Charge order in kagome superconductors
Why does charge order break symmetry differently across the AV3Sb5 kagome superconductor family?
Why does charge order break symmetry differently across the AV3Sb5 kagome superconductor family?
Do the excitations of the 5/2 fractional quantum Hall state exhibit non-Abelian exchange statistics?
Can an isolated two-dimensional disordered interacting system avoid thermalization indefinitely?
Is the field-induced state of α-RuCl3 a Kitaev spin liquid with fractional excitations?
Why do flowing mixtures with very different grain sizes form repeated layers?
How does slow fault slip develop into the unstable rupture of a natural earthquake?
How do earthquakes occur hundreds of kilometres down, where ordinary brittle failure is suppressed?
What supplied the energy to sustain Earth’s magnetic dynamo before the solid inner core grew?
How much water do subducting rocks carry deep into the mantle, and how is it exchanged?
How does fast electrical breakdown become a lightning leader in natural thunderstorm fields?
How will low clouds change under sustained warming, and how will that change affect Earth’s energy balance?
Some giant planets close to their stars are larger than ordinary cooling models predict. What keeps them inflated?
Stars within one globular cluster can have different light-element abundances. Their common origin is still debated.
A pulsar’s rotating beam is familiar. The plasma process that makes its exceptionally bright radio waves is less certain.
A star’s core and outer layers exchange rotational motion. Which internal processes set that exchange as stars evolve?
Saturn’s icy rings look relatively clean. Does that reveal when they formed, or how they lose and retain pollution?
An unidentified absorber darkens Venus’s clouds in near-ultraviolet light. Which chemicals produce it and keep it present?
Ganymede generates its own magnetic field. What keeps the conducting material inside it moving?
Some pulsars suddenly spin faster. What triggers the rapid transfer of rotational motion that produces a large glitch?
Turbulent motion concentrates into rare, intense bursts. Can the fluid equations predict how those bursts scale?
Quark distributions change when protons and neutrons are bound in nuclei. What physical mechanism causes those changes?
A proton’s total spin is known. How is it shared among quark spin, gluon spin and their orbital motion?
Different methods still disagree on parts of the hadronic contribution to the muon’s magnetic moment. Which data or corrections explain the differences?
Cow-like transients brighten and fade rapidly while emitting powerful X-rays and radio waves. Which stellar events produce them?