collaborators

10 papers

astro-ph.IM2026

NASA ASTRA Initiative White Paper: Space-Based Mission for Ultrahigh Energy Particles

Mauricio Bustamante, Johannes Eser, Ke Fang +9

Ultra-high-energy cosmic rays ( EeV) are the highest-energy particles known, signaling extreme particle processes at work in the universe. However, many aspec…

hep-ph2026

Electron stability constrains neutrino time delays

Mauricio Bustamante, José Manuel Carmona, José Luis Cortés +2

Superluminal neutrino propagation, induced by Lorentz-invariance violation (LIV), is strongly constrained by vacuum pair emission, , a process ordinarily forbi…

hep-ph2026

Are neutrinos Majorana? Fixed-target and high-energy astrophysical searches decide

Gabriela Barenboim, Mauricio Bustamante, Qinrui Liu

Determining whether the neutrino is a Dirac or Majorana fermion remains a fundamental open question. Conventional searches rely on neutrinoless double beta decay, but this electron…

hep-ph2026

Astrophysical bounds on the high-energy evolution of neutrino mixing

Mauricio Bustamante, Qinrui Liu, Gabriela Barenboim

While conventional oscillation experiments measure neutrino mixing parameters with high precision, these measurements are strictly confined to sub-TeV scales. At higher energies, r…

hep-ph2026

Measuring neutrino mixing above 1 TeV with astrophysical neutrinos

Mauricio Bustamante, Qinrui Liu, Gabriela Barenboim

We assess the potential for measuring neutrino mixing parameters at energies above 1~TeV, for the first time, using the flavor composition of TeV--PeV astrophysical neutrinos, i.e.…

hep-ph2026

No Flavor Anisotropy in the High-Energy Neutrino Sky Upholds Lorentz Invariance

Bernanda Telalovic, Mauricio Bustamante

Discovering Lorentz-invariance violation (LIV) would upend the foundations of modern physics. Because LIV effects grow with energy, high-energy astrophysical neutrinos provide the…