Evidence is now compelling that elements heavier than helium in many white dwarf
atmospheres have accumulated by accretion from orbiting rocky bodies, often larger than …

The study of structure, thermodynamic state, equation of state (EOS) and transport properties
of warm dense matter (WDM) has become one of the key aspects of laboratory astrophysics …

We investigate a new class of habitable planets composed of water-rich interiors with
massive oceans underlying H 2-rich atmospheres, referred to here as Hycean worlds. With …

Carbon is the fourth-most prevalent element in the Universe and essential for all known life.
In the elemental form it is found in multiple allotropes, including graphite, diamond and …

The composition of a planet's atmosphere is determined by its formation, evolution, and
present-day insolation. A planet's spectrum therefore may hold clues on its origins. We …

The search for life in the Universe is a fundamental problem of astrobiology and modern
science. The current progress in the detection of terrestrial-type exoplanets has opened a …

Aims. We present an inversion method based on Bayesian analysis to constrain the interior
structure of terrestrial exoplanets, in the form of chemical composition of the mantle and core …

The recent discovery of more than a thousand planets outside our Solar System,, together
with the significant push to achieve inertially confined fusion in the laboratory, has prompted …

Traditionally, the search for life on exoplanets has been predominantly focused on rocky
exoplanets. The recently proposed Hycean worlds have the potential to significantly expand …

Abstract Machine learning interatomic force fields are promising for combining high
computational efficiency and accuracy in modeling quantum interactions and simulating …