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ORGANIZER;CN=Heungman Park:MAILTO:Heungman.Park@tamuc.edu
ATTENDEE;ROLE=REQ-PARTICIPANT;PARTSTAT=NEEDS-ACTION;RSVP=FALSE;CN=phas-dept
 @tamuc.edu:MAILTO:phas-dept@tamuc.edu
DESCRIPTION;LANGUAGE=en-US:When: Thursday\, September 3\, 2020 4:00 PM-5:00
  PM. (UTC-06:00) Central Time (US & Canada)\nWhere: Online\n\n*~*~*~*~*~*~
 *~*~*~*\n\nJoin Zoom Meeting\nhttps://tamuc.zoom.us/j/92605940950\n\n\nMee
 ting ID: 926 0594 0950\n\n\n\n\nFall 2020 Colloquium\nDepartment of Physic
 s & Astronomy\, A&M-Commerce\nSep 3\, Thursday\, 4-5 PM in a Zoom Virtual 
 Meeting\nhttps://tamuc.zoom.us/j/92605940950\nAstrophysics\nNew Results on
  Stellar Neutrinos\nDr. Frank Timmes\nArizona State University\n\n\n[https
 ://lh4.googleusercontent.com/Roc8tNB7JI4kI9nwYFnDgRXUWIqpYVmwfvwXRdw-pS2j3
 vtijZOBNRCaY4PeNg55kgkZXdxEGhBGoidKSXhNna3D14e_W3RogBc6DIcXasm3Y0oFulklmWJ
 _SEcFaifJ5HSkH8gs]\nFrank Timmes is a Professor in the School of Earth and
  Space Exploration at Arizona State University. He has expertise in stella
 r astrophysics\, nuclear astrophysics\, chemical evolution\, astrobiology\
 , gamma-ray astronomy from radioactive isotopes\, community-driven softwar
 e instruments\, and teaching large online astronomy courses. He is a Fello
 w of the American Physical Society and a Simons Fellow in Theoretical Phys
 ics. Frank provides service to the international astronomy & astrophysics 
 community through the American Astronomical Society Journals\, where he ha
 s been a Scientific Editor since 2009\, Lead Editor of the "High Energy Ph
 enomena and Fundamental Physics" corridor since 2016\, and driving content
  on the AAS YouTube channel\, https://www.youtube.com/c/AAStronomy since 2
 019.  His website is http://cococubed.asu.edu/\n\n\nAbstract\n\nStars radi
 ate energy by releasing photons from the stellar surface and neutrinos fro
 m the stellar interior. In the stellar interior\, weak reactions produce e
 lectron neutrinos by thermal processes\, electron and positron captures on
  nuclei\, and nuclear decays. Neutrinos interact feebly with baryonic matt
 er\, escaping from the star unhindered in circumstances where photons are 
 trapped. Neutrino astronomy has been limited\, so far\, to the Sun\, super
 nova 1987A\, and blazar TXS 0506+056. However\, the Super-Kamiokande with 
 Gadolinium\, Jiangmen Underground Neutrino Observatory\, and XENON experim
 ents usher in a new generation of multi-purpose neutrino detectors designe
 d to open new avenues for potentially observing currently undetected neutr
 inos. In this talk we'll explore recent results on stellar neutrinos that 
 provide new targets for current\, forthcoming\, and future generations of 
 neutrino detectors\, new estimates of the stellar neutrino background sign
 al\, and new opportunities for nuclear reaction data that can make sizable
  differences in stellar evolution.\n\n
SUMMARY;LANGUAGE=en-US:Zoom for Colloquium Today at 4 PM
DTSTART;TZID=Central Standard Time:20200903T160000
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