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Gravity Waves Gravity Waves

Gravity Waves - PowerPoint Presentation

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Gravity Waves - PPT Presentation

Dennis Stewart November Smu Modern Physics 1 Outline for this talk Einstein Einsteins Contribution Joseph Weber LIGO The Machine and How it works The Chrip Conclusion 2 Albert Einstein ID: 556408

waves org light measurements org waves measurements light physics gravitational ligo iop http aps wave iopscience einstein distance signal

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Slide1

Gravity Waves

Dennis Stewart

NovemberSmuModern Physics

1Slide2

Outline for this talk

Einstein

Einsteins Contribution

Joseph Weber

LIGO

The Machine and How it works

The ChripConclusion

2Slide3

Albert Einstein

German Born Theoretical Physicist (1879-1955)

Developed the General Theory of RelativityBest known for his mass energy equivalent principle E=mc^2

3Slide4

A 100 year old prediction thanks to GR

Developed between 1907 and 1915

Explains the cause of space-time warpingGravitational waves were predicted in 1916 as ‘ripples’

4Slide5

Joseph Weber

Studied gravitational radiation

Developed ‘Weber Bars’ in the 60’sApollo 17 Lunar MissionNever produced solid evidence

5Slide6

6

LIGO

Laser Interferometer Gravitational-Wave ObservatorySlide7

Inside LIGO

To spot a signal, LIGO uses a special mirror to split a beam of laser light and sends the beams down

two 4-kilometer-long arms, at a 90 degree angle to each other. After ricocheting back and forth 400 times, turning each beam’s journey into a

1,600 kilometer round-trip

, the light recombines near its source.

7Slide8

The Signal

Produced by the inspired and merger of the first observation of such black holes Each with a mass 25X greater than our sun which is 1.989 × 10^30 kgTravel at the speed of lightstretching spacetime in the plane perpendicular to the direction they’re moving in

8Slide9

9

The experiment is designed so that, in normal conditions, the

light waves

cancel

one another out when they recombine,

sending no light signal to the nearby detector.

But a gravitational wave

stretches

one tube while

squeezing

the other, altering the distance the two beams travel relative to each other.

Because of this difference in distance

, the recombining

waves are no longer perfectly aligned

and therefore don’t cancel out. The detector picks up a faint glow, signaling a passing wave.

How Detection WorksSlide10

10

http://physics.aps.org/assets/8cbf3dfb-7849-485b-8626-1276bc044ddf/video1.mp4Slide11

11

100 Years LaterSlide12

12

Measurements Used

Masses of BlackholesSlide13

13

Measurements Used

Merger RateSlide14

14

Measurements Used

Periastron DistancesSlide15

15

Measurements Used

Maximum luminosity distance (

DL

)

Redshift (

z

)

On the right a measure for the surveyed volume (V[bar]_c) for the initial LIGO/Virgo detectors, the current aLIGO, and future expectationsSlide16

16

The ChirpSlide17

In Closing

For the first time we have observational evidence that BBH systems actually form in nature, with properties such that they merge in the local universe.

We are looking forward to the development of GW astronomy as a new way of probing the universe.17Slide18

18

The End!Slide19

Sources

http://www.nature.com/news/einstein-s-gravitational-waves-found-at-last-1.19361

http://physics.aps.org/articles/v9/17http://iopscience.iop.org/article/10.3847/2041-8205/818/2/L22/meta;jsessionid=9B49F1CD55E9BBF9ADD8F5261D7C3DB4.c1.iopscience.cld.iop.org\http://iopscience.iop.org/article/10.1088/0264-9381/32/7/074001/metal

https://physics.aps.org/story/v16/st19

19