160 lines
7.0 KiB
TeX
160 lines
7.0 KiB
TeX
\documentclass[12pt,journal,onecolumn]{IEEEtran}
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\usepackage{graphicx}
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\usepackage{amsmath}
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\begin{document}
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%\title{Report on Uemura's lectures\\ Rotons in superfluid helium}
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\title{Learning about Rotons}
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\author{Tran Hoai Nam}
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\maketitle
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%\begin{abstract}
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%This is abstract text: This simple document shows very basic features of \LaTeX{}.
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%\end{abstract}
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%\chapter{First Chapter}
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\section{Theoretical framework: Landau and Feynman}
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%Explain contribution of Landau and Feynman on studies of rotons
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In 1938, P. Kapitza \cite{kapitza}, and simultaneously, J.F. Allen and A.D.
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Misener \cite{allen} reported experimental evidence
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of an anomalous behavior of liquid helium below 2.2 K, which is later called ``superfluidity''.
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In the same year, F. London \cite{london} suggested that superfluidity is
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consequence of Bose-Einstein condensation (BEC), and L. Tisza proposed a ``two fluid
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model'' to explain the observation. Both of these ideas connected to BEC.
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The two fluid model was subsequently developed by L.D. Landau \cite{landau1}, however without
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reference to BEC. In his theory, Landau considered energy states of the liquid instead of
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individual atoms, it means without giving
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an underlying microscopic basis (such as Bose statistics of the $^4$He atoms).
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%(c.f. Bose condensed gases at finite temperature, p. 329)
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Landau assumed that single
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particle states were replaced by collective modes of two different kinds:
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phonons, i.e. sound quanta, and quantized vortices called ``rotons''.
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Phonons have basically a linear dispersion relation:
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\begin{equation}
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\omega = ck,
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\label{eq:phonon}
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\end{equation} and rotons
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have a quadratic one with a gap:
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\begin{equation}
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\epsilon = \Delta + p^2/2\mu,
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\label{eq:roton1}
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\end{equation}
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Later \cite{landau2}, Landau
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modified the dispersion relation of rotons in order to obtain better agreement
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with thermodynamic properties. The phonon branch evolved continuously into a
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roton branch:
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\begin{equation}
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\epsilon = \Delta + (p-p_0)^2/2\mu,
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\label{eq:roton2}
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\end{equation}
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where $\Delta$ and $p_0$ are the energy and momentum of the minimum, and
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$\mu$ is effective mass of excitation.
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M. Cohen and R.P. Feynman \cite{cohen} then proposed to verify Landau's theory by neutron
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scattering experiments. These experiments were strong support to Landau's
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theory. Nevertheless, Feynman thought that there are weaknesses in Landau's theory. Notably,
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Landau's quantum hydrodynamical approach treated helium II as a continuous
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medium, which right from the beginning sacrificed the atomic structure of the
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liquid and thus forestalled the possibility to calculate various characteristics
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of the system. By writing
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partition function as an integral over trajectories, using the space-time
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approach to quantum mechanics, Feynman \cite{feynman1953} could derive a Landau-type energy
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spectrum and further demonstrate how phonon-like excitation evolved into
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roton-like ones at large momenta.
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\section{Experimental evidence}
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%Choose one experiment probing rotons, explain principle, describe what results
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%indicate.
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In this section, I want to introduce about one neutron scattering experiment to
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probe rotons. The experiment was done by D.G. Henshaw and A.D.B. Woods in
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1960 \cite{exp}.
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\subsection{Principle of the experiment}
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%It is refered to Cohen and Feynman's paper --> should look at it before
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%proceeding.`
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In this experiment, inelastically scattered neutrons from superfluid
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$^4$He were measured. Changes in energy and momentum of scattered neutrons
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are equal to the energy and momentum of an excitation produced in the liquid.
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By measuring wavelength distribution of
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scattered neutrons, the authors could infer a dispersion curved for liquid
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$^4$He at 1.12 K. The dispersion curved was compared with Landau's theory of
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rotons.
