A5076377853- Astrophysics and Cosmic Phenomena
- Neutrino Physics Research
- Dark Matter and Cosmic Phenomena
- Radio Astronomy Observations and Technology
- Gamma-ray bursts and supernovae
- Pulsars and Gravitational Waves Research
- Particle physics theoretical and experimental studies
- Particle Detector Development and Performance
- Radio, Podcasts, and Digital Media
- Particle accelerators and beam dynamics
- Computational Physics and Python Applications
- Motor Control and Adaptation
- Arctic and Antarctic ice dynamics
- Superconducting Materials and Applications
- CCD and CMOS Imaging Sensors
- Atomic and Subatomic Physics Research
- Gyrotron and Vacuum Electronics Research
- Earthquake Detection and Analysis
- Neural and Behavioral Psychology Studies
- Cryospheric studies and observations
- Ionosphere and magnetosphere dynamics
- Solar and Space Plasma Dynamics
- Radio Wave Propagation Studies
- Particle Accelerators and Free-Electron Lasers
- Atmospheric Ozone and Climate
The University of Texas at Arlington
2019-2025
Curtin University
2023
University of California, Irvine
2021
University of California, Santa Cruz
2018-2020
With the advent of a new generation neutrino experiments which leverage high-intensity beams for precision measurements, it is timely to explore physics topics beyond standard neutrino-related physics. Given that realm model (BSM) has been mostly sought at high-energy regimes colliders, such as LHC CERN, exploration BSM in will enable complementary measurements energy balance LHC. This concert with ideas fixed target and beam-dump world-wide, e.g., those CERN. The combination high intensity...
136 Xe is used as the target medium for many experiments searching 0νββ.Despite underground operation, cosmic muons that reach laboratory can produce spallation neutrons causing activation of detector materials.A potential background difficult to veto using muon tagging comes in form 137 created by capture on Xe.This isotope decays via beta decay with a half-life 3.8 minutes and Q β ∼4.16 MeV.This work proposes explores concept adding small percentage 3 He xenon means thermal reduce number...
Neutrino telescopes provide strong sensitivity to sterile neutrino oscillations through matter-enhanced oscillation, occurring in the few TeV energy range for eV$^{2}$-scale mass-squared splittings. Prior searches have focused on $\nu_\mu$ disappearance, which has a particularly mixing angle $\theta_{24}$ via $\nu_\mu\rightarrow\nu_s$ transitions. Nowadays, $\nu_\mu\rightarrow\nu_e$ and $\nu_\mu\rightarrow\nu_\tau$ appearance channels been considered less promising at telescopes, due part...
The properties of 60-{\mu}m thick Ultra-Fast Silicon Detectors (UFSD) detectors manufactured by Fondazione Bruno Kessler (FBK), Trento (Italy) were tested before and after irradiation with minimum ionizing particles (MIPs) from a 90Sr \b{eta}-source . This FBK production, called UFSD2, has UFSDs gain layer made Boron, Boron low-diffusion, Gallium, Carbonated Carbonated. neutrons took place at the TRIGA reactor in Ljubljana, while proton CERN SPS. sensors exposed to neutron fluence 4*10e14,...
Abstract Previous research on movement preparation identified a period of corticospinal suppression about 200 ms prior to initiation. This phenomenon has been observed for different types motor tasks typically used investigate (e.g., reaction time, self-initiated, and anticipatory actions). However, we recently discovered that this is not when actions must be initiated under time pressure. In the present study, investigated urgency effects throughout course an timing task. Participants were...