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authorBlaise Thompson <blaise@untzag.com>2018-04-15 17:04:18 -0500
committerBlaise Thompson <blaise@untzag.com>2018-04-15 17:04:18 -0500
commit58a5425154d4d7eec55463e5e2a89b7ade067781 (patch)
treeaab9a57676b084fa66bd49a4f69a13367ad14ce7
parent0f87beb9b3cbf8447f4850be0eb9874e9c4fb64f (diff)
2018-04-15 17:04
-rw-r--r--bibliography.bib23
-rw-r--r--spectroscopy/auto/chapter.el3
-rw-r--r--spectroscopy/chapter.tex152
-rw-r--r--todo.org13
4 files changed, 97 insertions, 94 deletions
diff --git a/bibliography.bib b/bibliography.bib
index 4e1e234..2651b25 100644
--- a/bibliography.bib
+++ b/bibliography.bib
@@ -1537,6 +1537,20 @@
publisher = {{AIP} Publishing},
}
+@article{KoivistoinenJuha2017a,
+ author = {Juha Koivistoinen and Pasi Myllyperki\"{o} and Mika Pettersson},
+ title = {Time-Resolved Coherent Anti-Stokes Raman Scattering of Graphene: Dephasing
+ Dynamics of Optical Phonon},
+ journal = {The Journal of Physical Chemistry Letters},
+ volume = 8,
+ number = 17,
+ pages = {4108--4112},
+ year = 2017,
+ doi = {10.1021/acs.jpclett.7b01711},
+ month = {aug},
+ publisher = {American Chemical Society ({ACS})},
+}
+
@article{KraatzIngvarT2014a,
author = {Kraatz, Ingvar T and Booth, Matthew and Whitaker, Benjamin J and Nix, Michael G D
and Critchley, Kevin},
@@ -3481,9 +3495,14 @@
url = {http://docs.h5py.org/en/latest/high/group.html#groups},
}
+@misc{nanoram,
+ note = {Accessed: 2018-04-15},
+ title = {NanoRam Handheld Raman Spectrometer for Material ID},
+ url = {http://bwtek.com/products/nanoram/},
+}
+
@misc{pyqtgraph,
note = {Accessed: 2018-03-27},
title = {PyQtGraph: Scientific Graphics and GUI Library for Python},
url = {http://pyqtgraph.org/},
-}
-
+} \ No newline at end of file
diff --git a/spectroscopy/auto/chapter.el b/spectroscopy/auto/chapter.el
index 731ac34..41829c0 100644
--- a/spectroscopy/auto/chapter.el
+++ b/spectroscopy/auto/chapter.el
@@ -3,7 +3,6 @@
(lambda ()
(LaTeX-add-labels
"cha:spc"
- "spc:eqn:E"
- "spc:fig:ranges"))
+ "spc:eqn:E"))
:latex)
diff --git a/spectroscopy/chapter.tex b/spectroscopy/chapter.tex
index 819fe94..805bce8 100644
--- a/spectroscopy/chapter.tex
+++ b/spectroscopy/chapter.tex
@@ -38,7 +38,7 @@ many photons. %
The basics of light matter interaction have been covered in many texts. %
For a beginners introduction I recommend ``How a Photon is Created or Absorbed'' by
-\textref{HendersonGiles1994a}. %
+\textcite{HendersonGiles1994a}. %
Here I present a very minimal overview. %
Consider a two state system: ``a'' and ``b''. %
@@ -61,8 +61,8 @@ For simplicity, we consider a single transition dipole, $\mu$. %
The Hamiltonian which controls the coupling of or simple system to the electric field described in
\autoref{spc:eqn:E} can be written. %
\begin{eqnarray}
- H &=& H_{0} - \mu \cdot E \\
- &=& H_{0} - \mu \cdot \frac{E^0}{2}\left[ \me^{i(kz-\omega t)} + \me^{-i(kz-\omega t)} \right]
+ H &=& H_{0} + \mu \cdot E \\
+ &=& H_{0} + \mu \cdot \frac{E^0}{2}\left[ \me^{i(kz-\omega t)} + \me^{-i(kz-\omega t)} \right]
\end{eqnarray}
Solving for the time-dependent coefficients, then:
@@ -79,15 +79,11 @@ Where $\omega_a$ and $\omega_b$ are the fast (and familiar) Bohr frequencies and
In Dirac notation \cite{DiracPaulAdrienMaurice1939a}, an observable (such as $\mu(t)$) can be
written simply: %
\begin{equation}
- \mu(t) = \left< c_aa + c_bb \left| \hat{H} \right| c_aa + c_bb \right>
+ \mu(t) = |c_a(t)|^2 \langle \phi_a | \mu | \phi_a \rangle + |c_b(t)|^2 \langle \phi_b | \mu | \phi_b \rangle + c_a(t) c_b^*(t) \langle \phi_b | \mu | \phi_a \rangle +
+ c_b(t) c_a^*(t) \langle \phi_a | \mu | \phi_b \rangle
\end{equation}
The complex wavefunction is called a \emph{ket}, represented $\left|b\right>$. %
The complex conjugate is called a \emph{bra}, represented $\left<a\right|$. %
-When expanded,
-\begin{equation}
- \mu(t) = c_a^2\mu_a + c_b^2\mu_b + \left< c_aa \left| \hat{H} \right| c_bb \right> +
- \left<c_bb \left| \hat{H} \right| c_aa \right>
-\end{equation}
The first two terms are populations and the final two terms are coherences. %
The coherent terms will evolve with the rapid Bohr oscillations, coupling the dipole observable
with the time-dependent electric field. %
@@ -146,18 +142,19 @@ These are workhorse experiments, like absorbance, reflectance, FTIR, UV-Vis, and
ordinary Raman spectroscopy (COORS). %
These experiments are incredibly robust, and are typically performed using easy to use commercial
desktop instruments. %
-There are now even handheld Raman spectrometers for use in industrial settings. [CITE] %
+There are now even handheld Raman spectrometers for use in industrial settings. \cite{nanoram} %
