structural evolution in the ( n,z,i p ) coordinate frame for a~100

28
Structural Evolution in the ( N,Z,I ) Coordinate Frame for A~100 Paddy Regan* Dept. of Physics University of Surrey,UK E-mail: [email protected]. uk *partially supported by WNSL-Yale Flint and Science Development Fund

Upload: kali

Post on 21-Jan-2016

28 views

Category:

Documents


0 download

DESCRIPTION

Structural Evolution in the ( N,Z,I p ) Coordinate Frame for A~100. Paddy Regan* Dept. of Physics University of Surrey,UK E-mail : [email protected] * partially supported by WNSL-Yale Flint and Science Development Fund. Sr-Mo region ‘famous’ for dramatic collapse in I p =2 + energy - PowerPoint PPT Presentation

TRANSCRIPT

Page 1: Structural Evolution in the ( N,Z,I p ) Coordinate Frame for A~100

Structural Evolution in the (N,Z,I) Coordinate Frame for A~100

Paddy Regan*

Dept. of Physics

University of Surrey,UK

E-mail: [email protected]

*partially supported by WNSL-Yale Flint and Science Development Fund

Page 2: Structural Evolution in the ( N,Z,I p ) Coordinate Frame for A~100

Sr-Mo region ‘famous’ for dramatic collapse in I=2+ energy going from N=58 to N=60

Page 3: Structural Evolution in the ( N,Z,I p ) Coordinate Frame for A~100

Explanation by Federman & Pittel in terms of quadrupoledeformation ‘driving’ T=0 (pn) interaction.

Particularly noticeable forprotons and neutron orbitalswith large spatial overlaps

(e.g., Spin Orbit Partners such as g9/2 and g7/2 in A~100)

Page 4: Structural Evolution in the ( N,Z,I p ) Coordinate Frame for A~100

Other aspects ?Correlation betweendeformation & populationof ‘deformation aligned’,low-h11/2 neutronintruder orbitals.

Classic ‘chicken and egg’.Does population of orbital ‘cause’ deformationor is deformation there from the core and thush11/2 orbital lies closerto the Fermi Surface ?

How does this situationevolve with spin ?

Page 5: Structural Evolution in the ( N,Z,I p ) Coordinate Frame for A~100

Alignment (rotational picture at least) driven by Coriolis interaction on high-j, low- orbitals (ie. ones with large jx on collective rotation axis.

Vcor = -jx.

eg.

h11/2 [550]1/2 ‘intruder’

FS for N~57, 2~0.15->0.2

jx

50

82

[550]1/2-

1h11/2

1g9/2

[541]3/2-

Page 6: Structural Evolution in the ( N,Z,I p ) Coordinate Frame for A~100

= 101Mo,new data,see later

Page 7: Structural Evolution in the ( N,Z,I p ) Coordinate Frame for A~100

Alignments and rotational motion in ‘vibrational’ 106Cd (Z=48, N=58),

PHR et al. Nucl. Phys. A586 (1995) p351

Page 8: Structural Evolution in the ( N,Z,I p ) Coordinate Frame for A~100

Detailed spectroscopy allowed by investigating gamma-decay sequences from high-spin states. YRASTBALL allows triples to show band-like structures in 101Ru.

see A.D.Yamamoto et al., Phys. Rev. C66 (2002) 024302

Page 9: Structural Evolution in the ( N,Z,I p ) Coordinate Frame for A~100

TRS calculations for 101Ru by F.R. Xu (Bejing) for differentparity (and signature) configs.

2

=0.2MeV

=0.4MeV

=0.3MeV

=0.6MeV

A.D.Yamamoto et al. Phys. Rev. C66 (2002) 024302

Page 10: Structural Evolution in the ( N,Z,I p ) Coordinate Frame for A~100

Crossing and alignments well reproduced by CSM, although AHVs see PHR et al., Phys. Rev. C68 (2003) 044313

Page 11: Structural Evolution in the ( N,Z,I p ) Coordinate Frame for A~100

PHR, Beausang, Zamfir, Casten, Zhang et al., Phys. Rev. Lett. 90 (2003) 152502

24

24

2 :Rotor

0 : Vibrator

)2(

242

),1(2

:Rotor

,2

:Vibrator

22

22

J

J

J

n

JR

JR

J

JJER

JEJJE

EJ

nE

Page 12: Structural Evolution in the ( N,Z,I p ) Coordinate Frame for A~100

PHR, Beausang, Zamfir, Casten, Zhang et al., Phys. Rev. Lett. 90 (2003) 152502

Page 13: Structural Evolution in the ( N,Z,I p ) Coordinate Frame for A~100

PHR, Beausang, Zamfir, Casten, Zhang et al., Phys. Rev. Lett. 90 (2003) 152502

Page 14: Structural Evolution in the ( N,Z,I p ) Coordinate Frame for A~100

Vibrator-Rotator phase change is a feature of near stable (green) A~100.

‘Rotational alignment’ can be a crossing between quasi-vibrational GSB & deformed rotational sequence.(stiffening of potential by population of high-j, equatorial (h11/2) orbitals).

PHR, Beausang, Zamfir, Casten, Zhang et al., Phys. Rev. Lett. 90 (2003) 152502

Page 15: Structural Evolution in the ( N,Z,I p ) Coordinate Frame for A~100

Simon et al., Nucl. Inst. Meth. A452, 205 (2000)

BLF

TLF

beam tlftlf

blfblf

Ge

TOF ~5-10 ns.ns-s isomers can de-excite in bestopped by CHICO position detector. Delayeds can still be viewedby GAMMASPHERE.

