We demonstrate that the ultra-high-energy cosmic rays (UHECRs) produced in the nuclear cascade in the jets of low-luminosity gamma-ray bursts (LL-GRBs) can describe the UHECR spectrum and composition, and at the same time, the diffuse neutrino flux at the highest energies. The radiation density in the source simultaneously controls the neutrino production and the development of the nuclear cascade, leading to a flux of nucleons and light nuclei describing even the cosmic-ray ankle at 5 centerdot 1018 eV. The derived source parameters are consistent with population studies, indicating a baryonic loading factor of about 10. Our results motivate the continued experimental search of LL-GRBs as a unique GRB population
A model is proposed for the origin of cosmic rays (CRs) from ~10^14 eV to the highest energies, >10^...
It is natural to consider the possibility that the most energetic particles detected (> 10^18 eV), u...
Abstract: The detection of an astrophysical source of Ultra High Energy (& 1 PeV) neutrinos and Ultr...
We demonstrate that the UHECRs produced in the nuclear cascade in the jet of Low-Luminosity Gamma-Ra...
We discuss neutrino and cosmic-ray emission from Gamma-Ray Bursts (GRBs) with the injection of nucle...
We discuss neutrino and cosmic-ray emission from Gamma-Ray Bursts (GRBs) with the injection of nucle...
Aim. We discuss neutrino and cosmic ray emission from gamma-ray bursts (GRBs) with the injection of ...
We discuss neutrino and cosmic-ray emission from Gamma-Ray Bursts (GRBs) with the injection of nucle...
Aim. We discuss neutrino and cosmic ray emission from gamma-ray bursts (GRBs) with the injection of ...
We demonstrate that a population of active galactic nuclei (AGN) can describe the observed spectrum ...
We reconsider the possibility that gamma-ray bursts (GRBs) are the sources of the ultra-high energy ...
Gamma-ray bursts (GRBs) are sources of energetic, highly variable fluxes of gamma rays, which demons...
We reconsider the possibility that gamma-ray bursts (GRBs) are the sources of the ultra-high energy ...
The recently discovered gamma-ray burst (GRB) 060218/SN 2006aj is classified as an X-ray Flash with ...
A complete model for the origin of high-energy ( >∼ 1014 eV) cosmic rays from gamma-ray bursts (GRB...
A model is proposed for the origin of cosmic rays (CRs) from ~10^14 eV to the highest energies, >10^...
It is natural to consider the possibility that the most energetic particles detected (> 10^18 eV), u...
Abstract: The detection of an astrophysical source of Ultra High Energy (& 1 PeV) neutrinos and Ultr...
We demonstrate that the UHECRs produced in the nuclear cascade in the jet of Low-Luminosity Gamma-Ra...
We discuss neutrino and cosmic-ray emission from Gamma-Ray Bursts (GRBs) with the injection of nucle...
We discuss neutrino and cosmic-ray emission from Gamma-Ray Bursts (GRBs) with the injection of nucle...
Aim. We discuss neutrino and cosmic ray emission from gamma-ray bursts (GRBs) with the injection of ...
We discuss neutrino and cosmic-ray emission from Gamma-Ray Bursts (GRBs) with the injection of nucle...
Aim. We discuss neutrino and cosmic ray emission from gamma-ray bursts (GRBs) with the injection of ...
We demonstrate that a population of active galactic nuclei (AGN) can describe the observed spectrum ...
We reconsider the possibility that gamma-ray bursts (GRBs) are the sources of the ultra-high energy ...
Gamma-ray bursts (GRBs) are sources of energetic, highly variable fluxes of gamma rays, which demons...
We reconsider the possibility that gamma-ray bursts (GRBs) are the sources of the ultra-high energy ...
The recently discovered gamma-ray burst (GRB) 060218/SN 2006aj is classified as an X-ray Flash with ...
A complete model for the origin of high-energy ( >∼ 1014 eV) cosmic rays from gamma-ray bursts (GRB...
A model is proposed for the origin of cosmic rays (CRs) from ~10^14 eV to the highest energies, >10^...
It is natural to consider the possibility that the most energetic particles detected (> 10^18 eV), u...
Abstract: The detection of an astrophysical source of Ultra High Energy (& 1 PeV) neutrinos and Ultr...