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Self-consistent description of multipole strength

in exotic nuclei

J. Terasaki, J. Engel, M. Bender, J. Dobaczewski, W. Nazarewicz, and M. Stoitsov

Mar. 31, 2005

http://www.nndc.bnl.gov/nudat2/

Nuclear chart

Z

N

Strength function

∑∑−=

=J

JMkJMk

kJ ELΨFΨES )(ˆ)(

2

0

Lorenzian (

isovector and isoscalar

operator transition

forces pairing type-volume and Skyrme

ion,approximat phase random clequasiparti

state ground

state excited

:)

)(:ˆ

:

:

0

EL

ΩYrF

ΨΨ

k

JMn

JM

k

←⎭⎬⎫

PRC 71, 034310 (2005)

124Sn120Sn 118Sn

116Sn

Cro

ss s

ectio

n [m

b]

Photon energy [MeV]

B.L. Berman and S.C Fultz, Rev.Mod.Phys. 47 (1975) 713 Our calculation (SkM*)

Isovector 1−

Isoscalar 1− strength functions

N=50 82 126

A=100 132 176

Isoscalar 1− strength functions

Isoscalar 1− strength functions

Isoscalar 1− strength functions

Isoscalar 1− strength functions

Isoscalar 1− strength functions

Isoscalar 1− strength functions

Isoscalar 1− strength functions

Isoscalar 1− strength functions

Isoscalar 1− strength functions

Isoscalar 1− strength functions

Isoscalar 1− strength functions

Isoscalar 1− strength functions

Isoscalar 1− strength functions

Isoscalar 1− strength functions

Isoscalar 1− strength functions

Isoscalar 1− strength functions

Isoscalar 1− strength functions

Isoscalar 1− strength functions

Isoscalar 1− strength functions

Isoscalar 1− strength functions

Isoscalar 1− strength functions

Isoscalar 1− strength functions

Isoscalar 1− strength functions

Isoscalar 1− strength functions

Isoscalar 1− strength functions

Isoscalar 1− strength functions

At A = 154 - 162 (N = 104 - 112)ground states : deformed

Isoscalar 1− strength functions

Isoscalar 1− strength functions

Isoscalar 1− strength functions

Isoscalar 1− strength functions

Isoscalar 1− strength functions

Isoscalar 1− strength functions

Isoscalar 1− strength functions

Transition density

0)(ˆ);( ΨrρΨkrρ k p or ntr

p or n =

);()();( 02 krρΩYΩdrkrρ J

trp or n

trp or n ∫=

One-dimensional

↓↓

Transition densities ofa stable nucleus

c.c.+≅−

tωik

tFitFi

eΨrρΨΨrρΨΨerρeΨ

0

000)(ˆ)(ˆ

0

)(ˆ)(ˆ)(ˆ

Near neutron drip line

Recent experimental studies near 132Sn

D.C. Radford et al. Phys.Rev.Lett. 88 (2002) 222501,D.C. Radford, talk at conf. “Exotic Nuclei and Atomic Masses 2004”

Measurement of 1− strength of 132Sn is in progress at GSI.

Summary

• Strength functions of even Sn isotopes have beeninvestigated from the proton drip line to neutron drip line.

1. Strength of Isoscalar 1− mode increases dramaticallyin a low-energy region as N approaches the neutrondrip line.

2. The state of the low-energy peak looks like a “neutron-skin oscillation” or continuum-energy state.

• We can obtain isoscalar 1− solutions accurately without contamination of the center-of-mass motion.