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The Leidenfrost effect — in which droplets levitate above hot surfaces — is well-known, but the ultimate fate of the evaporating droplets is unexplored. New experiments show that droplets either fly away or explode, depending on their initial size and purity.
Women remain under-represented in science, and in particular in physics. Effective action to remedy this situation should be based on rigorous analysis of high-quality data.
The percentage of women in post-graduate physics positions has stalled just below 20%. The most precipitous drop in women’s representation occurs between high school and university; however, women at all career stages struggle with ongoing cultural burdens and obstacles.
The Event Horizon Telescope collaboration has released images and data showing the dark shadow of the supermassive black hole at the centre of galaxy Messier 87. This release is the result of years of development in instrumentation and data processing.
We examine the arguments for and against building the next big particle collider and explore the technologies for different future particle accelerator projects.
Oliver Brüning and Lucio Rossi discuss an upgrade of the Large Hadron Collider (LHC), the High-Luminosity LHC (HL-LHC), which aims to significantly increase the luminosity.
Edda Gschwendtner and Patric Muggli discuss the concept of plasma wakefield acceleration and its potential for future particle colliders and other applications.
Michael Benedikt and Frank Zimmermann describe the Future Circular Collider, a proposed collider-based research infrastructure that can be realized in successive steps.
Shinichiro Michizono describes the International Linear Collider, a proposed 250 GeV electron–positron collider using superconducting radiofrequency technology.
Calculations show that contrary to the commonly accepted idea, sound waves carry a tiny negative mass and create a gravitational field that is associated with it.
New experiments on swarms of Caenorhabditis elegans reveal that the worm can form a dynamical network that can be understood using active matter physics, and controlled using genetic manipulation.
How the mass of super-Earths affects mantle convection is a key question for understanding rocky exoplanet structure and thermal dynamics. New material models based on ab initio mineral calculations characterize convection, with implications for magnetism, planetary cooling, atmospheric composition and habitability.