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1 Nuclear Structure 2016 – Knoxville, TN, USA July 24-29, 2016 Office of Science The 30 Mg(t, p) 32 Mg “Puzzle” Revisited

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Page 1: The Mg(t, p) Mg “Puzzle” Revisited · Nuclear Structure 2016 – Knoxville, TN, USA! July 24-29, 2016! Office of Science Outline! Short Introduction The 30Mg(t,p)32Mg Reaction

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Nuclear Structure 2016 – Knoxville, TN, USA!July 24-29, 2016!

Office of Science

The 30Mg(t, p)32Mg “Puzzle” Revisited!

Page 2: The Mg(t, p) Mg “Puzzle” Revisited · Nuclear Structure 2016 – Knoxville, TN, USA! July 24-29, 2016! Office of Science Outline! Short Introduction The 30Mg(t,p)32Mg Reaction

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Nuclear Structure 2016 – Knoxville, TN, USA!July 24-29, 2016!

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Outline!

Short Introduction

The 30Mg(t,p)32Mg Reaction Fortune’s analysis The “Puzzle” Revisited Three-level Mixing

Energies, wavefuntions, and cross-sections Summary

Page 3: The Mg(t, p) Mg “Puzzle” Revisited · Nuclear Structure 2016 – Knoxville, TN, USA! July 24-29, 2016! Office of Science Outline! Short Introduction The 30Mg(t,p)32Mg Reaction

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Nuclear Structure 2016 – Knoxville, TN, USA!July 24-29, 2016!

Office of Science

“Classic”  magic  numbers  are  generally  correct  only  for  stable  and  near  stable  isotopes    Experimental  studies  of  new  exo:c  isotopes  has  provided  insight  on  the  important  role  play  by  the  tensor  and  3-­‐body  forces  in  the  changes  in  shell  structure  and  collec:vity:        A  delicate  balance  between  the  monopole  field  and  correla3ons.  

Evolu:on  of  Shell  Structure  and  Collec:vity  R.V.F  Janssens,    Nature,  Vol.  435,  2005.

Page 4: The Mg(t, p) Mg “Puzzle” Revisited · Nuclear Structure 2016 – Knoxville, TN, USA! July 24-29, 2016! Office of Science Outline! Short Introduction The 30Mg(t,p)32Mg Reaction

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Nuclear Structure 2016 – Knoxville, TN, USA!July 24-29, 2016!

Office of Science

“Classic”  magic  numbers  are  generally  correct  only  for  stable  and  near  stable  isotopes    Experimental  studies  of  new  exo:c  isotopes  has  provided  insight  on  the  important  role  play  by  the  tensor  and  3-­‐body  forces  in  the  changes  in  shell  structure  and  collec:vity:        A  delicate  balance  between  the  monopole  field  and  correla3ons.  

Evolu:on  of  Shell  Structure  and  Collec:vity  R.V.F  Janssens,    Nature,  Vol.  435,  2005.

N=20  Island  of  Inversion  

32Mg,  at  the  center  of  this  region,  has  been  a  subject  of  intense  work  for  many  years,  both  experimental  and  theore3cal.        à  Much  evidence  has  been  obtained  for  the  existence  of  deformed  ground  states.      

Page 5: The Mg(t, p) Mg “Puzzle” Revisited · Nuclear Structure 2016 – Knoxville, TN, USA! July 24-29, 2016! Office of Science Outline! Short Introduction The 30Mg(t,p)32Mg Reaction

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Nuclear Structure 2016 – Knoxville, TN, USA!July 24-29, 2016!

Office of Science

“Classic”  magic  numbers  are  generally  correct  only  for  stable  and  near  stable  isotopes    Experimental  studies  of  new  exo:c  isotopes  has  provided  insight  on  the  important  role  play  by  the  tensor  and  3-­‐body  forces  in  the  changes  in  shell  structure  and  collec:vity:        A  delicate  balance  between  the  monopole  field  and  correla3ons.  

Evolu:on  of  Shell  Structure  and  Collec:vity  R.V.F  Janssens,    Nature,  Vol.  435,  2005.

N=20  Island  of  Inversion  

32Mg,  at  the  center  of  this  region,  has  been  a  subject  of  intense  work  for  many  years,  both  experimental  and  theore3cal.        à  A  clear  fingerprint  :    Rota3onal  ground  state  band      

Cf.      Heather  Crawford’s  talk

Page 6: The Mg(t, p) Mg “Puzzle” Revisited · Nuclear Structure 2016 – Knoxville, TN, USA! July 24-29, 2016! Office of Science Outline! Short Introduction The 30Mg(t,p)32Mg Reaction

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Nuclear Structure 2016 – Knoxville, TN, USA!July 24-29, 2016!

Office of Science

The 30Mg(t,p)32Mg reaction!

