Differences between revisions 3 and 9 (spanning 6 versions)
Revision 3 as of 2007-11-16 01:13:12
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Editor: RobertWard
Comment:
Revision 9 as of 2012-01-03 23:02:41
Size: 506
Editor: localhost
Comment: converted to 1.6 markup
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 * Multi-color interferometers (maybe this is only 2.5G)  * 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)