Shape Isomerism in 66 Ni S. Leoni, B. Fornal, N. Marginean, M. - - PowerPoint PPT Presentation

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Shape Isomerism in 66 Ni S. Leoni, B. Fornal, N. Marginean, M. - - PowerPoint PPT Presentation

Shape Isomerism in 66 Ni S. Leoni, B. Fornal, N. Marginean, M. Sferrazza, Y. Tsunoda, T. Otsuka, et al., University of Milano and INFN sez. Milano, Italy IFJ-PAN, The Ins=tute of Nuclear Physics, Krakow, Poland IFIN HH, Bucharest,


slide-1
SLIDE 1

“Shape Isomerism in 66Ni”

  • S. Leoni, B. Fornal, N. Marginean, M. Sferrazza,
  • Y. Tsunoda, T. Otsuka, et al., …

University of Milano and INFN sez. Milano, Italy IFJ-PAN, The Ins=tute of Nuclear Physics, Krakow, Poland IFIN HH, Bucharest, Romania Departement de Physique, Universite libre de Bruxelles, Belgium Center for Nuclear Study, University of Tokyo, Japan

slide-2
SLIDE 2

Outline

  • Introduction

isomers in molecular chemistry

  • Atomic nucleus

shell structure, deformation, potential energy surpace (PES)

  • Discovery of nuclear fission (shape) isomers
  • Experimental search for shape coexistence/shape isomers
  • The unique case of 66Ni
  • Relevance for THEORY – SHELL Model

MICROSCOPIC origin of Nuclear Deformation

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SLIDE 3

In chemistry, an isomer is a molecule with the same molecular formula as another molecule, but with different arrangement of the atoms.

Subgroup: stereoisomers or spa=al isomers Sub-subgroup: conforma=onal isomers (conformers) Sub-sub-subgroup: rotamers

ISOMERS in chemistry

slide-4
SLIDE 4

Rotation about single bond of butane

Butane molecule C4H10

Conformational isomers

C C C C

C C C C CH3 H H CH3 H H 60°

rotation

CH3 H H CH3 H H

Free energy diagram of butane

as a function of dihedral angle

free energy

60°

rotation

slide-5
SLIDE 5

Potential energy surface (PES) of a nucleus

0.0 0.2 0.1 0.3

1 2 3

  • 0.2
  • 0.3
  • 0.1

4 5

ONE-dimensional representation

ENERGY

TWO-dimensional contour Spheroidal Deforma<on β

)] , ( 1 [ ) , (

,

ϕ θ ϕ θ

lm m l lmY

a R R

+ =

γ β cos

20 =

a

γ β sin ) 2 1 (

22 =

a

β > 0 β < 0

Z Z

Parametriza<on

  • f the NUCLEAR SHAPE

If we consider only quadrupole deforma<on

slide-6
SLIDE 6

Where do we find secondary minima in the nuclear chart considering only sta<c deforma<on ?

(no addi=onal degree of freedom involved … angular momentum, excita=ons …)

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SLIDE 7

Already in 1953, Hill and Wheeler discussed possible consequences of the existence of two well separated minima in the potential energy surface for the ground state of the system. 1953

Cigare form becoms stable

slide-8
SLIDE 8

8 2 2 8 20 28 50 82 28 20 50 126 82

1961 - discovery of the first spontaneously fissioning isomer in 242Am with a half-life 14 msec

  • C. M. Polikanov et al., Zh. Eksp. Teor. Fiz. 42, 1464

(1962) [Sov. Phys.- JETP 15, 1016 (1962)].

slide-9
SLIDE 9

1968 1973

Liquid Drop Model

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SLIDE 10

Shape isomers in actinides

  • HIGH Poten<al BARRIER
  • Nucleus trapped In the second minimum
  • Spontaneous fission from the second minimum

8 2 2 8 20 28 50 82 28 20 50 126 82

TWO EXCEPTIONS

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SLIDE 11

SHAPE ISOMERS very peculiar metastable states

  • HIGH Poten<al BARRIER
  • Nucleus trapped In the minimum
  • very retarded photon decay (107 hindrance)

Can OTHER (lighter) nuclei exhibit these features ?

γ

236,238U

95% 5% B(E2)=1.54 x10-7 W.u. !!!

