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Quantum Transport and Mesoscopic Physics60ZR

1 IntroductionZ4MT

1.1  Recommended Textbooks

  • J.M. Ziman Principles of the theory of solids, 2nd Edition
  • A. Atland and B. Simons, Condensed Matter Field Theory
  • S.M. Girvin and Kun Kang, Modern Condensed Matter Physics

1.2  Presentation Topics

  • Coulomb blockade.
  • Kondo effect
  • Orthogonality catastrophe and quantum speed limit
  • Mott transition
  • Spin Hall effect
  • Composite fermions and the fractional quantum Hall effect
  • Charge density waves
  • Strongly coupled large polarons

2 Brownian Motion0ZE2

2.1 Stationary 1D Brownian MotionDFZJ

Definition 2.1.1  A quantum particle exhibits coherent motion iff its lifetime $t_\ell$ is much greater than $\frac{\hbar}{E}$.
\[t_\ell >> \frac{\hbar}{E}\]

Definition 2.1.2  A quantum particle exhibits incoherent motion iff its lifetime $t_\ell$ less than $\frac{\hbar}{E}$.
\[t_\ell \leq \frac{\hbar}{E}\]

Definition 2.1.3  A stationary 1D Brownian particle is a system of a stationary 1D particle experiencing many fast collisions with momentum $p_i$ integrated over a small time step $\Delta t$. Defined the force experienced by the particle $f(t)$ as a function of time.
\[f(t) = \frac{2}{\Delta t}\sum_i{p_i}\]

Definition 2.1.4  The ensemble average denoted $\langle x \rangle$ of a random variable $x$ is the integral of the variable weighted by the probability density function $P_{x}(x)$ across all possible values.
\[\langle x \rangle = \int_{-\infty}^{\infty}{x P_{x} dx}\]

Definition 2.1.5  The momentum diffusion coefficient is defined $D=2\nu\langle p_i^2\rangle = 2\nu m_{mol} k_B T$ where $\nu$ is the average frequency of collisions and $m^*$ is the effective mass of the particles.

Result 2.1.6  $\langle f\rangle = 0$

Result 2.1.7  $\langle f^2\rangle = \frac{4}{(\Delta t)^2} \sum_i{\langle p_i^2 \rangle}=\frac{4}{\Delta t}\nu\langle p_i^2\rangle = \frac{2D}{\Delta t}$

Result 2.1.8  $\langle f^{2n+1} \rangle = 0$

Result 2.1.9  $\langle f^{2n} \rangle = \langle f^2 \rangle^n (2n-1)!! =\left(\frac{4}{\Delta t}\nu\langle p_i^2\rangle\right)^n (2n-1)!! = \left(\frac{2D}{\Delta t}\right)^n (2n-1)!!$

Definition 2.1.10  A Gaussian Distribution with variance $\sigma=\langle f^2 \rangle$ is a distribution of the form:
\[P_f(x) = \frac{1}{\sqrt{2\pi\sigma}}e^{-x^2/2\sigma}\]

Definition 2.1.11  A probability density function of a variable is a function that when integrated over a region of possible values represents the probability of the variable being in that region.

Result 2.1.12  The probability density function of $f(t)$ at a particular time is Gaussian with $\sigma = \langle f^2 \rangle = \frac{2D}{\Delta t}$.

Definition 2.1.13  A functional probability density function is a probability density function that is integrated over different functions.

Result 2.1.14  The functional probability density of $f(t)$ is \[\mathcal{P}(f(t)) = C \text{exp}\left[{-\frac{1}{4D}\int_{-\infty}^{\infty}{f^2(t)dt}}\right]\]

2.2 1D Brownian Motion with Friction9ET5

Definition 2.2.1  The friction coefficient is a constant that describes the amount of friction experienced by a 1D Brownian particle.
\[\Gamma = \frac{m_{mol}\nu}{M}\]

