This Week at Physics

<< April 2018 >>
Sun Mon Tue Wed Thu Fri Sat
 1   2   3   4   5   6   7 
 8   9   10   11   12   13   14 
 15   16   17   18   19   20   21 
 22   23   24   25   26   27   28 
 29   30   
Add an Event

This Week at Physics

<< Fall 2017 Spring 2018 Fall 2018 >>
Subscribe your calendar or receive email announcements of events

Events During the Week of April 29th through May 6th, 2018

Monday, April 30th, 2018

Council Meeting
Council Meeting
Time: 4:00 pm
Place: 2314 Chamberlin Hall
Add this event to your calendar

Tuesday, May 1st, 2018

Chaos & Complex Systems Seminar
Year-end celebration
Time: 12:05 pm
Place: 4274 Chamberlin (Refreshments will be served)
Speaker: General discussion, UW Madison
Abstract: Following the tradition of recent years in which we had a delightful discussion of where we have come and where we might go with the seminars, this last seminar of the semester will be devoted to a continuation of that discussion without any formal speaker. We will also discuss what we want to do during our informal weekly lunches on the Memorial Union Terrace which begin on May 8th. This celebration will include expanded refreshments, to which your own culinary contribution is welcome.
Host: Clint Sprott
Add this event to your calendar

"Physics Today" Undergrad Colloquium (Physics 301)
LZ and Dark Matter at UW
Time: 1:20 pm
Place: 2241 Chamberlin Hall
Speaker: Kimberly J. Palladino, UW Madison Department of Physics
Host: Wesley Smith
Add this event to your calendar

Wednesday, May 2nd, 2018

Department Meeting
Department Meeting
Time: 12:15 pm
Place: 5310 Chamberlin Hall
Add this event to your calendar

Thursday, May 3rd, 2018

NPAC (Nuclear/Particle/Astro/Cosmo) Forum
Fission and the formation of the r-process rare-earth abundance peak in neutron star mergers
Time: 2:30 pm
Place: 5280 Chamberlin Hall
Speaker: Nicole Vassh, University of Notre Dame
Abstract: The recent observations of the GW170817 electromagnetic counterpart
suggest lanthanides were produced in this neutron star merger event.
However many questions regarding heavy element production in mergers
remain: can such events account for all the r-process lanthanide material
observed in the galaxy? are precious metals such as gold produced in
sufficient amounts? are actinides produced? where within the merger
environment does nucleosynthesis occur and under what specific conditions?
Such questions can only be answered with careful studies of the nuclear
physics uncertainties affecting r-process calculations. Here I will
discuss recent extended calculations of beta-delayed fission and their
implications for r-process nucleosynthesis. The influence of fission
fragment distributions will also be addressed with a particular emphasis
on the unknown origin of the r-process rare-earth peak at A~164. Since the
rare-earth peak is formed as the r-process path begins to draw closer to
stability, the rare-earth nuclei contributing to peak formation will soon
be within reach of nuclear physics experiments performed at, for example,
the CPT at CARIBU and the upcoming FRIB. Here I will present the latest
results for the masses found to produce the rare-earth peak in a low
entropy accretion disk wind scenario and compare directly with recent mass
measurements from the CPT at CARIBU. Such collaborative efforts between
theory and experiment could soon be in a position to make definitive
statements regarding the mechanism of rare-earth peak formation and thus
the astrophysical site of the r process.
Host: Baha Balantekin
Add this event to your calendar

Friday, May 4th, 2018

Physics Department Colloquium
The microphysics of the GW170817 kilonova
Time: 3:30 pm
Place: 2241 Chamberlin Hall
Speaker: Rebecca Surman, Notre Dame University
Abstract: The optical signal that accompanied the GW170817 gravitational wave event
provided the first firm proof that neutron star mergers produce heavy
elements. Still, it is not known exactly which elements are produced by
mergers and in what proportions. A full understanding of neutron star
mergers and their role in galactic chemical evolution requires progress in
a number of areas. Two key areas are neutrino and nuclear physics.
Neutrino physics shapes the initial conditions for element synthesis, and
the nuclear physics of extreme neutron-rich nuclei governs how the
nucleosynthesis proceeds. Here we will review these microphysics aspects
of neutron star merger nucleosynthesis and discuss how current
uncertainties influence our interpretations of observed abundance patterns
and kilonova signals. We will then explore the promise of experimental
campaigns at rare isotope beam facilities to both reduce these
uncertainties and provide insight into astrophysical environments of heavy
element production.
Host: Baha Balantekin
Add this event to your calendar

Physics Awards Banquet
Time: 5:30 pm
Place: The University Club
Abstract: Awards presentation for student and alumni award winners.
Host: Sridhara Dasu
Add this event to your calendar
©2013 Board of Regents of the University of Wisconsin System