Events Daily

Wednesday, May 14, 2025
      

Classical and Quantum Detection of Gravitational Waves
Sebastian Ellis, University of Geneva
Event Type: Informal HEP Talk
Time: 11:00 AM - 12:15 PM
Location: 726 Broadway, 940, CCPP Seminar
Abstract: There are many reasons to hope for the further detection of gravitational waves, especially from non-astrophysical sources. In particular, detecting cosmogenic gravitational waves could be our best hope of probing theories in the far UV with Earth-bound detectors. We will discuss how the detection of gravitational waves can be understood using simple heuristics. These will enable us to derive best-case scenarios for a variety of real and hypothetical detector technologies. We will see that quantum states will almost certainly be necessary to detect the most interesting gravitational wave signals, further motivating the development of quantum sensors.

Link to the Event Video


HEP Journal Club
Event Type: HEP Journal Club
Time: 12:30 PM - 1:30 PM
Location: 726 Broadway, 940, CCPP Seminar

Searching for coupled, hyperlight scalars across cosmic history
Zach Weiner, Perimeter Institute
Event Type: Informal HEP Talk
Time: 4:00 PM - 4:30 PM
Location: 726 Broadway, 940, CCPP Seminar
Abstract: New scalar fields may couple to the Standard Model by modulating its fundamental parameters in space and time. I will discuss a class of models in which a coupled scalar shifts the electron mass or the electromagnetic fine-structure constant before recombination, paying careful attention to the scalar's gravitational effects, the impact of Standard Model matter on its evolution, and its signatures relevant to complementary probes of fundamental constants at other epochs. I will show that a hyperlight, coupled scalar's gravitational effects open up new degeneracies in cosmological parameters and present quantitative constraints on theoretically consistent scenarios using cosmological data. In the process, I will expound the observational status of early-recombination models in relation to cosmological tensions and comment on the implications of these results for cosmological neutrino mass measurements.