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Black Hole

Lensing of space time around a black hole. At Oxford we study black holes observationally and theoretically on all size and time scales - it is some of our core work.

Credit: ALAIN RIAZUELO, IAP/UPMC/CNRS. CLICK HERE TO VIEW MORE IMAGES.

Dr Peter Hatfield

Visitor

Research theme

  • Astronomy and astrophysics
  • Lasers and high energy density science

Sub department

  • Astrophysics

Research groups

  • Galaxy formation and evolution
  • Hintze Centre for Astrophysical Surveys
peter.hatfield@physics.ox.ac.uk
  • About
  • Publications

Observation of He-like satellite lines of the H-like potassium K XIX emission

Astrophysical Journal American Astronomical Society 881:2 (2019) 92

Authors:

ME Weller, P Beiersdorfer, TE Lockard, GV Brown, A McKelvey, J Nilsen, R Shepherd, VA Soukhanovskii, MP Hill, LMR Hobbs, D Burridge, DJ Hoarty, J Morton, L Wilson, Steven Rose, P Hatfield

Abstract:

We present measurements of the H-like potassium (K xix) X-ray spectrum and its He-like (K xviii) satellite lines, which are situated in the wavelength region between 3.34 and 3.39 Å, which has been of interest for the detection of dark matter. The measurements were taken with a high-resolution X-ray spectrometer from targets irradiated by a long-pulse (2 ns) beam from the Orion laser facility. We obtain experimental wavelength values of dielectronic recombination satellite lines and show that the ratio of the Lyα lines and their dielectronic satellite lines can be used to estimate the electron temperature, which in our case was about 1.5 ± 0.3 keV.

Enhanced fluorescence from x-ray line coincidence pumping of K-pumped Cl and Mg-pumped Ge plasmas

Proceedings of SPIE Society of Photo-optical Instrumentation Engineers 11111 (2019)

Authors:

J Nilsen, D Burridge, LMR Hobbs, D Hoarty, P Beiersdorfer, GV Brown, N Hell, D Panchenko, MF Gu, AM Saunders, HA Scott, RA London, P Hatfield, MP Hill, R Charles, L Wilson, CRD Brown, Steven Rose

The blind implosion-maker: Automated inertial confinement fusion experiment design

Physics of Plasmas AIP Publishing 26:6 (2019) 062706

Authors:

Peter W Hatfield, Steven Rose, R Scott

Abstract:

The design of inertial confinement fusion (ICF) experiments, alongside improving the development of energy density physics theory and experimental methods, is one of the key challenges in the quest for nuclear fusion as a viable energy source [O. A. Hurricane, J. Phys.: Conf. Ser. 717, 012005 (2016)]. Recent challenges in achieving a high-yield implosion at the National Ignition Facility (NIF) have led to new interest in considering a much wider design parameter space than normally studied [J. L. Peterson et al., Phys. Plasmas 24, 032702 (2017)]. Here, we report an algorithmic approach that can produce reasonable ICF designs with minimal assumptions. In particular, we use the genetic algorithm metaheuristic, in which “populations� of implosions are simulated, the design of the capsule is described by a “genome,� natural selection removes poor designs, high quality designs are “mated� with each other based on their yield, and designs undergo “mutations� to introduce new ideas. We show that it takes ∼5 × 104 simulations for the algorithm to find an original NIF design. We also link this method to other parts of the design process and look toward a completely automated ICF experiment design process—changing ICF from an experiment design problem to an algorithm design problem.

Transforming education with the Timepix detector - Ten years of CERN@school

Radiation Measurements Elsevier BV (2019) 106090

Authors:

B Parker, L Thomas, E Rushton, P Hatfield

IRIS opens pupils' eyes to real space research

Astronomy & Geophysics Oxford University Press (OUP) 60:1 (2019) 1.22-1.24

Authors:

Peter Hatfield, W Furnell, A Shenoy, E Fox, B Parker, L Thomas, EAC Rushton

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