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Astrophysics (information studies) PhD Projects, Programs & Scholarships

We have 5 Astrophysics (information studies) PhD Projects, Programs & Scholarships

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  Theoretical and numerical studies of relativistic laser-plasma interaction and applications
  Prof Z Sheng
Applications accepted all year round

Funding Type

PhD Type

You might be a potential candidate if you are interested in using high performance computing to discover novel physics or solve key problems in high intensity laser-matter interactions and their applications, particularly in advanced particle accelerators and radiation sources (from THz to X-rays).
  Numerical and analytical studies of early universe Einstein-Euler-scalar field models
  Dr F Beyer
Applications accepted all year round

Funding Type

PhD Type

The point of this project is to study the Einstein’ equation (as a model of gravity) coupled to the Euler equations (as a model of cosmological matter) and the scalar field equations (as a model of the “inflaton” driving “inflation”) in the cosmological setting close to a big bang singularity.
  The variability of the Earth’s electron radiation belt
  Prof R Horne, Dr G Del-Zanna, Dr S Glauert
Application Deadline: 15 April 2020

Funding Type

PhD Type

The Earth’s electron radiation belts consist of high energy (relativistic) electrons which are trapped by the Earth’s external magnetic field and which circulate around the Earth.
  Cosmic-Ray Muons in Different Applications
  Research Group: Particle Physics and Particle Astrophysics
  Dr V Kudryavtsev
Applications accepted all year round

Funding Type

PhD Type

Cosmic-ray muons are known to be useful in applications beyond particle astrophysics. They have helped with mapping structure of volcanoes and with finding voids in various geological structures.
  Properties of evolved, hot luminous stars from large spectroscopic surveys
  Research Group: Astronomy and Astrophysics
  Dr P Crowther
Applications accepted all year round

Funding Type

PhD Type

Massive stars are rare, though dominate the radiative, mechanical and chemical feedback in star-forming galaxies. Historically, spectroscopic studies of hot massive stars in the Milky Way and nearby galaxies have been restricted to small sample sizes.
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