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<div style="text-align:center"><span style="font-family:Cambria; background-color:rgb(255,255,255); vertical-align:baseline; white-space:pre-wrap"><span id="docs-internal-guid-748f50ce-f689-54d2-9b41-5a3c77a9e486" style=""><span id="docs-internal-guid-44741882-f788-0e32-c8e8-2b168c3681ef" style=""><span id="docs-internal-guid-d5bed97d-3f42-6ae7-0034-104ccf7b3897" style=""><span id="docs-internal-guid-498729f8-679a-0a20-28d6-2d9b55698270" style=""><span id="docs-internal-guid-51391753-8bcf-ef16-57fc-e1b7affdfc5f" style=""><span id="docs-internal-guid-42e41036-7fff-21b4-7d44-d4dd211c366f" style=""><span id="docs-internal-guid-5f05f5c9-7fff-beba-2406-c965c2ae057c" style=""><span id="docs-internal-guid-b54610e0-7fff-3506-dfd5-090d1f414dc8"><span id="docs-internal-guid-bccd1570-7fff-2f10-1577-65d92a6f7f88">
<p dir="ltr" style="line-height: 1.38; margin-top: 0pt; margin-bottom: 0pt;"><span style="font-size: 28pt; color: rgb(192, 0, 0); background-color: transparent; font-weight: 700; vertical-align: baseline;">Fall 2018 Colloquium</span></p>
<p dir="ltr" style="line-height: 1.38; margin-top: 0pt; margin-bottom: 0pt;"><span style="font-size: 16pt; background-color: transparent; font-weight: 700; vertical-align: baseline;">Department of Physics & Astronomy, TAMU-Commerce</span></p>
<p dir="ltr" style="line-height: 1.38; margin-top: 0pt; margin-bottom: 0pt;"><span style="font-size: 16pt; color: rgb(192, 0, 0); background-color: transparent; font-weight: 700; vertical-align: baseline;">Sep 27, Thursday, 4-5 PM in Science Building 127</span></p>
<p dir="ltr" style="line-height: 1.38; margin-top: 0pt; margin-bottom: 0pt;"><span style="font-size: 14pt; background-color: transparent; vertical-align: baseline;">(coffee and cookies will be served at 3:50 PM)</span></p>
<p dir="ltr" style="line-height: 1.38; margin-top: 0pt; margin-bottom: 0pt;"><span style="font-size: 14pt; color: rgb(0, 176, 80); background-color: transparent; font-weight: 700; vertical-align: baseline;">Astrophysics, Nuclear physics</span></p>
<p dir="ltr" style="line-height: 1.38; margin-top: 0pt; margin-bottom: 0pt;"><span style="font-size: 18pt; color: rgb(0, 0, 255); background-color: transparent; font-weight: 700; vertical-align: baseline;">Symmetry energy in nuclear matter
</span><span style="font-size: 18pt; color: rgb(0, 0, 255); background-color: transparent; font-weight: 700; vertical-align: baseline;"><br class="kix-line-break">
</span><span style="font-size: 18pt; color: rgb(0, 0, 255); background-color: transparent; font-weight: 700; vertical-align: baseline;">and in neutron star matter</span><span style="font-size: 18pt; color: rgb(0, 0, 255); background-color: transparent; font-weight: 700; vertical-align: baseline;"><br class="kix-line-break">
</span><span style="font-size: 14pt; background-color: transparent; font-weight: 700; vertical-align: baseline;">Dr. Jorge Lopez</span></p>
<p dir="ltr" style="line-height: 1.38; margin-top: 0pt; margin-bottom: 0pt;"><span style="font-size: 14pt; color: rgb(11, 83, 148); background-color: transparent; font-weight: 700; vertical-align: baseline;">University of Texas at El Paso</span><span style="font-size: 14pt; background-color: transparent; font-weight: 700; vertical-align: baseline;">
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<img src="https://lh6.googleusercontent.com/Rd42utw75qOafUB2OXmSTNnEoFyrRi7XnV6iyYBP7iO565Vx4LXAv3a9iaTKUpCFWWzBSugifQvfdk_cRg72-jzDrbQGNIcgsQ01ZH-oWvhZ9MS7SRu2Md77_xFVftf28uM7Ec4v" width="150" height="179" style="border: none; transform: rotate(0.00rad); -webkit-transform: rotate(0.00rad);">
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<span style="font-size: 12pt; vertical-align: baseline;">Dr. Jorge A. Lopez earned BS and MS degrees at the University of Texas at El Paso, and a PhD at the Texas A&M University. He was a postdoctoral researcher at the Niels Bohr Institute and at the Lawrence
Berkeley National Lab. His area of research has been nuclear physics with specialization in heavy ion reactions, but he has also performed research in materials science. In 2018 he received the Presidential Award for Excellence in Science, Mathematics, and
Engineering Mentoring from the White House, and was inducted into the Academy of Distinguished Former Students of Texas A&M University.
</span><span style="font-size: 11pt; vertical-align: baseline;">More information about Dr. Lopez can be found at</span><span style="font-size: 11pt; vertical-align: baseline;"><br class="kix-line-break">
</span><a href="https://urldefense.proofpoint.com/v2/url?u=https-3A__academics.utep.edu_Default.aspx-3Ftabid-3D18741&d=DwMF-g&c=oqyuZuih6ykib6aKiBq22_bich4AVfYGoLertJN0bEc&r=hjwEO_XYlnwAQWUGeaCrW47w4mK-Al28-BKyRvaivBs&m=ic9LAlrdKBNcP_3tNvY8SGvDKcYKSfcGc_vYjWUKuh0&s=qfp0MfenmuceLpKXAs2GYQ_8YucMMiMUqijAvlDLhjw&e=" style="text-decoration-line: none;"><span style="font-size: 12pt; color: rgb(17, 85, 204); text-decoration-line: underline; vertical-align: baseline;">https://academics.utep.edu/Default.aspx?tabid=18741</span></a></p>
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<p dir="ltr" style="line-height:1.38;margin-top:0pt;margin-bottom:4pt;"><span style="font-size: 12pt; background-color: transparent; font-weight: 700; vertical-align: baseline;">Abstract</span></p>
<p dir="ltr" style="line-height:1.38;margin-top:0pt;margin-bottom:0pt;text-align: justify;">
<span style="font-size: 12pt; vertical-align: baseline;">Results from classical molecular dynamics simulations of infinite nuclear systems with varying density, temperature and isospin content are used to calculate the symmetry energy at low nuclear densities
at several temperatures. The results show an excellent agreement with the experimental data (from Texas A&M Cyclotron Institute) and corroborate the claim that the formation of clusters has a strong influence on the symmetry energy in the liquid–gas coexistence
region.</span></p>
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