Proton-Proton Fusion: Powering the Sun
Large-scale simulations of quarks promise precise view of reactions of astrophysical importance.
Large-scale simulations of quarks promise precise view of reactions of astrophysical importance.
Gravitational wave observations combined with optical and gamma-ray data confirm earlier predictions, offer insights into how the galaxy produces lead, mercury, and other elements.
For one of the strongest known materials, calculations clarify a long-standing debate about how atoms pack together.
Theory predicts that bending a film will control spin direction and create a spin current for next-generation electronics.
New materials could turn water into the fuel of the future.
Neutrons provide the solution to nanoscale examination of living cell membrane and confirm the existence of lipid rafts.
New supercomputing capabilities help understand how to cope with large-scale instabilities in tokamaks.
For the first time, scientists modeled the spontaneous bifurcation of turbulence to high-confinement mode, solving a 35-year-old mystery.
Calculations of a subatomic particle called the sigma provide insight into the communication between subatomic particles deep inside the heart of matter.
Water table depth and groundwater flow are vital to understanding the amount of water that plants transmit to the atmosphere.
Heating the core of fusion reactors causes them to develop sheared rotation that can improve plasma performance.
A new model identifies a high degree of fluctuations in the glue-like particles that bind quarks within protons as essential to explaining proton structure.