I am a PhD student at the Anton Pannekoek Institute for Astronomy at the University of Amsterdam. I study thermonuclear X-ray bursts on Neutron Stars, in particular the dynamics of ocean layers of the star during these bursts. I am part of Dr. Anna Watts' European Research Council (ERC) funded group.
Email: F.R.N.Chambers (at) uva.nl
Visitors' address: Science Park 904, 1098 XH Amsterdam
Mailing address: PO Box 94249, 1090 GE Amsterdam
Neutron stars are the smallest and most dense stars in our universe. They contain about as much mass as our sun, however, this mass is compressed into a sphere about 10 - 20 km in radius. This density gives rise to exotic forms of matter, strong gravitational fields, and strong magnetic fields. Neutron stars constitute one of the most extreme astrophysical environments available for study, and so are a perfect laboratory to test fundamental physics.
Many neutron stars come in pairs called binaries with a sun-like companion. These stars orbit around each other quite rapidly, and if they are close enough together, matter can be stripped off the surface of the companion. This process is call accretion and occurs because of the neutron star's large gravitational pull. The matter falling to the surface acts as fuel for nuclear fusion and, given the right conditions, this burning process can become unstable and results in a violent thermonuclear explosion called a Type I X-ray burst.
X-ray timing analysis reveals periodic frequencies during these bursts. These frequencies are offset from the spin frequency of the neutron star by several Hz, and can drift by 1-3 Hz during the cooling phase of the burst. It is unknown exactly what causes these frequencies, but a possible explanation is that a wave exists in the ocean layers of the star that changes in frequency as the star cools.
I am also involved in a collaboration with Ferran Garcia (HZDR) investigating thermal convection with many applications including neutron star oceans.
Burning in the tail: implications for a burst oscillation model [arxiv link] In this paper we calculate modes during short waiting time bursts, these are hydrogen/helium triggered bursts in quick succession. The calculation involves an accurate background model that includes a realistic composition and full nuclear reaction network. We find that using this background reduces frequency drift compared to previous calculations, which didn't account for composition changes, and was a problem for matching the mode model of burst oscillations to observations.
Superburst Oscillations: ocean and crustal modes excited by Carbon-triggered Type I X-ray bursts [arxiv link] In this paper we calculate modes during superbursts which are triggered by unstable carbon burning in the deep ocean and last hours. We find that frequency of the mode (in the rotating frame) varies during the burst from 4–14 Hz and is sensitive to the background parameters, in particular the temperature of the ocean and ignition depth.
Polar travelling waves in thin rotating spherical shells [arxiv link]
Thermal convection in rotating spherical shells: temperature-dependent internal heat generation using the example of triple-alpha burning [arxiv link]
The onset of low Prandtl number thermal convection in thin spherical shells [arxiv link]
New Burning Physics and Burst Oscillations, COSPAR, Pasedena, USA, June 2018
New Burning Physics and Burst Oscillations, BERN18, Prato, Italy, June 2018
Superburst Oscillations, JINA-CEE: Frontier in Nuclear Astrophysics, Notre Dame, USA, May 2018
Superburst Oscillations, IAU: 50 Years of Pulsars, Manchester, UK, September 2017
Currently completing a PhD at the Anton Pannekoek Institute for Astronomy, on the topic: Surface Patterns on Neutron Stars. Taught a Bachelor course Introduction to Astronomy and Masters course Fluid Dynamics. Was the PhD representitive on the PhD/PostDoc council academic year 2017/2018.
Graduated with First Class Honours. Awarded Trinity College Gold Medal for academic excellence upon graduating. Obtained Foundation Scholarship for outstanding performance in voluntary examinations.
Calculated properties of bi-layered materials using high performance computing software and Density Functional Theory techniques.
I have also held jobs as a server in Trinity College Dining Hall, an intern in Pacemetrics, a mark layer for the Dublin Bay Sailing Club, and a tutor in secondary school maths, physics, applied-maths and technical graphics.