Structures living in “separate worlds”

MAIN FINGER PRINT: hindrance

  • f deexciSng transiSons
slide-12
SLIDE 12

SEARCH for SHAPE ISOMERS in LIGHTER nuclei:

  • MOST CLEAR-CUT cases of SHAPE Coexistence
  • a PROBE of MICROSCOPIC origin of nuclear deforma<on

within a pure SHELL Model Approach

(Ac<nides are NOT doable by SHELL Model …)

Ideal Cases are 0+ states – to avoid ambiguity given by spin effects

slide-13
SLIDE 13

8 2 2 8 20 28 50 82 28 20 50 126 82

SHAPE Coexistence in Atomic Nuclei

Appearence of different shapes at low excitaSon energy

  • K. Heyde and J. L. Wood, Rev. Mod. Phys. 83, 1467 (2011)

Through the last 40 years of experimental acSviSes, the concept has evolved:

186Pb

Oblate Prolate Spherical

0+

1

0+

2

0+

3

  • A. Andreyev et al., Nature 405 (2000) 430

1) exo<c rarity (1970’) 2) islands of occurrence (1990’) 3) current believe: occurrence in all (but the lightest) nuclei

Shape Isomers in acSnides

Polikanov - 1973

70Ni

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SLIDE 14

0.0 0.0 0.2 0.1 0.3 0.1 0.2 0.3 0.4

235U target 241Pu target

N=82 Z=50 Z=28 N=50

N=60 100Zr 98Sr 0+ 2+ 0+ B(E2) 93 W.u. 102Mo B(E2) 69 W.u. 0+ 2+ 0+ 100Zr

B(E2) 63 W.u.

0+ 2+ 0+

slide-15
SLIDE 15
  • E. Clément, M. Zielińska et al.,

Phys.Rev. Lej. 116, 022701 (2016)

B(E2)=16 W.u.

235U target 241Pu target

N=82 Z=50 N=50

N=60

96Sr 98Sr B(E2)=93 W.u.

No retardaSon in γ decay is observed !!!! Poten<al barrier NOT sizable enough to prevent fast shape changes

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SLIDE 16

Macro-Microscopic Model – P. Moeller et al. 2012

Global Calculation Searching for Nuclear Shape Isomers

Study of 7206 nuclei from A=31 to A=209

Ni

actinides

66Ni

1989

PredicSons for SHAPE ISOMERS - Mean Field Based

64Cr 66Fe

66Ni

68Ni 72Zn Energy of second minimum

Barrier hight Microscopic Hartree-Fock plus BCS calculations

1989

64Ni 68Ni 66Ni

2012

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SLIDE 17

PredicSons for SHAPE ISOMERS – SHELL Model Based state-of-the-art SHELL Model: possible for A <= 100

new calcula<ons scheme, very powerfull computer

Monte Carlo SHELL Model (T. Otsuka’s Group – K computer 106 processors)

66Ni – 78Ni: FULL pf + g9/2 + d5/2 for both neutrons and protons

Inves<ga<on of MICROSCOPIC NATURE - wave func<ons, B(Eλ/Mλ), …

66Ni 68Ni

N=40

70Ni

Z=28

78Ni

N=50

  • Y. Tsunoda et al., PRC 89 (2014) 031301R

64Ni

stable

[Otsuka group and Nowacki, Lenzi, Poves, …]

66Ni 68Ni

  • blate

spherical prolate

70Ni

  • blate

spherical prolate

slide-18
SLIDE 18

Experimentally … No retardaSon is found in 68Ni and 70Ni

2.4 W.u. 7 W.u.

  • B. P. Crider et al., Phys. LeP. B 763, 108 (2016)

70Ni 68Ni

prolate spherical

  • blate

prolate spherical

B(E2) B(E2)

slide-19
SLIDE 19

64Cr 66Fe

66Ni

68Ni 72Zn

Energy of second minimum Barrier hight

66Ni 66Ni

PredicSons of four models à shape isomerism in 66Ni

Macro-Microscospic Model Microscopic Hartree-Fock plus BCS Microscopic Hartree-Fock-Bogoliubov Monte Carlo Shell Model

2012 1989 66Ni 1989 2016

slide-20
SLIDE 20

0.006 W.u. 0.01 W.u. 4.1 W.u.

MONTE CARLO SHELL MODEL Calculations

  • Y. Tsunoda and T. Otsuka, Univ. of Tokyo

66Ni

prolate spherical spherical

  • blate

0+4 0+3 0+2 0+1

Detailed Microscopic Inves<ga<on:

