Thessaloniki ΘΕΣΣΑΛΟΝΙΚΗ Solúň Salonico Salonique Salonik 315 B.C.
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Transcript of Thessaloniki ΘΕΣΣΑΛΟΝΙΚΗ Solúň Salonico Salonique Salonik 315 B.C.
ThessalonikiΘΕΣΣΑΛΟΝΙΚΗ
SolúňSalonico
SaloniqueSalonik
315 B.C.
ARISTOTLE UNIVERSITYΑΡΙΣΤΟΤΕΛΕΙΟ ΠΑΝΕΠΙΣΤΗΜΙΟ
75 000 students14 Faculties
53 Departments
Section of Nuclear & Particle Physics
Theory Group C. KoutroulosG. LalazissisS. MassenC. PanosC. Moustakidis
R. FossionK. Chatzisavvas
S. KaratzikosV. PrassaB. Psonis
Zagreb, Sofia, Catania, Munich, Hamburg, Oak Ridge, Mississippi, Giessen
Experimental Group M. Chardalas S. DedoussisC. EleftheriadisM. ZamaniA. Liolios M. ManolopoulouE. SavvidisA. IoannidouK. PapastefanouS. Stoulos
M. FragopoulouC. LamboudisTh. Papaevagelou
Paris (CEA), Dubna, CERN (CAST, n-TOF)
Covarinat density functional theory: isospin
dependence of the effective nuclear force
Covarinat density functional theory: isospin
dependence of the effective nuclear force
Georgios A. LalazissisAristotle University of Thessaloniki, Greece
Georgios A. LalazissisAristotle University of Thessaloniki, Greece
Collaborators: Collaborators: T. Niksic (Zagreb), N. Paar (Darmstadt), T. Niksic (Zagreb), N. Paar (Darmstadt), P. Ring (Munich), D. Vretenar (Zagreb)P. Ring (Munich), D. Vretenar (Zagreb)
Table of Isotopes
Evolution of the Table of IsotopesEvolution of the Table of Isotopes
A large portion of this table is less than ten years old !A large portion of this table is less than ten years old !
1940 - 20001940 - 20001940 - 20001940 - 2000
Large gaps on the heavy neutron rich side !Large gaps on the heavy neutron rich side !
Evolution of the Table of IsotopesEvolution of the Table of Isotopes
Need for improved isovector channel ofthe effective nuclear interaction.
EOS of asymmetric nuclear matter and neutron matter
Structure and stability of exotic nuclei with extremeproton/neutron asymmetries
Formation of neutron skin and halo structures
Isoscalar and isovectordeformations Mapping the drip-lines
Evolution of shell structure Structure of superheavy elements
EE Slater determinant density matrix
A
iii
1
)()(),(ˆ r'rr'r
ˆ
E
h iiih ˆ
))()(( 11 AA rr A
Mean field: Eigenfunctions:
ˆ
2
E
V
Interaction:
effHH
DFT very successful because being effective theories, adjusted to experiment, include globally a large number of important effects, which go beyond simple Hartree theory, such as:
Brueckner correlations, ground state correlations, vacuum polarizations, exchange terms etc.
Why relativistic? Why relativistic?
* Simplicity and elegance
Non-relativistic kinematics !!!Non-relativistic kinematics !!!
* Large spin-orbit term in nuclear physics (magic numbers)
* Success of relativistic Brueckner calculations (Coester line)
* Weak isospin dependence of spin-orbit (isotopic shifts)
* Pseudospin symmetry (nuclear spectra)
* Relativistic saturation mechanism
* Nuclear magnetism (magnetic moments) (moments of inertia)
Covariant density functional theory:Covariant density functional theory:Covariant density functional theory:Covariant density functional theory:
system of Dirac nucleons coupled by the exchange mesons and the photon field through an effective Lagrangian.
(J,T)=(0+,0) (J,T)=(1-,0) (J,T)=(1-,1)
Sigma-meson: attractive scalar field:
Omega-meson: short-range repulsive
Rho-meson:isovector field
)()( rr gS )()()()( rrrr eAggV
Covariant density functional theory Covariant density functional theory
A
iii
1
)()(),(ˆ r'rr'r
Dirac operator:
)(
)(
r
r
i
ii g
f
No sea approximation: i runs over all states in the Fermi sea
..)()()()(ˆ ),(ˆˆˆ rαVrrrrpα VSmh
)(
)(ˆSVm
SVmh
αp
αp
EFFECTIVE INTERACTIONSEFFECTIVE INTERACTIONS (NL1, NL2, NL3, NL-Z2, …) (NL1, NL2, NL3, NL-Z2, …)
model parameters: meson masses m, m, m, meson-nucleon coupling constants g, g, g, nonlinear self-interactions coupling constants g2, g3, ...
