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Influence of the ni 13/2 orbital on the structure of Tl & 187Os ...13/2 orbital on the structure of...

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Influence of the ni 13/2 orbital on the structure of 197 Tl & 187 Os nuclei S.Nandi 1,2* , G.Mukherjee 1,2 On behalf of VENUS and INGA collaboration 1 Variable Energy Cyclotron Center, Kolkata; 2 HBNI, Training School Complex, Anushaktinagar, Mumbai-400094, India *[email protected] Workshop on Nuclear Astrophysics Opportunities at ATLAS 2019, 12 th -13 th July 2019
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Page 1: Influence of the ni 13/2 orbital on the structure of Tl & 187Os ...13/2 orbital on the structure of 197Tl & 187Os nuclei S.Nandi1,2*, G.Mukherjee1,2 On behalf of VENUS and INGA collaboration

Influence of the ni13/2 orbital on the

structure of 197Tl & 187Os nuclei

S.Nandi1,2*, G.Mukherjee1,2

On behalf of VENUS and INGA collaboration 1Variable Energy Cyclotron Center, Kolkata;

2HBNI, Training School Complex, Anushaktinagar, Mumbai-400094, India

*[email protected]

Workshop on Nuclear Astrophysics Opportunities at ATLAS 2019, 12th -13th July 2019

Page 2: Influence of the ni 13/2 orbital on the structure of Tl & 187Os ...13/2 orbital on the structure of 197Tl & 187Os nuclei S.Nandi1,2*, G.Mukherjee1,2 On behalf of VENUS and INGA collaboration

Outline

Introduction

Active single particle orbitals in mass A~180-200 region

Motivation behind the study of 197Tl, 187Os

Different modes of excitation in 197Tl &187Os based on

ni13/2 orbital

Summary

Page 3: Influence of the ni 13/2 orbital on the structure of Tl & 187Os ...13/2 orbital on the structure of 197Tl & 187Os nuclei S.Nandi1,2*, G.Mukherjee1,2 On behalf of VENUS and INGA collaboration

Introduction

• The neutron rich nuclei with proton

and/or neutron numbers close to the

shell closures are of paramount interest

to understand the r-process nuclear synthesis.

• Observed r-process abundance peak at around A∼ 195 originates from the

waiting point nuclei at N=126 neutron

magic number and the nuclear structure

properties are important to understand nuclear synthesis.

• On the above context, neutron rich Os, and Ir isotopes are important to study.

• Structure of near shell closure nuclei is

important to understand the r –process nuclear synthesis.

Page 4: Influence of the ni 13/2 orbital on the structure of Tl & 187Os ...13/2 orbital on the structure of 197Tl & 187Os nuclei S.Nandi1,2*, G.Mukherjee1,2 On behalf of VENUS and INGA collaboration

The Nucleus

Proton

Neutron

GS

ES Jp

Jp

• Single Particle Excitation

• Collective Excitation

Page 5: Influence of the ni 13/2 orbital on the structure of Tl & 187Os ...13/2 orbital on the structure of 197Tl & 187Os nuclei S.Nandi1,2*, G.Mukherjee1,2 On behalf of VENUS and INGA collaboration

Z=82

N=

126

Neutron (N)

Pro

ton

(Z

)

4He Beam

Page 6: Influence of the ni 13/2 orbital on the structure of Tl & 187Os ...13/2 orbital on the structure of 197Tl & 187Os nuclei S.Nandi1,2*, G.Mukherjee1,2 On behalf of VENUS and INGA collaboration

Motivations

• The isotopes, near the stability line of

heavier nuclei near Z=82, mostly produced

as end products of the b decay of the r-

process elements and the slow neutron

capture.

• The active high j single particle orbitals like

ph11/2, ph9/2, nh9/2, ni13/2 etc. control the

nuclear structural properties in A ~ 190

region.

• Different novel excitations like chiral band,

gamma band, wobbling band are expected

in these nuclei due to the interplay of single

particle and collective degrees of freedom.

• Recently we have studied the excited states

in 197Tl, an odd proton system and 187Os, an

odd neutron system.

• These odd A systems are ideal laboratory to

understand the effects of the single particle

orbitals on the structure of nuclei.

