Fusion hindrance and SHE D. Boilley GANIL and Univ. Caen CEA, - - PowerPoint PPT Presentation

fusion hindrance and she
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Fusion hindrance and SHE D. Boilley GANIL and Univ. Caen CEA, - - PowerPoint PPT Presentation

Fusion hindrance and SHE D. Boilley GANIL and Univ. Caen CEA, Saclay: On the prediction for the SHE production RCNP, Osaka: B. Giraud ( ) Yasuhisa Abe GANIL, Caen: ( )


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SLIDE 1

On the prediction for the SHE production Kazimierz Dolny, Sept. 20011

Fusion hindrance and SHE

 CEA, Saclay:

 B. Giraud

 GANIL, Caen:

 Anthony Marchix  Yoann Lallouet

 Ankara university:

 Bülent Yilmaz 

RCNP, Osaka:

(大阪大学核物理研究センター)

Yasuhisa Abe

(阿部恭久) 

Huzhou Teachers’ College:

(湖州师范学院)

Caiwan Shen

(沈彩万)

  • D. Boilley

GANIL and Univ. Caen

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SLIDE 2

On the prediction for the SHE production Kazimierz Dolny, Sept. 20011

Questions for theoreticians

 Can we guide the experiments ?  What is the shell correction energy ?  Models cannot be extrapolated from

lighter systems

 Fusion hindrance

 Extremely low cross sections

 Few data with few information

Difficulties

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SLIDE 3

On the prediction for the SHE production Kazimierz Dolny, Sept. 20011

Blocking technique in crystals

 Introduction

 Premier point

 Chapitre 1

 Section 1

 …

  • F. Goldenbaum et al.,

PRL 82 (1999) 5012

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SLIDE 4

On the prediction for the SHE production Kazimierz Dolny, Sept. 20011

Direct evidence for long fission times

Quasi-elastic (target)

  • M. Morjean et al, Eur. Phys. J. D45 (2007) 27

& PRL101, 072701 (2008)

Z = 124 A = 312 At least 12 % of the capture events with a life time longer than 10-18 s Z = 120 A = 296 At least 10 % of the capture events with a life time longer than 10-18 s Z = 114 A = 282 Very low statistic or no events with a life time longer than 10-18 s Fission barriers

From P. MÖLLER et al.,

  • At. Dat. And Nucl. Dat. Tab.

59 (1995) 185

Mesurements at GANIL by crystal blocking techniques

1f 1021s

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SLIDE 5

On the prediction for the SHE production Kazimierz Dolny, Sept. 20011

KEWPIE 2 Main ingredients

 Formalism:

 Weisskopf or Hauser-

Feshbach

 Bohr-Wheeler

 Level density:

 Bohr-Mottelson with

angular dependence

 Level density

parameter:

 Töke-Swiatecki  Suppression of shell

energy corrections according to Ignatyuk

 Collective

enhancement included

  • A. Marchix, PhD thesis, Univ. Caen (2007)

dP

i

dt = i1

n P i1(t) (i f + i n)P i(t)

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SLIDE 6

On the prediction for the SHE production Kazimierz Dolny, Sept. 20011

Simplified model

 Fission vs neutron

evaporation

 Bn=6 MeV & Bf

constant along the chain

 Long fission times

mean:

 Bf ≈ Bn  Long fission time

events occur after evaporation of several neutrons

 We cannot

extract Bf of each isotope

Fission time Bf=Bn

Pre-scission neutrons

D.B. et al, IJMP E17 (2008) 1681-1693

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SLIDE 7

On the prediction for the SHE production Kazimierz Dolny, Sept. 20011

What about ΔEshell?

 Experimental results for Z=120 and 124

cannot be reproduced with Möller’s table

 Very large ΔEshell for the first isotopes of

the evaporation chain

 Potential structure effects ?

aground = a.(1+ (1 eE*/ Ed ).Eshell E * ) Bf eE*/ Ed .Eshell

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SLIDE 8

On the prediction for the SHE production Kazimierz Dolny, Sept. 20011

Structure effect 2

E ? = 0 E = 5MeV E* = 20MeV E* = 2MeV

Preliminary

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SLIDE 9

On the prediction for the SHE production Kazimierz Dolny, Sept. 20011

Residue cross sections

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SLIDE 10

On the prediction for the SHE production Kazimierz Dolny, Sept. 20011

 It is not a Monte-Carlo code to calculate very low

probabilities

 It is based on a discretisation in bins of the energy

spectra:

KEWPIE 2 Specificity

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SLIDE 11

On the prediction for the SHE production Kazimierz Dolny, Sept. 20011

Residue cross sections

Important parameters of KEWPIE2

 Shell correction energy -> correction factor  Damping Energy Ed

 Originally, Ed=18.5 MeV

 Reduced friction

Eshell = f .EMoller

aground = a.(1+ (1 eE*/ Ed ).Eshell E * )

  • A. Marchix, PhD thesis, Univ. Caen (2007)

β=2.1021s-1

Bf eE*/ Ed .Eshell

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SLIDE 12

On the prediction for the SHE production Kazimierz Dolny, Sept. 20011

Results

 Fitting the residue cross sections gives

very strong constraint on ΔEshell…

  • Precision of 1 MeV

 … if we know the fusion cross section

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SLIDE 13

On the prediction for the SHE production Kazimierz Dolny, Sept. 20011

Reaction

Reseparation

Coulomb barrier

Quasi-fission

Inner barrier

Fission

SHE

How to assess the fusion model?

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SLIDE 14

On the prediction for the SHE production Kazimierz Dolny, Sept. 20011

Experimental fusion hindrance

K.-H. Schmidt & W. Morawek Rep. Prog. Phys. 54 (1991) 949

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SLIDE 15

On the prediction for the SHE production Kazimierz Dolny, Sept. 20011

Position of the inner barrier

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On the prediction for the SHE production Kazimierz Dolny, Sept. 20011

Importance of the neck

The value of the neck parameter differs from authors

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On the prediction for the SHE production Kazimierz Dolny, Sept. 20011

Neck dynamics

V(ε)=f. ε ε

1

We solved the Smoluchowski equation

Neck equilibrates very quickly  <ε> ≈ 0.1

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SLIDE 18

On the prediction for the SHE production Kazimierz Dolny, Sept. 20011

Fusion hindrance for symmetric reactions

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SLIDE 19

On the prediction for the SHE production Kazimierz Dolny, Sept. 20011

Fusion hindrance for symmetric reactions

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SLIDE 20

On the prediction for the SHE production Kazimierz Dolny, Sept. 20011

Influence of the shift

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SLIDE 21

On the prediction for the SHE production Kazimierz Dolny, Sept. 20011

Borderline between hindered and non hindered reactions

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SLIDE 22

On the prediction for the SHE production Kazimierz Dolny, Sept. 20011

Adiabatic approximation

Fast degree of freedom (neck) vs slow degree of freedom (r)

Tensor coupling

Shift of the initial condition in r

Larger hindrance due to dynamical coupling!

V(ε)=f. ε ε

1

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SLIDE 23

On the prediction for the SHE production Kazimierz Dolny, Sept. 20011

Test on a simple case

Exact solution for a saddle made with 2 parabolas

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SLIDE 24

On the prediction for the SHE production Kazimierz Dolny, Sept. 20011

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