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VERSION:2.0
CALSCALE:GREGORIAN
PRODID:UW-Madison-Physics-Events
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SEQUENCE:2
UID:UW-Physics-Event-9232
DTSTART:20260327T203000Z
DTEND:20260327T213000Z
DTSTAMP:20260413T083859Z
LAST-MODIFIED:20260304T185444Z
LOCATION:Chamberlin 2241
SUMMARY:Neutrinos in the Universe\, Physics Department Colloquium\, Ce
 cilia Lunardini\, Arizona State University
DESCRIPTION:Neutrinos are unique cosmic messengers. Produced in the mo
 st extreme\nenvironments in the Universe\, they escape dense astrophy
 sical regions\nthat are opaque to photons and carry information acros
 s vast\ncosmological distances. Over the past decade\, neutrino astro
 nomy has\nexpanded dramatically\, opening new windows on phenomena ra
 nging from\ncore-collapse supernovae to the highest-energy cosmic acc
 elerators.\n\nI will present a broad view of neutrino astrophysics\
 nacross the energy spectrum — from MeV neutrinos emitted in stellar
 \nexplosions to TeV–PeV neutrinos observed from powerful extragalact
 ic sources. I will emphasize the multimessenger perspective\, highligh
 ting the\nconnections between neutrinos\, electromagnetic signals\, c
 osmic rays and\ngravitational waves. In particular\, I will discuss h
 ow neutrinos and\ngravitational waves together probe the physics of c
 ompact objects\,\nstellar collapse\, and the dynamics of extreme cosm
 ic environments.\n\nI will also outline future developments in neutr
 ino detection and\nmultimessenger astronomy\, and how next-generation
  experiments will\ndeepen our understanding of fundamental physics an
 d astrophysics alike.\n
URL:https://www.physics.wisc.edu/events/?id=9232
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