Page 7: The Mg(t, p) Mg “Puzzle” Revisited · Nuclear Structure 2016 – Knoxville, TN, USA! July 24-29, 2016! Office of Science Outline! Short Introduction The 30Mg(t,p)32Mg Reaction

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Nuclear Structure 2016 – Knoxville, TN, USA!July 24-29, 2016!

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The 30Mg(t,p)32Mg reaction!

E(02+) = 1058(2) keV!

!σ(g.s.) = 10.5(7) mb!σ(02

+) = 6.5(5) mb !!σ(02

+)/σ(g.s.) = 0.62(6)!

Page 8: The Mg(t, p) Mg “Puzzle” Revisited · Nuclear Structure 2016 – Knoxville, TN, USA! July 24-29, 2016! Office of Science Outline! Short Introduction The 30Mg(t,p)32Mg Reaction

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Nuclear Structure 2016 – Knoxville, TN, USA!July 24-29, 2016!

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The 30Mg(t,p)32Mg “puzzle”!

| 0gs+ >=α | sph > +β | def >

α 2 ≈ 0.8 β 2 ≈ 0.2

Page 9: The Mg(t, p) Mg “Puzzle” Revisited · Nuclear Structure 2016 – Knoxville, TN, USA! July 24-29, 2016! Office of Science Outline! Short Introduction The 30Mg(t,p)32Mg Reaction

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Nuclear Structure 2016 – Knoxville, TN, USA!July 24-29, 2016!

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A paradigm shift: 2-Level to 3-Level Mixing J!

Guided by shell model we consider the need for 3 configurations to describe the low-energy structure in 32Mg.!

Caurier,  Nowacki,  Poves  PRC  90,  0914302  (2014).  -­‐-­‐  SDPF-­‐U-­‐MIX  interac3on  

Page 10: The Mg(t, p) Mg “Puzzle” Revisited · Nuclear Structure 2016 – Knoxville, TN, USA! July 24-29, 2016! Office of Science Outline! Short Introduction The 30Mg(t,p)32Mg Reaction

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!Construct a mixing matrix of the form:!!!!!!!!Take e0 (0p0h) = 1.4 MeV, e2 (2p2h) = 0.2 MeV, and e4 (4p4h) = 0.0 MeV.!!Diagonalize to extract energies and 0+ wavefunctions of the form:!

3-Level Mixing!

Page 11: The Mg(t, p) Mg “Puzzle” Revisited · Nuclear Structure 2016 – Knoxville, TN, USA! July 24-29, 2016! Office of Science Outline! Short Introduction The 30Mg(t,p)32Mg Reaction

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Diagonalization Solution!

•  Constrain Vmixing by matching to experimental E(02+) = 1058(2) keV!

Page 12: The Mg(t, p) Mg “Puzzle” Revisited · Nuclear Structure 2016 – Knoxville, TN, USA! July 24-29, 2016! Office of Science Outline! Short Introduction The 30Mg(t,p)32Mg Reaction

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Diagonalization Solution!

 SDPF-­‐U-­‐MIX  interac3on  

Page 13: The Mg(t, p) Mg “Puzzle” Revisited · Nuclear Structure 2016 – Knoxville, TN, USA! July 24-29, 2016! Office of Science Outline! Short Introduction The 30Mg(t,p)32Mg Reaction

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Nuclear Structure 2016 – Knoxville, TN, USA!July 24-29, 2016!

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Page 14: The Mg(t, p) Mg “Puzzle” Revisited · Nuclear Structure 2016 – Knoxville, TN, USA! July 24-29, 2016! Office of Science Outline! Short Introduction The 30Mg(t,p)32Mg Reaction

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Cross-Section Analysis!

Page 15: The Mg(t, p) Mg “Puzzle” Revisited · Nuclear Structure 2016 – Knoxville, TN, USA! July 24-29, 2016! Office of Science Outline! Short Introduction The 30Mg(t,p)32Mg Reaction

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32Mg:!

T0,2 & T2,4! T0,0 & T2,2!

Cross-Section Analysis!

Page 16: The Mg(t, p) Mg “Puzzle” Revisited · Nuclear Structure 2016 – Knoxville, TN, USA! July 24-29, 2016! Office of Science Outline! Short Introduction The 30Mg(t,p)32Mg Reaction

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Cross-Section Ratio and the 30Mg Wavefunction!

V [MeV]0.2 0.3 0.4 0.5 0.6 0.7 0.8

Mg

|0p0

h> F

ract

ion

30

0.8

0.9

1 + 10m/ + 20

m

00.10.20.30.40.50.60.70.80.91•  Constrain the 30Mg ground

state wavefunction based on the cross-section ratio !

σ(02+)/σ(g.s.) = 0.62(6)!

•  32Mg is dominated by 2p2h and 4p4h components (>95%) while 30Mg is predominantly 0p0h, in agreement with experiment !

