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BEGIN:VEVENT

CATEGORIES:Lectures/Conferences
CATEGORIES:Utilities
CATEGORIES:Panel/Seminar/Colloquium
CATEGORIES:Research
CATEGORIES:Main
CONTACT;X-BEDEWORK-UID=00f1fcdb-0f068baf-010f-068baf83-00000004:None
CREATED:20250204T221958Z
DESCRIPTION:Since their original proposal\, neutrinos have been linked to 
 nuclear physics. We can use neutrinos to probe the properties of nuclei\,
 and use nuclei as targets for detecting neutrinos. In this seminar\, I wi
 ll present my past research on COHERENT and nEXO\, and describe my experi
 mental research program measuring nuclear matrix elements important for n
 eutrinoless double beta decay of germanium-76\, searching for Dark Matter
  in naturally occurring minerals with the PALEOCCENE collaboration\, and 
 developing new technology to detect some of the lowest energy neutrinos p
 roduced on Earth. I'll describe how the resources available at TUNL can h
 elp characterize backgrounds for these experiments and provide supporting
  measurements to enable this program.
DURATION:PT1H
DTSTAMP:20250219T153800Z
DTSTART;TZID=America/New_York:20250304T133000
LAST-MODIFIED:20250219T153800Z
LOCATION;X-BEDEWORK-UID=18832edc-1b27e154-011b-28387b11-00000077:Physics 1
 28
STATUS:CONFIRMED
SUMMARY:TUNL Seminar - Using Neutrinos to Study Nuclei\, and Nuclei to Det
 ect Neutrinos
UID:CAL-8a000483-92c3adf6-0194-d30c7e86-00005472demobedework@mysite.edu
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Main:/user/public-user/Utili
 ties/Main
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Panel_Seminar_Colloquium:/us
 er/public-user/Lectures_Conferences/Panel_Seminar_Colloquium
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Research:/user/public-user/T
 opics/Research
X-BEDEWORK-STUDENT-CONTACT;X-BEDEWORK-PARAM-EMAIL=phil.barbeau@duke.edu:Ph
 illip Barbeau
X-BEDEWORK-DUKE-SERIES:TUNL Seminar
X-BEDEWORK-SUBMITTEDBY:rlf41 for Physics (agrp__ArtsandSciences_Physics)
X-BEDEWORK-SPEAKER:Sam Hedges
END:VEVENT
BEGIN:VEVENT

CATEGORIES:Natural Sciences
CATEGORIES:Lectures/Conferences
CATEGORIES:Utilities
CATEGORIES:Panel/Seminar/Colloquium
CATEGORIES:Main
CONTACT;X-BEDEWORK-UID=00f1fcdb-0f068baf-010f-068baf83-00000004:None
CREATED:20251103T190222Z
DESCRIPTION:Nuclear reactions drive the energy generation and nucleosynthe
 sis in stars and compact objects. Understanding nuclear structure includi
 ng resonances and the properties of bulk nuclear matter is necessary for 
 constraining the stellar behaviour. In this talk\, I will discuss some of
  my research focusing on how nuclear structure studies can be used to inf
 orm stellar behaviour with particular focus on how experiments can be use
 d to constrain elemental abundances and the properties of neutron stars.
DURATION:PT1H
DTSTAMP:20251103T190511Z
DTSTART;TZID=America/New_York:20251113T150000
LAST-MODIFIED:20251103T190511Z
LOCATION;X-BEDEWORK-UID=18832edc-1b27e154-011b-28387b11-00000077:Physics 1
 28
STATUS:CONFIRMED
SUMMARY:TUNL Seminar - How to understand stars through nuclear structure?
UID:CAL-8a00ec8b-979413b9-019a-4b195695-00003928demobedework@mysite.edu
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Main:/user/public-user/Utili
 ties/Main
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Panel_Seminar_Colloquium:/us
 er/public-user/Lectures_Conferences/Panel_Seminar_Colloquium
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Natural Sciences:/user/publi
 c-user/Topics/Natural Sciences
X-BEDEWORK-STUDENT-CONTACT;X-BEDEWORK-PARAM-EMAIL=sean.finch@duke.edu:Sean
  Finch
X-BEDEWORK-SPEAKER:Philip Adsley
X-BEDEWORK-DUKE-WEBCAST:https://duke.zoom.us/j/94580918793?pwd=LubgRabPznU
 b2DirzaRJ6RRavDxbWp.1
X-BEDEWORK-SUBMITTEDBY:asc for TUNL Seminar Series (agrp_TUNL_SeminarSerie
 s)
X-BEDEWORK-CS;X-BEDEWORK-PARAM-DESCRIPTION="/principals/users/agrp__Artsan
 dSciences_Physics,":Physics
END:VEVENT
BEGIN:VEVENT

