About the SKA
Outline of Fields Expected to be Advanced by the SKA
Cosmology - The universe on the largest scale
- The Dark Ages: Structures beyond redshift 5
- Structures: Radio tracers a thousand times fainter
- Fundamental Constants: Ho, qo
- The Heavy Elements: When did they start to form?
High Energy Astrophysics - The radio, X-ray, gamma-ray connection
- Giant Gamma-Ray Burst Sources: Identification to physics
- Relativistic Phenomena: Formation of superluminal jets
- Black Hole Identification: Setting the limits in galactic nuclei
- The S-Z Effect: The interaction of the CMB with hot matter
Cosmogony - Origins, Evolution
- Large-Scale Structures: Galaxy clusters and voids
- Galaxies: Formation, evolution, and mergers
- Heavy Elements: Generation as the universe evolves
- Stars: From the interstellar medium to protostars
- Planetary Systems: Evolution of circumstellar disks
Fundamental Physics - Gravitation: Testing GR in the strong field case
- Black Holes: Schwarzschild or Kerr?
- Nuclear Density: What is the equation of state?
- Dark Matter: What is it?
Constituents of the Universe
- Pulsars: A complete census, plus those in other galaxies
- X-ray Binaries: Tying radio and X-rays together
- Giant Stars: Physics and dynamics
- Main Sequence Stars: Their chromospheres and coronae
- Planets: Finding planets of other stars
- SETI: Searching for other intelligent civilizations