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UID:Baylor_CMS_Event-51061
DTSTAMP:20260609T041029Z
SUMMARY:CASPER Seminar: Mike Montgomery, UT Austin: 
DESCRIPTION;ENCODING=QUOTED-PRINTABLE: White dwarf stars are the endpoints of stellar evolution for the vast=0D=0A=
majority of stars. They lack nuclear reactions and are mainly supported=0D=0A=
by electron degeneracy pressure, making them simpler to model. Since=0D=0A=
they are essentially cooling off, their temperatures are diagnostic of=0D=0A=
their ages, and they can be used as cosmic clocks. In addition, a subset=0D=0A=
of them pulsate, and we can use these pulsations to probe their=0D=0A=
interiors. This allows us to test many "exotic" processes such as=0D=0A=
neutrino and (hypothetical) axion emission rates, crystallization of a=0D=0A=
dense plasma, the physics of turbulent convection, and it also allows us=0D=0A=
to detect the presence of orbiting planets. =0D=0A=

LOCATION:BSB C231
DTSTART;TZID=US_Central:20081003T140000
DTEND;TZID=US_Central:20081003T150000
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