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Time-Dependent Density Functional Theory (TDDFT) part-2
Takashi NAKATSUKASA Theoretical Nuclear Physics Laboratory RIKEN Nishina Center Density-Functional Theory (DFT) Time-dependent DFT (TDDFT) Applications CNS-EFES Summer RIKEN Nishina Hall
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Time-dependent HK theorem
First theorem Runge & Gross (1984) One-to-one mapping between time-dependent density ρ(r,t) and time-dependent potential v(r,t) except for a constant shift of the potential Condition for the external potential: Possibility of the Taylor expansion around finite time t0 The initial state is arbitrary. This condition allows an impulse potential, but forbids adiabatic switch-on.
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Schrödinger equation:
Current density follows the equation (1) Different potentials, v(r,t) , v’(r,t), make time evolution from the same initial state into Ψ(t)、Ψ’(t) Continuity eq.
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Problem: Two external potentials are different, when their expansion
has different coefficients at a certain order Using eq. (1), show
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Second theorem The universal density functional exists, and the variational principle determines the time evolution. From the first theorem, we have ρ(r,t) ↔Ψ(t). Thus, the variation of the following function determines ρ(r,t) . The universal functional is determined. v-representative density is assumed.
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Time-dependent KS theory
Assuming non-interacting v-representability Time-dependent Kohn-Sham (TDKS) equation Solving the TDKS equation, in principle, we can obtain the exact time evolution of many-body systems. The functional depends on ρ(r,t) and the initial state Ψ0 .
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Time-dependent quantities → Information on excited states
Energy projection Finite time period → Finite energy resolution
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Time Domain Energy Domain Basic equations Time-dep. Schroedinger eq.
Time-dep. Kohn-Sham eq. dx/dt = Ax Energy resolution ΔE〜ћ/T All energies Boundary Condition Approximate boundary condition Easy for complex systems Basic equations Time-indep. Schroedinger eq. Static Kohn-Sham eq. Ax=ax (Eigenvalue problem) Ax=b (Linear equation) Energy resolution ΔE〜0 A single energy point Boundary condition Exact scattering boundary condition is possible Difficult for complex systems
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Photoabsorption cross section of rare-gas atoms
Zangwill & Soven, PRA 21 (1980) 1561
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TDHF(TDDFT) calculation in 3D real space
H. Flocard, S.E. Koonin, M.S. Weiss, Phys. Rev. 17(1978)1682.
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3D lattice space calculation Application of the nuclear Skyrme-TDHF technique to molecular systems
Local density approximation (except for Hartree term) →Appropriate for coordinate-space representation Kinetic energy is estimated with the finite difference method
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Real-space TDDFT calculations
Time-Dependent Kohn-Sham equation 3D space is discretized in lattice Each Kohn-Sham orbital: N : Number of particles Mr : Number of mesh points Mt : Number of time slices y K. Yabana, G.F. Bertsch, Phys. Rev. B54, 4484 (1996). T. Nakatsukasa, K. Yabana, J. Chem. Phys. 114, 2550 (2001). X
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Calculation of time evolution
Time evolution is calculated by the finite-order Taylor expansion Violation of the unitarity is negligible if the time step is small enough: The maximum (single-particle) eigenenergy in the model space
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Real-time calculation of response functions
Weak instantaneous external perturbation Calculate time evolution of Fourier transform to energy domain ω [ MeV ]
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1. External perturbation t=0
Real-time dynamics of electrons in photoabsorption of molecules 1. External perturbation t=0 2. Time evolution of dipole moment E at t=0 Ethylene molecule
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TDDFT Exp Comparison with measurement (linear optical absorption)
TDDFT accurately describe optical absorption Dynamical screening effect is significant PZ+LB94 with Dynamical screening without TDDFT Exp + - Without dynamical screening (frozen Hamiltonian) T. Nakatsukasa, K. Yabana, J. Chem. Phys. 114(2001)2550.
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Photoabsorption cross section in C3H6 isomer molecules
Nakatsukasa & Yabana, Chem. Phys. Lett. 374 (2003) 613. TDLDA cal with LB94 in 3D real space 33401 lattice points (r < 6 Å) Isomer effects can be understood in terms of symmetry and anti-screening effects on bound-to-continuum excitations. Cross section [ Mb ] Photon energy [ eV ]
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Nuclear response function Dynamics of low-lying modes and giant resonances
Skyrme functional is local in coordinate space → Real-space calculation Derivatives are estimated by the finite difference method.
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Skyrme TDHF in real space
Time-dependent Hartree-Fock equation 3D space is discretized in lattice Single-particle orbital: N: Number of particles Mr: Number of mesh points Mt: Number of time slices y [ fm ] Spatial mesh size is about 1 fm. Time step is about 0.2 fm/c Nakatsukasa, Yabana, Phys. Rev. C71 (2005) X [ fm ]
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E1 resonances in 16,22,28O 16O 22O 28O 50 σ [ mb ]
Leistenschneider et al, PRL86 (2001) 5442 50 22O Berman & Fultz, RMP47 (1975) 713 σ [ mb ] 50 20 40 28O SGII parameter set Г=0.5 MeV Note: Continnum is NOT taken into account ! E1 resonances in 16,22,28O σ [ mb ] 20 40 E [ MeV ]
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18O 16O Prolate 10 30 20 40 Ex [ MeV ]
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26Mg 24Mg Ex [ MeV ] Ex [ MeV ] Prolate Triaxial 10 20 30 40 10 20 30
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28Si 30Si Oblate Oblate 10 20 30 40 Ex [ MeV ] 10 20 30 40 Ex [ MeV ]
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44Ca 48Ca 40Ca Ex [ MeV ] Ex [ MeV ] Ex [ MeV ] Prolate 10 20 30 10 20
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Giant dipole resonance in stable and unstable nuclei
Classical image of GDR p n
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Choice of external fields
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Neutrons 16O Time-dep. transition density δρ> 0 δρ< 0 Protons
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Skyrme HF for 8,14Be 8Be 14Be ∆r=12 fm R=8 fm Adaptive coordinate x z
Neutron Proton S.Takami, K.Yabana, and K.Ikeda, Prog. Theor. Phys. 94 (1995) 1011.
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8Be Solid: K=1 Dashed: K=0 14Be
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Peak at E〜6 MeV 14Be
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Picture of pygmy dipole resonance
Halo neutrons Neutrons Protons n Core n p Ground state Low-energy resonance
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Nuclear Data by TDDFT Simulation
T.Inakura, T.N., K.Yabana Ground-state properties Create all possible nuclei on computer Investigate properties of nuclei which are impossible to synthesize experimentally. Application to nuclear astrophysics, basic data for nuclear reactor simulation, etc. n Photoabsorption cross sections TDDFT Kohn-Sham equation n Real-time response of neutron-rich nuclei
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Non-linear regime (Large-amplitude dynamics)
N.Hinohara, T.N., M.Matsuo, K.Matsuyanagi Quantum tunneling dynamics in nuclear shape-coexistence phenomena in 68Se Cal Exp
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Summary (Time-dependent) Density functional theory assures the existence of functional to reproduce exact many-body dynamics. Any physical observable is a functional of density. Current functionals rely on the Kohn-Sham scheme Applications are wide in variety; Nuclei, Atoms, molecules, solids, … We show TDDFT calculations of photonuclear cross sections using a Skyrme functional. Toward theoretical nuclear data table
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Postdoctoral opportunity at RIKEN
Click on “Carrier Opportunity” FPR (Foreign Postdoctoral Researcher)
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