14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015 1 PRE-EQUILIBRIUM (EXCITON)...
-
Upload
clyde-chambers -
Category
Documents
-
view
216 -
download
3
Transcript of 14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015 1 PRE-EQUILIBRIUM (EXCITON)...
![Page 1: 14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015 1 PRE-EQUILIBRIUM (EXCITON) MODEL AND THE HEAVY-ION REACTIONS WITH CLUSTER EMISSION.](https://reader035.fdocuments.in/reader035/viewer/2022062802/56649e915503460f94b96f7f/html5/thumbnails/1.jpg)
14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015
1
PRE-EQUILIBRIUM (EXCITON) MODELAND THE HEAVY-ION REACTIONS
WITH CLUSTER EMISSION
E. BětákInst. of Physics, Slovak Acad. Sci., Bratislava,
Slovakia([email protected])
J. CsehATOMKI, Debrecen, Hungary
![Page 2: 14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015 1 PRE-EQUILIBRIUM (EXCITON) MODEL AND THE HEAVY-ION REACTIONS WITH CLUSTER EMISSION.](https://reader035.fdocuments.in/reader035/viewer/2022062802/56649e915503460f94b96f7f/html5/thumbnails/2.jpg)
14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015 2
1. Motivation2. Consistency of the exciton model – master eq.
approach3. Coalescence and Iwamoto-Harada model for cluster
emission in its density formulation4. Extensions of the Iwamoto-Harada model5. Cluster emission with angular momentum
variables6. Cluster emission from heavy-ion collisions
![Page 3: 14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015 1 PRE-EQUILIBRIUM (EXCITON) MODEL AND THE HEAVY-ION REACTIONS WITH CLUSTER EMISSION.](https://reader035.fdocuments.in/reader035/viewer/2022062802/56649e915503460f94b96f7f/html5/thumbnails/3.jpg)
14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 20153
MOTIVATION
Candidates for hyperdefomed nuclei are expected to be formed (relatively easily) in (light) heavy-ion reactions at not too high energy (say, incident energy of few tens or as a maximum few hundreds of MeV).
Some combinations of colliding ions have been suggested.
The question is, which energies seem to be favourable for their creation.
We aim to get some hints for this process, and illustrate it on the 20Ne + 20Ne -> 36 Ar (plus something: α, 2n+2p, n+p+d, …)
The production cross section serves as the main indiucator. Therefore we applied statistical pre-equilibrium model with additions suitable to this aim.
![Page 4: 14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015 1 PRE-EQUILIBRIUM (EXCITON) MODEL AND THE HEAVY-ION REACTIONS WITH CLUSTER EMISSION.](https://reader035.fdocuments.in/reader035/viewer/2022062802/56649e915503460f94b96f7f/html5/thumbnails/4.jpg)
14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 20154
CONSISTENCY OF THE EXCITON MODEL - MASTER EQUATIONS APPROACH
Master equations are capable to describe the whole process in time from the very creation of the composite system through its equilibration up to the decay of compound nucleus within a single formalism, not mixing various approaches.
Using the density-dependent formulation of the so-called Iwamoto-Harada model (Dobes and Betak, 5 years before I+H) for cluster emission, pick-up as well as knock-out can be included. Obviously, one pays for the single approach with the lost of majority details, like details of the structures in spectra, but the cross sections describe the average trends rather satisfactorilly.
A technical handicap remains: the set of master
equations is huge, but we have a suitable algorithm to solve it.
