Density matrices for atoms and solids. I. Effective potential matrix and the Bloch equation

By recognizing that the canonical density matrix C can be expressed in terms of an effective potential matrix, U , intimately related to the potential V in which the particles move, a powerful approximate analytic solution of the Bloch equation has been obtained. This solution for U reduces ( a ) to first-order perturbation theory on C when V is weak and ( b ) to the correct Thomas–Fermi result when V is almost constant in space. For an attractive defect centre in a metal, represented by a screened Coulomb potential which is not strong enough to bind an electron, it is shown that this approximate analytic solution may be used successfully in a numerical iterative solution of the Bloch equation and final numerical results are presented. For more strongly attractive centres, however, where bound states appear, the same numerical iterative scheme proves inadequate. A method is developed which orthogonalizes the approximate analytical density matrix to the wave function product for the lowest bound state. The new density matrix thereby formed is tested, and found to work successfully for an unscreened Coulomb field. This approach is then worked out for a screened potential created by a charge Z = 4 in a Fermi gas of density equal to that in Cu metal. Such a charged centre brings down a bound state from the conduction band and it is shown that the method employed successfully for the bare Coulomb field also leads to an accurate solution of the Bloch equation in this case. It is concluded that we have here a sufficiently powerful iterative scheme to carry out Hartree self-consistent calculations based on the Dirac density matrix, both for atoms, where the Fermi level lies in the bound state region, and for defects in metals, where the Fermi energy falls in the continuum. Such calculations are now in progress.

Recent work by Hilton, March & Curtis (1967) has shown how the Bloch density matrix may be calculated for an attractive scattering centre in a Fermi gas which is strong enough to lead to bound states. Using this pseudoatom description, and expressing the zero order approximation of independent pseudoatoms by writing the total partition function as a product of the single-centre functions, we develop a systematic procedure for calculating energy band structures. The convergence of the method depends on the magnitude of the overlaps of the effective potential matrix U introduced by Hilton, March & Curtis, for pseudoatoms on adjacent sites. To illustrate the method, calculation of the partition function of metallic Be is carried out from the earlier one-centre results for a charge Z = 4 in a Fermi gas. A preliminary estimate of the density of states in Be is reported, from this partition function.


Author(s):  
XD Dongfang

The quantum model of valence electron generation orbital penetration of alkali metal elements with unique stable structure is investigated. The electric field outside the atomic kernel is usually expressed by the Coulomb field of the point charge mode, and the composite electric field in atomic kernel can be equivalent to the electric field inside the sphere with uniform charge distribution or other electric fields without divergence point. The exact solutions of two Schrödinger equations for the bound state of the Coulomb field outside the atom and the binding state of the equivalent field inside the atom determine two different quantization energy formulas respectively. Here we show that the atomic kernel surface is the only common zero potential surface that can be selected. When the orbital penetration occurs, the law of conservation of energy requires that the energy level formulas of the two bound states must have corresponding quantum numbers to make them equal. As a result, there is no solution to the quantum number equation, indicating that the two quantum states of the valence electron are incompatible. This irreconcilable contradiction shows that the quantized energy of quantum mechanics cannot absolutely satisfy the law of conservation of energy.


2014 ◽  
Vol 29 (35) ◽  
pp. 1450180 ◽  
Author(s):  
N. Candemir ◽  
O. Bayrak

Bound state solutions of the Dirac equation for the generalized Woods–Saxon potential are examined for arbitrary κ states by using the approximation to the Coulomb and centrifugal potentials in pseudospin symmetry (PSS) and spin symmetry (SS) limits, respectively. The energy eigenvalues and corresponding eigenfunctions are obtained in closed forms. Some numerical examples are given for proton or anti-proton in a nucleus. The correlations between the energy splitting and some parameters of the effective potential in PSS limit are examined for several pseudospin doublets.


2020 ◽  
Vol 35 (23) ◽  
pp. 2050140
Author(s):  
Eduardo López ◽  
Clara Rojas

We solve the one-dimensional time-independent Klein–Gordon equation in the presence of a smooth potential well. The bound state solutions are given in terms of the Whittaker [Formula: see text] function, and the antiparticle bound state is discussed in terms of potential parameters.


2012 ◽  
Vol 2012 ◽  
pp. 1-15 ◽  
Author(s):  
M. Eshghi ◽  
M. Hamzavi ◽  
S. M. Ikhdair

The spatially dependent mass Dirac equation is solved exactly for attractive scalar and repulsive vector Coulomb potentials including a tensor interaction potential under the spin and pseudospin (p-spin) symmetric limits by using the Laplace transformation method (LTM). Closed forms of the energy eigenvalue equation and wave functions are obtained for arbitrary spin-orbit quantum number κ. Some numerical results are given too. The effect of the tensor interaction on the bound states is presented. It is shown that the tensor interaction removes the degeneracy between two states in the spin doublets. We also investigate the effects of the spatially-dependent mass on the bound states under the conditions of the spin symmetric limit and in the absence of tensor interaction (T=0).


2005 ◽  
Vol 14 (06) ◽  
pp. 931-947 ◽  
Author(s):  
F. PILOTTO ◽  
M. DILLIG

We investigate the influence of retardation effects on covariant 3-dimensional wave functions for bound hadrons. Within a quark-(scalar) diquark representation of a baryon, the four-dimensional Bethe–Salpeter equation is solved for a 1-rank separable kernel which simulates Coulombic attraction and confinement. We project the manifestly covariant bound state wave function into three dimensions upon integrating out the non-static energy dependence and compare it with solutions of three-dimensional quasi-potential equations obtained from different kinematical projections on the relative energy variable. We find that for long-range interactions, as characteristic in QCD, retardation effects in bound states are of crucial importance.


1992 ◽  
Vol 07 (09) ◽  
pp. 1935-1951 ◽  
Author(s):  
G.A. KOZLOV

A systematic discussion of the probability of eta and KL bound-state decays—[Formula: see text] and [Formula: see text](l=e, μ)—within a three-dimensional reduction to the two-body quantum field theory is presented. The bound-state vertex function depends on the relative momentum of constituent-like particles. A structure-transition form factor is defined by a confinement-type quark-antiquark wave function. The phenomenology of this kind of decays is analyzed.


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