The parameters are determined from properties of nuclear matter (symmetric and asymmetric) and bulk properties of finite nuclei (binding energies, charge radii, neutron radii, surface thickeness ...)
Effective density dependence Effective density dependence
through a non-linear potential: Boguta and Bodmer, NPA. 431, 3408 (1977)NL1,NL3,TM1..
43
32
2222
4
1
3
1
2
1)(
2
1 ggmUm 4
33
22222
4
1
3
1
2
1)(
2
1 ggmUm
through density dependent coupling constants:
T.W.,DD-ME..Here, the meson-nucleon couplings
)(),(),(,, gggggg )(),(),(,, gggggg
are replaced by functions depending on the density r)
number of param.
How many parameters ?How many parameters ?
symmetric nuclear matter: E/A, ρ0
finite nuclei (N=Z):
E/A, radii
spinorbit for free
m
g
m
g
m
Coulomb (N≠Z): a4
m
g
density dependence: T=0 K∞
7 parameters
rn - rpT=1
g2 g3
aρ
One- and two-neutron separation energies
surface thicknesssurface diffuseness
Neutron densities
groundstates of Ni-SnGround states of Ni and Sn isotopesGround states of Ni and Sn isotopes
combination of the NL3 effective interaction for the RMF Lagrangian, and the Gogny interaction with the parameter set D1S in the pairing channel.
G.L., Vretenar, Ring, Phys. Rev. C57, 2294 (1998)
RHB description of neutron rich N=28 nuclei. NL3+D1S effective interaction.
Strong suppression of the spherical N=28 shell gap.
1f7/2 -> fp core breaking Shape coexistence
G.L., Vretenar, Ring, Stoitsov, Robledo, Phys. Rev. C60, 014310 (1999)
Ground-state quadrupole deformation
Average neutronpairing gaps
Shape coexistence in the N=28 regionShape coexistence in the N=28 region
Neutron single-particle levels for 42Si, 44S, and 46Ar against of the deformation. The energies in the canonical basis correspond to qround-state RHB solutions with constrained quadrupole deformation.
Total binding energy curves
SHAPE COEXISTENCE
Evolution of the shell structure, shell gaps and magicity with neutron number!Evolution of the shell structure, shell gaps and magicity with neutron number!
Ground-state proton emitters
Self-consistent RHB calculations -> separation energies, quadrupole deformations, odd-proton orbitals, spectroscopic factors
G.L., Vretenar, RingPhys.Rev. C60, 051302 (1999)
Proton emitters I
characterized by exotic ground-state decay modes such as the direct emission of charged particles and -decays with large Q-values.
Vretenar, G.L., Ring, Phys.Rev.Lett. 82, 4595 (1999)
Nuclei at the proton drip line:Nuclei at the proton drip line:
How far is the proton-drip line from the experimentallyknown superheavy nuclei?
G.L. Vretenar, Ring, PRC 59 (2004) 017301
Proton drip-line in the sub-Uranium region Proton drip-line in the sub-Uranium region
Possible ground-state protonemitters in this mass region?
Proton drip-line for super-heavy elements: Proton drip-line for super-heavy elements:
Pygmy: 208-PbPaar et al, Phys. Rev. C63, 047301 (2001)
Exp GDR at 13.3 MeV
Exp PYGMY centroid at 7.37 MeV
In heavier nuclei low-lying dipole states appear that are characterized by a more distributed structure of the RQRPA amplitude.Among several single-particle transitions, a single collective dipole state is
found below 10 MeV and its amplitude represents a coherent superposition of many neutron particle-hole configurations.
