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What's happening at the INT:

  INT Calendar

   :: Live at the INT: Schedule and access to INT talks online today
   :: Current Program
   :: Seminar Schedule
   :: Upcoming INT Programs and Workshops
   :: INT/Nuclear Theory Group Seminars
   :: INT Special Seminars
   :: UW Physics Dept. Seminars
   :: 2016 National Nuclear Physics Summer School
   :: REU Program

  INT News

   :: Map of where our RAPs, postdocs and grad students are now.
   :: Stealthy dark matter, research done at the INT by former post-doc M. Buchoff & collaborators
   :: Nuclear magnetic moments from Lattice QCD
   :: INT introduces a Wiki for program attendees to share information on childcare in Seattle - please contact INT staff for the password.

  Other News

   :: Congratulations UW Professor Emeritus David J. Thouless, 2016 Nobel Prize Winner in Physics
   :: Joseph Carlson is the 2017 recipient of the Herman Feshbach Prize in Theoretical Nuclear Physics
   :: NRC Nuclear Physics Decadal Survey and Videos
   :: Upcoming Conferences
 
Recent Activity at INT:

Exploring the QCD Phase Diagram through Energy Scans (INT-16-3)
(INT Program September 19 - October 14, 2016)

Reported by Volker Koch, Michael Lisa, Hannah Petersen, Paul Sorensen
Reported on January 10, 2017
The goal of this program was to deepen our theoretical understanding of the phase structure of QCD-in particular the de-confinement transition and possible critical point-from present experimental programs, and to provide theoretical guidance to upcoming programs at several facilities worldwide. All talks and discussions were centered around this goal and highlighted different facets of this overarching task. Read more...






Flavor Observations with Supernova Neutrinos (INT-16-61W)
(INT Workshop August 15 - 19, 2016)

Reported by Chuck Horowitz, H.-Thomas Janka, Sanjay Reddy, and Kate Scholberg
Reported on August 23, 2016
Supernova (SN) neutrinos, as astrophysical messengers, carry unique flavor, time and energy information that may be crucial for understanding neutrino oscillations, the SN explosion mechanism, neutron star properties, and nucleosynthesis. Historically, about 20 electron anti-neutrinos were detected from SN 1987A. Read more...











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