a recap of the main points so far… observers moving uniformly with respect to each other

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A recap of the main points so far… Observers moving uniformly with respect to each other • do not agree on time intervals or distance intervals • do not agree about the simultaneity or otherwise of events A moving clock appears to run slow – time dilation A moving ruler appears short – length contraction •A moving object has an increased relativistic mass

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A recap of the main points so far… Observers moving uniformly with respect to each other do not agree on time intervals or distance intervals do not agree about the simultaneity or otherwise of events A moving clock appears to run slow – time dilation - PowerPoint PPT Presentation

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Page 1: A recap of the main points so far… Observers moving uniformly with respect to each other

A recap of the main points so far…

Observers moving uniformly with respect to each other

• do not agree on time intervals or distance intervals

• do not agree about the simultaneity or otherwise of events

A moving clock appears to run slow – time dilation

A moving ruler appears short – length contraction

•A moving object has an increased relativistic mass

•Mass can be converted into energy (and vice-versa)

E = m c2

Page 2: A recap of the main points so far… Observers moving uniformly with respect to each other

The Twins Paradox

Page 3: A recap of the main points so far… Observers moving uniformly with respect to each other

Symmetry

As far as the observer on the spaceship is concerned, a clock left on Earth is running slow and lengths are contracted in the direction of motion.

As far as the observer on Earth is concerned, a clock on the spaceship is running slow and lengths are contracted in the direction of motion.

The frames of reference are equivalent?

Page 4: A recap of the main points so far… Observers moving uniformly with respect to each other

Hammer and feather on the moon

Page 5: A recap of the main points so far… Observers moving uniformly with respect to each other

Underlying principles of General Underlying principles of General RelativityRelativity

The Equivalence Principle

No difference between a steady acceleration and a gravitational field

Page 6: A recap of the main points so far… Observers moving uniformly with respect to each other

Gravity and Acceleration cannot be distinguished

Page 7: A recap of the main points so far… Observers moving uniformly with respect to each other

h

V = a h/c

Page 8: A recap of the main points so far… Observers moving uniformly with respect to each other

h Gravitational field

Equivalence principle – this situation should be the same

Page 9: A recap of the main points so far… Observers moving uniformly with respect to each other

Consequences I. Gravitational Redshift

Size of effect (doppler shift equivalent speed)

Earth 0.2 m/s

Sun 0.6 km/s

White Dwarf 70 km/s

Neutron Star 100,000 km/s

Black-hole infinite

Page 10: A recap of the main points so far… Observers moving uniformly with respect to each other

Gravitational redshift of Sirius B

Equivalent velocity 80 km/s

Page 11: A recap of the main points so far… Observers moving uniformly with respect to each other

Corrections to GPS

Orbital radius 26,000 km

gh/c2 = 0.0000000026

Clocks “on the ground” would lose about 0.2 ms per day (actually a bit less).

Clocks on the GPS satellites run intentionally slowly!

Page 12: A recap of the main points so far… Observers moving uniformly with respect to each other
Page 13: A recap of the main points so far… Observers moving uniformly with respect to each other
Page 14: A recap of the main points so far… Observers moving uniformly with respect to each other
Page 15: A recap of the main points so far… Observers moving uniformly with respect to each other

Lensing of distant galaxies by a foreground cluster

Page 16: A recap of the main points so far… Observers moving uniformly with respect to each other
Page 17: A recap of the main points so far… Observers moving uniformly with respect to each other
Page 18: A recap of the main points so far… Observers moving uniformly with respect to each other

QSO 2237+0305

The Einstein cross

Page 19: A recap of the main points so far… Observers moving uniformly with respect to each other

Abell 1689

Plus derived

Mass Map

Page 20: A recap of the main points so far… Observers moving uniformly with respect to each other

Galaxies at 3, 6 and 11 billion light years away

Einstein Rings

Page 21: A recap of the main points so far… Observers moving uniformly with respect to each other
Page 22: A recap of the main points so far… Observers moving uniformly with respect to each other