strawman red caltech - physics.gla.ac.uk

Post on 19-May-2022

13 Views

Category:

Documents

0 Downloads

Preview:

Click to see full reader

TRANSCRIPT

Overview

Stefan Hild Slide 2 Strawman Caltech, Jan 2012

Task description

Stefan Hild Slide 3 Strawman Caltech, Jan 2012

Some working assumptions

Stefan Hild Slide 4 Strawman Caltech, Jan 2012

To avoid misunderstandings …

Stefan Hild Slide 5 Strawman Caltech, Jan 2012

Suspension Thermal Noise

  Boosted aLIGO Quad with 1.2m long last stage and 160kg test masses.

Stefan Hild Slide 6 Strawman Caltech, Jan 2012

Suspension Thermal Noise

Stefan Hild Slide 7 Strawman Caltech, Jan 2012

Suspension R&D

Stefan Hild Slide 8 Strawman Caltech, Jan 2012

Newtonian Noise

Stefan Hild Slide 9 Strawman Caltech, Jan 2012

Used seismic from:

Newer data from LLO

Stefan Hild Slide 10 Strawman Caltech, Jan 2012

New data from LLO seem to suggest that Strawman red underestimates the GGN level by about a factor 2. Work in progress!

Seismic barrages

  2D finite-difference time-domain simulations for barrages of 40x40m.

  Attenuation of seismic by about a factor 2.

Stefan Hild Slide 11 Strawman Caltech, Jan 2012

Coating Brownian noise

Stefan Hild Slide 12 Strawman Caltech, Jan 2012

Increasing the beam size

  Assume an increase of beam size by a factor 1.6.

  Keep aspect ratio of test masses as it is => 160kg.

Stefan Hild Slide 13 Strawman Caltech, Jan 2012

Optical coatings with reduced thermal noise

 Continued improvement of tantala coatings.   Loss related to local atomic structure of material

 High-temperature annealing of coatings.   Heat treatment in the range of 500-1000 degrees centigrade

 Amorphous silicon as a high-index coating material   n=3.5 => quarter-wave layer is thinner. In addition need fewer layers.   Potential improvement = 4.6   Requires change of laser wavelength

 Crysatalline coatings (AlGaAs)

Stefan Hild Slide 14 Strawman Caltech, Jan 2012

Khalili cavities

Stefan Hild Slide 15 Strawman Caltech, Jan 2012

Khalili cavities

 Extremely hardware intensive.

 Lots of technical challenges:   Thermal lensing   Cavity stability   Control

Stefan Hild Slide 16 Strawman Caltech, Jan 2012

Thermal lensing in K-cavity

Stefan Hild Slide 17 Strawman Caltech, Jan 2012

Waveguide mirrors

Stefan Hild Slide 18 Strawman Caltech, Jan 2012

Quantum noise

Stefan Hild Slide 19 Strawman Caltech, Jan 2012

Squeezing losses

Stefan Hild Slide 20 Strawman Caltech, Jan 2012

= 9% in total

Cavity losses in literature

Assuming losses are independent of cavity length

Speedmeter an alternative?

Stefan Hild Slide 21 Strawman Caltech, Jan 2012

Strawman Red Costs

Stefan Hild Slide 22 Strawman Caltech, Jan 2012

sthild
Rectangle
Cost are removed from this public version.If you are an LSC member you can find the full slides at LIGO-T1200005-v2
sthild
Rectangle
sthild
Rectangle
sthild
Rectangle

Stefan Hild Slide 23 Strawman Caltech, Jan 2012

sthild
Rectangle
Cost are removed for the public version. If you are an LSC member you can find the cost in LIGO-T1200005-v2

Stefan Hild Slide 24 Strawman Caltech, Jan 2012

sthild
Rectangle
Costs removed for public version. If you are an LSC member you can find the cost is LIGO-T1200005-v2
sthild
Rectangle

Overview

Stefan Hild Slide 25 Strawman Caltech, Jan 2012

 For details please see document on the DCC:

 https://dcc.ligo.org/cgi-bin/private/DocDB/ShowDocument?docid=78100

Stefan Hild Slide 26 Strawman Caltech, Jan 2012

top related