Production of High Energy Neutrinos in the Coronae of Ultraluminous X-ray Sources

arXiv:2608.02269 · astro-ph.HE · Submitted 2026-08-03 · Read on arXiv

Norita Kawanaka, Shigeo S. Kimura

astro-ph.HE

Submitted: 2026-08-03

Comments: 13 pages, 5 figures, 1 table

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• AGN — 14× in this paper · explained in 1 episode
• Accretion Flows — 9× in this paper · explained in 1 episode
• Adam — 2× in this paper · explained in 2 episodes
• Little Red Dots — 1× in this paper · explained in 2 episodes

Related papers

• Accreting Neutron Stars in Low-Mass X-ray Binaries
• Numerical Studies of Accretion Flows onto a Neutron Star Engulfed in a Massive Star
• Early panchromatic spectra reveal helium in the thermonuclear supernova 2024kce
• Multiwavelength Classification of Chandra Sources in Omega Centauri
• Impact of the equation of state on core collapse supernovae I: the low- T/W instability
• Secular Evolution of Quasiperiodic Eruptions: eRO-QPE2