Magnetic and electric properties of a quantum vacuum

R Battesti, C Rizzo - Reports on Progress in Physics, 2012 - iopscience.iop.org
In this report we show that a vacuum is a nonlinear optical medium and discuss what the
optical phenomena are that should exist in the framework of the standard model of particle …

Atmospheres and radiating surfaces of neutron stars

AY Potekhin - Physics-Uspekhi, 2014 - iopscience.iop.org
The early 21st century is witnessing a breakthrough in the study of the thermal radiation of
neutron stars. Observations with modern space telescopes have provided a wealth of …

Cyclotron lines in highly magnetized neutron stars

R Staubert, J Trümper, E Kendziorra… - Astronomy & …, 2019 - aanda.org
Cyclotron lines, also called cyclotron resonant scattering features are spectral features,
generally appearing in absorption, in the X-ray spectra of objects containing highly …

Physics of strongly magnetized neutron stars

AK Harding, D Lai - Reports on Progress in Physics, 2006 - iopscience.iop.org
There has recently been growing evidence for the existence of neutron stars possessing
magnetic fields with strengths that exceed the quantum critical field strength of 4.4× 10 13 G …

The magnificent seven: magnetic fields and surface temperature distributions

F Haberl - Astrophysics and Space Science, 2007 - Springer
Presently seven nearby radio-quiet isolated neutron stars discovered in ROSAT data and
characterized by thermal X-ray spectra are known. They exhibit very similar properties and …

New views of thermonuclear bursts

T Strohmayer, L Bildsten - arXiv preprint astro-ph/0301544, 2003 - arxiv.org
Since the advent of powerful new X-ray observatories, NASA's Rossi X-ray Timing Explorer
(RXTE), the Italian-Dutch BeppoSAX mission, XMM-Newton and Chandra, a number of …

Surface emission from neutron stars and implications for the physics of their interiors

F Özel - Reports on Progress in Physics, 2012 - iopscience.iop.org
Neutron stars are associated with diverse physical phenomena that take place in conditions
characterized by ultrahigh densities as well as intense gravitational, magnetic and radiation …

Isolated neutron stars: the challenge of simplicity

R Turolla - Neutron stars and pulsars, 2009 - Springer
The seven soft, thermal sources discovered by ROSAT offer an unprecedented opportunity
to unveil the temperature and magnetic field surface distribution of isolated neutron stars …

Axion emission can explain a new hard X-ray excess from nearby isolated neutron stars

M Buschmann, RT Co, C Dessert, BR Safdi - Physical review letters, 2021 - APS
Axions may be produced thermally inside the cores of neutron stars (NSs), escape the stars
due to their feeble interactions with matter, and subsequently convert into x rays in the …

Atmosphere models of magnetized neutron stars: QED effects, radiation spectra and polarization signals

M Van Adelsberg, D Lai - Monthly Notices of the Royal …, 2006 - academic.oup.com
Observations of surface emission from isolated neutron stars (NSs) provide unique
challenges to theoretical modelling of radiative transfer in magnetized NS atmospheres …