CATEGORIES:Natural Sciences
CATEGORIES:Lectures/Conferences
CATEGORIES:Utilities
CATEGORIES:Panel/Seminar/Colloquium
CATEGORIES:Main
CONTACT;X-BEDEWORK-UID=00f1fcdb-0f068baf-010f-068baf83-00000004:None
CREATED:20251124T161001Z
DESCRIPTION:A growing body of experimental data on single-particle energie
 s in weakly bound systems has materialized over the past decade or so. Th
 e most illuminating of these data has been for the neutron-rich nuclei ar
 ound N = 20 and 28. A smooth decrease in the separation of the 2p3/2-2p1/
 2 spin-orbit splittings is observed as they approach zero binding\, which
  is at odds with the well-accepted scaling\, with mass\, of measured spin
 -orbit splittings across the chart of nuclides for well-bound states as e
 stablished by Mairle [Phys. Lett. B 304\, 39 (1993)]. In studying the con
 trast between experimental data\, the mean-field descriptions\, and the t
 rends established by Mairle for both well-bound and weakly bound systems 
 across the nuclear chart\, with a focus on neutron spin-orbit partners\, 
 a seemingly universal behavior emerges that could prove predictive. Many 
 of the regions explored have connections to other prominent topics in nuc
 lear physics\, such as r-process nucleosynthesis\, where the ordering of 
 single-particle energies near threshold in weakly bound systems plays a r
 ole in reaction rates. Throughout\, I will highlight one of the principal
  techniques used to extract such data: the solenoidal spectrometer techni
 que\, now used at ATLAS\, CERN\, and FRIB. This material is based upon wo
 rk supported by the U.S. Department of Energy\, Office of Science\, Offic
 e of Nuclear Physics\, under Contract Number DE-AC02-06CH11357.
DURATION:PT1H
DTSTAMP:20251124T161001Z
DTSTART;TZID=America/New_York:20251204T150000
LAST-MODIFIED:20251124T161001Z
LOCATION;X-BEDEWORK-UID=18832edc-1b27e154-011b-28387b11-00000077:Physics 1
 28
STATUS:CONFIRMED
SUMMARY:A universal fate for spin-orbit partners in the weak-binding regim
 e?
UID:CAL-8a00ec9e-9a83ce7f-019a-b6a11889-00007eeedemobedework@mysite.edu
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Main:/user/public-user/Utili
 ties/Main
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Panel_Seminar_Colloquium:/us
 er/public-user/Lectures_Conferences/Panel_Seminar_Colloquium
X-BEDEWORK-ALIAS;X-BEDEWORK-PARAM-DISPLAYNAME=Natural Sciences:/user/publi
 c-user/Topics/Natural Sciences
X-BEDEWORK-CS;X-BEDEWORK-PARAM-DESCRIPTION="/principals/users/agrp__Artsan
 dSciences_Physics,":Physics
X-BEDEWORK-SPEAKER:Ben Kay
X-BEDEWORK-DUKE-WEBCAST:https://duke.zoom.us/j/94580918793?pwd=LubgRabPznU
 b2DirzaRJ6RRavDxbWp.1
X-BEDEWORK-STUDENT-CONTACT;X-BEDEWORK-PARAM-EMAIL=sean.finch@duke.edu:Sean
  Finch
X-BEDEWORK-SUBMITTEDBY:asc for TUNL Seminar Series (agrp_TUNL_SeminarSerie
 s)
END:VEVENT
END:VCALENDAR