![Page 5: 14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015 1 PRE-EQUILIBRIUM (EXCITON) MODEL AND THE HEAVY-ION REACTIONS WITH CLUSTER EMISSION.](https://reader035.fdocuments.in/reader035/viewer/2022062802/56649e915503460f94b96f7f/html5/thumbnails/5.jpg)
14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 201
5 5
COALESCENCE MODEL FOR CLUSTER EMISSION
Kalbach (Cline, Kalbach-Cline, Kalbach-Walker), Ribanský & Obložinský
Emision rate (nucleons):
Coalescence clusters:
)(),,(
),,1()(
12),,( *
32pR
Ehp
UhpsEn xxINVxx
xx
cx
x
xxxxx
xxINVxx
xx
cx g
BppR
Ehp
UhppsEn
),0,()(
),,(
),,()(
12),,( *
32
![Page 6: 14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015 1 PRE-EQUILIBRIUM (EXCITON) MODEL AND THE HEAVY-ION REACTIONS WITH CLUSTER EMISSION.](https://reader035.fdocuments.in/reader035/viewer/2022062802/56649e915503460f94b96f7f/html5/thumbnails/6.jpg)
14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 20156
coalescence IH model IHB model knock-out
COALESCENCE (IWAMOTO-HARADA) MODEL FOR CLUSTER EMISSION IN ITS DENSITY FORMULATION
![Page 7: 14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015 1 PRE-EQUILIBRIUM (EXCITON) MODEL AND THE HEAVY-ION REACTIONS WITH CLUSTER EMISSION.](https://reader035.fdocuments.in/reader035/viewer/2022062802/56649e915503460f94b96f7f/html5/thumbnails/7.jpg)
Generalized (coalescence + pickup) Iwamoto & Harada, Dobeš & Běták, Bisplinghoff
EMISSION RATE PROPORTIONAL to the CLUSTER FORMATION PROBABILITY
SINGLE-CLUSTER DENSITY INVERSELY PROPORTIONAL to the CLUSTER FORMATION PROBABILITY
12*
1*
11
* ),,0(),0,(),,(
),0,(),,(
*
dpppEhpp
BpUhpp
x
p
p
E
B
xxxx
x
xx
THEREFORE the result is PARAMETERLESS !
7
![Page 8: 14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015 1 PRE-EQUILIBRIUM (EXCITON) MODEL AND THE HEAVY-ION REACTIONS WITH CLUSTER EMISSION.](https://reader035.fdocuments.in/reader035/viewer/2022062802/56649e915503460f94b96f7f/html5/thumbnails/8.jpg)
Bisplinghoff
Pickup limited by the binding energy of nucleons in the cluster (i.e. about 28 MeV for alphas and 2 MeV for deuterons)
Now Limitation due to binding energy for all clusters
Only low-exciton configurations with pickup (CN limit!)
Thermal “blurring” considered
Admixture allowed for all potential well (Heisenberg uncertainty relation)
Possibility of knockout (initial stage only) for alphas
E
dU0
),0,1(),4,0(
14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015
8
![Page 9: 14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015 1 PRE-EQUILIBRIUM (EXCITON) MODEL AND THE HEAVY-ION REACTIONS WITH CLUSTER EMISSION.](https://reader035.fdocuments.in/reader035/viewer/2022062802/56649e915503460f94b96f7f/html5/thumbnails/9.jpg)
14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June
2015 9
Calculations without spin (old)
a) deuterons
![Page 10: 14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015 1 PRE-EQUILIBRIUM (EXCITON) MODEL AND THE HEAVY-ION REACTIONS WITH CLUSTER EMISSION.](https://reader035.fdocuments.in/reader035/viewer/2022062802/56649e915503460f94b96f7f/html5/thumbnails/10.jpg)
14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015 10
Bb) alphas
![Page 11: 14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015 1 PRE-EQUILIBRIUM (EXCITON) MODEL AND THE HEAVY-ION REACTIONS WITH CLUSTER EMISSION.](https://reader035.fdocuments.in/reader035/viewer/2022062802/56649e915503460f94b96f7f/html5/thumbnails/11.jpg)
14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June
2015 11
c) α-knockout admixtures from the fit to the data
![Page 12: 14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015 1 PRE-EQUILIBRIUM (EXCITON) MODEL AND THE HEAVY-ION REACTIONS WITH CLUSTER EMISSION.](https://reader035.fdocuments.in/reader035/viewer/2022062802/56649e915503460f94b96f7f/html5/thumbnails/12.jpg)
14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015 12
Cluster emissionCluster emission withwith
angular momentumangular momentumvariablesvariables
![Page 13: 14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015 1 PRE-EQUILIBRIUM (EXCITON) MODEL AND THE HEAVY-ION REACTIONS WITH CLUSTER EMISSION.](https://reader035.fdocuments.in/reader035/viewer/2022062802/56649e915503460f94b96f7f/html5/thumbnails/13.jpg)
Spin variables:
Coupling of nucleons to form a coalescence or pickup cluster may be – in a very rough approximation – considered included in the formation probability.
Therefore, no additional couplings appear in the emission rates and the only place affected by the angular momentum are different transition coefficients and via competitions to other (nucleon,γ) channels.
Exception: knock-out – α-particle is not formed during reaction, but it is already present in the target nucleus.
