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1 %!TEX root = /Users/charles/Desktop/nanoglass/nanoglass.tex
2
3 \section{Computational Methodology}
4 \label{sec:details}
5
6 \subsection{Initial Geometries and Heating}
7
8 Cu-core / Ag-shell and random alloy structures were constructed on an
9 underlying FCC lattice (4.09 {\AA}) at the bulk eutectic composition
10 $\mathrm{Ag}_6\mathrm{Cu}_4$. Both initial geometries were considered
11 although experimental results suggest that the random structure is the
12 most likely structure to be found following
13 synthesis.\cite{Jiang:2005lr,gonzalo:5163} Three different sizes of
14 nanoparticles corresponding to a 20 \AA radius (2382 atoms), 30 {\AA}
15 radius (6603 atoms) and 40 {\AA} radius (15683 atoms) were
16 constructed. These initial structures were relaxed to their
17 equilibrium structures at 20 K for 20 ps and again at 300 K for 100 ps
18 sampling from a Maxwell-Boltzmann distribution at each
19 temperature. All simulations were conducted using the {\sc oopse}
20 molecular dynamics package.\cite{Meineke:2004uq}
21
22 To mimic the effects of the heating due to laser irradiation, the
23 particles were allowed to melt by sampling velocities from the Maxwell
24 Boltzmann distribution at a temperature of 900 K. The particles were
25 run under microcanonical simulation conditions for 1 ns of simualtion
26 time prior to studying the effects of heat transfer to the solvent.
27 In all cases, center of mass translational and rotational motion of
28 the particles were set to zero before any data collection was
29 undertaken. Structural features (pair distribution functions) were
30 used to verify that the particles were indeed liquid droplets before
31 cooling simulations took place.
32
33 \subsection{Modeling random alloy and core shell particles in solution
34 phase environments}
35
36 To approximate the effects of rapid heat transfer to the solvent
37 following a heating at the plasmon resonance, we utilized a
38 methodology in which atoms contained in the outer $4$ {\AA} radius of
39 the nanoparticle evolved under Langevin Dynamics,
40 \begin{equation}
41 m \frac{\partial^2 \vec{x}}{\partial t^2} = F_\textrm{sys}(\vec{x}(t))
42 - 6 \pi a \eta \vec{v}(t) + F_\textrm{ran}
43 \label{eq:langevin}
44 \end{equation}
45 with a solvent friction ($\eta$) approximating the contribution from
46 the solvent and capping agent. Atoms located in the interior of the
47 nanoparticle evolved under Newtonian dynamics. The set-up of our
48 simulations is nearly identical with the ``stochastic boundary
49 molecular dynamics'' ({\sc sbmd}) method that has seen wide use in the
50 protein simulation
51 community.\cite{BROOKS:1985kx,BROOKS:1983uq,BRUNGER:1984fj} A sketch
52 of this setup can be found in Fig. \ref{fig:langevinSketch}. In
53 Eq. (\ref{eq:langevin}) the frictional forces of a spherical atom
54 of radius $a$ depend on the solvent viscosity. The random forces are
55 usually taken as gaussian random variables with zero mean and a
56 variance tied to the solvent viscosity and temperature,
57 \begin{equation}
58 \langle F_\textrm{ran}(t) \cdot F_\textrm{ran} (t')
59 \rangle = 2 k_B T (6 \pi \eta a) \delta(t - t')
60 \label{eq:stochastic}
61 \end{equation}
62 Due to the presence of the capping agent and the lack of details about
63 the atomic-scale interactions between the metallic atoms and the
64 solvent, the effective viscosity is a essentially a free parameter
65 that must be tuned to give experimentally relevant simulations.
66 \begin{figure}[htbp]
67 \centering
68 \includegraphics[width=5in]{images/stochbound.pdf}
69 \caption{Methodology used to mimic the experimental cooling conditions
70 of a hot nanoparticle surrounded by a solvent. Atoms in the core of
71 the particle evolved under Newtonian dynamics, while atoms that were
72 in the outer skin of the particle evolved under Langevin dynamics.
73 The radius of the spherical region operating under Newtonian dynamics,
74 $r_\textrm{Newton}$ was set to be 4 {\AA} smaller than the original
75 radius ($R$) of the liquid droplet.}
76 \label{fig:langevinSketch}
77 \end{figure}
78
79 The viscosity ($\eta$) can be tuned by comparing the cooling rate that
80 a set of nanoparticles experience with the known cooling rates for
81 similar particles obtained via the laser heating experiments.
