2020 Fall.Includes bibliographical references.As the Short-Baseline Neutrino Program Far Detector, the ICARUS liquid argon time-projection chamber will operate at shallow depth and therefore be exposed to the full surface flux of cosmic rays. This poses a problematic background to the sterile neutrino search. A direct way to reject this background is to surround the cryostat with a detector capable of tagging incident cosmic muons with high efficiency, the Cosmic Ray Tagging System (CRT). I have worked to develop the CRT detector hardware and the simulation and reconstruction software. This system, currently undergoing installation, is approximately 25% commissioned and taking data. I have developed a powerful method for cosmogenic backgrou...
The Fermilab Short Baseline Neutrino (SBN) program aims to observe and reconstruct thousands of neut...
Since the discovery of neutrino oscillation in atmospheric neutrinos by the Super-Kamiokande experim...
Since the discovery of neutrino oscillation in atmospheric neutrinos by the Super-Kamiokande experim...
As the SBN far-detector, the ICARUS liquid argon time-projection chamber will operate at shallow dep...
The uncertainties associated with neutrino-nucleus cross section modelling need to be redu...
When a cosmic ray particle collides with the upper atmosphere, it creates a shower of particles that...
Thanks to the good tracking and calorimetric capabilities of a Liquid Argon Time Projection Chamber ...
CHIPS (CHerenkov detectors In mine PitS) is an R&D project aiming to develop novel cost-effective de...
The Short Baseline Neutrino Program at Fermilab aims to discover, or definitely rule out, the existe...
ManuscriptWe have investigated the possibility of ντ detection using Cosmic Ray Tau Neutrino Telesc...
The Short Baseline Neutrino Program aims to discover, or definitely rule out, the existence of steri...
Ultra high energy neutrinos are important astrophysical messengers that carry information on process...
Neutrino physics is approaching the precision era, with current and future experiments aiming to per...
Cosmic ray (CR) interactions can be a challenging source of background for neutrino oscillation and ...
The Short Baseline Neutrino (SBN) program at Fermilab will search for new physics in the neutrino os...
The Fermilab Short Baseline Neutrino (SBN) program aims to observe and reconstruct thousands of neut...
Since the discovery of neutrino oscillation in atmospheric neutrinos by the Super-Kamiokande experim...
Since the discovery of neutrino oscillation in atmospheric neutrinos by the Super-Kamiokande experim...
As the SBN far-detector, the ICARUS liquid argon time-projection chamber will operate at shallow dep...
The uncertainties associated with neutrino-nucleus cross section modelling need to be redu...
When a cosmic ray particle collides with the upper atmosphere, it creates a shower of particles that...
Thanks to the good tracking and calorimetric capabilities of a Liquid Argon Time Projection Chamber ...
CHIPS (CHerenkov detectors In mine PitS) is an R&D project aiming to develop novel cost-effective de...
The Short Baseline Neutrino Program at Fermilab aims to discover, or definitely rule out, the existe...
ManuscriptWe have investigated the possibility of ντ detection using Cosmic Ray Tau Neutrino Telesc...
The Short Baseline Neutrino Program aims to discover, or definitely rule out, the existence of steri...
Ultra high energy neutrinos are important astrophysical messengers that carry information on process...
Neutrino physics is approaching the precision era, with current and future experiments aiming to per...
Cosmic ray (CR) interactions can be a challenging source of background for neutrino oscillation and ...
The Short Baseline Neutrino (SBN) program at Fermilab will search for new physics in the neutrino os...
The Fermilab Short Baseline Neutrino (SBN) program aims to observe and reconstruct thousands of neut...
Since the discovery of neutrino oscillation in atmospheric neutrinos by the Super-Kamiokande experim...
Since the discovery of neutrino oscillation in atmospheric neutrinos by the Super-Kamiokande experim...