Conclusions

• Mounting evidence that non-baryonic Dark Matter and Dark Energy exist

• Immediately imply physics beyond the SM

• Dark Matter likely to be TeV-scale physics

• Search for Dark Matter via

  • Collider experiment
  • Direct Search (e.g., CDMS-II)
  • Indirect Search (e.g., ICECUBE)

• Dark Energy best probed by SNAP (LSST?)

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