production of rare nuclear species with proton and heavy ion beams in various regimes martin...
TRANSCRIPT
Production of rare nuclear species with proton and heavy ion beams in various regimes
Martin Veselský
Institute of Physics, Slovak Academy of Sciences, Bratislava, Slovakia
Exotic nuclei
- only 2500 out of approx 6000 possible nuclei known - large region of very neutron-rich nuclei still unknown- region of superheavy nuclei
Physics questions
- properties of nuclear surface ( neutron skin )- nuclear astrophysics ( r-process ) - hyperheavy nuclei, nuclear molecules
Participant-spectator reactions at relativistic energies ( above 100 AMeV ). Applicable to both spallation reactions ( normal kinematics ) and fragmentation
( inverse kinematics ) ?
Production of exotic nuclei in spallation with proton beams ISOLDE facility ( CERN ), beam energies ~ 1 GeVA,
Production of exotic nuclei in relativistic fragmentation Separator FRS ( GSI Darmstadt ), beam energy 1 GeVA, Separátor LISE ( GANIL ), beam energy 70-100 MeVA.
FRS
Task 11 - Subtask 1- Heavy Ion Benefits for Driver Accelerator
Driver-Beam Scenarios to be Covered
1. The three HI driver beam options described in the report of the Driver Accelerator group (App. B, Sect. 4.2 of the EURISOL report)a) A/q = 2 at 43 A MeV and A/q = 3 at 28 A MeVb) A/q = 2 at 500 A MeVc) A/q = 3 at 100 A MeV and A/q = 2 at 150 A MeV
2. The HI driver beam option described in the Target and Ion Source group (App C, Sect. 2.2.3 of the EURISOL report)
A/q = 6 at 166.5 A MeV and A/q = 3 at 333 A MeV
3. 3He beam accelerated to 1 A GeV in the main linac with minor cavity modifications.
All these options will be compared with the standard 1 GeV proton-driver case.
- peripheral elastic and quasi-elastic ( QE ) collisions - semi-peripheral deep-inelastic collisions ( DIT ) collisions - incomplete ( ICF ) and complete ( CF ) fusion in central collisions - pre-equilibrium emision typically preceding ICF/CF and DIT
( detailed description in M. Veselský, Nuclear Physics A 705(2002)191 )
Nucleus-nucleus collisions at beam energies below 100 AMeV:
Standard DIT ( Tassan-Got and Stefan, NPA 524 (1991) 121 )
86Kr + 64Ni at 25 AMeV
Solid - GEMINI, dash-SMM
86Kr + 112Sn at 25 AMeV Modified DIT (nucl-th/0507026):
solid - GEMINI, dash -SMM Dash-dotted - SMM, s > 0.8 fm
How to reach the extremely neutron-rich nuclei ( e.g. around 78Ni ) :
- Optimize projectile-target combination
- Optimize energy. Energies lower than 20 AMeV ?
How close to e.g. 78Ni can one get with 86Kr+64Ni at 25 AMeV?
Experimental data ( 1-3 deg ) vs modified DIT + SMM
With 86Kr one cannot get too close to 78Ni, how about 82Se ?
Calculated yields for reaction 82Se+64Ni at 25 AMeV.
Reaction 82Se+64Ni - results of simulations :
- cross sections of exotic nuclei around 78Ni at 0.1 - 1 b level
- cross sections depend weakly on beam energy
- with 100pnA beam, 20 mg/cm2 target ( settings assumed in G. Souliotis et al. PLB 543 (2002) 163 ), the intensities of secondary beams around 78Ni of 10 - 100 /s can be expected
- what is the maximum achievable current of the primary beam ?
Observed excess of neutron-rich nuclei in reactions 124Sn+124Sn at 20 AMeV .
solid symbols - experimental data
open symbols - DIT+Gemini
dashed line - EPAX
Test of low energy data 58Ni+208Pb at 5.66 AMeV, angle-integrated data( L. Corradi et al., Phys. Rev. C 66 (2002) 24606 )
Z=22
Z=27 Z=26 Z=25
Z=24 Z=23
Z=28
Experimental data vs DIT calculation ( after de-excitation )
DIT calculation with radius of nuclear potential extended by 0.75 fm. Possible explanation : deformation, neck structure ?
