Survival of ultraheavy nuclei in astrophysical sources: applications to protomagnetar outflows
astro-ph.HE, hep-ph, nucl-th
Submitted: 2026-03-06
Updated: 2026-09-14
Comments: 14 pages, 5 figures, 1 table. This matches the version published in PRD
Journal ref: Phys.Rev.D 114 (2026) 063031
DOI: 10.1103/p1n3-hc7k
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- The Pierre Auger Cosmic Ray Observatory
- Observation of the suppression of the flux of cosmic rays above 4x10^19eV
- Constraining the sources of ultra-high-energy cosmic rays across and above the ankle with the spectrum and composition data measured at the Pierre Auger Observatory
- Unmasking the tail of the cosmic ray spectrum
- Ultraheavy Ultrahigh-Energy Cosmic Rays
- Radio Quiet AGNs as Possible Sources of Ultra-high Energy Cosmic Rays
- Blazars as Ultra-High-Energy Cosmic-Ray Sources: Implications for TeV Gamma-Ray Observations
- High Energy Neutrinos and Cosmic-Rays from Low-Luminosity Gamma-Ray Bursts?
- High-energy cosmic-ray nuclei from high- and low-luminosity gamma-ray bursts and implications for multi-messenger astronomy
- Spectrum and Composition of Ultra-high Energy Cosmic Rays from Semi-relativistic Hypernovae
- Newly-born pulsars as sources of ultrahigh energy cosmic rays
- Testing the Newborn Pulsar Origin of Ultrahigh Energy Cosmic Rays with EeV Neutrinos
- High-Energy Radiation from Remnants of Neutron Star Binary Mergers
- Binary Neutron Star Merger Remnants as Sources of Cosmic Rays Below the "Ankle"
- Energetics of High-Energy Cosmic Radiations
- Binary neutron star mergers as the source of the highest energy cosmic rays
- "Espresso" Acceleration of Ultra-high-energy Cosmic Rays
- Ultrahigh-energy Cosmic-ray Nuclei from Black Hole Jets: Recycling Galactic Cosmic Rays through Shear Acceleration
- Bottom-up Acceleration of Ultra-High-Energy Cosmic Rays in the Jets of Active Galactic Nuclei
- High-Energy Neutrino Emission from Espresso-Reaccelerated Ions in Jets of Active Galactic Nuclei
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