Results 221 to 230 of about 1,798 (265)

All‐Solution‐Processed HgTe Quantum Dot Photodetectors for Extended Short‐Wavelength Infrared Range Enhanced by Plasmonic ITO Nanocrystals

open access: yesAdvanced Functional Materials, EarlyView.
All‐solution‐processed, low‐cost extended short‐wavelength infrared photodetectors are realized by coupling colloidal HgTe quantum dots to plasmonic In2O3:Sn,F nanocrystals. Localized surface plasmon resonances boost and spectrally tailor light absorption between 1500 and 3000 nm, enabling responsivities above 40 A W−1.
Kseniia A. Sergeeva   +9 more
wiley   +1 more source

Theoretical evidence of H-He demixing under Jupiter and Saturn conditions. [PDF]

open access: yesNat Commun
Chang X   +14 more
europepmc   +1 more source

Direct aluminium-alloy upcycling from entire end-of life vehicles. [PDF]

open access: yesNat Commun
Krall P   +8 more
europepmc   +1 more source

State shifts in the deep Critical Zone drive landscape evolution in volcanic terrains. [PDF]

open access: yesProc Natl Acad Sci U S A
Karlstrom L   +11 more
europepmc   +1 more source

Exploring pulsar glitches with dipolar supersolids

open access: yes
Bland T   +4 more
europepmc   +1 more source

Neutron stars interiors: Theory and reality [PDF]

open access: yesThe European Physical Journal A, 2016
There are many fascinating processes in the universe which we observe in more detail thanks to increasingly sophisticated technology. One of the most interesting phenomena is the life cycle of stars, their birth, evolution and death. If the stars are massive enough, they end their lives in a core-collapse supernova explosion, one of the most violent ...
J. R. Stone
openaire   +2 more sources

Physics and neutron star interiors

Philosophical Transactions of the Royal Society of London. Series A: Physical and Engineering Sciences, 1992
Abstract Conditions in neutron stars are more extreme than almost any encountered on Earth: densities exceed those of atomic nuclei, and matter has a large neutron excess. During the past quarter of a century, the challenge of understanding neutron stars has stimulated physicists to confront conditions far different from those ...
C. J. Pethick, D. G. Ravenhall
openaire   +1 more source

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