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Ab Initio Calculations of Three and Four Body Dynamics
M. Tomasellia,b
Th. Kühla, D. Ursescua
a Gesellschaft für Schwerionenforschung, D-64291 Darmstadt,Germanyb Technical University Darmstadt, D-64289 Darmstadt, Germany
Marco Tomaselli 2006Brasil: Few body 18
The Equation of Motion (EoM) in the zero The Equation of Motion (EoM) in the zero order dynamic linearization (GLA)order dynamic linearization (GLA)
Marco Tomaselli 2006Brasil: Few body 18
The Equation of Motion (EoM) in The Equation of Motion (EoM) in the second order GLA-IIIthe second order GLA-III
Marco Tomaselli 2006Brasil: Few body 18
The Equation of Motion (EoM)-IVThe Equation of Motion (EoM)-IV
Marco Tomaselli 2006Brasil: Few body 18
The Non-Linear Eigenvalue EquationThe Non-Linear Eigenvalue Equation
Marco Tomaselli 2006Brasil: Few body 18
Analogy with cluster theoryAnalogy with cluster theory
0...)1(01
3211
N
ii
N
ii
iS aSSSae
211 aaS 6543213 aaaaaaS
iSiSeff HeeH
iSiSeff OeeO
.....43212 aaaaS Perturbation approximation possible. We prefer to calculate the
effective operators.
Correlations can be introduced via eiS method
The perturbative terms of the correlation operators Si correspond
to the diagram of the dynamic theory. The particle–hole terms
generated by the S3 operator are put to zero in the ladder perturbation.
Marco Tomaselli 2006Brasil: Few body 18
Configuration mixing wave functions Configuration mixing wave functions (CMWF)(CMWF)
Marco Tomaselli 2006Brasil: Few body 18
The wavefunction of the deuteronThe wavefunction of the deuteron
Marco Tomaselli 2006Brasil: Few body 18
Cluster model based on Dynamic Cluster model based on Dynamic Correlation Model (DCM)Correlation Model (DCM)
000],[1
11
11
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ii
N
ii
N
ii aaaaH
000],[2
1'
2
1'
1
11
1
11
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ii
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ii
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ii aaaaaaH
......
01
N
iiN a
...000...2
1
2
1''
1
11
12,21,1
N
i iii
N
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iiNNNtot aaaaa
Marco Tomaselli 2006Brasil: Few body 18
Effect of linearisation on commutator Effect of linearisation on commutator chain for two body clusterschain for two body clusters
Collect the resulting terms
Within the GLA the higher order terms (4p-2h) are calculated with the Wick's theorem by neglecting the normal order.
01313213
13222
13
2
13
2
hp
p
hp
p
hpVhpEEpVhp
hpVppVpEE
Dynamic eigenvalue equations for mixed mode amplitudes 2 particles => 3 particles – 1 hole
Marco Tomaselli 2006Brasil: Few body 18
Dynamics eigenvalue equation for one dressed Dynamics eigenvalue equation for one dressed dressed nucleon clustersdressed nucleon clusters
which is solvable self-consistentlywhich is solvable self-consistently
Marco Tomaselli 2006Brasil: Few body 18
Elastic proton scattering on Elastic proton scattering on 66LiLi
Marco Tomaselli 2006Brasil: Few body 18
Medium effects on the two body Medium effects on the two body matrix elements (matrix elements (1818O)O)
Marco Tomaselli 2006Brasil: Few body 18
Positive and Negative parity states in Positive and Negative parity states in 1818OO
Marco Tomaselli 2006Brasil: Few body 18
Comparison with VComparison with Vlow-klow-k potential: potential: 1818OO
Marco Tomaselli 2006Brasil: Few body 18
The EoM of the Three Nucleon ClustersThe EoM of the Three Nucleon Clusters
Marco Tomaselli 2006Brasil: Few body 18
Nuclear results for Li isotopesNuclear results for Li isotopes
Marco Tomaselli 2006Brasil: Few body 18
Elastic proton scattering on Elastic proton scattering on 1111LiLi
Summary of Charge RadiiSummary of Charge Radii
References: Method:[1] I. Tanihata, Phys. Lett B 206,592 (1988) Interaction Cross Sections with Glauber model,
HO distributions[2] P. Navratil, PRC 57,3119 (1998) Large-basis shell-model calculations[3] S. Pieper, Annu.Rev.Nucl.Part.Sci. 51, 53 (2001) Greens Function Monte Carlo AV18/IL2[4] S. Pieper, PRC 66, 044310 (2002) Greens Function Monte Carlo AV18/IL2[5] Suzuki, Progr.Theo.Phys.Suppl. 146, 413 (2002) Stochastic Variational Multicluster Method
on a correlated gaussian basis[6] M. Tomaselli et al., Can. J. Phys. 80, 1347 (2002) Dynamic Correlation model[7] Penionzhkevich, Nucl.Phys. A 616, 247 (1997) coupled channel calculations, double-folding
optical potential, M3Y effective interaction[8] C.W. de Jager, At.Dat.Nucl.Dat.Tab. 14, 479 (1974) Electron Scattering
Exp.[GSI] Exp.[8] Exp.+Th.[1] Exp+Th[1] Th.[2] Th.[3] Th.[4] Th.[5] Th.[6] Exp+Th[7]
Li - rms R c rms R c rms R p rms R c rms R p rms R p rms Rp rms R p rms R c rms R c
6 2,55 2.55 (4) 2.32 (3) 2.46 (2) 2,045 2,39 2,557 2,46 2.37 (3) 2.27 (2) 2.40 (2) 1,941 2,25 2,27 2,418 2,37 2.26 (2) 1,946 2,09 2,18 2,409 2,30 2.18 (2) 1,986 2,04 2,10 2,42
11 2,47 2.88 (2) 2,67 2,235
Rc = charge radius Rp = point radius
Marco Tomaselli 2006Brasil: Few body 18
Charge distributions for A=3 nucleiCharge distributions for A=3 nuclei
Marco Tomaselli 2006Brasil: Few body 18
Charge distribution: alpha particle Charge distribution: alpha particle
RMS (Bonn)=1.50 fm
RMS (Yale)=1.51 fm
Marco Tomaselli 2006Brasil: Few body 18
Energy splitting and BE(E2;2Energy splitting and BE(E2;2+ + 0 0++) ) transition for transition for 1616CC
Marco Tomaselli 2006Brasil: Few body 18
Cluster Factorization Theory ICluster Factorization Theory I
Marco Tomaselli 2006Brasil: Few body 18
Cluster Factorization Theory IICluster Factorization Theory II
Marco Tomaselli 2006Brasil: Few body 18
Cluster Factorization Theory IIICluster Factorization Theory III
Marco Tomaselli 2006Brasil: Few body 18
Cluster Factorization Theory IVCluster Factorization Theory IV
Marco Tomaselli 2006Brasil: Few body 18
Factorisation of the model CMWFs in terms of Factorisation of the model CMWFs in terms of cluster coefficientscluster coefficients
The factorisation method is presently applied to reduce complex Feynman diagrams to simple form
Particle line Hole line Interaction between nucleons