Conveners
Plenary
- Brendan Casey (Fermilab)
Plenary
- Brendan Casey (Fermilab)
Plenary
- Brendan Casey (Fermilab)
Plenary
- Brendan Casey (Fermilab)
Plenary
- Brendan Casey (Fermilab)
Plenary
- Brendan Casey (Fermilab)
Plenary
- Brendan Casey (Fermilab)
Plenary
- Brendan Casey (Fermilab)
Plenary
- Brendan Casey (Fermilab)
Plenary: Summaries
- Brendan Casey (Fermilab)
Plenary: Summaries
- Brendan Casey (Fermilab)
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Keti Kaazde (Kansas State University)8/30/22, 8:00 AMNeutrino Masses and Neutrino MixingPlenary talk
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Asutosh Kotwal (Duke University)8/30/22, 8:30 AMPhysics at High EnergiesPlenary talk
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Martin Fertl (Johannes Gutenberg University Mainz)8/30/22, 9:00 AMPrecision Physics at High IntensitiesPlenary talk
The E989 collaboration has published the most precise measurement of the muon anomalous magnetic moment $a_\mu$ with an uncertainty of $\mathrm{460\,ppb}$ in 2021. The new experimental world average of $a_\mu$ deviates by 4.2 standard deviations from the Standard Model prediction provided by the Muon g-2 Theory Initiative. The emerging results from ab-initio lattice QCD calculations allow to...
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Soeren Prell (Iowa State University)8/30/22, 10:00 AMHeavy Flavors and the CKM MatrixPlenary talk
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Wolfgang Altmannshofer (University of California Santa Cruz)8/30/22, 10:30 AMHeavy Flavors and the CKM MatrixPlenary talk
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Shujie Li (Berkeley Lab)8/30/22, 11:00 AMNuclear Forces and Structure, NN Correlations, and Medium EffectsPlenary talk
At Jefferson Lab, high luminosity electron beam are used to perform precision measurements on asymmetric nuclei including 3H, 3He, 48Ca, and 208Pb. Those nuclear system with imbalanced number of protons and neutrons provide a unique testing ground for isospin and flavor dependent effects in nuclear and nucleon structure. The recent Hall A Tritium Project which used the simplest many-body...
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Andreas Metz (Temple University)8/30/22, 11:30 AMParton and Gluon Distributions in Nucleons and NucleiPlenary talk
The 3D parton structure of strongly interacting systems is encoded in generalized and transverse-momentum-dependent parton distributions. We discuss the status of this very active research field and identify open questions. This includes a brief discussion of the overarching 5D partonic Wigner functions and the prospects of related studies at the future electron ion collider (EIC).
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Robert Pattie (East Tennessee State University)8/31/22, 8:00 AMTests of Symmetries and the Electroweak InteractionPlenary talk
The $\beta$-decay of the free neutron contains a wealth of information about the charged weak interaction. Measurements of the lifetime and angular correlation coefficients can be use to determine $V_{ud}$, the first element of the Cabibbo–Kobayashi–Maskawa quark mixing matrix.Traditionally Super-allowed Fermi nuclear beta-decays have provided the most precise determination of $V_{ud}$, but...
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Dr Georg Bison (Paul Scherrer Institut)8/31/22, 8:30 AMPrecision Physics at High IntensitiesPlenary talk
We report on the result of the neutron electric dipole moment EDM search which took data in 2015 and 2016 at PSIs ultracold neutron source. The neutron EDM is deemed to be one of the most sensitive probes of physics beyond the standard model. The experiment measured the precession frequency of spin polarized neutrons as a function of a strong electric field. The electric dipole moment of the...
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Andrea Pocar (University of Massachusetts)8/31/22, 9:00 AMNeutrino Masses and Neutrino MixingPlenary talk
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Douglas Tucker (Fermi National Accelerator Laboratory)8/31/22, 10:00 AMCosmic Physics and Dark Energy, Inflation, and Strong-Field GravityPlenary talk
The Dark Energy Survey (DES) is an optical astronomical imaging survey of one-quarter of the Southern sky. The on-sky operations for the survey were completed in 2019, with observations conducted over the course of 6 years with a 3-square-degree wide-field mosaic camera -- the Dark Energy Camera, or DECam -- installed on the Blanco 4-meter telescope at the Cerro Tololo Interamerican...
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Kyle Dawson (University of Utah)8/31/22, 10:30 AMCosmic Physics and Dark Energy, Inflation, and Strong-Field GravityPlenary talk
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Zeesh Amed (Stanford Linear Accelerator Center)8/31/22, 11:00 AMCosmic Physics and Dark Energy, Inflation, and Strong-Field GravityPlenary talk
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Kaja Rotermund (Lawrence Berkeley National Lab)8/31/22, 11:30 AMCosmic Physics and Dark Energy, Inflation, and Strong-Field GravityPlenary talk
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Michael Wagman (Fermi National Accelerator lab)9/1/22, 8:00 AMNeutrino Masses and Neutrino MixingPlenary talk
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Ralph Massarczyk (Los Alamos National Laboratory)9/1/22, 8:30 AMNeutrino Masses and Neutrino MixingPlenary talk
The Baksan Experiment on Sterile Transitions (BEST) was designed to investigate the deficit of electron neutrinos, $\nu_e$, observed in previous gallium-based radiochemical measurements with high intensity neutrino sources, commonly referred to as the gallium anomaly. The BEST setup is comprised of two zones of liquid Ga target to explore neutrino oscillations on the meter scale. Any deficits...
