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Orbital Euler-Lagrange equations

With fixed n, 0. for variations of occupied orbitals that are unconstrained in the orbital Hilbert space, the variational condition implies orbital Euler-Lagrange equations [Pg.58]

The orbital functional derivative here defines an effective Hamiltonian [Pg.58]

The theory is usually expressed in terms of canonical equations [Pg.58]


Orbital Euler-Lagrange equations are determined by functional derivatives... [Pg.65]

The Levy construction [222] can be used to prove Hohenberg-Kohn theorems for the ground state of any such theory. It should be noted that any explicit model of the Hohenberg-Kohn functional F[p] implies a corresponding orbital functional theory. The relevant density function p(r) is that constructed from an OFT ground state. This has the orbital decomposition , as postulated by Kohn and Sham [205]. Unlike the density p,, for an exact A-electron wave function T, which cannot be determined for most systems of interest, the OFT ground-state density function is constructed from explicit solutions of the orbital Euler-Lagrange equations, and the theory is self-contained. [Pg.69]

Euler-Lagrange Equation for Intra-Orbit Optimization of p(r) 206... [Pg.170]

Euler-Lagrange Equations for the Intra-Orbit Optimization of... [Pg.170]

As indicated in Fig. 7, the next step after either an explicit or an implicit energy density functional orbit optimization procedure. For this purpose, one introduces the auxiliary functional Q[p(r) made up of the energy functional [p(r) 9 ]. plus the auxiliary conditions which must be imposed on the variational magnitudes. Notice that there are many ways of carrying out this variation, but that - in general - one obtains Euler-Lagrange equations by setting W[p(r) = 0. [Pg.206]

The computational effort of solving orbital Euler-Lagrange (OEL) equations is significantly reduced if the generally nonlocal exchange-correlation potential vxc can be replaced or approximated by a local potential vxc(r). A variationally defined optimal local potential is determined using the optimized effective potential (OEP) method [380, 398]. This method can be applied to any theory in which the model... [Pg.65]

A modified effective Hamiltonian Goep is defined by replacing vxc by a model local potential vxc(r). The energy functional is made stationary with respect to variations of occupied orbitals that are determined by modified OEL equations in which Q is replaced by Goep- 84>i is determined by variations 8vxc(r) in these modified OEL equations. To maintain orthonormality, <5, can be constrained to be orthogonal to all occupied orbitals of the OEP trial state , so that (r) = J]a(l — na)i). First-order perturbation theory for the OEP Euler-Lagrange equations implies that... [Pg.66]

It is assumed that Ec is so defined that the functional E is minimized for ground states. Ground-state orbital functions and the density function are determined by Euler-Lagrange equations expressed in terms of functional derivatives of E. For any density or orbital functional, with fixed n, infinitesimal orbital variations determine the functional variation... [Pg.4]

Euler-Lagrange equation for intra-orbit optimization of p(r, s)... [Pg.95]

Let us consider now the energy density functional [/j(r,a) W] of Eq. (50). In this functional, p r, 5) stands for any one of the final densities generated from the initial density pg(r,s) coming from the orbit-generating wavefunction W. Clearly, the extremum of this functional is attained at the optimal density /> t(r,s). This density satisfies the Euler-Lagrange equation arising from the variation of the functional [/>(r,a) M] - subject to the normalization condition f d xp(r,s) = N -with respect to the one-particle density p(r, s). Explicitly, this amounts to varying the auxiliary functional... [Pg.95]

Euler-Lagrange equations for the intra-orbit optimization of N orthonormal orbitals Kohn-Sham-like equations... [Pg.97]

Orbit Variational Principle and Euler-Lagrange Equation... [Pg.89]

As the electronic energy is a function of the nuclear positions as well as function of the orbitals (/ , its derivative is taken with respect to the nuclear positions but also with respect to the wavefunction. The Euler-Lagrange equations then read... [Pg.115]

The equations of motion corresponding to eqn [9] are obtained from the associated Euler-Lagrange equations, that for the orbitals read... [Pg.428]

Here, is the expectation value of the hamiltonian operator with a single-determinant wave function. The second term comes from the orthonormalization condition of the molecular orbitals, while the third one arises from each population restriction. The Euler-Lagrange equations from this problem lead to a matrix problem similar to Eq. (15) ... [Pg.34]


See other pages where Orbital Euler-Lagrange equations is mentioned: [Pg.58]    [Pg.157]    [Pg.2]    [Pg.10]    [Pg.58]    [Pg.157]    [Pg.2]    [Pg.10]    [Pg.425]    [Pg.298]    [Pg.55]    [Pg.63]    [Pg.65]    [Pg.70]    [Pg.88]    [Pg.5]    [Pg.73]    [Pg.247]    [Pg.201]    [Pg.4]    [Pg.436]   
See also in sourсe #XX -- [ Pg.58 ]

See also in sourсe #XX -- [ Pg.9 , Pg.10 ]




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Derivation orbital Euler-Lagrange equations

Euler

Euler equation

Euler-Lagrange

Euler-Lagrange equations

Lagrange

Lagrange equations

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