Short introduction to quantum mechanics
... . By completely is implied that the function Ψ(q1 , q2 , q3 , ..., qn ; t) contains all information obtainable by experiments. The qi , i = 1, .., n, are called characteristic variables such as space coordinates, t is the time dependence. The functions Ψ are called state functions or wavefunctions. ...
... . By completely is implied that the function Ψ(q1 , q2 , q3 , ..., qn ; t) contains all information obtainable by experiments. The qi , i = 1, .., n, are called characteristic variables such as space coordinates, t is the time dependence. The functions Ψ are called state functions or wavefunctions. ...
Theory and simulation of polar and nonpolar polarizable fluids
... we study both kinds of fluids. In fluids containing polar molecules that are also polarizable the molecules are modeled as anisotropic Drude oscillators in which the electronic motion along the direction of the permanent dipole and perpendicular to it have different force constants, or equivalently ...
... we study both kinds of fluids. In fluids containing polar molecules that are also polarizable the molecules are modeled as anisotropic Drude oscillators in which the electronic motion along the direction of the permanent dipole and perpendicular to it have different force constants, or equivalently ...
Quantum Field Theory in a Non-Commutative Space: Sphere ?
... expects to observe deviations with respect to the quantum theory on the commutative sphere. Although the derivation of the non-commutative anomaly in [61] was worked out for the µ2 > 0 case, one may expect that a similar phenomenon occurs when µ2 < 0, too. For QFT on the commutative sphere, the latt ...
... expects to observe deviations with respect to the quantum theory on the commutative sphere. Although the derivation of the non-commutative anomaly in [61] was worked out for the µ2 > 0 case, one may expect that a similar phenomenon occurs when µ2 < 0, too. For QFT on the commutative sphere, the latt ...
Kinetics of decay of metastable gas phase of polarized atomic
... background (see Ref. 8). This decrease of the energy A& increases with decreasing density, and if l AE l becomes larger than 2p,H, then the process of depolarization will have no threshold. Close to the usual density of the condensed state, the parameter I AE I is replaced by the width of the energy ...
... background (see Ref. 8). This decrease of the energy A& increases with decreasing density, and if l AE l becomes larger than 2p,H, then the process of depolarization will have no threshold. Close to the usual density of the condensed state, the parameter I AE I is replaced by the width of the energy ...
Elements of QFT in Curved Space-Time
... There are covariant equations for the matter (fields and particles, fluids etc) and Einstein equations for the gravitational field gµν ...
... There are covariant equations for the matter (fields and particles, fluids etc) and Einstein equations for the gravitational field gµν ...
Fast converging path integrals for time-dependent potentials
... and W represents the ideal effective potential, which ensures the exactness of the above expression. The latter depends not only on the coordinate mid-point x = (a + b)/2, the discretized velocity δ = b − a, and the time interval ε = tb − ...
... and W represents the ideal effective potential, which ensures the exactness of the above expression. The latter depends not only on the coordinate mid-point x = (a + b)/2, the discretized velocity δ = b − a, and the time interval ε = tb − ...