Nilsson Diagrams

Oblate Prolate

Proton

Page 7: Influence of the ni 13/2 orbital on the structure of Tl & 187Os ...13/2 orbital on the structure of 197Tl & 187Os nuclei S.Nandi1,2*, G.Mukherjee1,2 On behalf of VENUS and INGA collaboration

197Tl

• In the isotopic chain of Tl, 197Tl

nucleus lie in between moderately

deformed lighter Tl isotopes and very

less deformed (A>199) Tl isotopes.

• Therefore, the structural information

of 197Tl is very important to

understand the shape evolution of Tl

with neutron number.

• Neutron deficient isotopes show

shape co-existence near ground state

e.g. in 187,189Tl.

• Recently, doubly degenerate chiral

bands have been observed in 194,195Tl.

195Tl: 5-qp Chiral Band

Left- handed Right- handed

Page 8: Influence of the ni 13/2 orbital on the structure of Tl & 187Os ...13/2 orbital on the structure of 197Tl & 187Os nuclei S.Nandi1,2*, G.Mukherjee1,2 On behalf of VENUS and INGA collaboration

187Os

• Os nuclei are the transitional

nuclei lie between prolate

deformed Hf and spherical Pb.

• Os nuclei are known to be g-

soft, e.g-185,186Os.

• g-band observed in 186Os.

• In 187Os (N==111), the neutron

Fermi level lies in the mid

upper region of ni13/2 orbital.

• Coupling of odd-neutron in

ni13/2 with the g-band ?

g.s Band g Band

186Os

186Os

192Pb 182Hf

1

2

3

Page 9: Influence of the ni 13/2 orbital on the structure of Tl & 187Os ...13/2 orbital on the structure of 197Tl & 187Os nuclei S.Nandi1,2*, G.Mukherjee1,2 On behalf of VENUS and INGA collaboration

Experimental details

Reaction: 186W(4He,3n)187Os at 36 MeV

from K-130 cyclotron at VECC Kolkata.

Detector: Indian National Gamma Array

(INGA) Seven CLOVER and one LEPS

Target: A stack of three 186W foils each

300mg/cm2 thick on a 20mg/cm2 12C

backing.

Data Acquisition: 2 fold coincidence data

were recorded using PIXIE -16 digitizer

based system of UGC-DAE-CSR,

Kolkata.

Reaction: 197Au(4He,4n)197Tl at 50

MeV from K=130 cyclotron at VECC

Kolkata.

Detector: VECC Nuclear Spectroscopy

(VENUS) array with six Clover HPGe.

Target: Au target of thickness 5mg/cm2

Data Acquisition: VME based data

acquisition system was used.

90º

90º

90º

90º

125º 125º

40º 40º LEPS

INGA at VECC:

90º

90º

VENUS at

VECC:

197Tl

187Os

Page 10: Influence of the ni 13/2 orbital on the structure of Tl & 187Os ...13/2 orbital on the structure of 197Tl & 187Os nuclei S.Nandi1,2*, G.Mukherjee1,2 On behalf of VENUS and INGA collaboration

New level scheme of 197Tl

3-qp MR

band

pi13/2+1 ni13/2)

-2

ph9/2ni13/2-3 np3/2,f5/2)

5-qp MR

band

S. Nandi, G. Mukherjee et al. Physical Review

C 99, 054312 (2019)

28 new g transitions

Page 11: Influence of the ni 13/2 orbital on the structure of Tl & 187Os ...13/2 orbital on the structure of 197Tl & 187Os nuclei S.Nandi1,2*, G.Mukherjee1,2 On behalf of VENUS and INGA collaboration

Angular

Momentum

coincide with

the principle

axis

DI=2

rotational

band

Angular

Momentum lie

in the principle

plane

Two DI=2

bands

connected

by DI=1

transition

Angular

Momentum lie

in out of plane

Two

DI=1sequence

Case:197Tl

Case:195Tl

Geometrical representation of different band structures

Page 12: Influence of the ni 13/2 orbital on the structure of Tl & 187Os ...13/2 orbital on the structure of 197Tl & 187Os nuclei S.Nandi1,2*, G.Mukherjee1,2 On behalf of VENUS and INGA collaboration