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\subsection{Results}
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\begin{figure}[htpb]
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\begin{center}
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\includegraphics[width=0.7 \textwidth]{dispersion}
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\caption{The dispersion curve for helium liquid at 1.12 K}
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\label{fig:dispersion}
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\end{center}
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\end{figure}
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The dispersion curve for liquid helium at 1.12 K under its normal vapor pressure
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is shown in Fig. \ref{fig:dispersion}. The open circles are data points, showed
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the energy and momentum of excitations of the liquid. The smooth curve drawn
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through data points is the guide to the eye.
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The parabolic curve from the origin represents
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the theoretically calculated dispersion relation of free helium atoms at 0 K.
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The dispersion curve showed behavior similar to what is expected from Landau's
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theory: a linear phonon branch evolves to a quadratic branch of roton. In Fig.
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\ref{fig:dispersion}, the part rising linearly from about 0.2 A$^{-1}$ until 0.6
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A$^{-1}$ is the phonon branch. It has the slope of the velocity of sound of
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237 m/s. Beyond 0.6 A$^{-1}$, the curve falls below the phonon branch, has
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one maximum at 1.10 A$^{-1}$ and 13.7 K. The curve has a minimum at 1.91
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A$^{-1}$ and 8.65 K. When fitted with equation \eqref{eq:roton2}, parameters of
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the roton branch at 1.12 K are:
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\begin{align*}
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\Delta/k &= 8.65 \pm 0.04 \mathrm{K} \\
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p_0/ \hbar &= 1.91 \pm 0.01 \mathrm{A}^{-1}\\
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\mu &= 0.16\mathrm{ m_{He}}
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\label{eq:fittedpar}
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\end{align*}
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The authors also investigated temperature variations of above parameters in the
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range from 1.1 K to 4.2 K. All of them showed a remarkable change in slope at
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the superfluidity transition point. The plot of mean energy change of 4.039 A
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neutrons is shown in Fig. \ref{fig:tempvar}.
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\begin{figure}[htpb]
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\begin{center}
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\includegraphics[width=0.7\textwidth]{tempvar}
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\end{center}
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\caption{The temperature variation of the mean energy change of 4.039 A
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neutrons scattered through 80$^o$ from liquid helium.}
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\label{fig:tempvar}
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\end{figure}
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\section{My opinion on employing roton concept for superconductivity}
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I do not have enough background to judge if employing roton in
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superconductivity is good or not. However, I think that superfluidity and
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superconductivity are both manifestations quantum behaviors in
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macroscopic scale. So, in some limit, idea of roton might be applied to explain
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superconductivity.
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%Your own view on employing roton concepts for superconductivity.
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%%%%%%%%%
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%Ref
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%%%%%%%%%
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\begin{thebibliography}{9}
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\bibitem{kapitza}
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P. Kapitza, \emph{Nature} \textbf{141}, 74 (1938).
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\bibitem{allen}
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J.F. Allen and A.D. Misener, \emph{Nature} \textbf{141}, 75 (1938).
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\bibitem{london}
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F. London, \emph{Nature} \textbf{141}, 643 (1938).
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\bibitem{tisza}
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L. Tisza, \emph{Nature} \textbf{141}, 913 (1938).
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\bibitem{landau1}
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L.D. Landau, \emph{J. Phys. USSR} \textbf{5}, 71 (1941).
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\bibitem{landau2}
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L.D. Landau, \emph{J. Phys. USSR} \textbf{11}, 91 (1947).
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\bibitem{cohen}
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M. Cohen and R.P. Feynman, \emph{Phys. Rev.} \textbf{107}, 13 (1957).
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\bibitem{feynman1953}
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R.P. Feynaman, \emph{Phys. Rev. } \textbf{91}, 1291 (1953).
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\bibitem{exp}
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D.G. Henshaw and A.D.B. Woods, \emph{Phys. Rev.} \textbf{107}, 13 (1957).
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\end{thebibliography}
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\end{document}
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