Ian Padilla Gay
Research Assoc-Theoretical, SLAC National Accelerator Laboratory
Bio
Hi! I'm a postdoctoral research associate at SLAC and Stanford. My current research focuses on the role of neutrino oscillations in core-collapse supernovae and binary neutron star merger remnants.
Education & Certifications
-
PhD, Niels Bohr Institute - University of Copenhagen, Astroparticle Physics (2022)
-
MSc, Lund University, Theoretical Physics (2019)
All Publications
-
Symmetry breaking due to multi-angle matter-neutrino resonance in neutron star merger remnants
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
2024
View details for DOI 10.1088/1475-7516/2024/05/037
View details for Web of Science ID 001296044200031
-
Collisions and collective flavor conversion: Integrating out the fast dynamics
PHYSICAL REVIEW D
2024; 109 (6)
View details for DOI 10.1103/PhysRevD.109.063021
View details for Web of Science ID 001195716600017
-
Neutrino Flavor Pendulum Reloaded: The Case of Fast Pairwise Conversion
PHYSICAL REVIEW LETTERS
2022; 128 (12): 121102
Abstract
In core-collapse supernovae or compact binary merger remnants, neutrino-neutrino refraction can spawn fast pair conversion of the type ν_{e}ν[over ¯]_{e}↔ν_{x}ν[over ¯]_{x} (with x=μ, τ), governed by the angle-dependent density matrices of flavor lepton number. In a homogeneous and axially symmetric two-flavor system, all angle modes evolve coherently, and we show that the nonlinear equations of motion are formally equivalent to those of a gyroscopic pendulum. Within this analogy, our main innovation is to identify the elusive characteristic of the lepton-number angle distribution that determines the depth of conversion with the "pendulum spin." The latter is given by the real part of the eigenfrequency resulting from the linear normal-mode analysis of the neutrino system. This simple analogy allows one to predict the depth of flavor conversion without solving the nonlinear evolution equations. Our approach provides a novel diagnostic tool to explore the physics of nonlinear systems.
View details for DOI 10.1103/PhysRevLett.128.121102
View details for Web of Science ID 000786542500003
View details for PubMedID 35394327
-
Neutrino fast flavor pendulum. II. Collisional damping
PHYSICAL REVIEW D
2022
View details for DOI 10.1103/PhysRevD.106.103031
-
A three Higgs doublet model with symmetry-suppressed flavour changing neutral currents
JOURNAL OF HIGH ENERGY PHYSICS
2021
View details for DOI 10.1007/JHEP11(2021)079
View details for Web of Science ID 000717994300003
-
Multi-dimensional solution of fast neutrino conversions in binary neutron star merger remnants
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
2021
View details for DOI 10.1088/1475-7516/2021/01/017
View details for Web of Science ID 000620675000017
-
Neutrino propagation hinders fast pairwise flavor conversions
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
2020
View details for DOI 10.1088/1475-7516/2020/06/048
View details for Web of Science ID 000551875400057
-
Series solutions of single-field models of inflation
IOP PUBLISHING LTD. 2018
View details for DOI 10.1088/1742-6596/1030/1/012008
View details for Web of Science ID 000454778900008