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Subject: ** [ PSI-K ]   Postdoc: First-Principles Simulations/Modeling of Phonon Linewidths in Thermoelectric Materials
Status: RO
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X-UID: 1

An announcement has been updated in the "PSI-K" site at PSI-K (<a href=3D"h=
ttp://cselnx9.dl.ac.uk:8080/portal">http://cselnx9.dl.ac.uk:8080/portal</a>=
)<br />
<br />
<br />
Subject: Postdoc: First-Principles Simulations/Modeling of Phonon Linewidth=
s in Thermoelectric Materials<br />
<br />
Category: Job<br />
<br />
From: Olivier Delaire<br />
<br />
Date: 01-Oct-2011 01:00<br />
<br />
Message: <br />
<br />
<div class=3D"form_row" >
<div class=3D"form_label" >Description</div>
<div class=3D"form_data" >
<div class=3D"web_default_style" >
<p><font face=3D"TimesNewRomanPSMT" >Postdoc Position at Oak Ridge National=
  Laboratory (USA): First-Principles Simulations and Modeling of Phonon  Li=
newidths in Thermoelectric Materials.</font></p>
<p><font face=3D"TimesNewRomanPSMT" >The goal of this project is to gain kn=
owledge about phonon energies and linewidths (inverse of </font><font face=
=3D"TimesNewRomanPSMT" >lifetimes), and their systematic dependence on temp=
erature, composition, or the underlying </font><font face=3D"TimesNewRomanP=
SMT" >electronic structure, to predict their impact on thermoelectric effic=
iency [1,2,3,4,5]. The project </font><font face=3D"TimesNewRomanPSMT" >inv=
olves collaboration between leading experimentalists, ab-initio theorists, =
and computer </font><font face=3D"TimesNewRomanPSMT" >scientists at ORNL. T=
he research will involve performing detailed calculations of phonon </font>=
<font face=3D"TimesNewRomanPSMT" >energies and linewidths (using first-prin=
ciples as well as force-field methods), and benchmarking </font><font face=
=3D"TimesNewRomanPSMT" >against experimental measurements. </font></p>
<p><font face=3D"TimesNewRomanPSMT" >The tasks will include writing softwar=
e to fit experimental </font><font face=3D"TimesNewRomanPSMT" >data with pa=
rameterized models, and perform numerical optimization of phonon lifetimes.=
 The </font><font face=3D"TimesNewRomanPSMT" >software will be implemented =
on the high-performance computers at ORNL (including hybrid </font><font fa=
ce=3D"TimesNewRomanPSMT" >architecture based on General Purpose Graphical P=
rocessing Unit) to optimize our phonon </font><font face=3D"TimesNewRomanPS=
MT" >dynamics models, and directly fit the experimental datasets. The convo=
lution of phonon </font><font face=3D"TimesNewRomanPSMT" >simulations with =
the response function of neutron scattering spectrometers at the Spallation=
 </font><font face=3D"TimesNewRomanPSMT" >Neutron Source will produce reali=
stic simulated datasets, directly comparable with experiments.&nbsp; </font=
></p>
<p><font face=3D"TimesNewRomanPSMT" >The outcome of this research will enab=
le benchmarking microscopic theories of thermal </font><font face=3D"TimesN=
ewRomanPSMT" >conductivity, and developing more efficient thermoelectric ma=
terials. This research will leverage </font><font face=3D"TimesNewRomanPSMT=
" >the world-class computing and neutron scattering resources at ORNL.</fon=
t></p>
<p align=3D"left" ><font face=3D"TimesNewRomanPSMT" ><strong><font face=3D"=
TimesNewRomanPS-BoldMT" >References:</font></strong></font></p>
<ol>
    <li><font face=3D"TimesNewRomanPSMT" ><font face=3D"TimesNewRomanPSMT" =
>O. Delaire, K. Marty , M. B. Stone, P. R. C. Kent, M. S. Lucas, D. L. Aber=
nathy, D. </font><font face=3D"TimesNewRomanPSMT" >Mandrus, B. C. Sales, </=
font><strong><font face=3D"TimesNewRomanPS-BoldMT" >Proc. Natl. Acad. Sci. =
</font></strong><font face=3D"TimesNewRomanPSMT" >USA </font><strong><font =