Definition 2.2.2  A 1D Brownian Particle is a system of a 1D particle of mass $m_p$ moving at velocity $v_{p}$ which is experiencing many fast collisions. Define the force experienced by the particle $f_p(t)$ in terms of the force experienced by a stationary 1D Brownian particle $f(t)$ and the friction coefficient $\Gamma$.
\[f_v(t) = f(t) - 2\Gamma m_p v_p\]

Definition 2.2.3  The position diffusion coefficient denoted $\mathscr{D}$ is defined in terms of the noise intensity $D$, the friction coefficient $\Gamma$ and the mass of the particle $m_p$.
\[\mathscr{D} = \frac{D}{(2\Gamma m_p)^2} = \frac{k_B T}{2\Gamma m_p}\]

Result 2.2.4  The motion $q(t)$ and the momentum $p(t)$ of a 1D Brownian particle is described by the following equations.
\[p(t) = \int_0^t{e^{-2\Gamma(t-\tau)f(\tau)d\tau}}\]\[q(t) = \frac{1}{m_p}\int_0^t{p(\tau)d\tau} = \frac{1}{m_p}\int_0^\tau{f(\tau)\frac{1-e^{-2\Gamma(t-\tau)}}{2\Gamma}d\tau}\]

Result 2.2.5  $\langle q\rangle = 0$

Result 2.2.6  For $t>>\frac{1}{\Gamma}$, $\langle q^2\rangle = \langle (q(t)-q(0))^2 \rangle = 2\mathscr{D}\left[t - \frac{2}{2\Gamma}(1-e^{-2\Gamma t}) + \frac{1}{4\Gamma}(1-e^{-4\Gamma t})\right] \approx 2\mathscr{D}t$

2.3 Lagevin and Fokker-Plank Equations26RC

Definition 2.3.1  A 1D Brownian Particle in a Potential is a system of a 1D Brownian particle experiencing a potential $U(p)$. The system can be written in terms of position $q$ and momentum $p$ or as a time dependent force function $f_U(t)$
\[\dot{q} = \frac{p}{m_p},\quad \dot{p} = f(t) - 2\Gamma p - U'(q)\]\[f_U(t) = f(t) - 2\Gamma m_pv_p - U'\]

Theorem 2.3.2  The Lagevin and Fokker-Plank Equations describe the probability density function $\omega(q,p,t,q(0),p(0),0)$ of a 1D Brownian particle in a potential $U(q)$.
\[\omega(q,p,0,q(0),p(0),0) = \delta(q-q(0))\delta(p-p(0))\]\[\partial_t \omega(q,p,t)= -\partial_q\left( \frac{p}{m_p}\omega(q,p,t) \right) - \partial_p\left(- 2\Gamma p - U'(q) + D\partial_p^2\right)\omega(q,p,t)\]

Definition 2.3.3  The Diffusion Equation describes a Brownian particle where there is no potential or drift, that is $\Gamma = 0$ and $U(q)=0$.
\[\frac{\partial n}{\partial t} - \mathscr{D}\nabla_\mathbf{x}^2n = 0\]

Result 2.3.4  The solution to the diffusion equation is of the form
\[\partial_t\omega = \mathscr{D}\partial_x^2\omega\]\[\omega = \frac{C}{\sqrt{t}}e^{-x^2/4\mathscr{D}t}\]

Definition 2.3.5  The time average denoted $\langle x \rangle$ of a random variable $x(t)$ is the time integral of the variable over a very long period.
\[\langle x\rangle = \lim_{T\to\infty}\frac{1}{T}\int_0^T{x(t)dt}\]

Definition 2.3.6  A system is ergodic iff the ensemble average and the time average are equivalent.

2.4 Harmonic Oscillator DiffusionK69N

Definition 2.4.1  The Brownian harmonic oscillator is a system describing a Brownian particle in a harmonic oscillator potential $U(q)$
\[U(q) = \frac{1}{2}m\omega_0^2q^2\]\[\partial_t \omega(q,p,t) = -\partial_q\left( \frac{p}{m_p}\omega(q,p,t) \right) - \partial_p\left(- 2\Gamma p\omega(q,p,t) - m\omega_0^2q\omega(q,p,t) + D\partial_p^2\right)\omega(q,p,t)\]

Result 2.4.2  For a Brownian harmonic oscillator, $\langle \ddot{q}\rangle = -\omega_0^2\langle q \rangle - \frac{2\Gamma}{m}\langle \ddot{q}\rangle$

Definition 2.4.3  The time correlation function $Q_{qq}(t)$ of a variable $q(t)$ is defined $Q_{qq}(t) = \langle q(t)q(0)\rangle$.