82 Essentially, we tune the solvent viscosity until the thermal decay
83 profile matches a heat-transfer model using reasonable values for the
84 interfacial conductance and the thermal conductivity of the solvent.
85
86 Cooling rates for the experimentally-observed nanoparticles were
87 calculated from the heat transfer equations for a spherical particle
88 embedded in a ambient medium that allows for diffusive heat transport.
89 Following Plech {\it et al.},\cite{plech:195423} we use a heat
90 transfer model that consists of two coupled differential equations
91 in the Laplace domain,
92 \begin{eqnarray}
93 Mc_{P}\cdot(s\cdot T_{p}(s)-T_{0})+4\pi R^{2} G\cdot(T_{p}(s)-T_{f}(r=R,s)=0\\
94 \left(\frac{\partial}{\partial r} T_{f}(r,s)\right)_{r=R} +
95 \frac{G}{K}(T_{p}(s)-T_{f}(r,s) = 0
96 \label{eq:heateqn}
97 \end{eqnarray}
98 where $s$ is the time-conjugate variable in Laplace space. The
99 variables in these equations describe a nanoparticle of radius $R$,
100 mass $M$, and specific heat $c_{p}$ at an initial temperature
101 $T_0$. The surrounding solvent has a thermal profile $T_f(r,t)$,
102 thermal conductivity $K$, density $\rho$, and specific heat $c$. $G$
103 is the interfacial conductance between the nanoparticle and the
104 surrounding solvent, and contains information about heat transfer to
105 the capping agent as well as the direct metal-to-solvent heat loss.
106 The temperature of the nanoparticle as a function of time can then
107 obtained by the inverse Laplace transform,
108 \begin{equation}
109 T_{p}(t)=\frac{2 k R^2 g^2
110 T_0}{\pi}\int_{0}^{\infty}\frac{\exp(-\kappa u^2
111 t/R^2)u^2}{(u^2(1 + R g) - k R g)^2+(u^3 - k R g u)^2}\mathrm{d}u.
112 \label{eq:laplacetransform}
113 \end{equation}
114 For simplicity, we have introduced the thermal diffusivity $\kappa =
115 K/(\rho c)$, and defined $k=4\pi R^3 \rho c /(M c_p)$ and $g = G/K$ in
116 Eq. (\ref{eq:laplacetransform}).
117
118 Eq. (\ref{eq:laplacetransform}) was solved numerically for the Ag-Cu
119 system using mole-fraction weighted values for $c_p$ and $\rho_p$ of
120 0.295 $(\mathrm{J g^{-1} K^{-1}})$ and $9.826\times 10^6$ $(\mathrm{g
121 m^{-3}})$ respectively. Since most of the laser excitation experiments
122 have been done in aqueous solutions, parameters used for the fluid are
123 $K$ of $0.6$ $(\mathrm{Wm^{-1}K^{-1}})$, $\rho$ of $1.0\times10^6$
124 $(\mathrm{g m^{-3}})$ and $c$ of $4.184$ $(\mathrm{J g^{-1} K^{-1}})$.
125
126 Values for the interfacial conductance have been determined by a
127 number of groups for similar nanoparticles and range from a low
128 $87.5\times 10^{6} (\mathrm{Wm^{-2}K^{-1}})$ to $130\times 10^{6}
129 (\mathrm{Wm^{-2}K^{-1}})$.\cite{Wilson:2002uq} Wilson {\it
130 et al.} worked with Au, Pt, and AuPd nanoparticles and obtained an
131 estimate for the interfacial conductance of $G=130
132 (\mathrm{Wm^{-2}K^{-1}})$.\cite{Wilson:2002uq} Similarly, Plech {\it
133 et al.} reported a value for the interfacial conductance of $G=105\pm
134 15 (\mathrm{Wm^{-2}K^{-1}})$ for Au nanoparticles.\cite{plech:195423}
135
136 We conducted our simulations at both ends of the range of
137 experimentally-determined values for the interfacial conductance.