face=3D"TimesNewRomanPS-BoldMT" >108</font></strong><font face=3D"TimesNewR=
omanPSMT" >, 4725 (2011)</font><em><font face=3D"TimesNewRomanPS-ItalicMT" =
>.</font></em></font></li>
    <li><font face=3D"TimesNewRomanPSMT" ><font face=3D"TimesNewRomanPSMT" =
>B. C. Sales, O. Delaire, M. A. McGuire, and A. F. May, </font><strong><fon=
t face=3D"TimesNewRomanPS-BoldMT" >Phys. Rev. B 83</font></strong><font fac=
e=3D"TimesNewRomanPSMT" >, 125209 (2011).</font></font></li>
    <li><font face=3D"TimesNewRomanPSMT" ><font face=3D"TimesNewRomanPSMT" =
>O. Delaire </font><em><font face=3D"TimesNewRomanPS-ItalicMT" >et al.</fon=
t></em><font face=3D"TimesNewRomanPSMT" >, </font><strong><font face=3D"Tim=
esNewRomanPS-BoldMT" >Nature Materials, </font></strong><font face=3D"Times=
NewRomanPSMT" >doi:10.1038/nmat3035 (2011).</font></font></li>
    <li><font face=3D"TimesNewRomanPSMT" ><font face=3D"TimesNewRomanPSMT" =
>O. Delaire, A. F. May, M. A. McGuire, W. D. Porter, M. S. Lucas, M. B. Sto=
ne, D. L. </font><font face=3D"TimesNewRomanPSMT" >Abernathy, and G. J. Sny=
der, </font><strong><font face=3D"TimesNewRomanPS-BoldMT" >Phys. Rev. B 80<=
/font></strong><font face=3D"TimesNewRomanPSMT" >, 184302 (2009).</font></f=
ont></li>
    <li><font face=3D"TimesNewRomanPSMT" ><font face=3D"TimesNewRomanPSMT" =
>O. Delaire, M.S. Lucas, J.A. Mu&ntilde;oz, M. Kresch, and B. Fultz, </font=
><strong><font face=3D"TimesNewRomanPS-BoldMT" >Phys. Rev. Lett</font></str=
ong><font face=3D"TimesNewRomanPSMT" >. </font><strong><font face=3D"TimesN=
ewRomanPS-BoldMT" >101</font></strong><font face=3D"TimesNewRomanPSMT" >, 1=
05504 </font><font face=3D"TimesNewRomanPSMT" >(2008).</font></font></li>
</ol>
</div>
</div>
</div>
<div class=3D"form_spacer" >&nbsp;</div>
<div class=3D"form_row" >
<div class=3D"form_label" >Qualifications</div>
<div class=3D"form_data" >
<div class=3D"web_default_style" >
<p align=3D"left" ><font face=3D"TimesNewRomanPSMT" >Candidates with a rece=
nt Ph.D. in Physics, Materials Science, Chemistry, or </font><font face=3D"=
TimesNewRomanPSMT" >related fields will be considered. Expertise with first=
-principles simulations (density functional </font><font face=3D"TimesNewRo=
manPSMT" >theory), and in particular phonon simulations (with linear respon=
se or direct method), is a </font><font face=3D"TimesNewRomanPSMT" >require=
ment for this position. Experience with molecular dynamics simulations, anh=
armonicity </font><font face=3D"TimesNewRomanPSMT" >calculations, many-body=
 techniques, and numerical optimization will be helpful. Good </font><font =
face=3D"TimesNewRomanPSMT" >programming skills with modern computer languag=
es (C++, Python) will be a strong advantage. </font><font face=3D"TimesNewR=
omanPSMT" >Strong written and oral communication skills and the desire to w=
ork in a team environment on </font><font face=3D"TimesNewRomanPSMT" >scien=
tifically challenging problems are required.</font></p>
<p align=3D"left" ><font face=3D"TimesNewRomanPSMT" ><font face=3D"TimesNew=
RomanPSMT" >Applicants cannot have received their Ph.D. </font><font face=
=3D"TimesNewRomanPSMT" >more than five years prior to the date of applicati=
on and must complete all degree requirements </font><font face=3D"TimesNewR=
omanPSMT" >before starting their appointment.</font></font></p>
<p align=3D"left" ><font face=3D"TimesNewRomanPSMT" ><font face=3D"TimesNew=
RomanPSMT" >For further information, please visit:</font></font></p>
<p align=3D"left" >https://www3.orau.gov/ORNL_TOppS/Posting/Details/188</p>
<p align=3D"left" >(Reference Code ORNL11-123-NSSD)</p>
</div>
</div>
</div><br />
<br />
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