Relativistic black-hole jet sources are leading candidates for high energy (>> TeV) neutrino production. The relations defining (a) efficient photopion losses of cosmic ray protons on target photons and (b) gamma-gamma opacity of gamma rays through that same target photon field imply clear multiwavelength predictions for when and at what energies blazars and GRBs should be most neutrino bright and gamma-ray dim
Since 2010 IceCube observed around 50 high-energy neutrino events of cosmic origin above 60 TeV, but...
AbstractTop–down models of cosmic rays produce more neutrinos than photons and more photons than pro...
Das Hauptziel dieser Arbeit ist die Charakterisierung extrem starker Quellen, die höchstwahrscheinli...
AbstractThe IceCube Collaboration has reported neutrinos with energies between ∼30 TeV and a few PeV...
Various aspects of the high-energy emission from relativistic jets associated wi th compact astrophy...
Blazars have long been considered as accelerator candidates for cosmic rays. In such a scenario, had...
In the light of growing evidence that blazars are responsible for part of the astrophysical very-hig...
The recent spatial and temporal coincidence of the blazar TXS 0506+056 with the IceCube-detected neu...
In this paper, I present a qualitative discussion on the prospect of production of ultra-high photon...
We treat the production of neutrons, photons, and neutrinos through photomeson interactions of relat...
Neutrinos at energies ranging from sub-TeV to EeV from astrophysical sources can yield interesting p...
© Copernicus Gesellschaft 2001 Submitted to Cornell University’s online archive www.arXiv.org in 200...
Blazars and Gamma Ray Bursts (GRBs) are the fastest objects known so far. The radiation we see from ...
Three independent predictions follow from postulating the existence of protons co-accelerated with e...
Observations imply that gamma-ray bursts (GRBs) are produced by the dissipation of the kinetic energ...
Since 2010 IceCube observed around 50 high-energy neutrino events of cosmic origin above 60 TeV, but...
AbstractTop–down models of cosmic rays produce more neutrinos than photons and more photons than pro...
Das Hauptziel dieser Arbeit ist die Charakterisierung extrem starker Quellen, die höchstwahrscheinli...
AbstractThe IceCube Collaboration has reported neutrinos with energies between ∼30 TeV and a few PeV...
Various aspects of the high-energy emission from relativistic jets associated wi th compact astrophy...
Blazars have long been considered as accelerator candidates for cosmic rays. In such a scenario, had...
In the light of growing evidence that blazars are responsible for part of the astrophysical very-hig...
The recent spatial and temporal coincidence of the blazar TXS 0506+056 with the IceCube-detected neu...
In this paper, I present a qualitative discussion on the prospect of production of ultra-high photon...
We treat the production of neutrons, photons, and neutrinos through photomeson interactions of relat...
Neutrinos at energies ranging from sub-TeV to EeV from astrophysical sources can yield interesting p...
© Copernicus Gesellschaft 2001 Submitted to Cornell University’s online archive www.arXiv.org in 200...
Blazars and Gamma Ray Bursts (GRBs) are the fastest objects known so far. The radiation we see from ...
Three independent predictions follow from postulating the existence of protons co-accelerated with e...
Observations imply that gamma-ray bursts (GRBs) are produced by the dissipation of the kinetic energ...
Since 2010 IceCube observed around 50 high-energy neutrino events of cosmic origin above 60 TeV, but...
AbstractTop–down models of cosmic rays produce more neutrinos than photons and more photons than pro...
Das Hauptziel dieser Arbeit ist die Charakterisierung extrem starker Quellen, die höchstwahrscheinli...