Completed Physics & Astronomy Chemistry

Gekko2026

In plain English

AI plain-English summary

A team of UK physicists will fire powerful laser pulses at a gas target in Japan to recreate the conditions inside certain types of stars. The researchers have won competitive access to the Gekko XII laser facility in Japan for experiments scheduled in February 2026. They will create photo-ionised plasmas—superheated, electrically charged gases where atoms are stripped of electrons by intense X-ray radiation. Such plasmas are common in astrophysical objects like accretion disks around black holes and the atmospheres of white dwarf stars, but they are extremely difficult to study in the laboratory because they are hard to sustain in a steady state. This experiment introduces a new step: pre-ionising the plasma before probing it with L-shell radiation. This should create a more stable, steady-state plasma that better mimics the conditions in real astrophysical environments. The work builds on previous experiments at the Rutherford Appleton Laboratory in the UK, in Shanghai, and at the Omega-EP facility in the US. This is fundamental science. It will not produce an immediate practical application. However, understanding how matter behaves under extreme radiation fields is essential for interpreting astronomical observations and for testing the computer models used to simulate stars and galaxies.

View original technical description
This travel grant application is to support our use of the Gekko XII laser facility in Japan. The beamtime has been awarded after competitive bidding and will be scheduled for February 2026. We intend to carry out on experiment into photo-ionised plasmas that will be of relevance to studies of astrophysical plasmas. This is a follow up to experiments at RAL, Shanghai and Omega-EP and will introduce a new extension to the experiments that involves pre-ionising the plasma before probing with L-shell radiation, as described in the case attached. The advantage of this is that it allows us to move to a more steady state situation that is more appropriate to astrophysical plasmas.

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Researchers

David Riley (Principal Investigator)

Related Research

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Transient High Energy Density Plasmas Driven By Few Cycle Laser Pulses.
Support for photoionisation experiments at the OMEGA EP high-power laser facility
Capital Equipment 2018
IR-FEL/XUV HHG hybrid experiments for molecular science

Original classification

Research and Innovation

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