Astroplasmas Seminar
Fridays at 12:30pm, Dome Room, Peyton Hall
Fridays at 12:30pm, Dome Room, Peyton Hall
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Speaker: Matt Caplan (Illinois State University)
Abstract: At sufficiently high temperatures matter becomes fully ionized, but under sufficiently high pressure those plasmas freeze solid. These “strongly coupled” plasmas have Coulomb energies orders of magnitude greater than their thermal energies and can be found in systems spanning electrically charged dusts to the crusts of neutron stars. While many of the physically interesting combinations of temperature and density are inaccessible to laboratory experiments on earth, numerical simulations allow us to study the detailed microphysics of these crystals such as how they break, with implications for starquakes, pulsar glitches, and more.