14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 201513
![Page 14: 14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015 1 PRE-EQUILIBRIUM (EXCITON) MODEL AND THE HEAVY-ION REACTIONS WITH CLUSTER EMISSION.](https://reader035.fdocuments.in/reader035/viewer/2022062802/56649e915503460f94b96f7f/html5/thumbnails/14.jpg)
14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015 14
![Page 15: 14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015 1 PRE-EQUILIBRIUM (EXCITON) MODEL AND THE HEAVY-ION REACTIONS WITH CLUSTER EMISSION.](https://reader035.fdocuments.in/reader035/viewer/2022062802/56649e915503460f94b96f7f/html5/thumbnails/15.jpg)
14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015
15
Primary nucleon, deuteron, alpha and gamma energy spectra (gammas with cascades) from 197Au+p at 62 MeV
![Page 16: 14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015 1 PRE-EQUILIBRIUM (EXCITON) MODEL AND THE HEAVY-ION REACTIONS WITH CLUSTER EMISSION.](https://reader035.fdocuments.in/reader035/viewer/2022062802/56649e915503460f94b96f7f/html5/thumbnails/16.jpg)
14
th In
tern
at. C
on
f. Nu
cl. Reactio
n M
ech
an
isms, V
are
nn
a,
19
th Ju
ne 2
01
5
16
![Page 17: 14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015 1 PRE-EQUILIBRIUM (EXCITON) MODEL AND THE HEAVY-ION REACTIONS WITH CLUSTER EMISSION.](https://reader035.fdocuments.in/reader035/viewer/2022062802/56649e915503460f94b96f7f/html5/thumbnails/17.jpg)
HEAVY IONS – INITIAL CONFIGURATION(without spin variables today)
Cindro et al.:
for lower energies,
where
14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 201517
)(
)(08.038.009.0
arg
arg0
projt
projt
proj AA
AA
A
n
proj
Ccm
A
VE
![Page 18: 14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015 1 PRE-EQUILIBRIUM (EXCITON) MODEL AND THE HEAVY-ION REACTIONS WITH CLUSTER EMISSION.](https://reader035.fdocuments.in/reader035/viewer/2022062802/56649e915503460f94b96f7f/html5/thumbnails/18.jpg)
HEAVY IONS – CLUSTER BREAKUPKalbach Walker, www-nds.iaea.org/fendl3/docs/dBreakupRCM2.pdf
where the normalizatoion factor is only weakly sensitive to the projectile.
We use this as very rough initial approximation.
14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015
18
MeV
EEMeV
E
Dinc
inc
bu
14exp1[
170exp
)(2/1
20
![Page 19: 14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015 1 PRE-EQUILIBRIUM (EXCITON) MODEL AND THE HEAVY-ION REACTIONS WITH CLUSTER EMISSION.](https://reader035.fdocuments.in/reader035/viewer/2022062802/56649e915503460f94b96f7f/html5/thumbnails/19.jpg)
14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 201519
P r e l i m i n a r y
20 Ne + 20 Ne
![Page 20: 14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015 1 PRE-EQUILIBRIUM (EXCITON) MODEL AND THE HEAVY-ION REACTIONS WITH CLUSTER EMISSION.](https://reader035.fdocuments.in/reader035/viewer/2022062802/56649e915503460f94b96f7f/html5/thumbnails/20.jpg)
CONCLUSIONS Clusterization itself parameterless Effective only at initial stages, what enables proper equilibrium
(compound nucleus) limit Thermal blurring of nucleons allowed Pickup (IHB) generalized to all types of clusters For strongly bound ejectiles knockout possible: Included angular momentum, but the couplings of nucleons to form a
cluster are hidden in cluster formation probability Introduction of spin variables enhances the cluster emission compared
to spin-independent case. (It plays similar role as deformation according to Blann & Komoto)
All calculations presented here are just with default parameters (level densities, inverse c.s., transition matrix element).
Possibility to indicate various contributing mechanisms leading to the same (nearly equilibrated) composite system, and to select the most suitable conditions for structure studies, like existence of hyperdeformed nucli.
Further effort: heavy ions, cluster emission, pre-equilibrium with some elements of direct reactions and spin variables tgogether within one formalism
14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015
20
![Page 21: 14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015 1 PRE-EQUILIBRIUM (EXCITON) MODEL AND THE HEAVY-ION REACTIONS WITH CLUSTER EMISSION.](https://reader035.fdocuments.in/reader035/viewer/2022062802/56649e915503460f94b96f7f/html5/thumbnails/21.jpg)
Thank you
14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June 2015 21