Z=22
Z=27 Z=26 Z=25
Z=24 Z=23
Z=28
DIT calculation ( with extended radius of the nuclear potential ) for the reaction 64Ni+208Pb at 5.66 AMeV, angle-integrated data ( compared to experimental data for the reaction 58Ni+208Pb from L. Corradi et al., Phys. Rev. C 66 (2002) 24606 )
Isoscaling in nuclear processes
M.B. Tsang et al., PRL 86(2001)5023
G. Souliotis et al., PRC 68(2003)24605
M. Veselský et al., PRC 69(2004)44607
Comparison of various scenarios
- production cross sections compared, others factors such as target thickness, extraction efficiencies are important
- region around 78Ni selected as a test case
- spallation - GSI model used ( statistical abrasion-ablasion + de-excitation/fission )
- fragmentation - cross sections calculated using EPAX-2, optimized for each isotope over all stable beams
Calculated ( GSI model ) cross sections for 1 GeV proton beam colliding with U, Th, W and La (solid, dashed, dash-dotted and dotted lines, respectively).
Calculated ( GSI model ) cross sections for 1 GeV proton beam colliding with U (solid line), compared to cross sections measured at GSI
(P. Armbruster et al., PRL 93 (2004) 212701).
Calculated cross sections for 1 GeV proton beam colliding with U (solid line), compared to the optimal fragmentation cross sections (dashed line ), calculated
with EPAX-2 for each nuclide separately using all -stable beams .
Calculated cross sections for 1 GeV proton beam colliding with La (solid line), compared to fragmentation cross sections , calculated with EPAX-2 using La
beam and using all -stable beams ( dash-dotted and dashed lines ).
Calculated cross sections for 1 GeV proton beam colliding with U (solid line), compared to the calculated inclusive cross sections for reactions 86Kr,82Se+64Ni at 25 AMeV (dashed and dash-dotted line, respectively) and optimal fragmentation cross
sections (dotted line).
Relative cross sections calculated with EPAX-2 for each nuclide separately using all -stable beams in one-step and two-step scenarios (solid and dashed
line, respectively).
Contour plot of fragmentation cross sections (dashed lines ), calculated for 78Ni with EPAX-2 using both stable ( dash-dotted line ) and unstable beams .
Conclusions :
- spallation/fission, fragmentation and peripheral ( deep-inelastic ) collisions were considered as possible candidates for production of exotic ( neutron-rich ) nuclei around 78Ni
- U-target is optimal for spallation/fission with 1 GeV proton beam
- cross sections in peripheral ( deep-inelastic ) collisions largest of all for the most n-rich nuclei, technically plausible to explore them ?
- systematic cross sections data from peripheral ( deep-inelastic ) collisions are necessary at both Fermi-energy domain and low energies
18O + 181Ta at 35 AMeV, beryllium isotopes
7Be - fast component, intense pre-eq emission, ICF kinematically impossible, motion along classical Coulomb trajectory ? Transparency ?
Experiment (COMBAS) PE+DIT/ICF+SMM
7Be
7Be
EURISOL
- 6FP Project "EURISOL Design Study" started in Feb 2005 ( MV/Bratislava involved ) http://www.eurisol-ds.lnl.infn.it/
- theoretical and experimental studies of production mechanisms are planned
- open question - Heavy Ion capability for driver accelerator - yes or no ?
- selection of the key experiment(s)
Observed excess of neutron-rich nuclei in reactions 86Kr+64Ni at 25 AMeV.
solid symbols - experimental data
open symbols - DIT+Gemini
dashed line - EPAX
Correlation of skin thickness to isovector chemical potential(V. Kolomietz et al, PRC 64(2001)024315, extended Thomas-Fermi calculation)
ἸἩRn-R
p determines the difference
of N/Z at (Rn+R
p)/2 ( surface ) from the bulk N/Z,
correlates to isovector chemical potential
DIT (T-G) : macroscopic formula for ἸἩR
n-R
p used, values unrealistically large
but bulk N/Z dynamics described well
Modified DIT (nucl-th/0507026), phenomenological correction, effect of shell structure on nuclear periphery ( assuming validity of the R
n-R
p vs
n-
p correlation ) and thus on transfer probability
estimated as:
where S... = S
...exp - S
...mac , is a free parameter ( = 0.53 determined as optimal value ),
s > 0 fm ( only non-overlapping configurations considered )
Conclusions 86Kr + 64Ni, 112,124Sn at 25 AMeV
- a correction to DIT describes the effect of isospin asymmetry at nuclear periphery
- inversion of the bulk isospin flow due to microscopic structure at nuclear periphery
- consistent parameters for all reactions
- SMM reproduces the yields of n-rich species well while overestimating the yields of -stable isotopes close to the projectile
- GEMINI typically overestimates the width of mass distributions
- for p-rich target 112Sn stronger Coulomb interaction supresses the effect of isospin asymmetry at nuclear periphery at s < 1 fm
Conclusions - low energy
- deep-inelastic collisions a dominant mechanism for production of exotic nuclei
- systematic cross section data needed