WEBVTT

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In nineteen oh five, Einstein published
special relativity, and at its centre

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is a speed limit: no influence
of any kind travels faster than light.

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Ten years later he
published a theory of gravity.

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If you had to compress
that theory into three words,

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they would be: not even gravity.

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This is where we are going.

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It is the equation Einstein
arrived at in nineteen fifteen.

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The left hand side is a quantity that is
zero when spacetime is flat and not zero

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when spacetime is curved.

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The right hand side is matter and energy.

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You do not have to read it yet.

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Everything between here

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and there is Newton, one coincidence that
Newton himself noticed and shrugged at,

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and one change of mind
about what a straight line is.

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Here is the Sun,

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here is the Earth, and this arrow
is the pull the Sun exerts on it.

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Newton's law of gravity says
that pull is his constant,

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times one mass, times the other, divided
by the distance between them squared.

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Now jiggle the Sun.

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Read that formula literally:

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the instant the separation changes, the
force out at the Earth changes with it.

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Not eight minutes later.

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Now.

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But light itself takes eight
minutes to cross that gap.

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Watch a flash leave the Sun and reach us.

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Newton's force beat that flash across,

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which is exactly what
the speed limit forbids.

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One of the two has to give.

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Einstein had spent years hunting down
every way of sending a signal faster

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than light, and he was not about
to allow a gravitational telephone.

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So the law that has to change is Newton's.

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There is a precedent
for repairing an inverse square law.

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Electricity has one
of exactly the same shape:

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a constant, times one charge, times
the other, over the separation squared.

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Maxwell had already dressed
that law up properly.

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Once the charges move,

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magnetic effects appear, and the whole
package obeys the speed limit exactly.

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So copy the trick for gravity and be done.

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Two like charges push each other apart.

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Two masses pull each other together.

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Copy the electric calculation exactly

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and you get the electric answer, which is
that the Sun would shove the Earth away.

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There is the difference,
and it is one character wide.

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A plus on this side, a minus on that one.

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That single character is why gravity
cannot simply be copied from electricity.

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The reason lies in the messenger.

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The electric force is carried
by a particle of spin one, the photon.

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Gravity is carried
by a particle of spin two.

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That difference is exactly
the difference in sign.

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So Einstein could not copy.

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He had to find another route,

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and he had one clue: a coincidence sitting
in the middle of Newton's own equations.

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Look again at the two laws,
and at the letter m in each of them.

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In Newton's second law,

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the mass measures stubbornness: how
hard the body fights being accelerated.

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That is the inertial mass.

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In the law of gravity, the mass
measures something else entirely:

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how firmly gravity takes hold of the body.

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That is a completely different job,
and it is called the gravitational mass.

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In electricity those two jobs
are done by two unrelated numbers.

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A neutron is heavy
and carries no charge at all.

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An electron is light
and carries a full unit of it.

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So there is no relation whatsoever

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between how much a particle weighs and
how strongly it feels an electric field.

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Now watch what gravity does.

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In gravity, the number that resists

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and the number that gets pulled
are the same number. Not nearly the same.

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The same.

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That statement is the equivalence
principle, and here is what it does.

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Drop a brick and a feather

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in a vacuum chamber, with no
air to slow either one down.

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Gravity pulls the brick harder, because
the brick has more gravitational mass.

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The brick also resists harder,
because it has more inertial mass.

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The two effects cancel exactly,
and the two bodies fall together.

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Newton noticed this himself.

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He ran experiments on it,

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and found the two masses agreeing
to roughly one part in a thousand.

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By Einstein's day the agreement
was one part in a billion.

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Today it is one part
in ten to the fifteen,

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which makes it one of the most precisely
tested statements in all of physics.

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In Newton's physics
this is a pure coincidence.

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Two unrelated quantities,

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agreeing to fifteen decimal places,
for no reason anybody could give.

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Einstein refused
to accept that as an accident.

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Here is the other half of Einstein's clue.

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A bucket of water on a rope,
swung in a vertical loop.

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Down at the bottom nothing is mysterious:

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gravity pulls the water
into the base of it.

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Swing it fast enough and the water stays
put at the top, upside down though it is.

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Ride along with the water
and there is a second account of why.

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From inside, something presses the water
outward, into the base of the bucket.

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We call that the centrifugal force.

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It is not a real force.

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Nothing is pushing.

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It appears only because the frame you
chose to describe things in is spinning,

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and its size is your speed squared
over the radius, times your mass.

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And look which mass that is.

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Not some new centrifugal charge.

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It is the inertial mass, the very same
stubbornness from Newton's second law.

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Here, though, that is no coincidence.

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It could not have come out any other way.

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The reason you feel pressed outward
is precisely that your body wants

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to keep going straight.

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Inertia is the whole cause,
so inertia is the whole charge.

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So write two facts side by side.

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Any inertial force, by construction,
couples to the inertial mass.

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And gravity, as we measured
to fifteen decimal places,

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couples to the inertial mass as well.

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Which raises the question Einstein
called the happiest thought of his life.

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What if gravity is an inertial force?

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Not a force at all, but the price
of describing motion in the wrong frame.

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That guess is even permitted only
because the two masses are equal.

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Try the same move on electricity and it

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collapses at once, because electric charge
is nothing whatsoever like inertial mass.

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But it sounds mad,
and here is exactly why.

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An inertial force is what you feel when
you are not moving along a straight line.

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Move along a straight line
and you feel nothing at all.

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So if gravity is one of those,
then the astronaut floating in orbit,

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feeling nothing,
is the one going straight.

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And you, held up by your chair,
feeling that push in your back, are not.

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Which means we are about
to be very wrong about straight lines.

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Here is a graph of height
above the ground against time.

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This flat line is you,

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sitting in your chair, staying
at the same height while time runs on.

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And this arc is a piece of chalk,
thrown up and caught again.

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The chalk is in free fall
the whole way, so it feels nothing,

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while you feel the chair pressing
into your back the entire time.

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If gravity is an inertial force,

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then the chalk is the one travelling
in a straight line, and you are not.

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Drawn like this, that is plainly absurd.

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One of them is straight,
the other is bent, and I can see which.

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Unless the picture is lying to us.

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Which is a thing that pictures do.

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You have met this exact lie on an
aeroplane. Here is the map on the seat

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in front of you, with San Francisco
on the left and London on the right.

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The obvious shortest route
is the dashed line straight across.

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But the aircraft flies
the red one, up over Greenland,

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which on this map looks
like a wasteful detour.

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Now put the same two cities
on the actual Earth, which is a sphere.

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The shortest path between two points
on a sphere is an arc of a great circle.

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Here is that arc,

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and it does run up over the north,
exactly where the airline said it would.

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The detour was never a detour. The flat
map bent it, because that map is trying

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to draw a curved Earth on a flat page,
and something always has to give.

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What gives is your idea
of which lines are straight.

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Now back to our graph,
with the same accusation.

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That picture drew time
and height on a flat grid.

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Spacetime is not flat: matter curves it.

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On the curved thing,

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the arc is the straight line,
and the level line is the bent one.

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So the astronaut,
feeling nothing, goes straight.

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You, held up by your chair,

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are being pushed off the straight line,
and the weight you feel is the price.

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Gravity is not a force in the picture.

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It is a property of the picture.

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That leaves exactly one job:

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say precisely how much matter
curves spacetime, and how much.

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It took Einstein eight further years,
and this is the answer he arrived at.

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On the left, the curvature of spacetime.

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On the right, all the matter
and all the energy there is.

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Read it as a slogan:

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matter tells spacetime how to curve, and
curved spacetime tells matter how to move.

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Newton's law of gravity is gone.

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Newton's first law survives, and reads
better than before: with no force on you,

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you travel in a straight line.

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We simply had the wrong lines.

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Curved spacetime has consequences,
and the first is about clocks.

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Here is a mass, here is a clock sitting
close to it, and here is one far away.

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Neither of them is moving.

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The one down low ticks slower.

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Not because of any motion, but because it
sits deeper in the gravitational well.

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The whole effect is this square
root, and it is less than one.

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This has been measured for seventy years.

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Two atomic clocks at two
heights in one building disagree.

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Satellite navigation
has to correct for it,

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or the position it reports
would wander off within minutes.

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And notice that this is not the
symmetric effect of special relativity.

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There, each of two moving observers
sees the other one running slow.

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Here we both agree
who is deeper in the well,

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so we both agree whose
clock is the slow one.

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Now send a photon up
from the low clock to the high one.

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Everything down there looks slow

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from up here, and that includes
the oscillation of a light wave.

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So the light arrives with a lower
frequency than it left with.

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Lower frequency means shifted
toward the red end of the spectrum,

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and it means less energy carried.

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That is the gravitational redshift, and we
see it in light climbing out of the Sun.

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Turn it around,

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and light falling down arrives blue,
carrying more energy than it started with.

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Whatever the exchange rate
is for time between two heights,

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it is also the exchange rate for energy.

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The third consequence is that light bends.

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Here is the Sun, and here is a star far
off to the left, sending a ray past it.

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If gravity did nothing, that ray
would run dead flat along the dashed line.

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It does not.

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The ray is pulled toward the Sun, and the
observer over on the right, looking back

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along the direction it arrives from, sees
the star shifted away from the Sun's edge.

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Treat light as a fast particle

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and Newton's gravity predicts
a deflection of two G M over c squared b.

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Einstein's theory predicts four.

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Exactly twice as much.

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That factor of two was testable, if only
you could see stars right beside the Sun.

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You cannot, except during a total eclipse,

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when the Moon covers the disc
and the sky beside it goes dark.

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Eddington's expedition of nineteen
nineteen measured it, came back

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with Einstein's number rather than
Newton's, and made him famous overnight.

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A British expedition confirming
a German theory, months after the war.

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Newton unified the falling
apple and the planets.

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This unified the apple,
the planets, and the light.

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Now take the whole argument to its limit.

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To leave a body you need escape velocity:

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enough kinetic energy to pay off
the gravitational binding energy

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at its surface.

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Solve that for the speed and you get
the square root of two G M over r.

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For the Earth it comes
to eleven kilometres a second.

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Make the body more compact
and the speed climbs.

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Keep squeezing.

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Here, for comparison, is the speed

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of light, and there is the moment
the escape velocity matches it exactly.

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Set the two equal
and solve for the radius.

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The mass of the escaping object cancels,

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and what is left is two G M over c
squared, the Schwarzschild radius.

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People wrote that expression down
in the seventeen hundreds and wondered.

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Now we know.

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Newton's law says nothing special
happens at that radius. Einstein's does.

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For an observer trying to hover
at rest, the pull is the inverse

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square law multiplied by one
over that same square root.

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The grey curve is Newton.

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The red one is the truth, and it
sits above the grey one everywhere.

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Gravity in general relativity
is stronger at short range, not weaker,

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which is the opposite
of what would rescue us.

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Now walk inward.

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Hover out here and you need
a certain thrust. Closer in, more thrust.

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And at the Schwarzschild radius,

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the dashed line, the thrust
you need runs away to infinity.

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So there is no hovering
at that surface, or anywhere inside it.

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Fire your rocket as hard
as you like and you still go in.

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That surface is the event horizon.

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It is not a wall, and nothing
about crossing it feels violent.

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For a big enough hole the tidal
stretching there is gentle and you sail

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through noticing nothing at all.

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What kills you is the singularity
at the centre, much later.

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And from far away I never see you cross.

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Your clock, by that same square root,
runs slower and slower as you approach.

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Your light stretches redder and redder.

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You fade out rather than arrive.

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Let us put the whole thing back together.

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Einstein's equation states it in one line,

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and the argument that got
us there came in three steps.

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First, the speed limit.

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Nothing carries
an influence faster than light,

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and Newtonian gravity
plainly broke that rule.

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Second, the coincidence
Newton shrugged at.

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The mass that resists
being accelerated and the mass

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that gravity pulls on are one number,
agreeing to fifteen decimal places.

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And third, the price
of taking that seriously.

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Gravity is not a force at all.

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It is the shape of spacetime,

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and free fall is what a straight line
looks like once you admit the shape.

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It took Einstein ten years, and it grew
out of a coincidence that everyone else

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had already seen and let pass.