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Pauli equation exclusion principle

We will soon encounter the enormous consequences of this antisymmetry principle, which represents the quantum-mechanical generalization of Pauli s exclusion principle ( no two electrons can occupy the same state ). A logical consequence of the probability interpretation of the wave function is that the integral of equation (1-7) over the full range of all variables equals one. In other words, the probability of finding the N electrons anywhere in space must be exactly unity,... [Pg.23]

The rotational coordinates are Q 2 and Q 5. The rotational motion can be visualized by mapping the trough onto the surface of a 2D sphere the rotation is governed by the usual polar coordinate definitions, 6 and . This is also shown in equation (7) which has the usual form for a rotator with spherical harmonic solutions Ylm. The solutions will be written in the form I i//lo, hn ). For the high spin states case, it was found that l must be odd in order to obey the Pauli s exclusion principle and preserve the antisymmetric nature of the total wavefunctions at any point on the trough under symmetric operations [26]. In the current case, similar arguments show that l must be even. This is because the electronic basis is even under inversion and the whole vibronic wavefunction must also be even under inversion. A general mathematical proof can be found in Ref. [23],... [Pg.327]

Pauli s exclusion principle imposes that either (ri, r2) or x(si, S2) must be odd (the other one remaining even) with respect to the interchange of indices 1 and 2. If the Coulomb repulsion t/(ri, r2) = e /47reo ri - r2 between both electrons is small, this contribution to the Hamiltonian H may be considered as a perturbation. Let (Pair) (respectively, b(r)) be the eigenstate of the Hamiltonian Hi = Ti =p l2m (respectively, H2 = T2 =p /2m) characterized by the eigenvalue (respectively, E, ). In this framework, this approximation allows us to solve the well-known secular equation det(H - El) = 0 (where 1 is the identity matrix and H=Ti + T2 + U(ri, V2)). hi the subspace spanned by the spatially symmetrical and antisymmetrical wave functions (Psiri, V2) and (Phiri, V2) containing functions a(ri) and hiri), we have ... [Pg.211]

In atoms with more than one electron, wave functions should include the coordinates of each particle, and a new term representing the electrostatic interactions between electrons. Even for the case of only two electrons, such a wave equation is so complex that it has never been solved exactly. To analyse multielectron atoms some approximations have to be made. The most practical one is to assume that the electron considered moves in an electrical potential that is a combination of all other electrons and the nucleus, and that this potential has spherical symmetry. This approximation has proven very useful, as it allows a description of energy states in a similar manner to that employed for the H atom by using a comparable set of four quantum numbers. An important, additional condition appears no two electrons can have the same set of quantum numbers in other words, no more than one electron can occupy the same energy state. This is Pauli s exclusion principle. [Pg.103]

The above treatment can be extended to a semiconductor with the additional conditions that momentum conservation and Pauli s exclusion principle must hold [36]. As described in Equation 3.6, modifying the rate equations for semiconductors would for stimulated absorption lead to (rates are given in units s m )... [Pg.142]

While the two equations look similar, in Equation 1.12 a stands for the four quantum numbers n, I, mi and m, which describe the state of each i of the N electrons. These permutate to generate equally valid states following Pauli s exclusion principle, to yield anti-symmetric wave functions in the central field, which are solutions to the Schrodinger equation (Equation 1.4). [Pg.7]

Because single-electron wave functions are approximate solutions to the Schroe-dinger equation, one would expect that a linear combination of them would be an approximate solution also. For more than a few basis functions, the number of possible lineal combinations can be very large. Fortunately, spin and the Pauli exclusion principle reduce this complexity. [Pg.255]

Intrinsic Semiconductors. For semiconductors in thermal equiHbrium, (Ai( )), the average number of electrons occupying a state with energy E is governed by the Fermi-Dirac distribution. Because, by the Pauli exclusion principle, at most one electron (fermion) can occupy a state, this average number is also the probabiHty, P E), that this state is occupied (see Fig. 2c). In equation 2, K... [Pg.345]

The fundamental laws which determine the behavior of an electronic system are the Schrodinger equation (Eq. II. 1) and the Pauli exclusion principle expressed in the form of the antisymmetry requirement (Eq. II.2). We note that even the latter auxiliary condition introduces a certain correlation between the movements of the electrons. [Pg.217]

