Magnetic Amplification in Cosmic Field Explained
Experimental turbulence model matches the magnetic field amplification seen within the remains of a supernova.
Experimental turbulence model matches the magnetic field amplification seen within the remains of a supernova.
Realistic computational view of how atom stretches informs microscopic description of nuclear energy production.
Careful tuning of a surface at the nanoscale could lead to robust materials for solar panels, other uses.
Pairs of precisely tuned X-ray pulses uncover ultrafast processes and previously unmapped structures.
Researchers determine the reaction pathway to how soot and other toxic components form in combustion systems.
Atomic-scale defects in graphene are shown to selectively allow protons to pass through a barrier that is just one carbon atom thick.
New models reveal the impact of competing processes on helium bubble formation in plasma-exposed tungsten.
Computational algorithms show whirlpools, not disks, form and dissipate on fluid’s surface.
New structures could accelerate progress toward faster computing and high-security data transfer across fiber optic networks.
Lead and bismuth systems are being produced to fill the nation’s need for short-lived, alpha-emitting isotopes.
Scientists shed new light on a proton's spin, refining our understanding of nuclear physics.
Tiny semiconducting crystals show promise for solar cell architectures and light-emitting devices.