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Peter Denton, Robert Szafron (Brookhaven National Laboratory)22/10/2025, 09:00
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Karri DiPetrillo (University of Chicago)22/10/2025, 09:10
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Brian Batell (Chicago)22/10/2025, 09:50
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Ian Low (Argonne/Northwestern)22/10/2025, 11:00
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Michael Hank (member@upenn.edu;faculty@upenn.edu;employee@upenn.edu)22/10/2025, 11:40
The Standard Model of particle physics successfully describes many known interactions, but is known to be incomplete. In this talk, recent results of searches for beyond-the-Standard-Model signatures are reported. These use up to 140 fb-1 of pp collisions collected by the ATLAS and CMS experiments at sqrt(s)=13 TeV and up to 51.8 fb-1 collected at sqrt(s)=13.6 TeV. Searches for compressed...
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Anna Suliga (University of California, Berkeley)22/10/2025, 14:00
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Shaouly Bar-Shalom (Technion)22/10/2025, 14:00
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Clara Lavinia Del Pio (Brookhaven National Laboratory)22/10/2025, 14:18
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22. Neutrino Magnetic Moment, Charge Radius and Polarizability from MeV to GeV Neutrino InteractionsSam Carey (Wayne State University)22/10/2025, 14:18
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Spencer Ellis (Brown University)22/10/2025, 14:36
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Karan Kumar (Columbia University)22/10/2025, 14:36
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Lynn Tung (lynnt@fnal.gov)22/10/2025, 14:54
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Amartya Sengupta (SUNY Buffalo)22/10/2025, 14:54
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Mira Varma (Yale)22/10/2025, 15:12
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Vu Chi Lan Nguyen (UCSB)22/10/2025, 15:12
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Tao Han (UPittsburgh)22/10/2025, 16:00
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Carlos Blanco23/10/2025, 09:00
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Thomas Blum (University of Connecticut)23/10/2025, 09:40
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Glennys Farrar23/10/2025, 10:50
I will briefly review the observations of UHECRs, emphasizing what is robust and what remains uncertain and explain why a key piece of data strongly suggests that UHECRs are produced in BNS mergers. Then, I will discuss the likely acceleration mechanism and locus and explain how the spectral cutoff is determined; the no-free-parameter prediction of the cutoff energy for different nuclei agrees...
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Cristina Ana Mantilla Suarez (FNAL)23/10/2025, 11:30
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Jesse Liu (NYU)23/10/2025, 13:40
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Masaaki Tomii (Columbia University)23/10/2025, 13:40
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So Chigusa (MIT)23/10/2025, 13:58
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Anthony Maurel Carroll (University of Oregon)23/10/2025, 13:58
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Minori Fujimoto (SBU)23/10/2025, 14:16
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Pankaj Munbodh (UCSC)23/10/2025, 14:16
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Francesca Acanfora (UMass Amherst)23/10/2025, 14:34
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Pierce Giffin (UCSC)23/10/2025, 14:34
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Jaeok Yi (KAIST)23/10/2025, 14:52
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M. Grant Roberts (UCSC)23/10/2025, 14:52
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Shuhei Yamamoto23/10/2025, 15:10
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Lam Hui23/10/2025, 16:00
We will discuss the possibility that dark matter is composed of particles lighter than about 10 eV, the prime example being an axion or axion-like-particle. In this case, the dark matter galaxy halo is best thought of as a set of waves. The astrophysical consequences, and the experimental implications for axion detection, will be discussed.
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Kim Berghaus24/10/2025, 09:00
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Bhupal Dev (University of Maryland, College Park)24/10/2025, 09:40
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Karsten Heeger (Yale University)24/10/2025, 10:50
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Mark Ross Lonergan24/10/2025, 11:30
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Ethan Cline (Stony Brook University)
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