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X-WR-CALNAME:Physics &amp; Astronomy
X-ORIGINAL-URL:https://uwm.edu/physics
X-WR-CALDESC:Events for Physics &amp; Astronomy
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DTSTART:20240310T080000
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DTSTART:20251102T070000
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DTSTART:20260308T080000
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BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20251107T130000
DTEND;TZID=America/Chicago:20251107T140000
DTSTAMP:20260613T161805
CREATED:20250925T154451Z
LAST-MODIFIED:20250925T154451Z
UID:10435364-1762520400-1762524000@uwm.edu
SUMMARY:CGCA Seminar - Dr. Amy Steele
DESCRIPTION:Dr. Amy Steele\, Planetary Science Institute\nThe CGCA Friday Seminar Series is hosted by the Center for Gravitation\, Cosmology & Astrophysics at the University of Wisconsin-Milwaukee. These seminars cover a broad number of topics related to the Center’s research areas. Talk titles and abstracts will be posted when available.
URL:https://uwm.edu/physics/event/cgca-seminar-dr-amy-steele/
LOCATION:Kenwood IRC 2175\, Milwaukee\, WI\, 53211\, United States
CATEGORIES:CGCA Seminars
X-TRIBE-STATUS:
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BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20251107T153000
DTEND;TZID=America/Chicago:20251107T170000
DTSTAMP:20260613T161805
CREATED:20250919T154545Z
LAST-MODIFIED:20251105T181227Z
UID:10435353-1762529400-1762534800@uwm.edu
SUMMARY:CANCELLED: Physics Colloquium - Justin Goodrich
DESCRIPTION:Due to circumstances beyond our control\, the Physics Colloquium for Friday\, 11/7/2025 is cancelled. \nJustin Goodrich\, Brookhaven National Laboratory
URL:https://uwm.edu/physics/event/physics-colloquium-justin-goodrich/
LOCATION:Chemistry 108\, 2050 E Kenwood Blvd\, Milwaukee\, WI\, 53201\, United States
CATEGORIES:Physics Colloquia
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BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20251114T130000
DTEND;TZID=America/Chicago:20251114T140000
DTSTAMP:20260613T161805
CREATED:20250925T154637Z
LAST-MODIFIED:20251111T200515Z
UID:10435365-1763125200-1763128800@uwm.edu
SUMMARY:CGCA Seminar - Terrence Pierre Jacques
DESCRIPTION:Self-Consistent Simulations of the Bar-mode Instability in Rotating Quasi-Stable Neutron Stars\nDr. Terrence Pierre Jacques\nWest Virginia University \nRapidly rotating neutron stars (NSs) formed from core-collapse supernovae serve as excellent astrophysical laboratories for probing their equation of state (EoS) and internal structure. As these stars cool and contract\, their spin angular momentum may increase\, making them susceptible to the dynamical bar-mode instability. Once this instability sets in\, these stars experience a redistribution of matter and angular momentum\, producing gravitational waves that may be detectable by future observatories. \nIn this talk\, I will describe the numerical techniques used to model these quasi-stable NS configurations and demonstrate how gravitational wave signals produced from simulations can be used to constrain the NS EoS.
