Diff for "Balanced Homodyne Detection"

Differences between revisions 2 and 4 (spanning 2 versions)

Noise Budget

Simple BHD

BHD detection of a simple Michelson

BHD detection of the full 40m Interferometer

Requirements

1. Displacement noise of OMC/LMC mirrors 1. Scatter loss in mirrors 1. Cavity design: triangle, quad ring, quad zig-zag (reference the new OMC paper from Koj) 1. Laser amplitude / frequency noise including DC offsets in various other lock points and motions to simulate bilinear noise 1. Oscillator noise: AM / FM 1. Aux length noise: MICH/PRC/ SRC 1. Req. on offsets/asymmetries: arm finesse, arm reflectivity, mass imbalance of ETMs

-  ⇤ ← Revision 2 as of 2017-10-27 04:50:45 → 
  Size: 14
  Editor: KevinkunsATligoDOTorg
  Comment:
+   ← Revision 4 as of 2017-10-27 23:50:52 → ⇥
  Size: 621
  Editor: RanaadhikariATligoDOTorg
  Comment:
-Deletions are marked like this.
+Additions are marked like this.
 Line 1:
-Noise Budget
+=== Noise Budget ===

==== Simple BHD ====

==== BHD detection of a simple Michelson ====

==== BHD detection of the full 40m Interferometer ====

==== Requirements ====
1. Displacement noise of OMC/LMC mirrors
1. Scatter loss in mirrors
1. Cavity design: triangle, quad ring, quad zig-zag (reference the new OMC paper from Koj)
1. Laser amplitude / frequency noise including DC offsets in various other lock points and motions to simulate bilinear noise
1. Oscillator noise: AM / FM
1. Aux length noise: MICH/PRC/ SRC
1. Req. on offsets/asymmetries: arm finesse, arm reflectivity, mass imbalance of ETMs