142 lines
6.0 KiB
TeX
Executable File
142 lines
6.0 KiB
TeX
Executable File
\documentclass[a4paper, 11pt]{article}
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\usepackage[utf8]{inputenc}
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\usepackage[
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a4paper,
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headheight = 20pt,
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margin = 1in,
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tmargin = \dimexpr 1in - 10pt \relax
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]{geometry}
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\usepackage{fancyhdr} % for headers and footers
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\usepackage{graphicx} % for including figures
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\usepackage{booktabs} % for professional tables
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\setlength{\headheight}{14pt}
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\fancypagestyle{plain}{
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\fancyhf{}
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\fancyhead[L]{\sffamily Radboud University Nijmegen}
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\fancyhead[R]{\sffamily Superconductivity (NWI-NM117), Q3+Q4}
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\fancyfoot[R]{\sffamily\bfseries\thepage}
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\renewcommand{\headrulewidth}{0.5pt}
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\renewcommand{\footrulewidth}{0.5pt}
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}
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\pagestyle{fancy}
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\usepackage{siunitx}
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\usepackage{hyperref}
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\usepackage{float}
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\usepackage{mathtools}
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\usepackage{amsmath}
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\usepackage{todonotes}
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\setuptodonotes{inline}
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\usepackage{mhchem}
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\newcommand{\pfrac}[2]{\frac{\partial #1}{\partial #2}}
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\title{Superconductivity - Assignment 3}
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\author{
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Kees van Kempen (s4853628)\\
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\texttt{k.vankempen@student.science.ru.nl}
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}
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\AtBeginDocument{\maketitle}
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% Start from 8
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\setcounter{section}{7}
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\begin{document}
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\section{\ce{Nb3Sn} cylinder}
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Consider a cylinder of \ce{Nb3Sb}.
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From lecture 4, we have the following properties for \ce{Nb3Sn}:
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$T_c = \SI{18.2}{\kelvin}$,
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$\xi = \SI{3.6}{\nano\meter}$,
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$\lambda = \SI{124}{\nano\meter}$,
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$\kappa = \frac{\lambda}{\xi} = 34 > \frac{1}{\sqrt{2}}$,
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which means we are indeed dealing with a type-II superconductor.
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As $B_{c1} < B_E < B_{c2}$, the cylinder is in the vortex state.
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From the previous set of assignments, we know what the currents in the cylinder look like.
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From free energy considerations, we have found in lecture 4 that for type-II superconductors, it is favorable to allow flux quanta inside the superconductor in this vortex state.
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In this derivation, the contribution of one flux quantum is considered, but the consideration holds for many vortices, until they start to interact and repel eachother.
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At that point, the vortex-vortex interaction orders the vortices in a lattice.
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When the vortex cores start to overlap, there are no superconducting regions left, thus the material enters the normal conducting state.\footnote{I wanted to paint a complete picture althought it is not needed to answer the question.}
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Minimizing the free energy over the flux shows the energy is lowered for determined thresholds $B_{c1} < B_E < B_{c2}$.
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Let's start with the result from said free energy considerations.
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The average field inside the cylinder is given by the following self-consisting equation as
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\[
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B = B_E - \frac{\phi_0}{8\pi\lambda^2}\ln{\frac{\phi_0}{4\exp{(1)}\xi^2B}}.
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\]
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Plugging in the values for \ce{Nb3Sn}, $B_E = \SI{1}{\tesla}$, and $\phi_0 = \SI{2.0678}{\weber}$, $B$ is found as $B = \SI{.986}{\tesla} \approx B_E$ by intersection.
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%https://www.wolframalpha.com/input?i=B+%3D+1+-+%282.0678*10%5E-15%29%2F%288*pi*%28124*10%5E-9%29%5E2%29+*+ln%282.0678*10%5E-15%2F%284*exp%281%29*%283.65*10%5E-9%29%5E2+*+B%29%29
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This is in the range as provided in the assignment ($B = \SI[separate-uncertainty]{.981\pm.019}{\tesla}$).
