[Jlab-seminars] Fwd: Physics Colloquium - "Nuclear and neutrino physics of the r-process" - Prof. Gail McLaughlin
Mary Fox
mfox at jlab.org
Tue Oct 2 08:23:12 EDT 2018
-------- Forwarded Message --------
Subject: Physics Colloquium - "Nuclear and neutrino physics of the
r-process" - Prof. Gail McLaughlin
Date: Mon, 1 Oct 2018 20:35:00 +0000
From: Wilkinson, Ellie V <evwilk at wm.edu>
To: physics2017 at physics.wm.edu <physics2017 at physics.wm.edu>
CC: undergrads2017 at physics.wm.edu <undergrads2017 at physics.wm.edu>
*_PHYSICS COLLOQUIUM_*
Friday, October 5, 2018
4:00 PM
Small Hall, Room 111
*Prof. Gail McLaughlin **[***Host: M. Sher]**
North Carolina State University
**
*Title of Talk: “Nuclear and neutrino physics of the r-process”*
*_Abstract:_*
The production of the elements heavier than iron in the universe has
long been associated with neutron-capture processes. The most
neutron-rich isotopes are created by rapid (r ) neutron-capture
nucleosynthesis in extreme astrophysical environments. Specifics of
these environments and the location of the astrophysical sites in which
the r process occurs have remained open problems. It has been reported
that observations of the gravitational wave event GW170817 and its
electromagnetic counterpart suggest that neutron star mergers are a site
of r-process nucleosynthesis. Still many questions remain, such as the
nature of the astrophysical conditions within the merger responsible for
element synthesis and whether mergers can account for all galactic
r-process production. If we hope to fully understand the connection
between this discovery and the origin of r-process elements,
uncertainties in neutrino and nuclear astrophysics must be reduced. I
will highlight the role played by neutrinos and nuclear masses.
*//*
*/Cookies & Coffee will be served in Small 122 at 3:30pm/*
******
*Eleonor V. Wilkinson*
Administrative & Office Specialist
William & Mary-Physics
Small Hall, Room 123
300 Ukrop Way
Williamsburg, VA 23185
Telephone: 757-221-3503
Fax: 757-221-3540
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