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26 July 2016 Gabella Quarknet 2016 LIGO 1 LIGO, ground-based Gravitational LIGO, ground-based Gravitational Wave Detectors Wave Detectors LIGO Hanford, WA (LHO) LIGO Livingston, LA (LLO) LIGO – Laser Interferometric Gravitational Wave Observatory LSC – LIGO Scientific Collaboration, includes VIRGO (Italy) team, maybe India

LIGO, ground-based Gravitational Wave Detectorsgabellwe/qnweb/quarknet... · Gravitational Wave GW150914 Direct Discovery by LIGO of a gravitational wave announced on 11 February

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Page 1: LIGO, ground-based Gravitational Wave Detectorsgabellwe/qnweb/quarknet... · Gravitational Wave GW150914 Direct Discovery by LIGO of a gravitational wave announced on 11 February

26 July 2016 Gabella Quarknet 2016 LIGO 1

LIGO, ground-based Gravitational LIGO, ground-based Gravitational Wave DetectorsWave Detectors

LIGO Hanford, WA (LHO)

LIGO Livingston, LA (LLO)

LIGO – Laser Interferometric Gravitational Wave ObservatoryLSC – LIGO Scientific Collaboration, includes VIRGO (Italy) team, maybe India

Page 2: LIGO, ground-based Gravitational Wave Detectorsgabellwe/qnweb/quarknet... · Gravitational Wave GW150914 Direct Discovery by LIGO of a gravitational wave announced on 11 February

25 July 2016 Gabella GravWaves 2

Strain Curves from Moore et al. Strain Curves from Moore et al.

Ground-basedSpaced-based

Pulsar Timing Arrays

3e8wavelength, m 3e43e123e161pc 30km

Page 3: LIGO, ground-based Gravitational Wave Detectorsgabellwe/qnweb/quarknet... · Gravitational Wave GW150914 Direct Discovery by LIGO of a gravitational wave announced on 11 February

25 July 2016 Gabella GravWaves 3

Gravitational Wave SpectrumGravitational Wave Spectrum

Page 4: LIGO, ground-based Gravitational Wave Detectorsgabellwe/qnweb/quarknet... · Gravitational Wave GW150914 Direct Discovery by LIGO of a gravitational wave announced on 11 February

26 July 2016 Gabella Quarknet 2016 LIGO 4

Page 5: LIGO, ground-based Gravitational Wave Detectorsgabellwe/qnweb/quarknet... · Gravitational Wave GW150914 Direct Discovery by LIGO of a gravitational wave announced on 11 February

26 July 2016 Gabella Quarknet 2016 LIGO 5

LIGO HardwareLIGO Hardware● LIGO “Test Mass” in 4-element suspension

● LIGO Vacuum Tube

Ref: some hardware images

Page 6: LIGO, ground-based Gravitational Wave Detectorsgabellwe/qnweb/quarknet... · Gravitational Wave GW150914 Direct Discovery by LIGO of a gravitational wave announced on 11 February

26 July 2016 Gabella Quarknet 2016 LIGO 6

LIGO HardwareLIGO Hardware● LIGO “Test Mass” in suspension

● Beam Splitter

Page 7: LIGO, ground-based Gravitational Wave Detectorsgabellwe/qnweb/quarknet... · Gravitational Wave GW150914 Direct Discovery by LIGO of a gravitational wave announced on 11 February

26 July 2016 Gabella Quarknet 2016 LIGO 7

InterferenceInterference● Two arms, slightly different lengths, L and L+∆L, consider the

amplitudes coming together.

● Single amplitude like

● Sum them together for

Page 8: LIGO, ground-based Gravitational Wave Detectorsgabellwe/qnweb/quarknet... · Gravitational Wave GW150914 Direct Discovery by LIGO of a gravitational wave announced on 11 February

25 July 2016 Gabella GravWaves 8

Nature of Gravitational Waves, and Nature of Gravitational Waves, and Of all 10 possible components to h, it simplifies to two polarizations. One with a motion that shrinks (grows) in one direction while growing (shrinking) in the other direction. The other polarization is just rotated by 45 degrees.