  • Wave func<ons
  • B(Eλ/Mλ), …

8 2 2 8 20 28 50 82 28 20 50 126 82

State-of-the-art Shell Model calculations possible by employing new calculations schemes and very powerful computing systems

(K computer -106 processors)

FULL pf + g9/2 + d5/2 for both neutrons and protons

slide-21
SLIDE 21

0.006 W.u. 0.01 W.u. 4.1 W.u.

MONTE CARLO SHELL MODEL Calculations

  • Y. Tsunoda and T. Otsuka, Univ. of Tokyo

66Ni

prolate spherical spherical

  • blate

0+4 0+3 0+2 0+1

A quadruplet of 0+ states !!!!

Circles:

MCSM basis vectors projected on PES

(T-Plot)

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SLIDE 22
  • R. Broda et al., Phys. Rev. C 86, 064312 (2012)

0+4 0+3 0+2 (t,p) 0+1

Monte Carlo SHELL Model

prolate spherical spherical

  • blate

0+4 0+3 0+2 0+1

0.006(7) W.u. 0.15(2) W.u. 1.53(9) W.u. 0.0025(4) W.u. 1.12(9) W.u. 0.0028 5.9 0.07 0.0024 0.74

B(E2/M1) (from our Bucharest EXP) Excited states energies à One-to-one correspondence (including 0+ states !) à very well reproduced !!

Decay Scheme of 66Ni

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SLIDE 23

Iβ(%) log(l)

EXP

3.1(6) 29(3) 5(1) 63(4) 5.3(2) 4.4(1) 5.5(4) 4.8(1) log(l)

MCSM

4.3 4.1 5.6 4.5 General agreement with β-decay branches

66Feà 66Co à 66Ni

model predicSons:

popula<on of 0+ and 2+ spherical states from spherical 66Co g.s

Monte Carlo SHELL Model

prolate spherical spherical

  • blate

0+4 0+3 0+2 0+1

β-decay populaSon of 66Ni

  • D. Pauwels, P. Van Duppen et al., ARIS-2011 Conference
slide-24
SLIDE 24

N=40 Z=28

66Ni 64Ni

Our Bucharest Experiment (@IFIN HH)

18O + 64Ni à 16O + 66Ni (2n Transfer - 1 MeV below Coulomb Barrier)

18O (39 MeV) 64Ni

σ(66Ni) ≈ few mb - FUSION strongly suppressed

  • PLUNGER - 12 distances

From 10 to 3000 µm

v/c ≈ 2.2 % TOF of 155 ps in 1 mm

ROSPHERE

14 HPGe - 1.1% eff 11 LaBr3(Ce) - 1.75% eff

  • THICK Target – 5 mg/cm2

> 1.5 month

30 pnA beam current

γ

66Ni

16O

γ

slide-25
SLIDE 25

1018

THICK TARGET, gate: 1425 keV

1245

2974

0+

4

1549

gate: 1425 keV

1018 1245

66Ni

1425 2971 3+ 1546 THICK TARGET

2+ 0+

3

2671 2443

0+

2

1018 1245

1425

0+

1

1245

(t,p)

77 – 465 ps 1.5 – 15 ps

1245 1018

18O+64Ni à16O+66Ni

Ebeam = 39 MeV

2n transfer below Coulomb Barrier at IFIN HH Bucarest

1245

77 – 465 ps

All transi<ons belong to 66Ni !!

1.4 ps

(DSAM)

slide-26
SLIDE 26

1018

THICK TARGET, gate: 1425 keV

1245

2974

0+

4

1549

gate: 1425 keV

1018 1245

66Ni

1425 2971 3+ 1546 THICK TARGET

2+ 0+

3

2671 2443

0+

2

1018 1245

1425

0+

1

1245

(t,p)

77 – 465 ps 77 – 465 ps 1.5 – 15 ps

1245 1245 1018

2974

0+

4

1549

18O+64Ni à16O+66Ni

Ebeam = 39 MeV

2n transfer below Coulomb Barrier at IFIN HH Bucarest

All transi<ons belong to 66Ni !!

