activity
20062026
most citedHyper-Kamiokande Design Report

417 citations · 5.4k across the 123 of their papers we have counts for

collaborators

123 papers

astro-ph.HE2026

SN2025aico: An Interesting Case Of Ni Mixing, Ejecta Asymmetries, and Dust Formation in a Type IIb Supernova

Grace Davis, Kyle Medler, Chris Ashall +8

Stripped-envelope supernovae provide a window into how massive stars lose their layers, mix radioactive material, produce dust, and explode asymmetrically. We present optical, near…

astro-ph.HE2026

Little Red Dots as Shock-Powered High-Energy Neutrino Sources

Tyco Mera, Chris Ashall, Shunsaku Horiuchi +3

Little Red Dots (LRDs) are compact, high-redshift sources whose physical nature remains uncertain. Their optical spectra bear many similarities to Type IIn supernovae (SNe IIn), mo…

astro-ph.CO2026

Constraints on Annihilating Dark Matter from Gamma-Ray Background-Galaxy Shape Correlations: Model-independent Null Results and Moderate Template-based Signals

Masato Shirasaki, Deheng Song, Oscar Macias +2

We revisit the cross-correlation between the unresolved -ray background and galaxy shapes to constrain the annihilation cross section of particle dark matter. Our analysis uses…

astro-ph.HE2026

Ultra high-energy cosmic rays from relativistic outflows in accretion induced collapse of white dwarfs

Mainak Mukhopadhyay, Shunsaku Horiuchi

When a rapidly-rotating, highly magnetized white dwarf (WD) approaches the Chandrashekhar limit through mass accretion, it can undergo an accretion-induced collapse (AIC) to form a…

astro-ph.HE2026

Survival of ultraheavy nuclei in astrophysical sources: applications to protomagnetar outflows

Nick Ekanger, Mukul Bhattacharya, Kohta Murase +1

Outflows of rapidly rotating protomagnetars have been considered as attractive sites for the synthesis of nuclei heavier than iron, but the question remains whether these nuclei ar…

hep-ph2026

The Cosmic Neutrino Background is within Reach of Future Neutrino Telescopes

Gonzalo Herrera, Shunsaku Horiuchi, Xiaolin Qi +1

The cosmic neutrino background (CB) can be boosted to high energies due to scatterings with energetic cosmic rays (CRs) across cosmological scales. Previous calculations focused…