URL:https://uwm.edu/physics/event/cgca-seminar-terrence-pierre-jacques/
LOCATION:Kenwood IRC 2175\, Milwaukee\, WI\, 53211\, United States
CATEGORIES:CGCA Seminars
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BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20251114T153000
DTEND;TZID=America/Chicago:20251114T170000
DTSTAMP:20260613T161805
CREATED:20250919T154730Z
LAST-MODIFIED:20251105T181117Z
UID:10435354-1763134200-1763139600@uwm.edu
SUMMARY:CANCELLED: Physics Colloquium - Jong-Woo Kim
DESCRIPTION:Due to circumstances beyond our control\, the Physics Colloquium for Friday\, 11/14/2025 has been cancelled. \nJong-Woo Kim\, Argonne National Lab
URL:https://uwm.edu/physics/event/physics-colloquium-jong-woo-kim/
LOCATION:Chemistry 108\, 2050 E Kenwood Blvd\, Milwaukee\, WI\, 53201\, United States
CATEGORIES:Physics Colloquia
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BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20251115T130000
DTEND;TZID=America/Chicago:20251115T150000
DTSTAMP:20260613T161805
CREATED:20250925T155723Z
LAST-MODIFIED:20250925T182823Z
UID:10435369-1763211600-1763218800@uwm.edu
SUMMARY:Coffeeshop Astrophysics - Space Rocks and Stardust
DESCRIPTION:Space Rocks and Stardust\nSpeakers: Pratyasha Gitika\, Tamal RoyChowdhury\, Laila Vleeschower \nAre shooting stars really stars falling from the sky? Spoiler alert: they’re not! Those quick flashes of light are actually tiny bits of space dust and rock burning up in our atmosphere. In this talk\, we’ll take a journey through the leftovers of the formation of our Solar System: asteroids\, meteorites\, and comets. We’ll talk about how these cosmic “crumbs” sometimes light up our skies as meteor showers\, how a rock you could hold in your hand might be older than the Earth itself\, and how one very big space rock may have changed the path of life’s evolution on Earth by wiping out the dinosaurs. \nMore information is available on the Coffeeshop Astrophysics website.
URL:https://uwm.edu/physics/event/coffeeshop-astrophysics-space-rocks-and-stardust/
LOCATION:Anodyne Coffee Shop\, 224 W Bruce Street\, Milwaukee\, WI\, United States
CATEGORIES:Public Event
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BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20251121T130000
DTEND;TZID=America/Chicago:20251121T140000
DTSTAMP:20260613T161805
CREATED:20250925T154902Z
LAST-MODIFIED:20251113T211706Z
UID:10435366-1763730000-1763733600@uwm.edu
SUMMARY:CGCA Seminar - Prof. Sharon Morsink
DESCRIPTION:The masses and radii of the neutron stars observed by NICER\nProf. Sharon Morsink\nUniversity of Alberta \nNeutron stars are the densest known gravitationally-stable objects in the Universe. Their strong gravitational fields\, rapid rotation rates\, and supra-nuclear central densities allow for a fascinating interplay between general relativistic effects and nuclear physics theory. Pulse-profile modeling is a technique that uses the gravitationally-lensed X-ray flux emitted from hot spots on the neutron star’s surface to infer its mass and radius. General relativity is a crucial ingredient in this analysis. The Neutron Star Interior Composition ExploreR (NICER) is a NASA X-ray telescope mounted on the International Space Station. NICER is a timing instrument designed to make the measurements required to implement pulse-profile modelling. In this talk\, I will give an overview of how NICER data is used to infer a neutron star’s radius (and its mass)\, along with the latest results and future observations of other pulsars.
URL:https://uwm.edu/physics/event/cgca-seminar-dr-sharon-morsink/
LOCATION:Kenwood IRC 2175\, Milwaukee\, WI\, 53211\, United States
CATEGORIES:CGCA Seminars
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BEGIN:VEVENT
DTSTART;TZID=America/Chicago:20251121T153000
DTEND;TZID=America/Chicago:20251121T170000
DTSTAMP:20260613T161805
CREATED:20250919T154830Z
LAST-MODIFIED:20250919T154830Z
UID:10435355-1763739000-1763744400@uwm.edu
SUMMARY:Physics Colloquium - Julian May Mann
DESCRIPTION:Physics Colloquium – Julian May Mann\, Stanford University\nPresentation title and abstract will be announced when they are available.
URL:https://uwm.edu/physics/event/physics-colloquium-julian-may-mann/
LOCATION:Chemistry 108\, 2050 E Kenwood Blvd\, Milwaukee\, WI\, 53201\, United States
CATEGORIES:Physics Colloquia
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