2–6 Sept 2024
Università di Milano "La Statale"
Europe/Rome timezone

Modelling the very high-energy gamma-ray emission from accreting neutron stars in X-ray binaries: a theoretical framework for future observations

GAL
2 Sept 2024, 09:09
1m
Poster Poster hang

Speakers

Lorenzo Ducci (Istituto Nazionale di Astrofisica (INAF))Dr Patrizia Romano (Istituto Nazionale di Astrofisica (INAF))

Description

The search of gamma-ray emission from accreting pulsars in X-ray binaries (XRBs) has been ongoing for some time. Recent marginal detections in high-mass X-ray binaries (HMXBs) have sparked renewed interest in this area. Anticipating future advances in gamma-ray telescopes like the Cherenkov Telescope Array (CTA), we investigate the expected emission above 10 GeV from XRBs using an enhanced Cheng & Ruderman model. This model incorporates Monte Carlo simulations to account for cascade development inside and outside the accretion disc, including pair and photon production processes that involve interaction with nuclei, X-ray photons from the accretion disc, and the magnetic field. Our results yield a wide range of gamma-ray luminosities (up to ~1E35 erg/s) and spectra, with some exhibiting emission below ~100 GeV and others extending to 10-100 TeV. We compare our findings with existing Fermi/LAT and VERITAS data for two HMXBs, and look forward to more comprehensive comparisons with forthcoming, more sensitive instruments.

Primary authors

Lorenzo Ducci (Istituto Nazionale di Astrofisica (INAF)) Dr Patrizia Romano (Istituto Nazionale di Astrofisica (INAF))

Co-authors

Prof. Andrea Santangelo (University of Tuebingen) Dr Stefano Vercellone (Istituto Nazionale di Astrofisica (INAF))

Presentation materials