Papers
Ten published, one under review, around 410 citations. Everything is on the arXiv. Grouped by topic below, most recent first within each group; the complete lists are on INSPIRE and ORCID.
Axions and ultralight dark matter
- 2026 Searching for dark matter X-ray lines from the Large Magellanic Cloud with eROSITA A search for the X-ray line a decaying sterile neutrino or axion-like particle would leave in eROSITA data. No line is found, which sets limits on masses from 2 to 18 keV.
- 2025 Searching for axion-like particles with SPHEREx How deep a near-infrared all-sky survey can go in the search for decaying axion-like particles.
- 2025 Searches for signatures of ultralight axion dark matter in polarimetry data of the European Pulsar Timing Array Ultralight axion dark matter would slowly rotate the polarisation of pulsar light. The EPTA data shows no such effect, which constrains the coupling.
- 2022 Searching for dark-matter waves with PPTA and QUIJOTE pulsar polarimetry The first version of the pulsar polarimetry search, combining PPTA timing data with QUIJOTE observations.
Dark matter and the Standard Model
- 2026 Galactic Center Neutrinos from Cosmic Ray–Dark Matter Interactionsunder review Cosmic rays colliding with halo dark matter produce neutrinos. Computing that flux and recasting public ANTARES data gives some of the strongest bounds on keV–GeV dark matter.
- 2026 The Highest-Energy Neutrino Event Constrains Dark Matter–Neutrino Interactions What the most energetic neutrino ever detected, KM3-230213A, implies about scattering between dark matter and neutrinos.
- 2023 New physics searches at kaon and hyperon factories A large community review of dark sector searches at kaon and hyperon facilities. I contributed the dark photon results derived from our supernova cooling analysis.
- 2021 Supernova Constraints on Dark Flavored Sectors A supernova that cools too quickly would indicate that something invisible is carrying energy away. The first such bounds on dark sectors coupled to flavour.
Neutrino physics
- 2023 A seesaw model for large neutrino masses in concordance with cosmology Cosmology requires neutrinos to be light; laboratory experiments may yet find them heavier. A model in which both can hold.
- 2021 (g−2)e,μ in an extended inverse type-III seesaw model Whether a single model can account for both the muon and electron magnetic moment anomalies while also generating neutrino masses.
- 2020 High-energy constraints from low-energy neutrino nonstandard interactions My first paper: low-energy neutrino experiments turn out to constrain high-energy new physics about as well as colliders do.