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Search for diabolic pair transfer at
higher angular momentum states by
using heavy-ion induced reaction
2

1
Spokesperson

Dr. Samit Kr. Mandal
Department of Physics & Astrophysics
Delhi University
H. J. Wollersheim
GSI
Pair transfer as a function of spin
238U
40Ar
Spectroscopic quantities


A  2, I a a


 0
A, I

I  2, A Q I , A  B( E 2; I  I  2
Intrinsic quantities


 a a


 0
Parameters 


Q

pair transfer amplitude

A  2, I a  a 

 0
A, I
Nuclear Josephson Effects:
Enhanced transfer of nucleon pairs between two superfluid heavy
nuclei in a cold reaction correspond to a super-current.
alternating current JE:
Strong coupling situation
Flux oscillation in particular mass partition
Characteristic dependences on incident energy or reaction angle
Transfer probability values larger than 0.5
direct super current JE:
Weak coupling situation
Enhanced transfer of several nucleon pairs
Transfer probability values less than 0.5
G.Eckert et al. Z.Phys. A343 (1992), 276
I.Peter,W.von Oertzen et al., Eur.Phys. J.A16(2003),509
Berry's Phase, Diabolic Pair Transfer
Berry's phase is a simple mathematical fact. Berry considers
a

Hamiltonian, which depends on external parameters R  ( x, y, z )
Examples: (a) Nilsson Model R=β
(b) Cranked Shell Model R=(λ,Δ,ω)
E2(λ,ω)
En(λ,ω)
Φ0
C
Φ1
V
E1(λ,ω)
ω
iγ Φ
Φ
Φ1=
=e-Φ
00
λ
chemical potential λ, angular velocity ω, pairing gap Δ
A diabolical point, where two energy
surfaces touch and a closed path on
the lower surface encircling this point
Berry's Phase and the Backbending Effect
J  is   s  s   g
Two different paths around a diabolic point
The oscillating behavior of the pair transfer matrix
element has a close analogy to the oscillating behavior
of the electric current in Superconducting Quantum
Interference Devices as a function of the magnetic
field, the DC-Josephson effect
<A+2,J/(a+a+)l=0/A,J>
J   g
J(ђ)
Berry's Phase in Nuclear Physics
 open problem for experimentalist
Pair transfer matrix
Full horizontal arrow indicates pair transfer matrix elements with positive sign and dashed arrows
indicate those with negative sign . K quantum number for j=13/2 is shown.
Proposed Systems:
172,174Yb
on 206Pb
174,176Hf on 206Pb
The Hf and Yb-chain : The interaction strength in the level crossing between the
ground state band and the s-band characterized by the minimal distance between the
yrast band and the first excited band ΔEmin. Connected lines correspond to minimal
distances for the angular momenta I= 10-16ħ. Full dot symbols indicate the even
mass Yb-isotopes. The position of the deformed single-particle energies of the v i13/2
levels for the nucleus 166Yb and 170Hf are given on the abscissa.
Y. Sun et al, Z. Phys. A339 (1991) 51
2n-transfer probability as a function of spin
yrast-states
yrare-states
174Hf(206Pb,208Pb)172Hf
The calculation show the diabolic effect for 206Pb on 174Hf. This calculation assumes
174Hf transfers to 172Hf. The symbol o’s are non diabolic case and Δ’s are diabolic cases.
L F Canto et al PRC 47,2836(1993).
Experimental Setup
Beam: 174,176Hf and 172,174Yb, Target : 206Pb (500μg/cm2 thick),
 The experiment will be performed at X7 beam line
 The ion beam from UNILAC facility.

Annular proportional counter for
particle detection
 Cluster Ge–detector from
EUROBALL and segmented
Clover will be used for
gamma-ray detection
Super
Experimental Setup & Beam time request
Beam: 174,176Hf and 172,174Yb, Target : 206Pb (500μg/cm2 thick),
Beam Energy: 5-8 MeV/A .
Beam Current: 109 pps.
Estimated cross-sect ion (Coupled Channels Calculations- FRESCO)~ 1 μb for
excited state of interest
Yield ~ 200 counts/hr.
Gamma detection efficiency ~ 4%
For each isotope, shifts required = 14 shifts.
Setting up detectors & particle-γ coincidence = 2 shifts.
Total shift require : 30 for each experiment with two isotopes
50% of duty cycle of accelerator has been taken into account.
Beam Time Request
Two Experiments
Each experiment: 30 Shifts
Total : 60 Shifts.
Collaborators :
Sunil Kalkal , Mansi Saxsena
Department of Physics & Astrophysics, University of Delhi, India
&
Punita Verma
Kalindi College, University of Delhi, India
&
Jürgen Gerl, Magdalena Gorska, Henning Schaffner,Ivan
Kojouharov, Jurek Grebosz, R. Hoischen
Gesellschaft für Schwerionenforschung, Darmstad, Germany
Thanks