1.4 ps

(DSAM)

slide-27
SLIDE 27

134(9) ps 7.6(8) ps 20(7) ps

2974

0+4

1549

66Ni

1425 2971 3+ 1546

2+ 0+3

2671 2443

0+2

1018 1245

1425

0+1

0.006 W.u. 0.01 W.u. 4.1 W.u.

prolate spherical spherical

  • blate

0+4 0+3 0+2 0+1

1245 2671

slide-28
SLIDE 28

2974

0+4

1549

66Ni

1425 2971 3+ 1546

2+ 0+3

2671 2443

0+2

1018 1245

1425

0+1

0.006 W.u. 0.01 W.u. 4.1 W.u.

!!!!!!!!!!!!!

B(E2) ~ 0.2 Wu B(E2) = 0.1 Wu B(E2) = 4.3 Wu

prolate spherical spherical

  • blate

0+4 0+3 0+2 0+1

2 TRANSITIONS BELOW 1 W.u. !!!!

1245 2671

slide-29
SLIDE 29

2974

0+4

1549

66Ni

1425 2971 3+ 1546

2+ 0+3

2671 2443

0+2

1018 1245

1425

0+1

0.006 W.u. 0.01 W.u. 4.1 W.u.

B(E2) ~ 0.2 Wu B(E2) = 0.1 Wu B(E2) = 4.3 Wu

prolate spherical spherical

  • blate

0+4 0+3 0+2 0+1

1245 2671

0+

3 is spherical (very similar to 0+ 1): HINDRANCE due to cancellaSon of matrix elements

à independent measurement of τ(0+

3) at ISOLDE - B. Olaizola, L. Fraile et al., PRC95, 061303(R) (2017)

Shell Model with LNPS interac=on – A. Poves and F. Nowacki

PROTON NEUTRON

0+4 0+4 0+3 0+3 0+2 0+2 0+1 0+1

2 TRANSITIONS BELOW 1 W.u. !!!!

slide-30
SLIDE 30

2974

0+4

1549

66Ni

1425 2971 3+ 1546

2+ 0+3

2671 2443

0+2

1018 1245

1425

0+1

0.006 W.u. 0.01 W.u. 4.1 W.u.

B(E2) ~ 0.2 Wu B(E2) = 0.1 Wu B(E2) = 4.3 Wu

prolate spherical spherical

  • blate

0+4 0+3 0+2 0+1

1245 2671

0+

4 is prolate: HINDRANCE due to shape change through high poten<al barrier !!!! SHAPE ISOMER Like !!

PROTON NEUTRON

0+4

NEUTRON PROTON

0+4 0+3 0+3 0+2 0+2 0+1 0+1

2 TRANSITIONS BELOW 1 W.u. !!!!

slide-31
SLIDE 31

0.006 W.u. 0.01 W.u. 4.1 W.u.

prolate spherical spherical

  • blate

0+4 0+3 0+2 0+1

0+

4 is prolate: HINDRANCE due to shape change through high poten<al barrier !!! SHAPE ISOMER Like !!

PROTON NEUTRON

0+4

NEUTRON PROTON

0+4 0+3 0+3 0+2 0+2 0+1 0+1

reduced proton spin-orbit spli`ng

d5/2 s1/2 f5/2

WITHIN the SAME nucleus

change of major configura=ons: sizable excita=ons of ν in g9/2

STABILIZATION

  • f DEFORMED

Local Minima ê SHAPE COEXISTENCE

Type II SHELL EvoluSon (tensor force)

slide-32
SLIDE 32

66Ni:

lightest and unique example

  • apart from the ac=nides –
  • f 0+ deformed state deexci<ng

via HINDERED γ transi<on

a SHAPE-ISOMER-like structure !!!!

** Thank You for the Attention **

A probe of TYPE II SHELL EvoluSon:

rearrengement of nucleons in orbitals causes emergence of deforma<on

BORMIO

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SLIDE 33

PRIZES for Young Speakers

  • ffered by CAEN

Organizers: A. Bracco, F. Camera, G. Colò, S. Leoni;

  • Scient. Secretaries: F. Crespi, X. Roca-Maza

Deadline for ABSTRACT Submission 20 Sep. 2017 E-mail: wsbormio-milano@mi.infn.it

Web-Page: http://www.mi.infn.it/WSBormio-Milano2018/