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The 2017 Nobel Prize in Physics "for decisive contributions to the LIGO detector and the observation of gravitational waves" Peter Berg Department of Science.

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Presentation on theme: "The 2017 Nobel Prize in Physics "for decisive contributions to the LIGO detector and the observation of gravitational waves" Peter Berg Department of Science."— Presentation transcript:

1 The 2017 Nobel Prize in Physics "for decisive contributions to the LIGO detector and the observation of gravitational waves" Peter Berg Department of Science University of Alberta Source:

2 Gravitational waves: Three ingredients
Clocks can tick at different rates (time is relative) Gravitational fields can warp space (space is relative) Accelerating masses keep changing space-time How?

3 We observe time dilation!
Time is relative The speed of light, c, is constant. It has the same value in all reference frames. We observe time dilation!

4 https://physics.aps.org/articles/v9/17
Warping space Gedankenexperiment #1: Equivalence Principle The accelerated observer, or equivalently an observer in a gravitational field, observes bent light trajectories!

5 Time in a gravitational field
Gedankenexperiment #2: Free fall in a gravitational field We observe different time dilation in a gravitational field!

6 Einstein’s field equations of general relativity
“Simple” concept: mass-momentum distribution determines space-time: Equations have “just” the right (relativistic) form! Everything moves according to a minimization principle ⇒ new distribution of matter ⇒ new space-time metric And so forth… Above equations allow for gravitational waves, moving at speed of light & produced by accelerated masses, similar to electro-magnetic waves, moving at c & produced by accelerating charges. Causing minuscule changes in distance of objects (𝟏 in 𝟏𝟎 𝟐𝟐 ) Einstein: “This can never be measured!”

7 Physics Nobel Prize Winners 2017
Reiner Weiss (*1932, Berlin, Germany) PhD from MIT LIGO/VIRGO Collaboration, MIT interferometer, noise reduction, data collection (1/2) Barry Barish (*1936, Omaha, USA) PhD from University of California, Berkeley LIGO/VIRGO Collaboration, Caltech PI & Director, LIGO (Hanford, WA; Livingston, LA); LIGO collaboration (1/4) Kip Thorne (*1940, Logan, USA) PhD from Princeton University LIGO/VIRGO Collaboration, Caltech prediction of signature; wormholes & time travel; Interstellar (1/4)

8 LIGO: Observing gravitational waves
Tiny effect amidst a lot of noise ⇒ gigantic interferometer! Laser Interferometer Gravitational- wave Observatory

9 What was observed first?
14 Sep 2015: (5x by now) Two black holes merging (predicted theoretically) 1.3 billion years ago. Happens very quickly (0.1s). Correlation between several interferometers.

10 What was observed first?
.

11 What is so special about this?
Gravitational waves pass through all matter, electro-magnetic waves do not. ⇒ Looking deeper into space, i.e. further back in time (closer to Big Bang), then currently possible (Cosmic Microwave Background Radiation; 𝑡=380,000 years) Proof of existence of black holes Study new dynamics

12 What is so special about this?
.

13 Observing gravitational waves: The future
Besides several current interferometers (2x USA, x Germany, 1x Italy), there is space: LISA And then there is the Warp Drive…


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