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lab:2025-04-23
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lab:2025-04-23 [2025/01/30 09:51] singhj |
lab:2025-04-23 [2025/05/08 09:51] (current) singhj |
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| Host = Revel, Aldric [[revel@frib.msu.edu]] | Host = Revel, Aldric [[revel@frib.msu.edu]] | ||
| - | When = 2025-04-23 Wednesday **<color #ed1c24>15:30 (note the new time!)</color>** | + | When = 2025-04-23 Wednesday 15:30 |
| Where = FRIB 1300 | Where = FRIB 1300 | ||
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| <sortable> | <sortable> | ||
| ^ Start Time ^ End Time ^ Name ^ Building ^ Room ^ | ^ Start Time ^ End Time ^ Name ^ Building ^ Room ^ | ||
| - | | 09:00 | 09:30 | | | | | + | | 09:00 | 09:30 | Aldric Revel | FRIB | 1014 | |
| - | | 09:30 | 10:00 | | | | | + | | 09:30 | 10:00 | Jaideep Taggart Singh | FRIB | 2016 | |
| - | | 10:00 | 10:30 | | | | | + | | 10:00 | 10:30 | Personal Time | FRIB | 2102 | |
| - | | 10:30 | 11:00 | | | | | + | | 10:30 | 11:00 | Filomena Nunes | FRIB | 2107 | |
| - | | 11:00 | 11:30 | | | | | + | | 11:00 | 11:30 | Thomas Baumann | FRIB | 6304 | |
| - | | 11:30 | 12:00 | | | | | + | | 11:30 | 12:00 | George Zimba | FRIB | 2003 | |
| | 12:00 | 13:00 | Lunch with Graduate Students | FRIB | 2311 | | | 12:00 | 13:00 | Lunch with Graduate Students | FRIB | 2311 | | ||
| - | | 13:00 | 13:30 | | | | | + | | 13:00 | 13:30 | Personal Time | FRIB | 2102 | |
| - | | 13:30 | 14:00 | | | | | + | | 13:30 | 14:00 | Patrick McGlynn | FRIB | 2120 | |
| - | | 14:00 | 14:30 | | | | | + | | 14:00 | 14:30 | Personal Time | FRIB | 2102 | |
| - | | 14:30 | 15:00 | | | | | + | | 14:30 | 15:00 | Alex Brown | FRIB | 2043 | |
| | 15:00 | 15:30 | Speaker Prep time | FRIB | 1300 | | | 15:00 | 15:30 | Speaker Prep time | FRIB | 1300 | | ||
| | 15:30 | 16:30 | Seminar | FRIB | 1300 | | | 15:30 | 16:30 | Seminar | FRIB | 1300 | | ||
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| ===== Context ===== | ===== Context ===== | ||
| - | Title = TBD | + | Title = [[https://mediaspace.msu.edu/media/Nuclear+Science+Seminar+-+Julian+Kahlbow/1_upwvjibw|Magicity vs Superfluidity, and the structure of extremely neutron-rich O & F isotopes]] |
| Abstract | Abstract | ||
| <blockquote> | <blockquote> | ||
| - | TBD | + | The atomic nucleus is an intricate, strongly-interacting quantum many-body system with fascinating structure rooted in Quantum Chromodynamics. The shell model has been a successful cornerstone describing effectively nuclear structure and predicting magic numbers. However, in extremely neutron-rich nuclei, nuclear structure undergoes significant changes with often surprising effects due to neutron excess and weak binding. One particularly interesting region is around the isotope 28O. In this talk, I will discuss nuclear structure studies of neutron-rich Fluorine isotopes using high-resolution invariant-mass spectroscopy at the SAMURAI setup at RIBF/RIKEN (Japan). We measured the isotope 30F for the first time, confirming the breakdown of the neutron magic number N = 20. Based on shell-model calculations this causes a superfluid behavior. This finding leads to new questions about neutron correlations in a low-density environment, similar to conditions in the crust of neutron stars. |
| </blockquote> | </blockquote> | ||
lab/2025-04-23.1738248690.txt.gz · Last modified: 2025/01/30 09:51 by singhj
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