Foreground dependence of the 20 GeV Galactic halo gamma-ray excess and its proposed connection to the LUX-ZEPLIN event
astro-ph.HE, hep-ph
Submitted: 2026-10-16
Updated: 2026-10-16
Comments: 24 pages, 6 figures, 14 tables. Code: https://github.com/kabazajian/totani (https://doi.org/10.5281/zenodo.23420779); data: https://doi.org/10.5281/zenodo.23420896
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
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
- Collisionless Accretion of Finite-Angular-Momentum Plasma onto a Spinning Black Hole
- Impact of Magnetic Field Topology on Electromagnetic and Gravitational Waves from Binary Neutron Star Merger Remnants
- XRISM Resolve Spectroscopy of GX 5-1: Constraints on Iron Spectral Features in a Luminous Neutron-Star Binary
- SN 1006: A Cosmic Laboratory for Investigating Shock Acceleration Physics