138 This allows us to observe both the slowest and fastest heat transfers
139 from the nanoparticle to the solvent that are consistent with
140 experimental observations. For the slowest heat transfer, a value for
141 G of $87.5\times 10^{6}$ $(\mathrm{Wm^{-2}K^{-1}})$ was used and for
142 the fastest heat transfer, a value of $117\times 10^{6}$
143 $(\mathrm{Wm^{-2}K^{-1}})$ was used. Based on calculations we have
144 done using raw data from the Hartland group's thermal half-time
145 experiments on Au nanospheres,\cite{HuM._jp020581+} the true G values
146 are probably in the faster regime: $117\times 10^{6}$
147 $(\mathrm{Wm^{-2}K^{-1}})$.
148
149 The rate of cooling for the nanoparticles in a molecular dynamics
150 simulation can then be tuned by changing the effective solvent
151 viscosity ($\eta$) until the nanoparticle cooling rate matches the
152 cooling rate described by the heat-transfer Eq.
153 (\ref{eq:heateqn}). The effective solvent viscosity (in Pa s) for a G
154 of $87.5\times 10^{6}$ $(\mathrm{Wm^{-2}K^{-1}})$ is $4.2 \times
155 10^{-6}$, $5.0 \times 10^{-6}$, and
156 $5.5 \times 10^{-6}$ for 20 {\AA}, 30 {\AA}, and 40 {\AA} particles, respectively. The
157 effective solvent viscosity (again in Pa s) for an interfacial
158 conductance of $117\times 10^{6}$ $(\mathrm{Wm^{-2}K^{-1}})$ is $5.7
159 \times 10^{-6}$, $7.2 \times 10^{-6}$, and $7.5 \times 10^{-6}$
160 for 20 {\AA}, 30 {\AA} and 40 {\AA} particles. These viscosities are
161 essentially gas-phase values, a fact which is consistent with the
162 initial temperatures of the particles being well into the
163 super-critical region for the aqueous environment. Gas bubble
164 generation has also been seen experimentally around gold nanoparticles
165 in water.\cite{kotaidis:184702} Instead of a single value for the
166 effective viscosity, a time-dependent parameter might be a better
167 mimic of the cooling vapor layer that surrounds the hot particles.
168 This may also be a contributing factor to the size-dependence of the
169 effective viscosities in our simulations.
170
171 Cooling traces for each particle size are presented in
172 Fig. \ref{fig:images_cooling_plot}. It should be noted that the
173 Langevin thermostat produces cooling curves that are consistent with
174 Newtonian (single-exponential) cooling, which cannot match the cooling
175 profiles from Eq. (\ref{eq:laplacetransform}) exactly. Fitting the
176 Langevin cooling profiles to a single-exponential produces
177 $\tau=25.576$ ps, $\tau=43.786$ ps, and $\tau=56.621$ ps for the 20,
178 30 and 40 {\AA} nanoparticles and a G of $87.5\times 10^{6}$
179 $(\mathrm{Wm^{-2}K^{-1}})$. For comparison's sake, similar
180 single-exponential fits with an interfacial conductance of G of
181 $117\times 10^{6}$ $(\mathrm{Wm^{-2}K^{-1}})$ produced a $\tau=13.391$
182 ps, $\tau=30.426$ ps, $\tau=43.857$ ps for the 20, 30 and 40 {\AA}
183 nanoparticles.
184
185 \begin{figure}[htbp]
186 \centering
187 \includegraphics[width=5in]{images/cooling_plot.pdf}
188 \caption{Thermal cooling curves obtained from the inverse Laplace
189 transform heat model in Eq. (\ref{eq:laplacetransform}) (solid line) as
190 well as from molecular dynamics simulations (circles). Effective
191 solvent viscosities of 4.2-7.5 $\times 10^{-6}$ Pa s (depending on the
192 radius of the particle) give the best fit to the experimental cooling
193 curves. This viscosity suggests that the nanoparticles in these
194 experiments are surrounded by a vapor layer (which is a reasonable
195 assumptions given the initial temperatures of the particles). }
196 \label{fig:images_cooling_plot}
197 \end{figure}
198
199 \subsection{Potentials for classical simulations of bimetallic
200 nanoparticles}
201
202 Several different potential models have been developed that reasonably
203 describe interactions in transition metals. In particular, the
204 Embedded Atom Model ({\sc eam})~\cite{PhysRevB.33.7983} and
205 Sutton-Chen ({\sc sc})~\cite{Chen90} potential have been used to study
206 a wide range of phenomena in both bulk materials and
207 nanoparticles.\cite{Vardeman-II:2001jn,ShibataT._ja026764r,Sankaranarayanan:2005lr,Chui:2003fk,Wang:2005qy,Medasani:2007uq} Both
208 potentials are based on a model of a metal which treats the nuclei and
209 core electrons as pseudo-atoms embedded in the electron density due to
210 the valence electrons on all of the other atoms in the system. The
211 {\sc sc} potential has a simple form that closely resembles that of
212 the ubiquitous Lennard Jones potential,
213 \begin{equation}
214 \label{eq:SCP1}
215 U_{tot}=\sum _{i}\left[ \frac{1}{2}\sum _{j\neq i}D_{ij}V^{pair}_{ij}(r_{ij})-c_{i}D_{ii}\sqrt{\rho_{i}}\right] ,
216 \end{equation}
217 where $V^{pair}_{ij}$ and $\rho_{i}$ are given by
218 \begin{equation}
219 \label{eq:SCP2}
220 V^{pair}_{ij}(r)=\left( \frac{\alpha_{ij}}{r_{ij}}\right)^{n_{ij}}, \rho_{i}=\sum_{j\neq i}\left( \frac{\alpha_{ij}}{r_{ij}}\right) ^{m_{ij}}.