Multidimensional spectroscopy contains a lot more information about the material under
investigation. %
In this work, by ``multidimensional'' I mean higher-order spectroscopy. %
-I ignore ``correlation spectroscopy'' [CITE], which tracks linear spectral features against
-non-spectral dimensions like lab time, pressure, and temperature. %
+I ignore ``correlation spectroscopy'' (otherwise known as covariance spectroscopy), which tracks
+linear spectral features against non-spectral dimensions like lab time, pressure, and
+temperature. %
So, in the context of this dissertation, multidimensional spectroscopy is synonymous with nonlinear
spectroscopy. %
Nonlinear spectroscopy relies upon higher-order terms in the light-matter interaction. In a generic
-system, each term is roughly ten times smaller than the last. % TODO: cite?
+system, a rule of thumb states that each term is roughly ten times smaller than the last. %
This means that nonlinear spectroscopy is typically very weak. %
Still, nonlinear signals are fairly easy to isolate and measure using modern instrumentation, as
this dissertation describes. %
@@ -261,67 +258,68 @@ space. %
Since signal goes as $N^2$, signal decays much faster in homodyne-collected experiments. %
If signal decays as a single exponential, the extracted decay is twice as fast for homodyne vs
heterodyne-detected data. %
-[CITE DARIEN CORRECTION]
-
-\section{Instrumentation} % ======================================================================
-
-In this section I introduce the key components of the MR-CMDS instrument. %
-This also serves to introduce the reader to the particular components used in my research. %
-
-\subsection{LASER} % -----------------------------------------------------------------------------
-
-Light Amplified by Stimulated Emission of Radiation (LASER) light sources are absolutely crucial
-components of the modern MR-CMDS instrument. %
-The first laser was built in 1960 by \textcite{MaimanTheodore1960a}, and pulsed lasers were
-invented soon after. %
-Today, ultrafast light sources are relatively cheap and reliable. %
-Our SpectraPhysics ``Tsunami'' oscillator uses passive Kerr-lens mode-locking to generate $\sim$35
-fs seed pulses at $\sim$80 MHz (one pulse every 12.5 nanoseconds). \cite{Tsunami} %
-This seed is split and fed into two 1 KHz amplifiers, a picosecond ``Spitfire Ace''
-\cite{SpitfireAce} and a femtosecond ``Spitfire Pro'' \cite{SpitfirePro}. %
-These amplifiers each output several watts of ultrafast pulses at 1 KHz (one pulse per
-millisecond). %
-
-\subsection{Optical parametric amplifiers} % -----------------------------------------------------
-
-Optical Parametric Amplifiers (OPAs) are arguably the most crucial component of modern MR-CMDS, as
-they provide the frequency tunable light sources that we require. \cite{CerulloGiulio2003a} %
-OPAs provide tunability through three-wave sum and difference frequency generation processes. %
-``Fundamental'' tunability is achieved by splitting the 800 nm photons into two lower energy
-photons, with a splitting ratio determined by motorized optics. %
-These split photons are called ``signal'' and ``idler'', with signal being the higher energy and
-idler the lower energy photon. %
-
-% TODO: paragraph about phase matching conditions and polarization
-
-Signal and idler are then either used directly, or amplified through sum or difference frequency
-processes to provide broadband tuneability. %
-All available optical processes for the TOPAS-C OPAs \cite{TOPAS-C} used on the femtosecond table
-are shown in \autoref{spc:fig:ranges}. %
-Amazingly, these OPAs offer tunability from the mid-infrared to the ultraviolet. %
-Currently we do not have proper automated filters to make it possible to continuously scan between
-regions, but such things are possible. %
-
-On the picosecond table we have three separate kinds of OPAs, including one TOPAS-800
-\cite{TOPAS-800} and two OPA-800 models that have been modified with precision micro control
-\cite{PMC} servo motors to provide automated tunability. %
-
-\subsection{Delay stages} % ----------------------------------------------------------------------
-
-Delay stages are simple, one-motor devices which are used to control the relative arrival time of
-pulses at the sample. %
-The Wright Group currently owns four models of delay stage: 1. Newport MFA-CC [CITE], 2. Aerotech
-... [CITE], 3. Thorlabs LTS300 [CITE]. %
-The fourth ``model'' are actually homemade stages that are driven using PMC motors. %
-
-\subsection{Spectrometers} % ---------------------------------------------------------------------
-
-Spectrometers...
