Chapter 1: The Wave Function

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The Schrodinger equation for a single particle in one dimension: $$i \hbar \frac{\partial \Psi}{\partial t} = - \frac{\hbar^2}{2m} \frac{\partial^2\Psi}{\partial x^2} + V\Psi$$ where \(m\) is the mass of the particle, \(\hbar\) is the reduced planck constant, \(V\) is the potential the particle is in and \(\Psi\) is the wavefunction of the particle describes where the particle is; i.e: $$\int_a^b |\Psi(x,t)|^2 dx$$ describes the probability of finding particle between \(a\) and \(b\) at time t. Evidently, the particle must be somewhere, so we have that: $$\int_{-\infty}^{+\infty} |\Psi(x,t)|^2 dx = 1$$ Notice that any such \(\Psi\) a solution to the Shrodinger equation gives rise to an infinite number of solutions \(a\Psi\) where \(a\) is a constant, so we must normalize the solution by making sure that the probability of the particle being somewhere is 1. It is true that if we normalise the wavefunction at \(t = 0\) and let the function evolve dynamically by the Shrodinger equation, that the wavefunction stays normalised.


Problem 1.5
Consider the wavefunction $$\Psi(x,t) = A e^{-\lambda |x|}e^{-i\omega t}$$ where \(A,\lambda,\) and \(\omega\) are positive real constants.

$$\langle x \rangle = \int_{-\infty}^{+\infty} \Psi^*(x) \Psi dx$$ $$\langle p \rangle = m \frac{d\langle x \rangle}{dt} = \int \Psi^* \bigg(\frac{\hbar}{i} \frac{\partial}{\partial x}\bigg) \Psi dx$$ We say that the operator \(x\) "represents" position, and the operator \((\hbar/i)(\partial/\partial x)\) "represents" momentum, in quantum mechanics; to calculate expectation values we "sandwich" the appropriate operator between \(\Psi^*\) and \(\Psi\), and integrate. The nice thing is, all classical dynamical variables can be expressed in terms of position and momentum. Kinetic energy, for example, is: $$\langle T \rangle = \frac{p^2}{2m}$$ To calculate the expectation value of any such quantity, \(Q(x,p)\), we simply replace every \(p\) by it's associated operator, sandwich the resulting operator between the conjugate of the wavefunction and the wavefunction, and integrate: $$\langle Q(x,p) \rangle = \int \Psi^* Q\bigg(x,\frac{\hbar}{i}\frac{\partial}{\partial x} \bigg) \Psi dx$$ For example, the expectation value of kinetic energy is $$\langle T \rangle = -\frac{\hbar^2}{2m} \int \Psi^* \frac{\partial^2}{\partial x^2} \Psi dx$$


Problem 1.7

Show that \(d\langle p \rangle / dt = \langle - \partial V / \partial x \rangle\).


The de Broglie formula tells us that a particle's momentum and wavelength are related by: $$p = \frac{h}{\lambda} = \frac{2\pi \hbar}{\lambda}$$ Heisenberg's uncertainty principle tells us: $$\sigma_x \sigma_p \geq \frac{\hbar}{2}$$ where \(\sigma_x\) is the standard deviation of \(x\), and \(\sigma_p\) is the standard deviation of \(p\).


Problem 1.9

A particle of mass \(m\) is in the state $$\Psi(x,t) = A e^{-a[(mx^2/\hbar)+it]}$$ where \(A,a\) are positive real constants.

Problem 1.15

Suppose we want to describe an unstable particle, that spontaneously disintegrates with 'lifetime' \(\tau\); i.e. $$P(t) = \int \Psi^* \Psi dx = e^{-t/\tau}$$ A crude way of approximating this situation would be to throw away the assumption that \(V\) (our potential) must be real, and instead replace it with \(V = V_0 + i\Gamma\) where \(V_0, \Gamma\) are positive real constants. Show that instead of \(P(t) = 1\), we have: $$\frac{dP}{dt} = - \frac{2\Gamma}{\hbar} P$$ Solve for \(P(t)\), and find the lifetime of the particle \(\tau\).