Quantum states in phase space • classical vs. quantum statistics
... • classical vs. quantum statistics, quasi-probability distributions • operator expansion in phase space Classical vs. quantum statistics, quasi-probability distributions: The phase-space picture we have developed in the last lecture for coherent and squeezed states is not quite correct as it cannot ...
... • classical vs. quantum statistics, quasi-probability distributions • operator expansion in phase space Classical vs. quantum statistics, quasi-probability distributions: The phase-space picture we have developed in the last lecture for coherent and squeezed states is not quite correct as it cannot ...
Quantum transport equations for Bose systems taking into account
... The problems of building a kinetic equation for Bose systems based on the microscopic approach were considered by Akhiezer and Peletminsky [21] and by Kirkpatrick and Dorfman [22–24]. The results of [22, 23] were extended and used to describe the trapped weakly-interacting Bose gases at finite temper ...
... The problems of building a kinetic equation for Bose systems based on the microscopic approach were considered by Akhiezer and Peletminsky [21] and by Kirkpatrick and Dorfman [22–24]. The results of [22, 23] were extended and used to describe the trapped weakly-interacting Bose gases at finite temper ...
Solving the Time-Independent Schrödinger Equation Abstract
... values of E are allowed, so the energy levels are quantized. This also suggests a way to determine the solutions numerically. We start at the center of the well with a specified ψ and ψ 0 = 0, guess a value of E and integrate forward past the edge of the well. If the solution is diverging there, cha ...
... values of E are allowed, so the energy levels are quantized. This also suggests a way to determine the solutions numerically. We start at the center of the well with a specified ψ and ψ 0 = 0, guess a value of E and integrate forward past the edge of the well. If the solution is diverging there, cha ...
powerpoint
... and, depending on the relative orientations of the two moments, orbital energy can be slightly altered. We use the so-called Na D line as a paradigm. We use the first-order perturbation theory to describe the shifts in orbital energies. The spin-orbit interaction is a relativistic effect and its der ...
... and, depending on the relative orientations of the two moments, orbital energy can be slightly altered. We use the so-called Na D line as a paradigm. We use the first-order perturbation theory to describe the shifts in orbital energies. The spin-orbit interaction is a relativistic effect and its der ...
An Ab Initio Study of the Hydrogen Chloride – Ammonia Complex
... Taking in account this approximations and the fact that the first non-adiabatic couplings are zero for all except spatially degenerate wavefunctions ...
... Taking in account this approximations and the fact that the first non-adiabatic couplings are zero for all except spatially degenerate wavefunctions ...
The Interaction of Radiation and Matter: Quantum
... can be analyzed completely since the first term on the RHS of Equation [ VII-6 ] -- the damping term-- contains only the system variable. In general, this feedback term will included reservoir variables as well and the simplified model breaks down. The general case may, however, be analyzed if we ta ...
... can be analyzed completely since the first term on the RHS of Equation [ VII-6 ] -- the damping term-- contains only the system variable. In general, this feedback term will included reservoir variables as well and the simplified model breaks down. The general case may, however, be analyzed if we ta ...
Generalized variational principle for excited states using nodes of
... and inner have 1S symmetry, this is automatically satisfied and ensures that our theorem provides a true upper bound to the 1s2s 1S state. This kind of argument could be applied to other selected excited states of many-electron systems as well. In order to compute the expectation values of the Hami ...
... and inner have 1S symmetry, this is automatically satisfied and ensures that our theorem provides a true upper bound to the 1s2s 1S state. This kind of argument could be applied to other selected excited states of many-electron systems as well. In order to compute the expectation values of the Hami ...
