A5108051936- Astrophysics and Cosmic Phenomena
- Dark Matter and Cosmic Phenomena
- Neutrino Physics Research
- Particle physics theoretical and experimental studies
- Radio Astronomy Observations and Technology
- Particle Detector Development and Performance
- Radiation Therapy and Dosimetry
- Gamma-ray bursts and supernovae
- Atmospheric Ozone and Climate
- High-Energy Particle Collisions Research
- Atmospheric and Environmental Gas Dynamics
- History and Developments in Astronomy
- Pulsars and Gravitational Waves Research
- Cosmology and Gravitation Theories
- Ionosphere and magnetosphere dynamics
- Precipitation Measurement and Analysis
- Solar and Space Plasma Dynamics
- Atmospheric aerosols and clouds
- Noncommutative and Quantum Gravity Theories
- Particle Accelerators and Free-Electron Lasers
- Superconducting and THz Device Technology
- Research Data Management Practices
- Radio Wave Propagation Studies
- Advanced Optical Sensing Technologies
- Antenna Design and Optimization
Colorado School of Mines
2022-2025
Istituto Nazionale di Fisica Nucleare, Sezione di Lecce
2023
Université Libre de Bruxelles
2023
Instituto de Tecnologías en Detección y Astropartículas
2023
Consejo Nacional de Investigaciones Científicas y Técnicas
2023
National Technological University
2023
Pierre Auger Observatory
2023
Universidad Nacional de La Plata
2023
Institute of Astronomy and Space Physics
2023
University of Buenos Aires
2023
Abstract Ultra-high-energy neutrinos serve as messengers of some the highest energy astrophysical environments. Given that are neutral and only interact via weak interactions, can emerge from sources, traverse astronomical distances, point back to their origins. Their interactions require large target volumes for neutrino detection. Using Earth a converter, terrestrial, sub-orbital, satellite-based instruments able detect signals neutrino-induced extensive air showers. In this paper, we...
Cosmic Probes of Fundamental Physics take two primary forms: Very high energy particles (cosmic rays, neutrinos, and gamma rays) gravitational waves. Already today, these probes give access to fundamental physics not available by any other means, helping elucidate the underlying theory that completes Standard Model. The last decade has witnessed a revolution exciting discoveries such as detection high-energy neutrinos scope for major developments in next decades is dramatic, we detail this report.
The Pierre Auger Observatory (Auger) and the Telescope Array Project (TA) are two largest ultra-high-energy cosmic ray observatories in world. They operate Southern Northern hemispheres, respectively, at similar latitudes but with different surface detector (SD) designs. This difference design changes their sensitivity to various components of extensive air showers. over-arching goal Auger@TA working group is cross-calibrate SD arrays order identify or rule out systematic causes for apparent...
The Pierre Auger Observatory (Auger) and the Telescope Array Project (TA) are two largest ultra-high-energy cosmic ray (UHECR) observatories in world. One obstacle pursuing full-sky UHECR physics is apparent discrepancy flux measured by experiments. This could be due to astrophysical differences as TA observe Southern Northern skies, respectively. However, scintillation detectors used have very different sensitivity various components of extensive air showers than water-Cherenkov (WCD)...
Using the Earth as a neutrino converter, tau fluxes from astrophysical point sources can be detected by tau-lepton-induced extensive air showers (EASs). Both muon and induced upward-going EAS signals terrestrial, sub-orbital satellite-based instruments. The sensitivity of these telescopes evaluated with nuSpaceSim package, which includes nuPyProp simulation package. package propagates neutrinos ($\nu_\mu$, $\nu_\tau$) through to produce corresponding charged leptons (muons tau-leptons). We...
Ultra-high-energy neutrinos serve as messengers of some the highest energy astrophysical environments. Given that are neutral and only interact via weak interactions, can emerge from sources, traverse astronomical distances, point back to their origins. Their interactions require large target volumes for neutrino detection. Using Earth a converter, terrestrial, sub-orbital, satellite-based instruments able detect signals neutrino-induced extensive air showers. In this paper, we describe...
The composition of cosmic ray primaries at the highest energies is one biggest open questions in astroparticle physics, and directly related to understanding sources of ultra-high energy rays. At Pierre Auger Observatory, rays are studied via extensive air showers they produce Earth’s atmosphere. Improving the understanding primary motivation behind upgrade AugerPrime. Surface Detector Obser- vatory is, as part this upgrade, process receiving new electronics additional detectors. Most...