Results 201 to 210 of about 507,717 (322)
Electron Channeling Contrast Imaging of Ferroelastic Domains
A simple scanning electron microscopy technique, electron channeling contrast imaging, unveils nanoscale ferroelastic domains and their coupling to functional properties in oxide heterostructures. The work demonstrates high‐resolution mapping of both surface and buried domains, broadening the experimental toolbox for ferroic and quantum oxide systems ...
Wei Peng +13 more
wiley +1 more source
Water Versus Land on Temperate Rocky Planets. [PDF]
Guimond CM +8 more
europepmc +1 more source
High‐Concentration Antibody Formulation via Solvent‐Based Dehydration
Amorphous solid antibodies are encapsulated into hydrogel microparticles through a solvent‐based dehydration process. The solvent extracts water from antibody solution droplets, causing the antibody to concentrate, and precipitation of the antibody into amorphous solid is induced.
Talia Zheng +3 more
wiley +1 more source
Characterization of exoplanets in the James Webb Space Telescope era. [PDF]
Lunine JI, Bahcall N.
europepmc +1 more source
DID PLANET FORMATION BEGIN INSIDE PERSISTENT GASEOUS VORTICES? [PDF]
P. Barge, Joël Sommeria
openalex +1 more source
Coupling a dual‐gradient carbonized framework with Fe2O3/Fe‐N‐C catalytic sites enables spatially synchronized sulfur redox across the entire electrode thickness in high‐mass‐loading Li–S batteries. This synergistic structural–catalytic design effectively mitigates concentration, ohmic, and electrochemical polarization, thereby achieving high‐capacity ...
Yuxuan Zhang +6 more
wiley +1 more source
A first look at rocky exoplanets with JWST. [PDF]
Kreidberg L, Stevenson KB.
europepmc +1 more source
Can the tidal quality factors of terrestrial planets and moons scale as positive powers of the tidal frequency? [PDF]
Michael Efroimsky
openalex +1 more source
All‐perovskite tandem solar cells are evaluated under low‐intensity and low‐temperature (LILT) conditions relevant to space environments. Distinct loss regimes emerge, where weaker entropic mixing causes halide segragation below ≈240 K going along with a strong current imbalance, while poor electron transport in C60 dominates.
Sercan Ozen +10 more
wiley +1 more source
Building wet planets through high-pressure magma-hydrogen reactions. [PDF]
Horn HW +4 more
europepmc +1 more source

