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“the energies are (2.73) All energies are proportional to”
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
“where is the exponential operator (3.105)”
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
“ Moreover”
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
“It’s difficult to overstate the importance of the harmonic oscillator in quantum mechanics. It is”
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
“This is entirely analogous to the fact that for any energy eigenstate of the harmonic oscillator. But we know what we need to do to construct a state of the harmonic oscillator with a (reasonably) well-defined phase: this is precisely the coherent state (5.33)”
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
“We see that all memory of our previous measurement has been erased by the measurement of . There’s no longer any guarantee that we will still get this time around. Instead”
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
“We see that the Gaussian wavepacket is rather special: it saturates the bound from the Heisenberg uncertainty relation. The class of Gaussian wavefunctions”
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
“All of this means that”
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
“This means that if we have many systems”
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
“Solutions to the Schrödinger equation that behave as (2.85) are called bound states because they are necessarily trapped somewhere in the potential.”
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
“Gaussian wavepacket. Clearly it describes a state that is fairly well localised in space. But”
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
“The Schrödinger equation is (2.4)”
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
“Given an operator acting on some class of functions”
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
“The quantum novelty is that the wavefunction itself is not restricted only to the well: it leaks out into the surrounding region”
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
“Take two systems. We’ll call them system described by the Hilbert space”
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
“3.5.3 Ehrenfest Theorem We can look at how the expectation value of some operator changes with time. We’ll assume that the operator itself has no time dependence”
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
“we take a state with some fixed number of photons”
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
“Let’s look at some properties of the Wigner function. First, it is real. (This follows by taking the complex conjugate and changing variables to .) Second, if we integrate over momentum, and use the fact that , we have (5.78) But that’s rather nice: marginalising over momentum gives us , which we know is the probability distribution over position. Moreover, if we have a normalised wavefunction then we know that .”
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
“There is an algebraic way of formalising whether two observables can be simultaneously measured or whether”
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
“Given a wavefunction , the Wigner function is a function over classical phase space, defined by (5.77) We want to think of this as something akin to a probability distribution over phase space. At first glance that seems unlikely because, as we’ve seen, there is a difference between quantum states whose properties are undetermined and classical probability that can be ascribed to ignorance. This is reflected in the fact that and so we can’t ascribe simultaneous values to both observables. And, indeed, it will turn out that it’s not possible to interpret as a classical probability distribution. Nonetheless, it gets close. Let’s look at some properties of the Wigner function. First, it is real. (This follows by taking the complex conjugate and changing variables to .) Second, if we integrate over momentum, and use the fact that , we have (5.78) But that’s rather nice: marginalising over momentum gives us , which we know is the probability distribution over position. Moreover, if we have a normalised wavefunction then we know that .”
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
“the idea of parity”
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
“Rather than thinking of them as quantum probabilities for a single particle”
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
“The discreteness in quantities like momentum and energy is one of the characteristic features of quantum mechanics. However”
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
“The time-dependent Schrödinger equation is (4.49)”
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
“An eigenstate of a Hermitian operator obeys (3.66) where is the eigenvalue.”
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
“In quantum mechanics”
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
“If we want to write down the analogous quantum Hamiltonian”
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
“We learn that the Gaussian wavefunction (2.64) that we guessed earlier is actually the lowest energy state of the system”
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
“This means”
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics
― Quantum Mechanics: Volume 3: Lectures on Theoretical Physics




