Abstract: Neutrino physics aims to answer some of the most pressing questions in particle physics: why the Universe is dominated by matter, why the neutrino mass is so small and if there are more types of neutrinos. Due to the …
ABSTRACT: Halometry---mapping out the spectrum, location, and kinematics of nonluminous structures inside the Galactic halo---can be realized via effects that variable weak gravitational lensing induces on the proper motions of stars and other luminous background sources. Modern astrometric surveys provide …
Ken Van Tilburg (NYU/IAS) “The Structure of Dark Matter on Small Scales” Read More »
Abstract: While neutrino oscillation physics has entered an era of precision measurements, several anomalies in experiments at short baselines remain without a satisfactory answer. The MicroBooNE experiment has been recording neutrino interactions on Fermilab’s Booster Neutrino Beam since 2015 employing …
David Caratelli (Fermilab) “Neutrinos at Short Baselines: the MicroBooNE Experiment” Read More »
Abstract: The Mu2e experiment will search for the charged lepton flavor violating (CLFV) neutrino-less conversion of a negative muon into an electron in the field of a nucleus, reaching a 90% C.L. limit of 8x10^-17 on the conversion rate. …
Abstract: The effect of dark matter and dark energy in the universe can be inferred through measurements of anisotropies in the cosmic microwave background (CMB). The quantum effect of new physics on collisions at the Large Hadron Collider can be …
Tom Melia (Kavli IPMU – Japan)“ ‘CMB-ing’ the Search for New Physics at Colliders” Read More »
Abstract: The discovery of the Higgs boson has revealed that the quartic Higgs self-coupling becomes small at very high energy scales. Guided by this observation, I introduce Higgs Parity, which is a spontaneously broken symmetry exchanging the standard model Higgs …
Keisuke Harigaya (IAS) “ Physics beyond the standard model from Higgs Parity” Read More »
Abstract: Ever since the discovery, neutrinos have proven to be one of the most intriguing subatomic particles. In the past two decades, we have made tremendous progress in the establishment of the neutrino oscillation phenomenon. We are now able to …
Ka Vang Tsang (SLAC) “Imaging Neutrinos: Machine Learning in LArTPC” Read More »
ABSTRACT: Neutrino oscillation experiments such as NOvA and T2K search for the disappearance and appearance of muon and electron flavor neutrinos in a predominately muon-type beam. These experiments are currently measuring the oscillation parameters to greater precision but will not …
ABSTRACT: Theories beyond the Standard Model of particle physics often predict new, light, feebly interacting particles whose discovery requires novel search strategies. A light particle, the QCD axion, elegantly solves the outstanding strong-CP problem of the Standard Model; cousins of …
Masha Baryakhtar (NYU) ” New Physics Across the Spectra” Read More »
ABSTRACT: Neutrino oscillation is a well-established phenomenon. Over the past two decades, nearly all of the parameters governing these oscillations have been measured experimentally, using neutrinos from the atmosphere, the sun, nuclear reactors, and particle accelerators. The remaining unknowns have …
Abstract: The Mu2e experiment will search for the charged lepton flavor violating (CLFV) neutrino-less conversion of a negative muon into an electron in the field of a nucleus, reaching a 90% C.L. limit of 8x10^-17 on the conversion rate. This …
Abstract: The ability of current and next generation accelerator based neutrino oscillation measurements to reach their desired sensitivity requires a high-level of understanding of the neutrino-nucleus interactions. These include precise estimation of the relevant cross sections and the reconstruction of …
Adi Ashkenazi (Fermilab) “Probing V Interactions for V Physics” Read More »
ABSTRACT: The Gaia mission has provided distance and velocity measurements of over a billion stars in the Milky Way, making it the largest stellar catalog at hand. Simultaneously, recent developments in cosmological simulations have made it possible to track stars …
Lina Necib (Caltech) “Dark Matter in the Era of Gaia” Read More »