Synchrotron emission from a nearby zone of SgrA
arXiv:2103.01900 · doi:10.1093/mnras/stab682
Abstract
Quasi-linear diffusion (QLD), driven by the cyclotron instability, is proposed as a mechanism for the possible generation of synchrotron emission in the nearby zone of SgrA. For physically reasonable parameters, the QLD, by causing non-zero pitch angle scattering lets electrons with the relativistic factors of the order of emit synchrotron radiation in the hard -ray spectral band keV.
arXiv comment4 pages, 3 figures
References in corpus (12)
- Monitoring stellar orbits around the Massive Black Hole in the Galactic Center
- Acceleration of petaelectronvolt protons in the Galactic Centre
- A powerful flare from Sgr A* confirms the synchrotron nature of the X-ray emission
- Stochastic Electron Acceleration During the NIR and X-ray Flares in Sagittarius A*
- Spin and mass of the nearest supermassive black hole
- Data Compression for the Tomo-e Gozen with Low-rank Matrix Approximation
- On the very high energy spectrum of the Crab pulsar
- Electron-Positron pairs creation close to a black hole horizon. Red-shifted annihilation line in the emergent X-ray spectra of a black hole, part I
- On the simultaneous generation of high energy emission and submillimeter/infrared radiation from active galactic nuclei
- On the rotationally driven pevatron in the centre of the Milky Way
- Constraining cosmic-ray acceleration in the magnetospheric gaps of Sgr A*
- Radio emission of magnetars driven by the quasi-linear diffusion