Definition 2.4.4  The power spectrium $S_{qq}(\omega)$ of a variable $q(t)$ is the Fourier transform of the time correlation function $S_{qq}(\omega) = \int_{\infty}^\infty{e^{i\omega t}\langle q(t) q(0)\rangle dt}$,

Result 2.4.5  For a real variable $q(t)$ the power spectrum is $S_{qq}(\omega) = 2\text{Re}\left( \int_{-\infty}^\infty{e^{i\omega t}\langle q(t) q(0)\rangle dt} \right)$

Result 2.4.6  The stationary solution to the Brownian Harmonic oscillator is of the form
\[\omega(q,p,t) = C e^{-(\frac{p^2}{2m} + U(q))/\alpha}\]

Result 2.4.7  The power spectrum of $q$ for the Brownian harmonic oscillator is
\[S_qq(\omega) = \frac{2\Gamma \omega_0^2}{(\omega^2-\omega_0^2)^2 + 4\Gamma^2\omega^2}\]

2.5 Escape and Activation via Tunneling8553

Definition 2.5.1  The probability current $j(q)$ is the rate at which probability to crossing point $q_B$.
\[j(q_B) = \int{\frac{p}{m}\omega(q_B,p,t)}\]

Definition 2.5.2  The escape rate is the reciprocal of the average lifetime $\tau$ and can be written in terms of probability current.
\[W_{esc} = \frac{j}{N} = \frac{1}{\tau}\]

Definition 2.5.3  The number of trapped particles $N$ is defined
\[N = \int_{-\infty}^{\infty}dp\int_{-\infty}^{q_B}dq \omega(q,p,t)\]

Result 2.5.4  The time derivative of the number of particles $N$ is $\frac{\partial N}{\partial t} = - W_{esc}N$ and the decay over time is
\[N(t) = N(0)e^{-W_{esc}t}\]

2.6 Escape and Activation via Tunneling8553

Definition 2.6.1  The probability current $j(q)$ is the rate at which probability to crossing point $q_B$.
\[j(q_B) = \int{\frac{p}{m}\omega(q_B,p,t)}\]

Definition 2.6.2  The escape rate is the reciprocal of the average lifetime $\tau$ and can be written in terms of probability current.
\[W_{esc} = \frac{j}{N} = \frac{1}{\tau}\]

Definition 2.6.3  The number of trapped particles $N$ is defined
\[N = \int_{-\infty}^{\infty}dp\int_{-\infty}^{q_B}dq \omega(q,p,t)\]

Result 2.6.4  The time derivative of the number of particles $N$ is $\frac{\partial N}{\partial t} = - W_{esc}N$ and the decay over time is
\[N(t) = N(0)e^{-W_{esc}t}\]

3 Electron TransportZKM7

3.1 Bloch's Theorem and Berry Phase45C9

Theorem 3.1.1  Bloch's Theorem states that the solution any system with a periodic potential can be represented with a periodic function $u_{\mathbf{k},n}(\mathbf{r})$ and $e^{i\mathbf{k}\cdot\mathbf{r}}$, that is
\[H\Psi_{\mathbf{k},n}(\mathbf{r}) = E_{\mathbf{k},n}\Psi_{\mathbf{k},n}(\mathbf{r}),\quad \Psi_{\mathbf{k},n}(\mathbf{r})=e^{i\mathbf{k}\cdot\mathbf{r}}u_{\mathbf{k},n}(\mathbf{r})\]

Definition 3.1.2  The Berry connection denoted $\mathcal{A}_{n,\mathbf{k}}(\mathbf{r})$ is defined as $\mathcal{A}_{n,\mathbf{k}}(\mathbf{r}) = i\langle u_{\mathbf{k},n}(\mathbf{r}) | \nabla_{\mathbf{k}} u_{\mathbf{k},n}(\mathbf{r}) \rangle$

