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Peter Denton, Robert Szafron (Brookhaven National Laboratory)10/22/25, 9:00 AM
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Karri DiPetrillo (University of Chicago)10/22/25, 9:10 AM
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Brian Batell (Chicago)10/22/25, 9:50 AM
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Ian Low (Argonne/Northwestern)10/22/25, 11:00 AM
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Michael Hank (member@upenn.edu;faculty@upenn.edu;employee@upenn.edu)10/22/25, 11:40 AM
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)10/22/25, 2:00 PM
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Shaouly Bar-Shalom (Technion)10/22/25, 2:00 PM
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Clara Lavinia Del Pio (Brookhaven National Laboratory)10/22/25, 2:18 PM
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22. Neutrino Magnetic Moment, Charge Radius and Polarizability from MeV to GeV Neutrino InteractionsSam Carey (Wayne State University)10/22/25, 2:18 PM
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Spencer Ellis (Brown University)10/22/25, 2:36 PM
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Karan Kumar (Columbia University)10/22/25, 2:36 PM
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Lynn Tung (lynnt@fnal.gov)10/22/25, 2:54 PM
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Amartya Sengupta (SUNY Buffalo)10/22/25, 2:54 PM
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Mira Varma (Yale)10/22/25, 3:12 PM
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Vu Chi Lan Nguyen (UCSB)10/22/25, 3:12 PM
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Tao Han (UPittsburgh)10/22/25, 4:00 PM
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Carlos Blanco10/23/25, 9:00 AM
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Thomas Blum (University of Connecticut)10/23/25, 9:40 AM
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Glennys Farrar10/23/25, 10:50 AM
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)10/23/25, 11:30 AM
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Jesse Liu (NYU)10/23/25, 1:40 PM
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Masaaki Tomii (Columbia University)10/23/25, 1:40 PM
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So Chigusa (MIT)10/23/25, 1:58 PM
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Anthony Maurel Carroll (University of Oregon)10/23/25, 1:58 PM
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Minori Fujimoto (SBU)10/23/25, 2:16 PM
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Pankaj Munbodh (UCSC)10/23/25, 2:16 PM
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Francesca Acanfora (UMass Amherst)10/23/25, 2:34 PM
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Pierce Giffin (UCSC)10/23/25, 2:34 PM
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Jaeok Yi (KAIST)10/23/25, 2:52 PM
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M. Grant Roberts (UCSC)10/23/25, 2:52 PM
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Shuhei Yamamoto10/23/25, 3:10 PM
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Lam Hui10/23/25, 4:00 PM
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 Berghaus10/24/25, 9:00 AM
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Bhupal Dev (University of Maryland, College Park)10/24/25, 9:40 AM
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Karsten Heeger (Yale University)10/24/25, 10:50 AM
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Mark Ross Lonergan10/24/25, 11:30 AM
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Ethan Cline (Stony Brook University)
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