Module P10.4 The Schrödinger equation
... eigenfunctions, then the energy of that particle may be predicted with certainty. It is the eigenvalue equation for energy, more often referred to as the time-independent Schrödinger equation, that will be our main concern in this module. Section 2 reviews the notion of a de Broglie wave, and introd ...
... eigenfunctions, then the energy of that particle may be predicted with certainty. It is the eigenvalue equation for energy, more often referred to as the time-independent Schrödinger equation, that will be our main concern in this module. Section 2 reviews the notion of a de Broglie wave, and introd ...
Canonically conjugate pairs and phase operators
... from zero to infinity. For the case of fermions with a filled Dirac sea one often works with the number operator relative to the Dirac sea which has integer eigenvalues which run from minus infinity to plus infinity4–6 . A conceptionally simple P∞ case where the number operator is of the form N = −∞ ...
... from zero to infinity. For the case of fermions with a filled Dirac sea one often works with the number operator relative to the Dirac sea which has integer eigenvalues which run from minus infinity to plus infinity4–6 . A conceptionally simple P∞ case where the number operator is of the form N = −∞ ...
Derivation Of The Schwarzschild Radius Without General
... primitive form of quantum gravity). In this paper I have chosen the method based on the Planck units. In 2014 I published an article entitled The Special Quantum Gravitational Theory of Black Holes (Wormholes and Cosmic Time Machines) [2] where I derived (a) a general formula for the temperature of ...
... primitive form of quantum gravity). In this paper I have chosen the method based on the Planck units. In 2014 I published an article entitled The Special Quantum Gravitational Theory of Black Holes (Wormholes and Cosmic Time Machines) [2] where I derived (a) a general formula for the temperature of ...
