Bulletin of the American Physical Society
2024 APS April Meeting
Wednesday–Saturday, April 3–6, 2024; Sacramento & Virtual
Session HH02: V: Particle Physics IVirtual Only
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Sponsoring Units: DPF Chair: Vaia Papadimitriou, Fermilab Room: Virtual Room 02 |
Friday, April 5, 2024 5:30PM - 5:42PM |
HH02.00001: Upper Limits on WIMP Annihilation Cross Sections with IceCube DeepCore Brandon Pries Dark matter is approximately five times more abundant than baryonic matter, but its particle nature continues to elude physicists. One proposed candidate is a Weakly-Interacting Massive Particle (WIMP), which is predicted by supersymmetry and expected to have many of the observed properties of dark matter, including no electromagnetic interactions and interacting primarily via gravity and weak-scale forces. These weak-scale interactions open up the possibility of WIMPs annihilating into Standard Model particles like neutrinos, which are observable by neutrino detectors like IceCube. Under this hypothesis, IceCube can search for signals of neutrinos coming from WIMP annihilation, or set upper limits on the WIMP annihilation cross section in the event of a non-detection. One prime location for WIMP annihilation is a dwarf galaxy, which is relatively rich in dark matter and has a relatively low neutrino background compared to a Milky Way-sized galaxy. We present upper limits on the annihilation cross section for GeV-scale WIMPs annihilating in dwarf galaxies, highlighting a substantial improvement in the limits for WIMP annihilation into quarks. |
Friday, April 5, 2024 5:42PM - 5:54PM |
HH02.00002: Abstract Withdrawn
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Friday, April 5, 2024 5:54PM - 6:06PM |
HH02.00003: ADMX-G2 Run 2A: A Multi-Cavity QCD Axion Search Stefan P Knirck The QCD axion is among the best motivated particle dark matter (DM) candidates. Cavity haloscopes like ADMX (Axion Dark Matter eXperiment) resonantly detect conversion of DM axions to photons under a strong magnetic field in a high-Q resonant cavity. Recent ADMX runs with a single cavity excluded most of the QCD axion parameter range between 2.7µeV and 4.2µeV and are set to cover the range until about 5.4µeV. However, at higher masses the wavelength of the generated photons shrinks, generally leading to a smaller cavity volume and reduced sensitivity. In this talk we present an array of four cavities, tuning in sync to scan a broad mass range from 5.4µeV to 7.6µeV with QCD axion sensitivity. We discuss experimental measurements of the quality factor and other important electromagnetic characteristics at room temperature and 4K. We show recent R&D and experimental improvements, and outline the path towards commissioning and run of the full axion search experiment. |
Friday, April 5, 2024 6:06PM - 6:18PM |
HH02.00004: Opening up baryon number violating operators Diana Sokhashvili, Julian Heeck, Anil Thapa
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Friday, April 5, 2024 6:18PM - 6:30PM |
HH02.00005: Abstract Withdrawn
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Friday, April 5, 2024 6:30PM - 6:42PM |
HH02.00006: Constraining CP-odd contributions in the Higgs-strahlung process at FCC-ee using kinematic observables Valdis Slokenbergs Prospects to constrain CP-odd contributions in the Higgs-strahlung process at a future electron-positron collider e+e- => ZH are presented. A realistic study is performed in the framework of the FCC-ee collider at the center-of-mass energy of 240 GeV, with reconstruction of the IDEA detector performed using the DELPHES framework. A matrix-element package, MELA, is implemented that uses event weights to the Standard Model in order to optimally constrain the CP-odd contributions based on kinematic observables. |
Friday, April 5, 2024 6:42PM - 6:54PM |
HH02.00007: Abstract Withdrawn
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Friday, April 5, 2024 6:54PM - 7:06PM |
HH02.00008: Optimizing Observables for Experimental Measurements at the LHC Michalis Panagiotou We present a framework for modeling processes with anomalous interactions at the LHC. One application of this framework is the modeling of the EFT in both on-shell and off-shell Higgs boson production and decay. We use this framework to illustrate the matrix-element approach in calculation of the observables optimal for EFT application and how most of the relevant information can be stored in an optimal way for data analysis. |
Friday, April 5, 2024 7:06PM - 7:18PM |
HH02.00009: Probing the parameter space of two-dimensional QCD with eLCQ Uwe Trittmann Recently, exhaustively-symmetrized discretized light-cone quantization (eLCQ) has been applied to two-dimensional QCD with adjoint fermions (QCD2A) |
Friday, April 5, 2024 7:18PM - 7:30PM |
HH02.00010: Einstein's basement - A model of dark matter and dark energy? Fritz W Riehle, Sebastian Ulbricht The energy-momentum relationship (EMR) of a free particle in special relativity is regarded as the upper branch of an avoided crossing between the mass of the particle and its momentum. The corresponding EMR for the lower branch - a regime dubbed as Einstein's basement - is derived. From the associated Lagrangian and the conventional gravitational interaction a new kinematics in Einstein's basement is determined. It is shown that this can lead to a repulsion of the basement particles and a modified interaction with regular matter. The model suggests the identification of the basement particles with dark matter accompanied with a missing interaction with light. The expansion of the basement particles and the regular mass that is carried along could be interpreted as an expansion of the universe. Tests of the model by astronomical observations are suggested. |
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