Type I X-ray bursts as probes of the neutron star accretion flow

Neutron stars in low-mass X-ray binaries frequently exhibit Type I X-ray bursts caused by unstable nuclear burning of accreted matter on the neutron star surface. X-ray bursts offer the opportunity to constrain the neutron star radii and masses and hence the equation of state of one of the densest environments in the Universe. However, constraining neutron star parameters requires knowledge of the entire observed emission, which also includes the emission of the neutron star accretion flow. X-ray bursts irradiate it, leading to structural and emission changes. Therefore, understanding the evolution of the accretion flow emission not only allows us to constrain neutron star properties but also to probe its accretion environment. The body of this PhD thesis details my work examining the impact of Type I X-ray bursts on the neutron star accretion flow. My first project studies the observational impact of an X-ray burst on the corona. Combining an analytical model and a hybrid-emission plasma code reveals how the coronal emission decreases at high X-ray energies and increases at low X-ray energies due to Compton scattering with burst photons. The project furthermore shows how coronal cooling depends on burst and coronal properties. For my second project, I used a reflection code and post-processed general relativistic hydrodynamics simulation data of a disk being impacted by an X-ray burst to calculate how the reflection spectrum of an accretion disk evolves during an X-ray burst. The simulations of the third project examine the effect of neutron star spin on the Poynting-Robertson drag during the burst and demonstrate its importance, regardless of the neutron star's spin. I used this simulation data for the next project to calculate the evolution of the thermal disk emission. The project finds that the enhancement of the thermal disk emission is only weakly correlated with an increase in the mass accretion rate. The dissertation highlights the wealth of observational impact of Type I X-ray bursts on the accretion flow, which offers the opportunity to probe its properties and improve the analysis of burst observations.

Level thesis:degree_level

Doctoral

Department dc:contributor.department

Physics

Grantor dc:publisher

Georgia Institute of Technology

Year dc:date.issued

2025

Author dc:creator

• Speicher, Julia

Advisor dc:contributor.advisor

• Ballantyne, David

Committee members dc:contributor.committeemember

• Bogdanovic, Tamara
• Wise, John H.
• Otte, Nepomuk
• Strohmayer, Tod E.

• astrophysics
• X-ray binaries
• X-ray bursts
• neutron stars

Language dc:language.iso

en_US

Handle dc:identifier.uri

https://hdl.handle.net/1853/78684

OAI identifier oai:identifier

oai:repository.gatech.edu:1853/78684