Differences between revisions 2 and 8 (spanning 6 versions)
⇤ ← Revision 2 as of 2007-08-07 22:44:00 →
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Editor: RobertWard
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Editor: RobertWard
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 * Multi-color interferometers  * Multi-color (multi-springy) interferometers (maybe this is only 2.5G)
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 * local readout techniques  * [[local readout techniques]]
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 * VRSM

 * super-seismic cancellation (feed-forward from seismometers, gravity gradient cancellation)

 * [[white light signal cavities]]

Here we'll list and describe ideas for testing 3rd generation (i.e., beyond Advanced LIGO) interferometric techniques at the 40m.

  • Multi-color (multi-springy) interferometers (maybe this is only 2.5G)
  • Sloshing cavities
  • Long signal cavities
  • speed-meter interferometers

  • local readout techniques

  • injecting squeezed vacuum
  • VRSM
  • super-seismic cancellation (feed-forward from seismometers, gravity gradient cancellation)

  • white light signal cavities

3G@40M (last edited 2012-01-03 23:02:41 by localhost)