Contribution List

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  1. Peter Denton, Robert Szafron (Brookhaven National Laboratory)
    10/22/25, 9:00 AM
  2. Karri DiPetrillo (University of Chicago)
    10/22/25, 9:10 AM
  3. Brian Batell (Chicago)
    10/22/25, 9:50 AM
  4. Ian Low (Argonne/Northwestern)
    10/22/25, 11:00 AM
  5. 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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  6. Anna Suliga (University of California, Berkeley)
    10/22/25, 2:00 PM
  7. Shaouly Bar-Shalom (Technion)
    10/22/25, 2:00 PM
  8. Clara Lavinia Del Pio (Brookhaven National Laboratory)
    10/22/25, 2:18 PM
  9. Sam Carey (Wayne State University)
    10/22/25, 2:18 PM
  10. Spencer Ellis (Brown University)
    10/22/25, 2:36 PM
  11. Karan Kumar (Columbia University)
    10/22/25, 2:36 PM
  12. Lynn Tung (lynnt@fnal.gov)
    10/22/25, 2:54 PM
  13. Amartya Sengupta (SUNY Buffalo)
    10/22/25, 2:54 PM
  14. Mira Varma (Yale)
    10/22/25, 3:12 PM
  15. Vu Chi Lan Nguyen (UCSB)
    10/22/25, 3:12 PM
  16. Tao Han (UPittsburgh)
    10/22/25, 4:00 PM
  17. Carlos Blanco
    10/23/25, 9:00 AM
  18. Thomas Blum (University of Connecticut)
    10/23/25, 9:40 AM
  19. Glennys Farrar
    10/23/25, 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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  20. Cristina Ana Mantilla Suarez (FNAL)
    10/23/25, 11:30 AM
  21. Jesse Liu (NYU)
    10/23/25, 1:40 PM
  22. Masaaki Tomii (Columbia University)
    10/23/25, 1:40 PM
  23. So Chigusa (MIT)
    10/23/25, 1:58 PM
  24. Anthony Maurel Carroll (University of Oregon)
    10/23/25, 1:58 PM
  25. Minori Fujimoto (SBU)
    10/23/25, 2:16 PM
  26. Pankaj Munbodh (UCSC)
    10/23/25, 2:16 PM
  27. Francesca Acanfora (UMass Amherst)
    10/23/25, 2:34 PM
  28. Pierce Giffin (UCSC)
    10/23/25, 2:34 PM
  29. Jaeok Yi (KAIST)
    10/23/25, 2:52 PM
  30. M. Grant Roberts (UCSC)
    10/23/25, 2:52 PM
  31. Shuhei Yamamoto
    10/23/25, 3:10 PM
  32. Lam Hui
    10/23/25, 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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  33. Kim Berghaus
    10/24/25, 9:00 AM
  34. Bhupal Dev (University of Maryland, College Park)
    10/24/25, 9:40 AM
  35. Karsten Heeger (Yale University)
    10/24/25, 10:50 AM
  36. Mark Ross Lonergan
    10/24/25, 11:30 AM
  37. Ethan Cline (Stony Brook University)