Kelly, Ruth ME;
Marshall, Herman L;
Zane, Silvia;
Brice, Nabil;
Ravi, Swati;
Turolla, Roberto;
Taverna, Roberto;
(2025)
Exploring the Future of Soft X-Ray Polarimetry: The Capabilities of the REDSoX Instrument for X-Ray Dim Isolated Neutron Star and Magnetar Studies.
The Astrophysical Journal
, 987
(2)
, Article 113. 10.3847/1538-4357/adde58.
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Abstract
X-ray polarimetry offers a unique window into neutron star physics and can provide answers to questions that cannot otherwise be probed. The upcoming Rocket Experiment Demonstration of a Soft X-ray Polarimeter (REDSoX) sounding rocket mission will be the first experiment equipped with a detector able to explore polarized X-rays below 1 keV, observing in the 0.2–0.4 keV range. Although REDSoX will only be capable of short, one-off observations, it will crucially test the instrument performance. In this paper we investigate how a fully fledged orbital mission with a longer lifetime, based on an instrument design similar to REDSoX, will allow us to study thermal emission from X-ray dim isolated neutron stars (XDINSs) and magnetars, probing their magnetic fields and the physics of their outer surface layers, including vacuum effects and quantum electrodynamics (QED) mode conversion at the vacuum resonance. We discuss the potentially observable features for promising values of the star’s surface temperature, magnetic field, and viewing geometry. Assuming emission from the whole surface, we find that, for a source with a magnetic field B = 5 × 1013 G and surface temperature T ≈ 107 K, the instrument can resolve a proton cyclotron absorption feature in the spectrum with high significance when collecting ≈25,000 counts across a single observation. Similarly, for a source with B = 1014 G and T ≈ 107 K, a switch in the dominant polarization mode, caused by mode conversion at the vacuum resonance, can be detected by collecting ≈25,000 counts, allowing for a long-sought observational test of the presence of QED effects. We then present two case studies for XDINS targets: RX J1856.5–3754 and RX J0720.4–3125.
| Type: | Article |
|---|---|
| Title: | Exploring the Future of Soft X-Ray Polarimetry: The Capabilities of the REDSoX Instrument for X-Ray Dim Isolated Neutron Star and Magnetar Studies |
| Open access status: | An open access version is available from UCL Discovery |
| DOI: | 10.3847/1538-4357/adde58 |
| Publisher version: | https://doi.org/10.3847/1538-4357/adde58 |
| Language: | English |
| Additional information: | This work is licensed under a Creative Commons License. The images or other third-party material in this article are included in the Creative Commons license, unless indicated otherwise in the credit line; if the material is not included under the Creative Commons license, users will need to obtain permission from the license holder to reproduce the material. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/ |
| Keywords: | Science & Technology, Physical Sciences, Astronomy & Astrophysics, RX J1856.5-3754, POLARIZATION, SURFACE, EMISSION, ATMOSPHERES, RADIATION, SPECTRA, ABSORPTION, DISCOVERY, FEATURES |
| UCL classification: | UCL UCL > Provost and Vice Provost Offices > UCL BEAMS UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics |
| URI: | https://discovery.ucl.ac.uk/id/eprint/10211274 |
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