White dwarfs are the end products of the life cycles of more than 90% of all stars. This makes them important laboratories for studying stellar evolution and the behaviour of matter at extremes of temperature and density. There is growing evidence that many white dwarfs are swallowing up debris from, now destroyed, planetary systems. Measuring the abundance of this material in the atmospheres of the white dwarfs can tell us about the composition of these planets. However, we first need to understand the evolution of white dwarfs, including the composition of their atmospheres. We are using data from a variety of space missions and telescopes to study the population of white dwarfs to provide this insight.
We wish to appoint an enthusiastic PhD student to contribute to the exploitation of this data, drawn from several observational programmes. The work will involve the analysis of spectroscopic and imaging data from the the ESA Gaia mission, Hubble Space Telescope (HST) and ground-based telescopes. There will also be a theoretical element to the work, using the University’s supercomputer to simulate stellar atmospheres, for comparison with the data.
There are several lines of research in which the student can become involved, depending on personal interests:
We are closely involved in the European Space Agency Gaia mission. Launched in December 2013, the satellite is carrying out a detailed survey of the entire visible galaxy to measure the positions, space motion and distances of approximately 1 billion stars. Data release 2, including as many as 500,000 white dwarfs. Combine with follow-up data from other surveys and ground-based spectroscopy, the Gaia data will allow us to obtain measurements of masses and radii with unprecedented accuracy, search for hidden stellar/exo-planet companions and search for the elusive progenitors of type Ia supernova explosions.
Measurement of the abundances of C and Si in a large sample of white dwarfs shows that in all cases C is depleted, indicating that the material has a rocky origin – similar to that of asteroids. A likely explanation is that this material is collected from extra-solar planetary debris and then retained in the hot white dwarf’s envelope by the force of radiation. We now need to test this by adapting the atmospheric modelling computer programme to include these physical processes.
Recently, we have shown that high spectral resolution and signal-to-noise spectra of a single hot white dwarfs can be used to measure potential changes in the value of the fundamental physical constants, such as the fine structure constant and electron/proton mass ratio, in a strong gravitational field. The accuracy of the technique is limited by how well we know the wavelengths of atomic absorption features in the spectrum. We are currently acquiring improved atomic data and are obtaining more high quality spectra of other stars to continue this work.
UK Bachelor Degree with at least 2:1 in a relevant subject or overseas equivalent.
The University of Leicester English language requirements apply.
Home/EU students only subject to residency requirements.
When applying, please ensure we have received all of the following required documents by Wednesday 29th January 2020:
• Submit an online application form https://le.ac.uk/study/research-degrees/funded-opportunities/stfc-studentships
• 2 academic references
• STFC Research Interests Form
• Undergraduate transcripts
- If you have completed your undergraduate degree, we will also require your undergraduate degree certificate
- If you have completed a postgraduate degree, we will also require your transcripts and degree certificate
If we do not have the required documents by the closing date, your application may not be considered for the studentship.
26th February 2020 – In person
27th February 2020 – Skype only
28th February 2020 – Skype only
2nd March 2020 – Skype only
3rd March 2020 – Skype only
4th March 2020 – In person
1. J.C. Berengut, V.V. Flambaum, A. Ong, J.K. Webb, J.D. Barrow, M.A. Barstow, S.P. Preval and J.B. Holberg, 2013, “Limits on the dependence of the fine-structure constant on gravitational potential from white dwarf spectra”, Phys.Rev.Letters, 111. http://arxiv.org/abs/1305.1337
2. M.A. Barstow, J.K. Barstow, S.L. Casewell, J.B. Holberg and I. Hubeny, 2014, “Evidence for an external origin of heavy elements in hot DA white dwarfs”, MNRAS, 440, 1607-1625 (May, 10.1093/mnras/stu216).
3. Gaia Collaboration, C. Babusiaux, F. van Leeuwen, M.A. Barstow, et al., 2018, “Gaia Data Release 2. Observational Hertzspring-Russell diagrams”, A&A, 616, id.A10, 29 pp (August, DOI - 10.1051/0004-6361/201832843).
4. S.R.G. Joyce, M.A. Barstow, S.L. Casewell, M.R. Burleigh, J.B. Holberg and H.E. Bond, 2018, “Testing the white dwarf mass-radius relation and comparing optical and far-UV spectroscopic results with Gaia DR2, HST, and FUSE”, MNRAS, 479, 1612-1626 (September – DOI 10.1093/mnras/sty1425).