(W. Schwerdtfeger et al., Phys. Rev. Lett. #103, 012501 (2009).)!

!

Page 17: The Mg(t, p) Mg “Puzzle” Revisited · Nuclear Structure 2016 – Knoxville, TN, USA! July 24-29, 2016! Office of Science Outline! Short Introduction The 30Mg(t,p)32Mg Reaction

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Nuclear Structure 2016 – Knoxville, TN, USA!July 24-29, 2016!

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Sum Rule!

V  (MeV)  

Total  

Page 18: The Mg(t, p) Mg “Puzzle” Revisited · Nuclear Structure 2016 – Knoxville, TN, USA! July 24-29, 2016! Office of Science Outline! Short Introduction The 30Mg(t,p)32Mg Reaction

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A Spectrum of Solutions!

•  Shell model prefers a 30Mg ground state more consistent with 80% 0p0h – within 3-level model small modifications to the initial e0, e2 and e4 can yield a consistent solution sets!

3-level model robustly confirms 2p2h/4p4h dominated 32Mg, at the center of the Island of Inversion !

Page 19: The Mg(t, p) Mg “Puzzle” Revisited · Nuclear Structure 2016 – Knoxville, TN, USA! July 24-29, 2016! Office of Science Outline! Short Introduction The 30Mg(t,p)32Mg Reaction

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A comment on the mixing matrix elements!

< 0p0h |V | 2p2h >=< 2p2h |V | 4p4h >=V

Page 20: The Mg(t, p) Mg “Puzzle” Revisited · Nuclear Structure 2016 – Knoxville, TN, USA! July 24-29, 2016! Office of Science Outline! Short Introduction The 30Mg(t,p)32Mg Reaction

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Nuclear Structure 2016 – Knoxville, TN, USA!July 24-29, 2016!

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A comment on the mixing matrix elements!

< 0p0h |V | 2p2h >=< 2p2h |V | 4p4h >=V

< npnhJ |V | (n+ 2)p(n+ 2)hJ >∝< 0p0h0+ |V | 2p2h0+ >

< 2p2h |V | 4p4h >≈< 0p0h |V | 2p2h > /2Gerace  and  Green,    NPA  93,  110  (1967)  

Page 21: The Mg(t, p) Mg “Puzzle” Revisited · Nuclear Structure 2016 – Knoxville, TN, USA! July 24-29, 2016! Office of Science Outline! Short Introduction The 30Mg(t,p)32Mg Reaction

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A comment on the mixing matrix elements!

Page 22: The Mg(t, p) Mg “Puzzle” Revisited · Nuclear Structure 2016 – Knoxville, TN, USA! July 24-29, 2016! Office of Science Outline! Short Introduction The 30Mg(t,p)32Mg Reaction

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Nuclear Structure 2016 – Knoxville, TN, USA!July 24-29, 2016!

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A comment on the mixing matrix elements!

Page 23: The Mg(t, p) Mg “Puzzle” Revisited · Nuclear Structure 2016 – Knoxville, TN, USA! July 24-29, 2016! Office of Science Outline! Short Introduction The 30Mg(t,p)32Mg Reaction

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Inclusion  of  the  third  state,  namely  4p4h  configura:on  resolves  the  “puzzle”  of  32Mg  discussed  by  Fortune,  and  the  ground  state  emerges   naturally   as   dominated   at   the   95%   level   by   intruder  (2p2h  and  4p4h)  configura:ons.      Within   a   simple   three-­‐level   model,   self-­‐consistent   solu:ons  exist   that   provide   good   agreement   with   the   experimental  excita:on   energy   of   the   0+2   state,   the   cross-­‐sec:on   ra:o   and  the   summed   cross-­‐sec:ons   with   a   reasonable   value   for   the  cross-­‐sec:on  for  transfer  of  two  sd  neutrons.      These  scenarios  also  indicate  a  30Mg  ground-­‐state  dominated  by  the   0p0h   component,   in   line   with   experimental   evidence   and  shell-­‐model  expecta:ons  .  

Summary!

Page 24: The Mg(t, p) Mg “Puzzle” Revisited · Nuclear Structure 2016 – Knoxville, TN, USA! July 24-29, 2016! Office of Science Outline! Short Introduction The 30Mg(t,p)32Mg Reaction

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This  material  is  based  upon  work  supported  by  the  U.S.  Department  of  Energy,  Office    of  Science,  Office  of  Nuclear  Physics  under  Contract  No.  DE-­‐AC02-­‐05CH11231  (LBNL),  by  the  U.S.   NSF  Grant  No.   PHY-­‐1404442,   and   by   the   Spanish  Ministry   of   Ciencia   e   Innovacion  under   Grant   FPA2014-­‐57196   and   Program   Centros   de   Excelencia   Severo   Ochoa   -­‐  SEV-­‐2012-­‐0249.  

Acknowledgements!