208Pb
208Pb 208Pb
Neutron radiiNeutron radii
RHB/NL3RHB/NL3
NaNa SnSn
ME2ME2
2. 2. MODELS WITH DENSITY-DEPENDENTMODELS WITH DENSITY-DEPENDENTMESON-NUCLEON COUPLINGSMESON-NUCLEON COUPLINGS
2. 2. MODELS WITH DENSITY-DEPENDENTMODELS WITH DENSITY-DEPENDENTMESON-NUCLEON COUPLINGSMESON-NUCLEON COUPLINGS
A. THE LAGRANGIANA. THE LAGRANGIAN
B. B. DENSITY DEPENDENCE OF THEDENSITY DEPENDENCE OF THE COUPLINGSCOUPLINGS
the meson-nucleon couplings g, g, g -> functions of Lorentz-scalar bilinear forms of the nucleon operators. The simplest choice:
a) functions of the vector density
b) functions of the scalar density
PARAMETRIZATION OF THE DENSITY DEPENDENCEPARAMETRIZATION OF THE DENSITY DEPENDENCE
MICROSCOPIC: Dirac-Brueckner calculations of nucleon self-energies in symmetric and asymmetric nuclear matter g
PHENOMENOLOGICAL:
S.Typel and H.H.Wolter, NPA 656, 331 (1999) Niksic, Vretenar, Finelli, Ring, PRC 66, 024306 (2002)
g()
g()
g()
saturation density
Fit: DD-ME2Nuclei used in the fit for DD-ME2Nuclei used in the fit for DD-ME2
(%)
(%)
Nuclear matter: E/A=-16 MeV (5%), o=1,53 fm-1 (10%)
K = 250 MeV (10%), a4 = 33 MeV (10%)
Neutron Matter
DD-ME2 DD-ME1 TW-99 NL3 NL3*
ρο (fm-3) 0.152 0.152 0.153 0.149 0.150
Ε/Α (MeV) -16.14 -16.20 -16.25 -16.25 -16.31
K (MeV) 250.89 244.5 240.0 271.8 258.5
J (MeV) 32.3 33.1 32.5 37.9 38.3
m*/m 0.572 0.578 0.556 0.60 0.595
Nuclear Matter PropertiesNuclear Matter Properties
Masses: 900 keV
rms-deviations: masses: m = 900 keV radii: r = 0.015 fmrms-deviations: masses: m = 900 keV radii: r = 0.015 fmG.L., Niksic, Vretenar, Ring, PRC 71, 024312 (2005)
DD-ME2
SH-Elements
DD-ME2 Exp: Yu.Ts.Oganessian et al, PRC 69, 021601(R) (2004)
Superheavy Elements: Q-valuesSuperheavy Elements: Q-values
IS-GMRIsoscalar Giant Monopole: IS-GMRIsoscalar Giant Monopole: IS-GMR
The ISGMR represents the essential source of
experimental information on the nuclear
incompressibility
constraining the nuclear matter compressibility
RMF models reproduce the experimental data only if
250 MeV K0 270 MeV
Blaizot-concept:
T. Niksic et al., PRC 66 (2002) 024306
IV-GDRIsovector Giant Dipole: IV-GDRIsovector Giant Dipole: IV-GDR
the IV-GDR represents one of the sources of experimental informations on the nuclear matter symmetry energy
constraining the nuclear matter symmetry energy
32 MeV a4 36 MeV
the position of IV-GDR isreproduced if
T. Niksic et al., PRC 66 (2002) 024306
saturation density
LombardoLombardo
Relativistic (Q)RPA calculations of giant resonances
Isoscalar monopole response
Sn isotopes: DD-ME2 effectiveinteraction + Gogny pairing
Conclusions:Conclusions:
- Covariant Density Functional Theory provides Covariant Density Functional Theory provides a unified description of properties for ground a unified description of properties for ground states and excited states all over the periodic states and excited states all over the periodic tabletable
- The present functionals have 7-8 parameters.The present functionals have 7-8 parameters.- The density dependence (DD) is crucial:The density dependence (DD) is crucial: NL3 is has only DD in the T=0 channelNL3 is has only DD in the T=0 channel DD-ME1,… have also DD in the T=1 channelDD-ME1,… have also DD in the T=1 channel better neutron radiibetter neutron radii better neutron EOSbetter neutron EOS better symmetry energybetter symmetry energy consistent description of GDR and GMRconsistent description of GDR and GMR
Simpler parametrizations: - point coupling - simpler pairing
Improved energy functional: - Fock terms and tensor forces - why is the first order pion-exchange quenched? - is vacuum polarization important in finite nuclei?
-----Open Problems ------Open Problems:Open Problems: