·
1879-1953
In
1905 Einstein published papers on:
·
Brownian
motion. This is an animation of Einstein’s explanation.
·
The
Photo-Electric Effect – An oversimplified cartoon-like explanation, but it
gets the main idea across.
·
light
knocking electrons out of matter This is a bit more staid and informative,
but still not too technical.
·
He received the Nobel Prize for this
·
His doctoral thesis
·
and most importantly, “On the
Electrodynamics of Moving Bodies” – the paper that launched Special
Relativity. This is the actual paper, translated into English. In case you are
interested.
What’s so
special about Special Relativity?
.
Energy
·
Mass
and energy are not independent concepts.
·
When a body radiates energy of amount e it loses mass by an amount e/c2
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Therefore, in principle m = e/c2
·
Or more familiarly, e = mc2
·
Special Relativity concerns frames of reference that move inertially with respect to each other.
·
This is a special case.
·
All motion that is not
inertial is accelerated.
Acceleration
and Gravity
·
In
·
Acceleration is perceived as an effect on inertial mass due to a
force impressed.
·
Viz.,
·
Inertial mass is measured as resistance to change of motion
(acceleration).
·
Gravitational mass is measured as attraction between bodies, causing
acceleration.
·
But inertial mass = gravitational mass.
·
Inertial and gravitational mass are equal in value and ultimately
measured by the same effect: acceleration.
·
The Positivist viewpoint: Acceleration and gravity must be equivalent.
·
Einstein’s thought experiment
·
Look for a case where acceleration and gravity should produce different
effects according to classical (i.e., Newtonian) physics.
Einstein’s
Elevator, another
site
·
In a closed elevator,
acceleration feels like gravity.
·
Therefore, gravity should do the same to light as acceleration does,
namely pull it toward the attracting mass.
A
Real Experiment – The Angular
distance between two stars
·
Einstein’s thought experiment points out the anomaly in the theory but
is not testable as conceived because the distances are too short and the speed
of light too fast.
·
The only practical way to test this hypothesis is with an astronomical
event.
·
Consider two stars that can be observed (at night) and the angular
distance between them measured.
·
Were it possible to see the stars in the daytime, the light travelling from them should be bent by the gravitational
pull of the sun. The result would be that the stars would seem to be farther
apart in the daytime than at night.
·
During a complete solar eclipse, the sky is dark enough to see the
stars, but the sun lies in the path between the stars and the earth.
·
Einstein predicted that the starlight would be bent by 1.7 seconds of
arc. In 1919, Sir Arthur Eddington confirmed that result. Details of Eddington’s analysis.
·
This is when Einstein became know to the public as Mr. Genius.
Another
confirmation of General Relativity:
·
General Relativity “postdicts” the otherwise
unexplained advance of the perihelion
of Mercury by 43 seconds per century.