The role of Bethe-Heitler pair production in reconnection-driven flares in M87*
Maria Petropoulou, Despina Karavola, Lorenzo Sironi

TL;DR
This paper investigates how Bethe-Heitler pair production influences the emission and cascade processes in reconnection-driven flares from M87*, revealing its role in high-energy photon production and attenuation.
Contribution
It introduces a detailed numerical model of Bethe-Heitler pair production in the context of black hole magnetospheric reconnection flares, highlighting its impact on high-energy emission.
Findings
Disk photons serve as targets for Bethe-Heitler pair production.
Secondary pairs emit very high-energy synchrotron photons (>0.1 TeV).
Electromagnetic cascades enhance pion production and photon attenuation.
Abstract
Rapid TeV flares have been observed from the core of the active galaxy M87. These have been attributed to inverse Compton scattering of disk photons by electrons and positrons accelerated in transient reconnection layers formed in baryon-poor regions of the magnetosphere of the central black hole, M87*. It was previously shown that even a small number of protons accelerated in the same layers can lead to bright GeV proton-synchrotron flares, if protons receive of the dissipated power for reconnecting fields of 100 G. We aim to investigate the role of Bethe-Heitler pair production in the emission of reconnection-driven flares from M87* in this physical regime. We perform numerical calculations that incorporate inelastic collisions between relativistic protons and photons, as well as photon-photon pair production, and compute the non-thermal radiation from the layer.…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Astrophysics and Cosmic Phenomena · Galaxies: Formation, Evolution, Phenomena