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To investigate the inhomogenity of the field inside the cylinder, we look at the gradient $\nabla B$ inside the material.
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As we assume a vortex lattice that fully fills the cross section of the cylinder,
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and we assume that the fields due to each vortex die out quickly enough to not overlap,
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it suffices to calculate the gradient over just one vortex.
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These assumptions coincide with slide 15 of lecture 4, from which I took figure \ref{fig:lec4-vortexlattice}.
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\begin{figure}[H]
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\centering
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\label{fig:lec4-vortexlattice}
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\includegraphics[width=.4\textwidth]{lec4-vortexlattice.png}
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\caption{The vortices are arranged in a lattice to maximize their distance, as this lowers their repulsive interaction and thus the energy.}
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\end{figure}
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On slide 19 from the same week, we find an expression $B(r)$ for the field at distance $r$ from the vortex core as
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\[
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B = \frac{\phi_0}{2\pi\lambda^2} K_0(r/\lambda) = B_0 K_0(r/\lambda),
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\]
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where $K_0$ is the modified Bessel function of the second kind.
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For small $r$ (i.e. $r << \lambda$), we can approximate this and find that
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\[
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K_0 \propto - \ln{(r/\lambda)},
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\]
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and notice a singularity at $r = 0$.
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For the gradient we thus find
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\[
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\nabla B \propto \pfrac{K_0}{r}(r/\lambda) \propto \pfrac{-\ln{(r/\lambda)}}{r} = -\lambda/r.
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\]
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The size of the supercurrent density has the same relation, $J_S \propto 1/r$.
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\section{Superconducting wire}
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\textbf{(a)}
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The voltage $U = \SI{1.5e-5}{\volt}$ across the wire of length $\ell = \SI{.08}{\meter}$ induces a current $J_t$. % through the resistive wire with unknown resistivity $\rho$ according to Ohm's law.
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Due to the presence of the magnetic field $B = \SI{5}{\tesla}$, if the vortices move with velocity $v_L$, a Lorentz force $f_L$ per vortex acts on the vortices.
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This results in a power input $P_L = f_Lv_L = J_tBv_L$ per vortex.
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%$\epsilon = Bv_L$
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This power should come from the current induced by the voltage, thus $P_L = \epsilon J_t = \frac{U}{\ell}J_t$.
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Equating these expressions and rewriting yields
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\[
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v_L = \frac{U}{B\ell} = \SI{3.75e5}{\meter\per\second}.
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% https://www.wolframalpha.com/input?i=1.5*10%5E-5+%2F+%285*+.08%29
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\]
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\todo{Direction?}
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\textbf{(b)}
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The vortices are aranged in a lattice with separation $r_{sep} = \sqrt{\frac{\Phi_0}{B}}$.
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They move along the wire with velocity $v_L$ as determined above.
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The expected frequency is then given by their velocity over the separation, as that is the period of the changing fields due to the vortices:
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\[
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f = \frac{v_L}{r_{sep}} = \frac{U}{B\ell}\sqrt{\frac{B}{\Phi_0}} = \frac{U}{\ell\sqrt{B\Phi_0}} = \SI{1.84}{\kilo\hertz},
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% https://www.wolframalpha.com/input?i=1.5*10%5E-5+%2F+%28.08%29+%2Fsqrt%285+*+2.067*10%5E%28-15%29%29
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\]
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where we used that $\Phi_0 = \SI{2.067e-15}{\volt\second}$.
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This is very close to what is written in the assignment, but not precisely the same, so maybe I used a different value for $\Phi_0$.
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\section{Fine type-II superconducting wire}
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\section{Critical currents}
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\section{A weak junction}
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\bibliographystyle{vancouver}
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\bibliography{references.bib}
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%\appendix
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\end{document}
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