paper

Accreting strongly magnetised neutron stars: X-ray Pulsars

arXiv:2204.14185

Abstract

X-ray pulsars (XRPs) are accreting strongly magnetised neutron stars (NSs) in binary systems with, as a rule, massive optical companions. Very reach phenomenology and high observed flux put them into the focus of observational and theoretical studies since the first X-ray instruments were launched into space. The main attracting characteristic of NSs in this kind of system is the magnetic field strength at their surface, about or even higher than , that is about six orders of magnitude stronger than what is attainable in terrestrial laboratories. Although accreting XRPs were discovered about 50 years ago, the details of the physical mechanisms responsible for their properties are still under debate. Here we review recent progress in observational and theoretical investigations of XRPs as a unique laboratory for studies of fundamental physics (plasma physics, QED and radiative processes) under extreme conditions of ultra-strong magnetic field, high temperature, and enormous mass density.

Invited chapter for the "Handbook of X-ray and Gamma-ray Astrophysics" (Eds. C. Bambi and A. Santangelo, Springer Singapore, 2022), 69 pages, 33 figures. The updated chapter contains a short discussion of new data on X-ray polarimetry of XRPs, new discovered cyclotron lines and a number of additions throughout the text. The review will be periodically updated according to advances in the field

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