Rochester Group

Page 16: Structural Evolution in the ( N,Z,I p ) Coordinate Frame for A~100

-1

cos-1

by calculated then is correctionDoppler The

coscoscoscossinsinsinsin)cos(

where

)cos(r.r

by given is angleray -fragment/ the

k )cos( , j )sin()sin( ,i )cos()sin(

k, and j i, rsunit vectoCartesian For

2

2,1'

2121212112

122121

1,2

1,2

EE

rr

rzryrx

z

x

y

Page 17: Structural Evolution in the ( N,Z,I p ) Coordinate Frame for A~100

Use ‘isomer gating’ to identify h11/2 bandin N=59, 101Mo.

{180}{429,616,772,891}

total, DICprompts

delayed

delayed coincs with prompt 429, 616, 772 & 891 keV

891

772

429

616

180

Page 18: Structural Evolution in the ( N,Z,I p ) Coordinate Frame for A~100
Page 19: Structural Evolution in the ( N,Z,I p ) Coordinate Frame for A~100

See PHR, Yamamoto, Beausang, Zamfir, Casten, Zhang et al., AIP Conf. Proc. 656 (2002) p422

‘Weak Coupling’

E/(I-j) E-GOS extension for odd-A

Suggests 11/2- band is an anharmonic vibratoror -soft rotor?

seems to work ok for +ve parity bandsthough

Page 20: Structural Evolution in the ( N,Z,I p ) Coordinate Frame for A~100

case. 0 even)-(even for the toreduces which

22

2

24 by, simplified becan This

24

24

2

24

2

2

2

2

2

22

jI

E

jI

jRER

RKIRjI

jjIE

jIRjI

jE

jI

jI

I

I

I

EIR

jGOSE

j

jII

Wheldon suggested extension of E-GOS by ‘renormalising’ the rotational energies at the bandhead.

If the band-head spin of a sequence is given by j then substituting Ij in place of I, one obtains,

Page 21: Structural Evolution in the ( N,Z,I p ) Coordinate Frame for A~100

seems to work ok, h11/2 bands now look like rotors,

Even-Even yrast sequences and odd-A +ve parity only show rotational behaviour after (h11/2 )2 crossing….

Page 22: Structural Evolution in the ( N,Z,I p ) Coordinate Frame for A~100

Even simpler to just take E(I->!-2) / I for odd-A e.g., R = [ E(15/2- ->11/2-) / (11/2) ]

Page 23: Structural Evolution in the ( N,Z,I p ) Coordinate Frame for A~100

Other signatures of (perfect) vibrators and rotors

State lifetimes, i.e., B(E2) values and selection rules (eg. n=1).

Page 24: Structural Evolution in the ( N,Z,I p ) Coordinate Frame for A~100

Need to measure lifetimesB(E2) values of yraststretched E2 decays in

N=58 isotones (best cases)+ h11/2 bands in N=57isotones.

RDM measurements in 103,4Pd, 105,6Cd due Aug. 2004 at Yale to ‘prove’ vibrator-to-rotor picture.

( Frauendorf’s ‘tidal wave’ picture is similar).

Page 25: Structural Evolution in the ( N,Z,I p ) Coordinate Frame for A~100

From Dudek et al.,Phys. Rev. Lett.59 (1987) p1405

Single particle spectra (for minimised LDMenergy at spin 60 hbar) shows distinct gaps for 2~0.4 at Z=42, N=58 (100Mo).

Note these arethe homologs of A~80 SD (N=42)and A~130 SD (Z=58)

Page 26: Structural Evolution in the ( N,Z,I p ) Coordinate Frame for A~100

• SD (2=0.4) minimum predicted in 100Mo to become yrast around spins 25-30 h.

• ‘Doubly-Magic’ SD shell gaps at (Z=42, N=58) = 100Mo.

J. Skalski et al.,Nucl. Phys. A617 (1997) p282

DIC Pb + Mo proposal to Be submitted to upcomingGAMMASPHERE PAC (deadline 26th April!)

Page 27: Structural Evolution in the ( N,Z,I p ) Coordinate Frame for A~100

P.H. Regan1,2, C. Wheldon1,3, A.D. Yamamoto1,2, S. Ashley1, P. Mumby-Croft1, D. Seaborne1, C.Y. Wu4, A.O. Macchiavelli5,

D. Cline4, J.F. Smith6, R.S. Chakrawarthy6, M. Cromaz5, P. Fallon5, S.J. Freeman6, W. Gelletly1, A. Görgen5, A. Hayes4,

H. Hua4, S.D. Langdown1,2, I.Y. Lee5, C.J. Pearson1, Zs. Podolyák1, R. Teng4, J.J. Valiente-Dobón1,

1University of Surrey, UK2Wright Nuclear Structure Laboratory, Yale University, USA

3HMI, Berlin, Germany4Nuclear Structure Research Laboratory, University of Rochester, USA

5Nuclear Science Division, Lawrence Berkeley National Laboratory, USA6Department of Physics and Astronomy ,The University of Manchester, UK

E-GOS story, PHR, Con Beausang, Victor Zamfir, Rick Casten, Jing-Ye Zhang

Money from…EPSRC (UK) , DOE (USA) , NSF (USA), Yale Flint-Science Development Funds

Acknowledgments

Page 28: Structural Evolution in the ( N,Z,I p ) Coordinate Frame for A~100

International ConferenceOn NUclear STructure, Astrophysics & Reactions University of Surrey, Guildford, UK5-8 January 2005

http://www.ph.surrey.ac.uk/cnrp/nustar05