Wave headed into the page, Y up, X right.

hplus polarization hcross polarization

Page 9: LIGO, ground-based Gravitational Wave Detectorsgabellwe/qnweb/quarknet... · Gravitational Wave GW150914 Direct Discovery by LIGO of a gravitational wave announced on 11 February

26 July 2016 Gabella Quarknet 2016 LIGO 9

Effect of a perfectly aligned wave on LIGOEffect of a perfectly aligned wave on LIGO

Page 10: LIGO, ground-based Gravitational Wave Detectorsgabellwe/qnweb/quarknet... · Gravitational Wave GW150914 Direct Discovery by LIGO of a gravitational wave announced on 11 February

26 July 2016 Gabella Quarknet 2016 LIGO 10

Page 11: LIGO, ground-based Gravitational Wave Detectorsgabellwe/qnweb/quarknet... · Gravitational Wave GW150914 Direct Discovery by LIGO of a gravitational wave announced on 11 February

26 July 2016 Gabella Quarknet 2016 LIGO 11

Seismic Noise aLIGO and initialSeismic Noise aLIGO and initial

Page 12: LIGO, ground-based Gravitational Wave Detectorsgabellwe/qnweb/quarknet... · Gravitational Wave GW150914 Direct Discovery by LIGO of a gravitational wave announced on 11 February

26 July 2016 Gabella Quarknet 2016 LIGO 12

Pick out the Livingston Peaks in AbovePick out the Livingston Peaks in Above

Pick out the largest peaks, reconstruct thepossible noise.Assumed at t=0 all the modes are in phase.

stra

in,

1e-2

1st

rain

, 1e

-21

0sec 3sec

1sec 1.5sec

3.0

-3.0

Page 13: LIGO, ground-based Gravitational Wave Detectorsgabellwe/qnweb/quarknet... · Gravitational Wave GW150914 Direct Discovery by LIGO of a gravitational wave announced on 11 February

26 July 2016 Gabella Quarknet 2016 LIGO 13

Saulson, Saulson, If Light Waves…If Light Waves…

Ref: Saulson, If Light Waves…, AmJPhys 65, 501 (1997)

● Argues that in the expanding Universe, light continuously experiences the increase in scale by expanding continuously itself.

● NOT the case for a light wave in LIGO...

– The wave filling the cavity IS stretched by the sudden onset of the gravitational wave.

– Light travel time, 2x4km is 27μs,but GW oscillates at 20 Hz, 50ms. ΔLh_0

time

Page 14: LIGO, ground-based Gravitational Wave Detectorsgabellwe/qnweb/quarknet... · Gravitational Wave GW150914 Direct Discovery by LIGO of a gravitational wave announced on 11 February

26 July 2016 Gabella Quarknet 2016 LIGO 14

As the Wave runs through...As the Wave runs through...

bb

ΔL

Page 15: LIGO, ground-based Gravitational Wave Detectorsgabellwe/qnweb/quarknet... · Gravitational Wave GW150914 Direct Discovery by LIGO of a gravitational wave announced on 11 February

26 July 2016 Gabella Quarknet 2016 LIGO 15

Saulson, Saulson, If Light Waves…,If Light Waves…, says rods are says rods are still rigid!still rigid!

Page 16: LIGO, ground-based Gravitational Wave Detectorsgabellwe/qnweb/quarknet... · Gravitational Wave GW150914 Direct Discovery by LIGO of a gravitational wave announced on 11 February

26 July 2016 Gabella Quarknet 2016 LIGO 16

Strain Curve, Strain Sensitivity, Strain Curve, Strain Sensitivity, Amplitude Spectral Density, Power Amplitude Spectral Density, Power

Spectral Density...OH MY!Spectral Density...OH MY!

“per root Hz” is usually called the strain sensitivity, or sometimes amplitude spectral sensitivity

Page 17: LIGO, ground-based Gravitational Wave Detectorsgabellwe/qnweb/quarknet... · Gravitational Wave GW150914 Direct Discovery by LIGO of a gravitational wave announced on 11 February

26 July 2016 Gabella Quarknet 2016 LIGO 17

Strain Curve, etc...Strain Curve, etc...

square root of Power Spectral Density, really amplitude spectral density

Characteristic Strain, just h

Ref: Cole,s online app .

