH ODUJHU IRU KHDYLHU QXFOHL<br />

¾ higher-order terms in <strong>the</strong> series expansion of M 1 (kr)<br />

¾ isospin mixing<br />

¾ +HDYLHVW SDUWLFOH VWDEOH QXFOHXV ZLWK = 1 LV H[SHFWHG WR EH 6Q<br />

¾ +HDYLHVW SDUWLFOH VWDEOH QXFOHL ZLWK 7 ] DQG 7 ] DUH $J DQG 6H<br />

5HOLDEOH HIIHFWLYH LQWHUDFWLRQV<br />

'HDO ZLWK KLJK UDWHV<br />

=0.2<br />

Detector<br />

Segments<br />

Pulse-shape<br />

analysis and<br />

tracking<br />

F. Recchia, E. Farnea<br />

S.M. Lenzi - International Workshop on Physics with <strong>AGATA</strong> 26


S.M. Lenzi - International Workshop on Physics with <strong>AGATA</strong> 27

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