Einsteins Happiest Thought Microworld MacroWorld Lecture 7 Equivalence

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Einstein’s Happiest Thought Micro-world Macro-World Lecture 7

Einstein’s Happiest Thought Micro-world Macro-World Lecture 7

Equivalence between gravity & acceleration a Man in a closed box on Earth m

Equivalence between gravity & acceleration a Man in a closed box on Earth m Gg g Since m. G=m. I, if a=-g, the conditions are equivalent m. Ia Man in a closed box on an accelerating rocket in deep outer space.

The happiest thought I cannot tell the difference between being on earth or in

The happiest thought I cannot tell the difference between being on earth or in a deep-space rocket accelerating with a=-g

Imagination This cannot be due to coincidence. There must be some basic truth involved.

Imagination This cannot be due to coincidence. There must be some basic truth involved.

Einstein didn’t accept m. G=m. I as a coincidence These two environments must be

Einstein didn’t accept m. G=m. I as a coincidence These two environments must be exactly equivalent.

Einstein Equivalence Principle in his words we [. . . ] assume the complete

Einstein Equivalence Principle in his words we [. . . ] assume the complete physical equivalence of a gravitational field and a corresponding acceleration o the reference system [Einstein, 1907]

So what? What would happen if I were to shine a light beam through

So what? What would happen if I were to shine a light beam through a window on the rocket? sra igh t lin e

If the rocket is accelerating, the light beam bends ½at 2

If the rocket is accelerating, the light beam bends ½at 2

L Since the accelerating rocket and gravity are equivalent, gravity must cause light to

L Since the accelerating rocket and gravity are equivalent, gravity must cause light to bend on Earth’s surface ½gt 2 for our room L≈6 m: very, very tiny effect

Does gravity cause light to bend? Very tiny effect: need very strong gravity and

Does gravity cause light to bend? Very tiny effect: need very strong gravity and a long lever arm. Look at the bending of light from a star by the Sun. (Only possible at an eclipse. ) Sir Arthur Eddington 1882 -1944 gsun ≈ 27 xgearth

Eddington’s 1919 Expeditions

Eddington’s 1919 Expeditions

1919 Eclipse Africa 1919 eclipse Measurement: q =0. 000550± 0. 000030 in agreement with

1919 Eclipse Africa 1919 eclipse Measurement: q =0. 000550± 0. 000030 in agreement with Einstein’s prediction

New York Times:

New York Times:

Gravitational lensing

Gravitational lensing

“Dark Matter” astronomy

“Dark Matter” astronomy

Mass induces curvature in space-time

Mass induces curvature in space-time

The curvature is what we feel as gravity

The curvature is what we feel as gravity

Seou l 120 Ri o

Seou l 120 Ri o

Cartesian vs non-Cartesian coords 170 ul o e S io R

Cartesian vs non-Cartesian coords 170 ul o e S io R

The Earth is round 170 ? ? This is how KAL goes

The Earth is round 170 ? ? This is how KAL goes

Geodesics The shortest distance between 2 points is Along a “geodesic. ” It is

Geodesics The shortest distance between 2 points is Along a “geodesic. ” It is a straight line In Cartesian systems

Great Circles spherical geometry The shortest distance between two points on the Earth’s surface

Great Circles spherical geometry The shortest distance between two points on the Earth’s surface correspond to “Great Circles”: the intersections of planes passing through the center of the Earth with the Earth’s surface.

In this figure, the shortest distances are indicated by the blue lines.

In this figure, the shortest distances are indicated by the blue lines.