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Quantum mechanics density matrices

A more complete version of the second postulate assumes random a priori phases of the time-dependent factors in the wave functions and involves quantum-mechanical density matrices. We present only the simplest version of statistical mechanics. [Pg.1043]

A number of procedures have been proposed to map a wave function onto a function that has the form of a phase-space distribution. Of these, the oldest and best known is the Wigner function [137,138]. (See [139] for an exposition using Louiville space.) For a review of this, and other distributions, see [140]. The quantum mechanical density matrix is a matrix representation of the density operator... [Pg.270]

H. Nakatsuji and K. Yasuda, Direct determination of the quantum-mechanical density matrix using the density equation. Phys. Rev. Lett. 76, 1039 (1996). [Pg.56]

The quantitative characteristic of the alignment created is given, as already stated, by multipole moments of even rank. A more rigorous treatment of the expansion of the quantum mechanical density matrix over irreducible tensorial operators will be performed later, in Chapter 5 and in Appendix D. As an example we will write the zero, second and fourth rank polarization moments and [Pg.62]

Expressions which would be applicable for arbitrary angular momentum values can be obtained by using the quantum mechanical density matrix. [Pg.68]

In the present book we have used the cogredient expansion form (2.14), where, as distinct from the standard form, an additional normalizing factor has been introduced, namely (—l)< v/(2K + l)/4n. Our expansion of the classical probability density p(0, differs from the standard one in exactly the same way as the expansion of the quantum mechanical density matrix p over 2Tq differs from the expansion over lTg. In Section 5.3 we present a comparison between the physical meaning of the classical polarization moments pg, as used in the present book, and the quantum mechanical polarization moments fg, as determined by the cogredient method using normalization (D.ll). [Pg.263]

Numerical values of c(K), v(K), for K < 4 are given in Table D.3. For expansion coefficients we use, following [249, 251], the same notation Aq as for the expansion coefficients of the quantum mechanical density matrix over real Tq . Such a choice of notation may be justified by the fact that classical Aq constitute an asymptotic limit of quantum mechanical... [Pg.265]

The method of Feynman paths is based on generating the diagonal terms in the quantum mechanical density matrix. For a Hamiltonian with discrete eigenstates ... [Pg.43]

Employing the quantum mechanical density matrix formalism it is possible to take into account the whole reaction pathway of Fig. 21.12 where both coherent and incoherent reaction pathways are present in the case of a PHIP experiment and convert the PHIP experiment into a diagnostic tool for all stages of a hydrogenation reaction. Such an analysis was performed in Ref [62]. In these calculations the initial condition was that at the start of the reaction all molecules are in the P-H2 state of site C, i.e., a pure singlet spin state, represented as a circle in Fig. 21.12, which shows the different possible reaction pathways. Moreover, all in-termolecular exchange reactions were treated as one-sided reactions, i.e. the rates of the back reactions were set to zero. [Pg.665]

Fortunately, progress can be made because the Heisenberg operator involved in the evolution of time correlation functions or the quantum mechanical density matrix involves not only the forward time evolution operator but also its inverse. It is well understood that a dramatic phase cancellation takes place between these two propagation steps upon integration, and this cancellation is entirely responsible for the failure of Monte Carlo methods. To remedy this situation, Mgtoi and Thompson proposed a forward-backward semiclassical approximation (36) in which the time evolution operator and its inverse are combined into a single semiclassical treatment. This procedure is equivalent to a sta-... [Pg.403]

This chapter deals with the analogous quantum mechanical problem. Within the limitations imposed by its nature as expressed, for example, by Heisenberg-type uncertainty principles, the Schrodinger equation is deterministic. Obviously it describes a deterministic evolution of the quantum mechanical wavefunction. The analog of the phase space probability density f (r, p f) is now the quantum mechanical density operator (often referred to as the density matrix ), whose time evolution is detennined by the quantum Liouville equation. Again, when the system is fully described in terms of a well specified initial wavefunction, the two descriptions are equivalent. The density operator formalism can, however, be carried over to situations where the initial state of the system is not well characterized and/or... [Pg.347]

A diagrannnatic approach that can unify the theory underlymg these many spectroscopies is presented. The most complete theoretical treatment is achieved by applying statistical quantum mechanics in the fonn of the time evolution of the light/matter density operator. (It is recoimnended that anyone interested in advanced study of this topic should familiarize themselves with density operator fonnalism [8, 9, 10, H and f2]. Most books on nonlinear optics [13,14, f5,16 and 17] and nonlinear optical spectroscopy [18,19] treat this in much detail.) Once the density operator is known at any time and position within a material, its matrix in the eigenstate basis set of the constituents (usually molecules) can be detennined. The ensemble averaged electrical polarization, P, is then obtained—tlie centrepiece of all spectroscopies based on the electric component of the EM field. [Pg.1180]

Fane U 1957 Description of states in quantum mechanics by density matrix and operator techniques Rev. Mod. Phys. 29 74-93... [Pg.1225]

Thus, HyperChem occasionally uses a three-point interpolation of the density matrix to accelerate the convergence of quantum mechanics calculations when the number of iterations is exactly divisible by three and certain criteria are met by the density matrices. The interpolated density matrix is then used to form the Fock matrix used by the next iteration. This method usually accelerates convergent calculations. However, interpolation with the MINDO/3, MNDO, AMI, and PM3 methods can fail on systems that have a significant charge buildup. [Pg.230]

Chirgwin, B. H., Phys. Rev. 107, 1013, Summation convention and the density matrix in quantum mechanics. ... [Pg.351]

The treatment developed here is based on the density matrix of quantum mechanics and extends previous work using wavefunctions.(42 5) The density matrix approach treats all energetically accessible electronic states in the same fashion, and naturally leads to average effective potentials which have been shown to give accurate results for electronically diabatic collisions. 19) The approach is taken here for systems where the dynamics can be described by a Hamiltonian operator, as it is possible for isolated molecules or in models where environmental effects can be represented by terms in an effective Hamiltonian. [Pg.319]

Dead time A very short delay introduced before the start of acquisition that allows the transmitter gate to close and the receiver gate to open. Density matrix A description of the state of nuclei in quantum mechanical terms. [Pg.413]


See other pages where Quantum mechanics density matrices is mentioned: [Pg.58]    [Pg.59]    [Pg.116]    [Pg.476]    [Pg.330]    [Pg.342]    [Pg.622]    [Pg.342]    [Pg.255]    [Pg.158]    [Pg.21]    [Pg.499]    [Pg.276]    [Pg.1274]    [Pg.632]    [Pg.725]    [Pg.173]   
See also in sourсe #XX -- [ Pg.126 , Pg.127 , Pg.128 ]




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