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Showing 1–6 of 6 results

Advanced filters: Author: Ronald Redmer Clear advanced filters

Turning solid aluminium transparent by intense soft X-ray photoionization

The first experimental demonstration of saturable absorption in core-electron transitions in aluminium paves the way for investigating warm dense matter, which potentially has an important role in planetary science and the realization of inertial confinement fusion.

Bob Nagler
Ulf Zastrau
Justin S. Wark
Research26 Jul 2009
Nature Physics

Volume: 5, P: 693-696
Diamond precipitation dynamics from hydrocarbons at icy planet interior conditions

Experiments using high-intensity X-ray pulses incident on high-pressure hydrocarbons suggest that diamond formation can occur at shallower depths in icy planets and may play a role in the internal convection that generates their magnetic fields.

Mungo Frost
R. Stewart McWilliams
Alexander F. Goncharov
Research08 Jan 2024
Nature Astronomy

Volume: 8, P: 174-181
Publisher Correction: Diamond precipitation dynamics from hydrocarbons at icy planet interior conditions

Mungo Frost
R. Stewart McWilliams
Alexander F. Goncharov
Amendments and Corrections22 Jan 2024
Nature Astronomy

Volume: 8, P: 545
Evidence of shock-compressed stishovite above 300 GPa

Markus O. Schoelmerich
Thomas Tschentscher
Karen Appel
ResearchOpen Access23 Jun 2020
Scientific Reports

Volume: 10, P: 1-8
Release dynamics of nanodiamonds created by laser-driven shock-compression of polyethylene terephthalate

Ben Heuser
Armin Bergermann
Dominik Kraus
ResearchOpen Access28 May 2024
Scientific Reports

Volume: 14, P: 1-11
Understanding dense hydrogen at planetary conditions

Understanding the behaviour of materials at high pressures and temperatures is of great importance to planetary science and the physics of warm dense matter. This Review addresses the close connection between modelling the interiors of gaseous planets and the high-pressure physics of hydrogen and helium.

Ravit Helled
Guglielmo Mazzola
Ronald Redmer
Reviews01 Sept 2020
Nature Reviews Physics

Volume: 2, P: 562-574