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  <title>DSpace Community:</title>
  <link rel="alternate" href="http://hdl.handle.net/1803/569" />
  <subtitle />
  <id>http://hdl.handle.net/1803/569</id>
  <updated>2013-06-19T07:08:21Z</updated>
  <dc:date>2013-06-19T07:08:21Z</dc:date>
  <entry>
    <title>Simulation and optimization of pulsed Chemical Exchange Saturation Transfer for clinical application at 3T</title>
    <link rel="alternate" href="http://hdl.handle.net/1803/5229" />
    <author>
      <name>Dewey, Blake</name>
    </author>
    <id>http://hdl.handle.net/1803/5229</id>
    <updated>2013-05-15T17:21:33Z</updated>
    <published>2013-04-22T05:00:00Z</published>
    <summary type="text">Title: Simulation and optimization of pulsed Chemical Exchange Saturation Transfer for clinical application at 3T
Authors: Dewey, Blake
Abstract: Chemical Exchange Saturation Transfer (CEST) is often overlooked as a method&#xD;
for the investigation of metabolites in vivo due to the time required to&#xD;
obtain a full spectrum. We investigated the feasibility and optimization of&#xD;
a pulsed CEST technique that interleaves an echo planer imaging (EPI)&#xD;
readout with saturation in order to reduce time. In addition, we&#xD;
incorporated a multi-shot EPI sequence that reduces distortions. To achieve&#xD;
this, computer simulations based on the Bloch equations were used to&#xD;
optimize scan parameters while keeping scan time in the clinical timeframe.&#xD;
To analyze the data, a number of Lorentizian fitting algorithms were&#xD;
investigated to evaluate their ability to isolate CEST contrast. By using a&#xD;
30 ms pulse at 2 μT, we were able to achieve CEST contrast on the order of&#xD;
2% and could provide APT maps based on an adapted Lorentzian fitting method.&#xD;
In the process of this fitting, it was also discovered that MTR contrast&#xD;
could also be recovered from the CEST data, allowing for MT and CEST to be&#xD;
acquired at the same time.</summary>
    <dc:date>2013-04-22T05:00:00Z</dc:date>
  </entry>
  <entry>
    <title>High-energy attosecond-width electron diffraction simulations</title>
    <link rel="alternate" href="http://hdl.handle.net/1803/5204" />
    <author>
      <name>Kidd, Daniel</name>
    </author>
    <id>http://hdl.handle.net/1803/5204</id>
    <updated>2013-05-10T18:56:44Z</updated>
    <published>2013-04-22T05:00:00Z</published>
    <summary type="text">Title: High-energy attosecond-width electron diffraction simulations
Authors: Kidd, Daniel
Abstract: Electron microscopy has been the recent subject of molecular imaging&#xD;
due to the strength of the electrons' interaction with the target&#xD;
molecule making for a detailed pattern at a small scale.[1] To achieve&#xD;
the best 4D image of the target, one needs sufficient&#xD;
spatial and temporal resolution, the prior being an issue of using&#xD;
electrons in the keV regime as to achieve an optimally small deBroglie&#xD;
wavelength, and the latter being improved by the temporal width of the&#xD;
electron wave packet itself.[2] In order to image the motion of the&#xD;
electronic structure of the target molecule, this width must be within&#xD;
the attosecond regime. In this paper, we use the computational method&#xD;
of time-dependent density functional theory (TDDFT) to model our&#xD;
targets of Beryllium and the Nitrogen molecule, N2 , and an incoming&#xD;
electron wave packet with an energy of 1500 eV.</summary>
    <dc:date>2013-04-22T05:00:00Z</dc:date>
  </entry>
  <entry>
    <title>An anomalous measurement of delta m31 squared from neutrino oscillations at the Daya Bay Reactor Neutrino Experiment</title>
    <link rel="alternate" href="http://hdl.handle.net/1803/5203" />
    <author>
      <name>Burroughs, Hunter</name>
    </author>
    <id>http://hdl.handle.net/1803/5203</id>
    <updated>2013-05-09T21:42:23Z</updated>
    <published>2013-04-22T05:00:00Z</published>
    <summary type="text">Title: An anomalous measurement of delta m31 squared from neutrino oscillations at the Daya Bay Reactor Neutrino Experiment
Authors: Burroughs, Hunter
Abstract: In 2012, the collaboration overseeing the Daya Bay Reactor Neutrino&#xD;
Experiment announced results which determined the magnitude of the mixing&#xD;
angle \theta_{13} with unprecedented precision. However, no attempt was made&#xD;
in the collaboration’s publications to predict the value of the most&#xD;
relevant mass-squared difference to the observed oscillation, \delta&#xD;
m^2_{31}. This paper presents the results of an analysis which suggests that&#xD;
the Daya Bay data prefers a value of \delta m^2_{31} which is far greater&#xD;
than its presently recognized value. Specifically, it is found that Daya Bay&#xD;
predicts \delta m^2_{31} = 3.53_(-1.07)^(+.74) × 10^(-3) eV^2, where the&#xD;
cited uncertainties correspond to the 99% confidence bounds. This&#xD;
measurement excludes the most precise current measurement of \delta&#xD;
m^2_{31}, the MINOS result, at a 99% confidence level and is in turn&#xD;
excluded by the MINOS data at a 10 \sigma level. The possibility that&#xD;
sterile neutrino effects are the cause of this anomalous result is&#xD;
considered and used to suggest further work.</summary>
    <dc:date>2013-04-22T05:00:00Z</dc:date>
  </entry>
  <entry>
    <title>Simulating the universe with GPU-accelerated supercomputers: n-body methods, tests, and examples</title>
    <link rel="alternate" href="http://hdl.handle.net/1803/5192" />
    <author>
      <name>Wibking, Benjamin</name>
    </author>
    <id>http://hdl.handle.net/1803/5192</id>
    <updated>2013-05-02T19:53:23Z</updated>
    <published>2013-04-22T05:00:00Z</published>
    <summary type="text">Title: Simulating the universe with GPU-accelerated supercomputers: n-body methods, tests, and examples
Authors: Wibking, Benjamin
Abstract: We demonstrate the acceleration obtained from using GPU/CPU hybrid clusters&#xD;
and supercomputers for N-body simulations of gravity based in part on the&#xD;
author's new code development.  Validation tests are shown for cosmological&#xD;
simulations and for galaxy simulations, along with their respective speedups&#xD;
compared to traditional simulations.  Potential new applications for science&#xD;
enabled by this advance are highlighted.</summary>
    <dc:date>2013-04-22T05:00:00Z</dc:date>
  </entry>
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