Gravity Gradient Noise from Ground Waves

Wm. Robert Johnston
University of Texas at Brownsville
johnston@phys.utb.edu

LIGO Livingston SURF presentation
31 July 2002
supported by CIRE (NSF)



Outline

    I. Project plan

   II. Description of gravity gradient

  III. Description of ground waves

  IV. Previous data and estimates for LLO

   V. Description of model

  VI. Model results to date



Project plan

theoretical experimental
1. characterize Rayleigh waves
2. model ground motion from waves
3. model gravity gradient from waves
4. relate to LIGO noise spectrum
1. review equipment and software
2. prepare seismometers
3. deploy seismometers
4. gather data
combined
1. use model to find gravity gradient from observed ground motion
2. characterize gravity gradient noise for LIGO-Livingston

Supervisor: Mark Coles
Team members: William Quarles, Michael Cheung



Gravity gradient--any nonuniform component of the gravitational field.

On the Earth, both the magnitude and direction of gravitational acceleration varies due to:

There is also an apparent gradient due to the Earth's rotation for observers in the rotating
frame of reference.

Gravitational wave observations can be affected by time-dependent gravity gradients from:

This is a concern for interferometers more than for resonant bar detectors.



Examples of gravity gradient noise sources

Ground waves from seismic noise (Hughes and Thorne, 1998, gr-qc/9806018)
People walking near test masses (Thorne and Winstein, 1999, gr-qc/9810016)
Tumbleweeds blown into side of buildings (Creighton, 2001, gr-qc/0007050)



Types of seismic waves

body waves P waves (pressure, primary, longitudinal)
S waves (shear, secondary, transverse)
surface waves Rayleigh waves (vertical and longitudinal)
Love waves (transverse horizontal)
interface waves Stonley waves
free oscillations torsional oscillations
spheroidal oscillations

(wave illustrations from Fowler, The Solid Earth, 1990, 1992)



Rayleigh waves are the greatest concern in terms of producing gravity
gradient noise, since they fall off more slowly with distance than body waves and
represent most seismic energy from localized surface sources.

Rayleigh wave properties







LLO ground characteristics

source depth (m) Poisson's ratio CP (m/s) CS (m/s) CH (m/s)
LIGO survey (1995) 2
5
15
0.4 213
247
293
Hughes & Thorne (model, 1998) 0-5
5-105
105-905
905-3005
0.33
0.47
0.40
0.31
440
1660
1700
1900
220
400
700
1000
205
360
660
930
Coles (2001) shallow 0.48 1780 368-379 335



Existing estimates of gravity gradient noise for LIGO

Saulson, 1994

Hughes and Thorne, 1998, gr-qc/98061018



Elements of current model:

Expression for gravity gradient:

Strain from simulated gravity gradient (acceleration) amplitude:

where L = arm and B = transfer function





© 2002 by Wm. Robert Johnston.
Last modified 3 October 2002.
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