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11/05/2026, 09:00
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Nicole Vassh (TRIUMF)11/05/2026, 09:05
The astrophysical rapid neutron capture process (r-process) ventures far from the stable species found on Earth. Experimental facilities have made impressive inroads towards pinning down the properties of more exotic, neutron-rich nuclei, but the map of the nuclear chart is far from complete, with the r process being the case we know to have wandered furthest into uncharted territory. We will...
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Mengke Li (UC Berkeley)11/05/2026, 09:30
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Zach Meisel (Ohio University)11/05/2026, 09:55
In the beginning, X-ray burst modeling was data-poor and the number of high-impact nuclear mass measurement opportunities were many. Today the situation has changed. Opportunities still exist, but they are more subtle, requiring consideration of an expanded set of astrophysical conditions and more complex observables. I will argue that we are not at the end of rp-process nuclear mass...
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Nikolai Shchechilin (Universite Libre de Bruxelles)11/05/2026, 10:50
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Luis Gonzáles Miret11/05/2026, 11:15
The rapid neutron-capture process (or r-process) is responsible for the production of about half of the elements heavier than iron in the Universe and
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is expected to take place in neutron star mergers and possibly in exploding
massive stars. To estimate the composition of the ejecta, a reaction network
involving about 6000 neutron-rich nuclei with all reactions of interest needs
to be... -
Matthew Mumpower11/05/2026, 11:40
Mass is a fundamental observable in nuclear physics, encoding the integrated effect of nuclear interactions and anchoring a range of applications from astrophysics to tests of the Standard Model. Yet of the roughly 7,000 nuclei expected to be bound, only about half have ever been measured, leaving the rest to be predicted by theory. In this talk I survey today's modeling approaches, noting the...
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Sudhanva Lalit11/05/2026, 14:00
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11/05/2026, 14:25
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Alfredo Estrade (CMU), Sam Porter (University of Notre Dame)11/05/2026, 14:50
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Justin Placido12/05/2026, 09:00
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Hannah Erington (Facility for Rare Isotope Beams (Michigan State University))12/05/2026, 09:25
Determining the exact methods of nucleosynthesis, in which elements are produced by a variety of astrophysical processes, remains a crucial and open question in nuclear science. Nuclear mass data is a key input for astrophysical models, which constrain nucleosynthesis reaction pathways, impacting the abundance distribution of produced isotopes. As such, accurate and precise mass data in exotic...
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Klaus Blaum (Max Planck Society (DE))12/05/2026, 09:50
Precision measurements of nuclear masses provide critical input for modeling nucleosynthesis pathways and the structure of exotic nuclei far from stability. In this talk, I will present recent advances in trapped-ion mass spectrometry across European facilities, highlighting key results and methodological developments that have significantly improved accuracy and reach. A few highlights of how...
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Adrian Valverde12/05/2026, 10:15
ATLAS, the Argonne Tandemless Linac Accelerator System, has a long history of precision mass measurements for nuclear astrophysics, most recently focusing on mass measurements for the r-process rare earth peak at CARIBU with the Canadian Penning Trap. Into the next 25 years, ATLAS is developing new capabilities like nuCARIBU and the N=126 Factory which will enable further campaigns of mass...
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12/05/2026, 11:15
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12/05/2026, 11:30
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12/05/2026, 11:45
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12/05/2026, 12:00
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12/05/2026, 15:50
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12/05/2026, 16:15
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12/05/2026, 16:40
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12/05/2026, 17:05
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13/05/2026, 10:50
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13/05/2026, 11:30
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Adrian Valverde
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