PeV neutrons as origin of separated SS433 TeV signals
D. Fargion, P. G. De Sanctis Lucentini, S. Turriziani, M. Y. Khlopov, D. Sopin
TL;DR
SS433 exhibits distant, disconnected TeV gamma-ray twins whose origin remains puzzling. The authors propose that a past century eruption produced a collimated beam of tens PeV neutrons via photo-nuclear Delta-resonance in a UV photon bath, with neutrons beta-decaying in flight to tens of TeV electrons that upscatter ambient infrared photons to TeV gamma rays. Key quantitative links include the Delta-resonance energy condition $E_\gamma = \frac{(m_\Delta)^2}{2 E_p}$, neutron flight lengths $L_n \approx 75\,\text{ly}\left(\frac{E_n}{25\,\text{PeV}}\right)$, and Larmor-radius-based collimation for protons and electrons, which together reproduce the observed separation and brightness of the TeV tracks. If correct, this scenario connects SS433 to broader high-energy phenomena such as UHECRs and neutrino astronomy, while suggesting observational tests in other microquasars and upcoming gamma-ray surveys.
Abstract
The SS433, a well-known binary system with an internal black hole, have shown since half a century, an inner (a few year light distances) twin precessing jets spirals. These beams are made by tidal forces while stripping mass from large stellar companion feeding an inner BH accretion disk and an orthogonal accelerating twin jet. From it, the radio, X gamma jet emission. A couple of years ago H.E.S.S telescope as well as HAWC and LHAASO array detectors, discovered also the surprising signature of an unexpected far twin separated gamma beam at tens TeV energy. At a hundred light years distances from its central source. We suggest that it is the legacy of a past rare eruption, a century ago, of tens PeV (10^16 eV) relativistic twin neutron beams. Their beta decay in flight at far distances, into proton, neutrino and in particular into tens TeV electrons, could feed the observed TeV gamma traces. They are originated by the same secondary tens TeV electrons emitting hard gamma, by Inverse Compton Scattering onto interstellar infrared photons.