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Michael Smy (University of California Irvine)9/1/22, 9:00 AMPlenary talk
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Imre Bartos (University of Florida)9/1/22, 10:00 AMCosmic Physics and Dark Energy, Inflation, and Strong-Field GravityPlenary talk
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Christian Drischler (FRIB/MSU)9/1/22, 10:30 AMParticle and Nuclear AstrophysicsPlenary talk
Neutron stars are unique laboratories for studying strongly interacting, neutron-rich matter under extreme conditions. While much has already been learned about neutron stars in the era of multi-messenger astronomy, many key questions remain, especially regarding the composition and equation of state (EOS) of the ultra-compressed matter in their inner cores. At the same time, chiral effective...
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Juliette Mammei (University of Manitoba)9/1/22, 11:00 AMNuclear Forces and Structure, NN Correlations, and Medium EffectsPlenary talk
The density dependence of the symmetry energy is a quantity that has long been anticipated to inform the determination of the neutron matter equation of state (EOS). Knowledge of the neutron distribution in heavy nuclei impacts nuclear structure theory, our understanding of neutron star structure, nuclear spectroscopy, atomic parity measurements and more. Electron scattering has already...
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Ben Margalit (University of California Berkeley)9/1/22, 11:30 AMParticle and Nuclear AstrophysicsPlenary talk
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Brad Sherrill (Michigan State University)9/2/22, 8:00 AMNuclear Forces and Structure, NN Correlations, and Medium EffectsPlenary talk
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Heather Crawford (Lawrence Berkeley National Lab)9/2/22, 8:30 AMNuclear Forces and Structure, NN Correlations, and Medium EffectsPlenary talk
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Ronald Garcia Ruiz (Massachusetts Institute of Technology)9/2/22, 9:00 AMNuclear Forces and Structure, NN Correlations, and Medium EffectsPlenary talk
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Carla Marin Benito (Universitat de Barcelona)9/2/22, 9:30 AMPlenary talk
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Walter Pettus (Indiana University)9/3/22, 8:00 AMNeutrino Masses and Neutrino MixingPlenary talk
The ${\rm M{\scriptsize AJORANA}}$ ${\rm D{\scriptsize EMONSTRATOR}}$ is an experiment designed to search for neutrinoless double beta decay of $^{76}$Ge. The ${\rm D{\scriptsize EMONSTRATOR}}$ consisted of two modules of p-type point-contact germanium detectors operating at the 4850’ level of the Sanford Underground Research Facility in Lead, SD. The experiment recently concluded its...
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Pierre Sikivie (University of Florida)9/3/22, 8:30 AMDark MatterPlenary talk
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Scott Hertel (University of Massachusetts)9/3/22, 9:00 AMDark MatterPlenary talk
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Matt Shepherd (Indiana University)9/3/22, 10:00 AMQCD, Hadron Spectroscopy, and ExoticsPlenary talk
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Sylvester Joosten (Argonne National Lab)9/3/22, 10:30 AMQuark Matter and High Energy Heavy Ion CollisionsPlenary talk
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Emanuele Mereghetti (Los Alamos National Lab)9/3/22, 11:00 AMPhysics at High EnergiesPlenary talk
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Patrick Meade (State University of New York Stony Brook)9/3/22, 11:30 AMPhysics at High EnergiesPlenary talk
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Hector de la Torre Perez (Michigan State University (US))9/4/22, 8:00 AM
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Justin Stevens (William & Mary)9/4/22, 8:20 AM
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Maria Pia Zurita (University of Regensburg), Maria Zurek (Argonne National Laboratory)9/4/22, 8:40 AM
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Nadia Fomin (University of Tennesee - Knoxville), Russell Mammei (The University of Winnipeg)9/4/22, 9:00 AM
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Rongrong Ma (BNL)9/4/22, 9:20 AMPlenary talk
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Jaimin Hou Jaimin Hou (University of Florida)9/4/22, 10:00 AMPlenary talk
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Alejandro Vaquero Aviles-Casco (University of Utah)9/4/22, 10:20 AMPlenary talk
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Shujie Li (Berkeley Lab)9/4/22, 10:40 AMPlenary talk
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Bryan Ramson (Fermilab)9/4/22, 11:00 AMPlenary talk
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Sophie Middleton (Caltech)9/4/22, 11:20 AMPlenary talk
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Plenary talk
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Pierre Sikivie (University of Florida)Dark MatterPlenary talk
The axion is a hypothetical particle motivated by the Strong CP Problem
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of elementary particle physics and by the dark matter problem of cosmology.
Cold dark matter axions are naturally produced during the QCD phase
transition in the early universe by a process of vacuum realignment.
They may be detected on Earth by converting them to photons in an
electromagnetic cavity permeated by a... -
Plenary talk