Discussions on 3 & 5 –qp magnetic rotational band

5-qp MR Band

Symmetry axis

Rotational axis

Jp

Jn I

R q

Oblate core

𝑐𝑜𝑠 𝜃 =𝐽2 − 𝐽2𝜋 − 𝐽2𝜈

2𝐽𝜋𝐽𝜈

• I= J+R

• J= Jn+Jp

b2=0.05

3-qp

b2=0.09

Co

un

ts

5-qp

g= -300

Page 13: Influence of the ni 13/2 orbital on the structure of Tl & 187Os ...13/2 orbital on the structure of 197Tl & 187Os nuclei S.Nandi1,2*, G.Mukherjee1,2 On behalf of VENUS and INGA collaboration

MR BAND (3-qp & 5-qp)

ph9/2ni13/2-3 np3/2,f5/2)

V21p-1h =221.8 keV

V21p-1h =587.5 keV

pi13/2+1 ni13/2)

-2

• Input parameters used for SPAC

Page 14: Influence of the ni 13/2 orbital on the structure of Tl & 187Os ...13/2 orbital on the structure of 197Tl & 187Os nuclei S.Nandi1,2*, G.Mukherjee1,2 On behalf of VENUS and INGA collaboration

187Os

Page 15: Influence of the ni 13/2 orbital on the structure of Tl & 187Os ...13/2 orbital on the structure of 197Tl & 187Os nuclei S.Nandi1,2*, G.Mukherjee1,2 On behalf of VENUS and INGA collaboration

Band D

Anomalous signature splitting in high W orbital (Band D)

The band D, based on high-W n11/2+[615]

configuration, has been extended up to

particle alignment and shows large

signature splitting similar to 185Os.

g-softness may be responsible for the

anomalous signature splitting of band D.

Page 16: Influence of the ni 13/2 orbital on the structure of Tl & 187Os ...13/2 orbital on the structure of 197Tl & 187Os nuclei S.Nandi1,2*, G.Mukherjee1,2 On behalf of VENUS and INGA collaboration

0+×11/2+ of ni13/2

2+g×11/2+ of ni13/2

4+g×11/2+ of ni13/2

Estimated gamma

deformation ~ 32º

A S Davydov et al. Nucl. Phys. 8 (1958) 237

1 & 2 g phonon bands

2+g×11/2+ of ni13/2

257

618

894

1382

Page 17: Influence of the ni 13/2 orbital on the structure of Tl & 187Os ...13/2 orbital on the structure of 197Tl & 187Os nuclei S.Nandi1,2*, G.Mukherjee1,2 On behalf of VENUS and INGA collaboration

• 3- and 5-qp bands in 197Tl are MR in nature in contrast to chiral

doublet bands in 195Tl. This implies that as neutron number

moves away from i13/2 orbital in 197Tl (N = 116), the particle-hole

coupling with the core attains a planar, tilted-axis geometry.

• A new level scheme of 187Os, much improved compared to the

known one, has been proposed which reveals many interesting

features of the bands built on different single-particle

configurations (including band crossings).

• Bands corresponding to the coupling of ni13/2 with the 1-phonon

and 2-phonon quanta of the g-band in 186Os have been identified.

• Detailed analysis of 187Os is in progress.

Summary

Page 18: Influence of the ni 13/2 orbital on the structure of Tl & 187Os ...13/2 orbital on the structure of 197Tl & 187Os nuclei S.Nandi1,2*, G.Mukherjee1,2 On behalf of VENUS and INGA collaboration

Acknowledgement

Collaborating institutes

• Saha institute of nuclear physics

• UGC, DAE, CSR, Kolkata

• Presidency College, Kolkata

• GANIL, France

• We would like to thank to our collaborators for their supports.

• We would also thankful to the VECC cyclotron operators for

good quality of α beam throughout the experiment.

• We also acknowledge the efforts of all who has contributed in the

setting up of the VENUS and INGA array.

• We also thank the target lab staff of IUAC, New Delhi for their

help in making the target. The help of Dr. P. Nair and his group is

also acknowledged.

Page 19: Influence of the ni 13/2 orbital on the structure of Tl & 187Os ...13/2 orbital on the structure of 197Tl & 187Os nuclei S.Nandi1,2*, G.Mukherjee1,2 On behalf of VENUS and INGA collaboration

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