Page 18: LIGO, ground-based Gravitational Wave Detectorsgabellwe/qnweb/quarknet... · Gravitational Wave GW150914 Direct Discovery by LIGO of a gravitational wave announced on 11 February

26 July 2016 Gabella Quarknet 2016 LIGO 18

Strain Curve, etc...Strain Curve, etc...

bb

Power spectral Density

Page 19: LIGO, ground-based Gravitational Wave Detectorsgabellwe/qnweb/quarknet... · Gravitational Wave GW150914 Direct Discovery by LIGO of a gravitational wave announced on 11 February

25 July 2016 Gabella GravWaves 19

LinksLinks LIGO Scientific Collaboration, LSCLIGO Document ServerCalTech GW media assets page. Kelly Holley-Bockelman’s TEDx Nashville Talk 2016 about GW150914. Pulsar timing array, Nanograv

Page 20: LIGO, ground-based Gravitational Wave Detectorsgabellwe/qnweb/quarknet... · Gravitational Wave GW150914 Direct Discovery by LIGO of a gravitational wave announced on 11 February

26 July 2016 Gabella Quarknet 2016 LIGO 20

BackupBackup

Page 21: LIGO, ground-based Gravitational Wave Detectorsgabellwe/qnweb/quarknet... · Gravitational Wave GW150914 Direct Discovery by LIGO of a gravitational wave announced on 11 February

26 July 2016 Gabella Quarknet 2016 LIGO 21

LIGO InteferometerLIGO Inteferometer

● 4km long

Page 22: LIGO, ground-based Gravitational Wave Detectorsgabellwe/qnweb/quarknet... · Gravitational Wave GW150914 Direct Discovery by LIGO of a gravitational wave announced on 11 February

26 July 2016 Gabella Quarknet 2016 LIGO 22

Units?Units?

Page 23: LIGO, ground-based Gravitational Wave Detectorsgabellwe/qnweb/quarknet... · Gravitational Wave GW150914 Direct Discovery by LIGO of a gravitational wave announced on 11 February

26 July 2016 Gabella Quarknet 2016 LIGO 23

SI PrefixesSI Prefixes

Page 24: LIGO, ground-based Gravitational Wave Detectorsgabellwe/qnweb/quarknet... · Gravitational Wave GW150914 Direct Discovery by LIGO of a gravitational wave announced on 11 February

26 July 2016 Gabella Quarknet 2016 LIGO 24

Gravitational Wave GW150914Gravitational Wave GW150914

Direct Discovery by LIGO of a gravitational wave announced on 11 February 2016 for a wave on 14 September 2015---event labeled GW150914.

SNR = 24, 5 sigma detection!

Pretty after filtering out the known seismic frequencies.

Page 25: LIGO, ground-based Gravitational Wave Detectorsgabellwe/qnweb/quarknet... · Gravitational Wave GW150914 Direct Discovery by LIGO of a gravitational wave announced on 11 February

26 July 2016 Gabella Quarknet 2016 LIGO 25ref: http://www.techinsider.io/binary-black-holes-confirmed-gravitional-waves-2016-2

Merging Black HolesMerging Black Holes

Page 26: LIGO, ground-based Gravitational Wave Detectorsgabellwe/qnweb/quarknet... · Gravitational Wave GW150914 Direct Discovery by LIGO of a gravitational wave announced on 11 February

26 July 2016 Gabella Quarknet 2016 LIGO 26

Schematic, Map, and NoiseSchematic, Map, and Noise

Page 27: LIGO, ground-based Gravitational Wave Detectorsgabellwe/qnweb/quarknet... · Gravitational Wave GW150914 Direct Discovery by LIGO of a gravitational wave announced on 11 February

25 July 2016 Gabella GravWaves 27

GW strain for Circular OrbitGW strain for Circular Orbit

● rs1 is 2GM_1/c^2, Schwarzschild radius for mass M_1, etc.

● r is distance from Earth to system.● R is the separation of the two bodies.

ref: Maggiore around Eqn. 3.332.

Page 28: LIGO, ground-based Gravitational Wave Detectorsgabellwe/qnweb/quarknet... · Gravitational Wave GW150914 Direct Discovery by LIGO of a gravitational wave announced on 11 February

25 July 2016 Gabella GravWaves 28

Some ConstantsSome Constants

Schwarzschild radius 2GM/c^2 2953 m for Msun

GR Units, Mass GM/c^2 1477 m for Msun

GR Units, Power c^5/G 3.628e52 W

GR Units, Energy c^4/G 1.210e44 J/m

parsec, pc 3.09e16 m = 3.262 ly

astronomical unit, au 149.6e9 m

light-year, ly 0.946e16 m = 0.307 pc

fine structure constant e^2/(4pi eps0)/hbar c 0.00730 = 1/137.04

wavelength-energy h c 1.24 eV μm