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  2. Wave function - Wikipedia

    en.wikipedia.org/wiki/Wave_function

    Download as PDF; Printable version ... equation does take the form of a wave equation. ... of wavefunction in Schrodinger's time dependent wave equation, ...

  3. Schrödinger equation - Wikipedia

    en.wikipedia.org/wiki/Schrödinger_equation

    The time-dependent Schrödinger equation described above predicts that wave functions can form standing waves, called stationary states. These states are particularly important as their individual study later simplifies the task of solving the time-dependent Schrödinger equation for any state.

  4. Matter wave - Wikipedia

    en.wikipedia.org/wiki/Matter_wave

    Beyond the equations of motion, other aspects of matter wave optics differ from the corresponding light optics cases. Sensitivity of matter waves to environmental condition. Many examples of electromagnetic (light) diffraction occur in air under many environmental conditions.

  5. Relativistic wave equations - Wikipedia

    en.wikipedia.org/wiki/Relativistic_wave_equations

    Weyl found a relativistic equation in terms of the Pauli matrices; the Weyl equation, for massless spin-⁠ 1 / 2 ⁠ fermions. The problem was resolved by Dirac in the late 1920s, when he furthered the application of equation to the electron – by various manipulations he factorized the equation into the form:

  6. and this is the Schrödinger equation. Note that the normalization of the path integral needs to be fixed in exactly the same way as in the free particle case. An arbitrary continuous potential does not affect the normalization, although singular potentials require careful treatment.

  7. Rectangular potential barrier - Wikipedia

    en.wikipedia.org/wiki/Rectangular_potential_barrier

    In classical wave-physics, this effect is known as evanescent wave coupling. The likelihood that the particle will pass through the barrier is given by the transmission coefficient, whereas the likelihood that it is reflected is given by the reflection coefficient. Schrödinger's wave-equation allows these coefficients to be calculated.

  8. Energy operator - Wikipedia

    en.wikipedia.org/wiki/Energy_operator

    The Schrödinger equation describes the space- and time-dependence of the slow changing (non-relativistic) wave function of a quantum system. The solution of the Schrödinger equation for a bound system is discrete (a set of permitted states, each characterized by an energy level ) which results in the concept of quanta .

  9. Normalized solutions (nonlinear Schrödinger equation)

    en.wikipedia.org/wiki/Normalized_solutions...

    The nonlinear Schrödinger equation (NLSE) is a fundamental equation in quantum mechanics and other various fields of physics, describing the evolution of complex wave functions. In Quantum Physics, normalization means that the total probability of finding a quantum particle anywhere in the universe is unity.