pith. sign in

arxiv: 1006.1045 · v1 · pith:FVH3UH7Enew · submitted 2010-06-05 · 🌌 astro-ph.HE

Angular, spectral, and time distributions of highest energy protons and associated secondary gamma-rays and neutrinos propagating through extragalactic magnetic and radiation fields

F.A. Aharonian , S.R. Kelner , A.Y. Prosekin This is my paper
classification 🌌 astro-ph.HE
keywords angularenergyfieldsgamma-rayshighestmagneticneutrinospropagating
0
0 comments X
read the original abstract

The angular, spectral and temporal features of the highest energy protons and accompanying them secondary neutrinos and synchrotron gamma-rays propagating through the intergalactic magnetic and radiation fields are studied using the analytical solutions of the Boltzmann transport equation obtained in the limit of the small-angle and continuous-energy-loss approximation.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Simulating realistic radio morphologies of Fanaroff-Riley I jets in a self-regulating cool-core cluster

    astro-ph.GA 2026-06 unverdicted novelty 7.0

    Self-regulating AGN jets in MHD simulations of cool-core clusters yield realistic FRI radio morphologies viewed along the jet axis and account for frequency-independent lobe extents via 1-50 μG fields allowing both yo...

  2. Revisiting radio synchrotron diagnostics in star-forming galaxies

    astro-ph.GA 2026-04 conditional novelty 7.0

    Advection-only galactic wind models fail to reproduce observed vertical radio profiles without unrealistic velocities, synchrotron spectra are biased toward young electrons in dense regions, and bremsstrahlung/Coulomb...

  3. FR0 radio galaxy jets -- I. linking jet dynamics and high-energy emission in LEDA 55267 and LEDA 58287

    astro-ph.HE 2026-05 unverdicted novelty 4.0

    3D RHD simulations of FR0 jets in LEDA 55267 and LEDA 58287 show recollimation shocks driving compactness via turbulence and deceleration, with SED modeling predicting lepto-hadronic emission at TeV energies as a test...

  4. Extreme Transients in Gamma Rays

    astro-ph.HE 2026-05 unverdicted novelty 2.0

    A review of extreme gamma-ray transients defined as catastrophic events or extreme particle acceleration regimes, covering diagnostics, instruments, and source classes.