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Particle in a box - MIT OpenCourseWare
Particle in a box - MIT OpenCourseWare

... In 1877 he went to Berlin for a year of study with physicists Helmholtz and Kirchhoff. He wrote that Kirchhoff spoke in carefully prepared lectures which were dry and monotonous. He eventually became Kirchhoff’s successor in Berlin. The concept of the photon was initially rejected by Planck. He wrot ...
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... According to the investigations presented in the cited literature [2, 3] it is obvious that the classical theory gives the correct results only in a limited field of application. Thus, the qualifying theories are highly developing and widely applying at present time. In this paper we consider a thin ...
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... lowering relations (recall that for the 1D HO, a †n\ = n + 1 †n + 1\). Following the usual arguments, one finds that a complete set of energy eigenstates can be chosen to be °nx ny ] where nx , ny = 0, 1, 2, … The eigenenergies are Enx ny = nx + ny + 1. ...
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... I'm considering my approach to the final project, and am 99% sure that I will do something along the lines of computation / simulation. I have a strong background in programming, and have had lots of fun and success in simulating all sorts of classical physics scenarios. I'd like to expand my horizo ...
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... n) the energy difference between two levels vanishes, ∆E E = (n+1/2)~ω ≈ 0; thus the energy becomes continuous, as it would be in the classical case. Still, to find a quantum-to-classical correspondence it is not enough to choose a stationary eigenstate of the Hamiltonian with a high energy (high n) ...
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... • Operators have associated with them a set of eigenfuntions, that in turn have eigenvalues associated with them. • For an operator Ô, with wavefunctions, ψn related as: Ô ψn = an ψn • The functions are known as eigenfunctions and the a n are eigenvalues. • The eigenvalues for quantum mechanical o ...
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... but are closely spaced double lines. This feature is called fine structure. There is an obvious way to get such closely spaced spectral lines: they will be observed if the degenerate energy levels are not truly degenerate but separated in energy by a very small amount (Figure 9.4). Recall that a giv ...
Lecture 11 - 12 - Cambridge University Press
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... Equation and Quantum Numbers There are four different quantum numbers needed to specify the state of an electron in an atom. 1.  The principal quantum number n gives the total energy. 2.  The orbital quantum number  gives the angular momentum;  can take on integer values from 0 to n - 1. ...
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... Quantum mechanics provides a mathematical description of the behavior and interactions of very small particles that are not correctly described by classical mechanics. This course is designed to provide students with the knowledge, theoretical background and mathematical tools to understand theoreti ...
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... perturbation theory. The first nontrivial term is second order normally called the Fermi Golden Rule. There is no systematic study of higher order and/or convergence in the physics literature. Some of the first attempts at a mathematical theory are due to Friedrichs. A common theme in these studies ...
the problem book
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... An observer chooses a Cartesian coordinate system at the geographical altitude angle θ, such that the (x, y)-plane is tangential to the surface of the Earth, with the x-axis pointing to the North and the y-axis to the West; the z-axis points radially, away from the center of the Earth. A pendulum of ...
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Van der Waals Forces Between Atoms
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... and this is certainly zero, as are all the other leading terms.  Baym (Lectures on Quantum  Mechanics) concluded from this that there is no leading order energy correction between two  hydrogen atoms if one of them is in the ground state.  This is incorrect: the first excited state of  the two­atom ...
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Perturbation theory (quantum mechanics)

In quantum mechanics, perturbation theory is a set of approximation schemes directly related to mathematical perturbation for describing a complicated quantum system in terms of a simpler one. The idea is to start with a simple system for which a mathematical solution is known, and add an additional ""perturbing"" Hamiltonian representing a weak disturbance to the system. If the disturbance is not too large, the various physical quantities associated with the perturbed system (e.g. its energy levels and eigenstates) can be expressed as ""corrections"" to those of the simple system. These corrections, being small compared to the size of the quantities themselves, can be calculated using approximate methods such as asymptotic series. The complicated system can therefore be studied based on knowledge of the simpler one.
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