Supermassive black holes as possible sources of ultra high energy cosmic rays
arXiv:2004.07907 · doi:10.3847/1538-4357/ab8ae9
Abstract
Production and acceleration mechanisms of ultra-high-energy cosmic rays (UHECRs) of energy eV, clearly beyond the GZK-cutoff limit remain unclear that points to exotic nature of the phenomena. Recent observations of extragalactic neutrino may indicate the source of UHECRs being an extragalactic supermassive black hole (SMBH). We demonstrate that ultra-efficient energy extraction from rotating SMBH driven by the magnetic Penrose process (MPP) could indeed foot the bill. We envision ionization of neutral particles, such as neutron beta-decay, skirting close to the black hole horizon that energizes protons to over eV for SMBH of mass and magnetic field of strength G. Applied to Galactic center SMBH we have proton energy of order eV that coincides with the knee of the cosmic ray spectra. We show that large factors of high-energy particles along the escaping directions occur only in the presence of induced charge of the black hole that is known as the Wald charge in the case of uniform magnetic field. It is remarkable that the process neither requires extended acceleration zone, nor fine-tuning of accreting matter parameters. Further, this leads to certain verifiable constraints on SMBH's mass and magnetic field strength as UHECRs sources. This clearly makes ultra-efficient regime of MPP one of the most promising mechanisms for fueling UHECRs powerhouse.
14 pages, 6 figures
References in corpus (10)
- Jet Launching Structure Resolved Near the Supermassive Black Hole in M87
- Observation of a Large-scale Anisotropy in the Arrival Directions of Cosmic Rays above eV
- Study of Ultra-High Energy Cosmic Ray Composition Using Telescope Array's Middle Drum Detector and Surface Array in Hybrid Mode
- Possible signature of magnetic fields related to quasi-periodic oscillation observed in microquasars
- Accurate Simulations of Binary Black-Hole Mergers in Force-Free Electrodynamics
- Investigating the Relativistic Motion of the Stars Near the Supermassive Black Hole in the Galactic Center
- Magnetization degree at the jet base of M87 derived from the event horizon telescope data: Testing magnetically driven jet paradigm
- On The Efficiency of Jet Production in Radio Galaxies
- Cosmic Ray Acceleration by Relativistic Shocks: Limits and Estimates
- Induced Gravitational Collapse, Binary-Driven Hypernovae, Long Gramma-ray Bursts and Their Connection with Short Gamma-ray Bursts
Cited by in corpus (14)
- Charged particle and epicyclic motions around Einstein-Gauss-Bonnet black hole immersed in an external magnetic field
- Construction of explicit symplectic integrators in general relativity. II. Reissner-Nordstrom black holes
- Fifty years of energy extraction from rotating black hole: revisiting magnetic Penrose process
- Dynamics of charged particles and magnetic dipoles around magnetized quasi-Schwarzschild black holes
- Lyapunov exponent ISCO and Kolmogorov Senai entropy for Kerr Kiselev black hole
- Geodesic Model of HF QPOs Tested for Black Holes in Spacetimes Reflecting the Effect of Surrounding Dark Matter
- Impact of electric charges on chaos in magnetized spacetimes
- Dragged surfaces. On the accretion tori in the ergoregion
- Embedded BHs and multipole globules: Clustered misaligned thick accretion disks around static SMBHs
- Magnetized black holes: interplay between charge and rotation
- Blazar jets as possible sources of ultra-high energy photons: a short review
- Evolution of Braneworld Kerr-Newman Naked Singularities
- Charged fluids encircling compact objects: force representations and conformal geometries
- Electric Penrose process: high-energy acceleration of ionized particles by non-rotating weakly charged black hole