LIGO -- Studying the Fabric of the Universe - PowerPoint PPT Presentation

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LIGO -- Studying the Fabric of the Universe

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by gravitational radiation at the speed of light. Gmn= 8pTmn. 17-Feb-03. AAAS Annual Meeting ... their sources as a space-time warpage at the speed of light ... – PowerPoint PPT presentation

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Title: LIGO -- Studying the Fabric of the Universe


1
LIGO -- Studying the Fabric of the Universe
Barry C. BarishNational Science BoardLIGO
Livingston, LA4-Feb-04
LIGO-GOxxxx
2
A Conceptual Problem is solved !
Newtons Theory instantaneous action at a
distance
Gmn 8pTmn
Einsteins Theory information carried by
gravitational radiation at the speed of light
3
General Relativity
Einstein theorized that smaller masses travel
toward larger masses, not because they are
"attracted" by a mysterious force, but because
the smaller objects travel through space that is
warped by the larger object
  • Imagine space as a stretched rubber sheet.
  • A mass on the surface will cause a deformation.
  • Another mass dropped onto the sheet will roll
    toward that mass.

4
Einsteins Theory of Gravitation
  • a necessary consequence of Special Relativity
    with its finite speed for information transfer
  • gravitational waves come from the acceleration
    of masses and propagate away from their sources
    as a space-time warpage at the speed of light

gravitational radiation binary inspiral of
compact objects
5
Detecting Gravitational Waves
Gravitational Wave Astrophysical Source
Terrestrial detectors Virgo, LIGO, TAMA, GEO AIGO
Detectors in space LISA
6
Frequency range for EM astronomy
  • Electromagnetic waves
  • over 16 orders of magnitude
  • Ultra Low Frequency radio waves to high energy
    gamma rays

7
Frequency range of GW Astronomy
Audio band
  • Gravitational waves
  • over 8 orders of magnitude
  • Terrestrial space detectors

Space
Terrestrial
8
Detecting a passing wave .
Free masses
9
Detecting a passing wave .
Interferometer
10
Interferometer Concept
  • Laser used to measure relative lengths of two
    orthogonal arms
  • Arms in LIGO are 4km
  • Measure difference in length to one part in 1021
    or 10-18 meters

causing the interference pattern to change at
the photodiode
Suspended Masses
11
Simultaneous DetectionLIGO
Hanford Observatory
MIT
Caltech
Livingston Observatory
12
Gravitational Wave Astronomy
LIGO will provide a new way to view the dynamics
of the Universe
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