221 \end{equation}
222 $V^{pair}_{ij}$ is a repulsive pairwise potential that accounts for
223 interactions between the pseudoatom cores. The $\sqrt{\rho_i}$ term in
224 Eq. (\ref{eq:SCP1}) is an attractive many-body potential that models
225 the interactions between the valence electrons and the cores of the
226 pseudo-atoms. $D_{ij}$, $D_{ii}$ set the appropriate overall energy
227 scale, $c_i$ scales the attractive portion of the potential relative
228 to the repulsive interaction and $\alpha_{ij}$ is a length parameter
229 that assures a dimensionless form for $\rho$. These parameters are
230 tuned to various experimental properties such as the density, cohesive
231 energy, and elastic moduli for FCC transition metals. The quantum
232 Sutton-Chen ({\sc q-sc}) formulation matches these properties while
233 including zero-point quantum corrections for different transition
234 metals.\cite{PhysRevB.59.3527} This particular parametarization has
235 been shown to reproduce the experimentally available heat of mixing
236 data for both FCC solid solutions of Ag-Cu and the high-temperature
237 liquid.\cite{sheng:184203} In contrast, the {\sc eam} potential does
238 not reproduce the experimentally observed heat of mixing for the
239 liquid alloy.\cite{MURRAY:1984lr} In this work, we have utilized the
240 {\sc q-sc} formulation for our potential energies and forces.
241 Combination rules for the alloy were taken to be the arithmetic
242 average of the atomic parameters with the exception of $c_i$ since its
243 values is only dependent on the identity of the atom where the density
244 is evaluated. For the {\sc q-sc} potential, cutoff distances are
245 traditionally taken to be $2\alpha_{ij}$ and include up to the sixth
246 coordination shell in FCC metals.
247
248 %\subsection{Sampling single-temperature configurations from a cooling
249 %trajectory}
250
251 To better understand the structural changes occurring in the
252 nanoparticles throughout the cooling trajectory, configurations were
253 sampled at regular intervals during the cooling trajectory. These
254 configurations were then allowed to evolve under NVE dynamics to
255 sample from the proper distribution in phase space. Fig.
256 \ref{fig:images_cooling_time_traces} illustrates this sampling.
257
258
259 \begin{figure}[htbp]
260 \centering
261 \includegraphics[height=3in]{images/cooling_time_traces.pdf}
262 \caption{Illustrative cooling profile for the 40 {\AA}
263 nanoparticle evolving under stochastic boundary conditions
264 corresponding to $G=$$87.5\times 10^{6}$
265 $(\mathrm{Wm^{-2}K^{-1}})$. At temperatures along the cooling
266 trajectory, configurations were sampled and allowed to evolve in the
267 NVE ensemble. These subsequent trajectories were analyzed for
268 structural features associated with bulk glass formation.}
269 \label{fig:images_cooling_time_traces}
270 \end{figure}
271
272
273 \begin{figure}[htbp]
274 \centering
275 \includegraphics[width=5in]{images/cross_section_array.jpg}
276 \caption{Cutaway views of 30 \AA\ Ag-Cu nanoparticle structures for
277 random alloy (top) and Cu (core) / Ag (shell) initial conditions
278 (bottom). Shown from left to right are the crystalline, liquid
279 droplet, and final glassy bead configurations.}
280 \label{fig:cross_sections}
281 \end{figure}