Introduction of the half-integral spin of the electrons (values h/2 and —fe/2) alters the above discussion only in that a spin coordinate must now be added to the wavefunctions which would then have both space and spin components. This creates four vectors (three space and one spin component). Application of the Pauli exclusion principle, which states that all wavefunctions must be antisymmetric in space and spin coordinates for all pairs of electrons, again results in the T-state being of lower energy [equations (9) and (10)]. [Pg.63]

A spinning electron also has a spin quantum number that is expressed as 1/2 in units of ti. However, that quantum number does not arise from the solution of a differential equation in Schrodinger s solution of the hydrogen atom problem. It arises because, like other fundamental particles, the electron has an intrinsic spin that is half integer in units of ti, the quantum of angular momentum. As a result, four quantum numbers are required to completely specify the state of the electron in an atom. The Pauli Exclusion Principle states that no two electrons in the same atom can have identical sets of four quantum numbers. We will illustrate this principle later. [Pg.45]

In Eq. (1.16a), A is the antisymmetrizer operator that converts the orbital product into a Slater determinant, insuring satisfaction of the Pauli exclusion principle. In this equation (alone), the same spatial orbital might appear twice, with different indices to indicate the change in spin. For example, / i (0,(7 ypf HA) might be the same as i<0)(F K/>,0,0" 2). a doubly occupied spatial orbital (n]m> = 2), with a bar denoting opposite spin in the second spin-orbital. [Pg.43]

Equation 4.49 defines the exchange or Fermi hole. It is as if an electron of a given spin digs a hole around itself in space in order to exclude another electron of the same spin from coming near it (Pauli exclusion principle). The integrated hole charge is unity, i.e., there is exactly one electron inside the hole. Likewise, the correlation energy functional can be defined as... [Pg.51]

Further, if the wave function depends also on the electron spins, spin variables over all electrons should also be integrated we will see this below, in the calculation of exchange hole. The expression in the curly brackets above is exactly the XC hole PxCM(r, r ) defined in Equation 7.17. A comparison with Equation 7.19a shows that adding the hole to the density is similar to subtracting the density of one electron p(r )/N from it. The hole thus represents a deficit of one electron from the density. This is easily verified by integrating p tM(V, r ) over the volume dr, which gives a value of — 1. However, the structure of the hole is not simple and this is because of the motion of different electrons correlated due to the Pauli exclusion principle and the Coulomb interaction between them. Finally we note that the product p(r)p cM(r, r ) is symmetric with respect to an exchange in the variables... [Pg.88]

Every atom shows specific, discrete energy levels for electrons. These levels are either empty or occupied by one or two (spin-paired) electrons according to the Pauli exclusion principle. The energy of the levels can be found by solving the Schrodinger equation. Exact solutions, however, can only be obtained for single electron atoms (hydrogenic atoms). [Pg.150]

Here, the summation goes over all the individual electron wave functions that are occupied by electrons, so the term inside the summation is the probability that an electron in individual wave function ijx((r) is located at position r. The factor of 2 appears because electrons have spin and the Pauli exclusion principle states that each individual electron wave function can be occupied by two separate electrons provided they have different spins. This is a purely quantum mechanical effect that has no counterpart in classical physics. The point of this discussion is that the electron density, n r), which is a function of only three coordinates, contains a great amount of the information that is actually physically observable from the full wave function solution to the Schrodinger equation, which is a function of 3N coordinates. [Pg.10]

In addition to the Coulombic forces, there is a repulsive force which operates at short distances between ions as a result of the overlapping of filled orbitals, potentially a violation of the Pauli exclusion principle. This repulsive force may be represented by the equation ... [Pg.158]


See other pages where Pauli equation exclusion principle is mentioned: [Pg.4]    [Pg.33]    [Pg.123]    [Pg.65]    [Pg.34]    [Pg.130]    [Pg.408]    [Pg.20]    [Pg.32]    [Pg.429]    [Pg.201]    [Pg.10]    [Pg.3]    [Pg.13]    [Pg.89]    [Pg.548]    [Pg.437]    [Pg.442]    [Pg.21]    [Pg.23]    [Pg.123]    [Pg.19]    [Pg.113]    [Pg.974]    [Pg.23]    [Pg.248]   
See also in sourсe #XX -- [ Pg.7 , Pg.48 , Pg.323 ]




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