Definition 3.1.3  The Berry phase denoted $\gamma_{n,\mathbf{k}}$ is defined as $\gamma_{n,\mathbf{k}} = \int \mathcal{A}_{n,\mathbf{k}}(\mathbf{r}) \cdot d\mathbf{r}$

Result 3.1.4  For the band wavefunction $\Phi_n(\mathbf{r}) = \int{ c(\mathbf{k})\Psi_{\mathbf{k},n}(\mathbf{k})\Psi_{\mathbf{k},n}(\mathbf{r}) d\mathbf{k}}$, written in terms of eigenstates $\Psi_{\mathbf{k},n}$,
\[\mathbf{r} = i\partial_k + i\langle u_{\mathbf{k},n}(\mathbf{r}) | \nabla_{\mathbf{k}} u_{\mathbf{k},n}(\mathbf{r}) \rangle = i\partial_k + \mathcal{A}_n(\mathbf{r})\]\[\langle \mathbf{r} \rangle = \left( \frac{(2\pi)^d}{V} \right)^2\int{c^*(\mathbf{k}) \mathbf{r} c(\mathbf{k}) d\mathbf{k}} = \left( \frac{(2\pi)^d}{V} \right)^2\int{c^*(\mathbf{k})\left(i\partial_k + \mathcal{A}_{n,\mathbf{k}}(\mathbf{r})\right) c(\mathbf{k}) d\mathbf{k}}\]\[\langle \dot{\mathbf{r}} \rangle = \frac{\partial E_{\mathbf{k},n}}{\partial \mathbf{k}}\]

3.2 Anomalous Quantum Hall Effect63P4

Definition 3.2.1  The anomalous quantum hall effect Hamiltonian $H$ describes the behavior of many electrons in a lattice $H_0$ experiences an electric field $E$ pointing in the x direction.
\[H = H_0 - e_qEx\]

Definition 3.2.2  The Berry curvature denoted $\mathbf{\Omega}_{n,\mathbf{k}}(\mathbf{r})$ is defined as $\mathbf{\Omega}_{n,\mathbf{k}}(\mathbf{r}) = \nabla_\mathbf{r}\times \mathcal{A}_{n,\mathbf{k}}(\mathbf{r})$

Result 3.2.3  The average velocities for 2D electrons experiencing an electric field in the x direction are
\[\langle v_x\rangle = \frac{1}{\hbar} \frac{\partial E_{n\mathbf{k}}}{\partial k_x}\]\[\langle v_y \rangle = \frac{1}{\hbar} \frac{\partial E_{n\mathbf{k}}}{\partial k_x} + \frac{qE}{\hbar}\left(\mathbf{\Omega}_{n,\mathbf{k}}(\mathbf{r})\right)_z\]

Result 3.2.4  current

Definition 3.2.5  Churn number

Result 3.2.6  conductivity

3.3  Boltzmann Kinetic Equation

4 Scattering and ConductivityREZC

4.1  Impurity Scattering

4.2  Electric Conductivity

4.3  Thermal Conductivity

4.4  Magnetoconductivity

4.5  Cyclotron Resonance

5 Low-dimensional SystemsAW5M

5.1  Landauer 1D Conductivity

5.2  2D Electron Systems

5.3  Quantum Hall Effect

6 LocalizationD3P7

6.1  Weak Localization

6.2  Anderson Localization

6.3  Density Matrix and the Quantum Kinetic Equation

7 Phonon1EDE

7.1  Electron-phonon Interaction

7.2  Polaronic Effect

7.3  Ohmic Dissipation

7.4  The Orthogonality Catastrophe

7.5  Holstein Polarons

8 Topological MaterialsNMJH

8.1  Variable-range Hopping

8.2  The Coulomb Gap

8.3  The Berry Phase

8.4  Group Velocity in Topologically Nontrivial Solids

8.5  The Kitaev Chain