-
-\begin{figure}
- \includegraphics[width=\linewidth]{spectroscopy/ranges}
- \caption{
- CAPTION TODO
- }
- \label{spc:fig:ranges}
-\end{figure} \ No newline at end of file
+This fact is often forgotten, and papers have been corrected for forgetting this factor of
+two. \cite{KoivistoinenJuha2017a} %
+
+% \section{Instrumentation} % ======================================================================
+
+% In this section I introduce the key components of the MR-CMDS instrument. %
+% This also serves to introduce the reader to the particular components used in my research. %
+
+% \subsection{LASER} % -----------------------------------------------------------------------------
+
+% Light Amplified by Stimulated Emission of Radiation (LASER) light sources are absolutely crucial
+% components of the modern MR-CMDS instrument. %
+% The first laser was built in 1960 by \textcite{MaimanTheodore1960a}, and pulsed lasers were
+% invented soon after. %
+% Today, ultrafast light sources are relatively cheap and reliable. %
+% Our SpectraPhysics ``Tsunami'' oscillator uses passive Kerr-lens mode-locking to generate $\sim$35
+% fs seed pulses at $\sim$80 MHz (one pulse every 12.5 nanoseconds). \cite{Tsunami} %
+% This seed is split and fed into two 1 KHz amplifiers, a picosecond ``Spitfire Ace''
+% \cite{SpitfireAce} and a femtosecond ``Spitfire Pro'' \cite{SpitfirePro}. %
+% These amplifiers each output several watts of ultrafast pulses at 1 KHz (one pulse per
+% millisecond). %
+
+% \subsection{Optical parametric amplifiers} % -----------------------------------------------------
+
+% Optical Parametric Amplifiers (OPAs) are arguably the most crucial component of modern MR-CMDS, as
+% they provide the frequency tunable light sources that we require. \cite{CerulloGiulio2003a} %
+% OPAs provide tunability through three-wave sum and difference frequency generation processes. %
+% ``Fundamental'' tunability is achieved by splitting the 800 nm photons into two lower energy
+% photons, with a splitting ratio determined by motorized optics. %
+% These split photons are called ``signal'' and ``idler'', with signal being the higher energy and
+% idler the lower energy photon. %
+
+% % TODO: paragraph about phase matching conditions and polarization
+
+% Signal and idler are then either used directly, or amplified through sum or difference frequency
+% processes to provide broadband tuneability. %
+% All available optical processes for the TOPAS-C OPAs \cite{TOPAS-C} used on the femtosecond table
+% are shown in \autoref{spc:fig:ranges}. %
+% Amazingly, these OPAs offer tunability from the mid-infrared to the ultraviolet. %
+% Currently we do not have proper automated filters to make it possible to continuously scan between
+% regions, but such things are possible. %
+
+% On the picosecond table we have three separate kinds of OPAs, including one TOPAS-800
+% \cite{TOPAS-800} and two OPA-800 models that have been modified with precision micro control
+% \cite{PMC} servo motors to provide automated tunability. %
+
+% \subsection{Delay stages} % ----------------------------------------------------------------------
+
+% Delay stages are simple, one-motor devices which are used to control the relative arrival time of
+% pulses at the sample. %
+% The Wright Group currently owns four models of delay stage: 1. Newport MFA-CC [CITE], 2. Aerotech
+% ... [CITE], 3. Thorlabs LTS300 [CITE]. %
+% The fourth ``model'' are actually homemade stages that are driven using PMC motors. %
+
+% \subsection{Spectrometers} % ---------------------------------------------------------------------
+
+% Spectrometers...
+
+% \begin{figure}
+% \includegraphics[width=\linewidth]{spectroscopy/ranges}
+% \caption{
+% CAPTION TODO
+% }
+% \label{spc:fig:ranges}
+% \end{figure} \ No newline at end of file
diff --git a/todo.org b/todo.org
index 33942ff..54a48d9 100644
--- a/todo.org
+++ b/todo.org
@@ -1,16 +1,3 @@
-* CANCELED headers :int:
- CLOSED: [2018-04-15 Sun 15:50]
-* TODO cite important CMDS discoveries, reviews :int:
-* TODO incorporate Nancy's comments :int:
-* TODO incorporate Claire's comments :int:
-* TODO summarize PbSe chapter :int:
-* TODO summarize MX2 chapter :int:
-* TODO summarize PEDOT:PSS chapter :int:
-* TODO verify light-matter interaction content :spc:
-* TODO finish instrumentation section (darien) :spc:
-* IDEA linear vs multidimensional figure :spc:
-* IDEA see Paul's dissertation :spc:
-** re: loss of resonance advantage with very fast pulses
* TODO more references for object oriented programming :sof:
** in inbox
* IDEA incorporate StoddenVictoria2016a :sof: