A Century Ago, Einstein’s Theory of Relativity Changed Everything
PRINCETON, N.J. — By the fall of 1915, Albert Einstein was a bit grumpy.
And
why not? Cheered on, to his disgust, by most of his Berlin colleagues,
Germany had started a ruinous world war. He had split up with his wife,
and she had decamped to Switzerland with his sons.
He
was living alone. A friend, Janos Plesch, once said, “He sleeps until
he is awakened; he stays awake until he is told to go to bed; he will go
hungry until he is given something to eat; and then he eats until he is
stopped.”
Worse,
he had discovered a fatal flaw in his new theory of gravity, propounded
with great fanfare only a couple of years before. And now he no longer
had the field to himself. The German mathematician David Hilbert was breathing down his neck.
So Einstein went back to the blackboard. And on Nov. 25, 1915, he set down the equation that rules the universe.
As compact and mysterious as a Viking rune, it describes space-time as a
kind of sagging mattress where matter and energy, like a heavy sleeper,
distort the geometry of the cosmos to produce the effect we call
gravity, obliging light beams as well as marbles and falling apples to
follow curved paths through space.
This
is the general theory of relativity. It’s a standard trope in science
writing to say that some theory or experiment transformed our
understanding of space and time. General relativity really did.
Since
the dawn of the scientific revolution and the days of Isaac Newton, the
discoverer of gravity, scientists and philosophers had thought of
space-time as a kind of stage on which we actors, matter and energy,
strode and strutted.
With
general relativity, the stage itself sprang into action. Space-time
could curve, fold, wrap itself up around a dead star and disappear into a
black hole. It could jiggle like Santa Claus’s belly, radiating waves
of gravitational compression, or whirl like dough in a Mixmaster. It
could even rip or tear. It could stretch and grow, or it could collapse
into a speck of infinite density at the end or beginning of time.
Scientists have been lighting birthday candles for general relativity all year, including here at the Institute for Advanced Study,
where Einstein spent the last 22 years of his life, and where they
gathered in November to review a century of gravity and to attend
performances by Brian Greene, the Columbia University physicist and World Science Festival
impresario, and the violinist Joshua Bell. Even nature, it seems, has
been doing its bit. Last spring, astronomers said they had discovered an
“Einstein cross,”
in which the gravity of a distant cluster of galaxies had split the
light from a supernova beyond them into separate beams in which
telescopes could watch the star exploding again and again, in a cosmic
version of the movie “Groundhog Day.”
What Is General Relativity?
Einstein presented his general theory of relativity 100 years ago this month.
Hardly
anybody would be more surprised by all this than Einstein himself. The
space-time he conjured turned out to be far more frisky than he had
bargained for back in 1907.
It
was then — perhaps tilting too far back in his chair at the patent
office in Bern, Switzerland — that he had the revelation that a falling
body would feel weightless. That insight led him to try to extend his
new relativity theory from slip-siding trains to the universe.
According
to that foundational theory, now known as special relativity, the laws
of physics don’t care how fast you are going — the laws of physics and
the speed of light are the same. Einstein figured that the laws of
physics should look the same no matter how you were moving — falling,
spinning, tumbling or being pressed into the seat of an accelerating
car.
One
consequence, Einstein quickly realized, was that even light beams would
bend downward and time would slow in a gravitational field. Gravity was
not a force transmitted across space-time like magnetism; it was the
geometry of that space-time itself that kept the planets in their orbits
and apples falling.
It
would take him another eight difficult years to figure out just how
this elastic space-time would work, during which he went from Bern to
Prague to Zurich and then to a prestigious post in Berlin.
In
1913, he and his old classmate Marcel Grossmann published with great
fanfare an outline of a gravity theory that was less relative than they
had hoped. But it did predict light bending, and Erwin Freundlich, an
astronomer at the Berlin Observatory, set off to measure the deflection
of starlight during a solar eclipse in the Crimea.
When
World War I started, Freundlich and others on his expedition were
arrested as spies. Then Einstein discovered a flaw in his calculations.
“There are two ways that a theoretician goes astray,” he wrote to the physicist Hendrik Lorentz.
“1) The devil leads him around by the nose with a false hypothesis (for
this he deserves pity) 2) His arguments are erroneous and ridiculous
(for this he deserves a beating).”
And
so the stage was set for a series of lectures to the Prussian Academy
that would constitute the final countdown on his quest to grasp gravity.
A Breakthrough Moment
Midway
through the month, he used the emerging theory to calculate a puzzling
anomaly in the motion of Mercury; its egg-shaped orbit changes by 43
seconds of arc per century. The answer was spot on, and Einstein had
heart palpitations.
The
equation that Einstein wrote out a week later was identical to one that
he had written in his notebook two years before but had abandoned.
On
one side of the equal sign was the distribution of matter and energy in
space. On the other side was the geometry of the space, the so-called
metric, which was a prescription for how to compute the distance between
two points.
Albert Einstein and Relativity in the Pages of The Times
When Albert Einstein and his work first became known to
the broader public, articles in The Times often seemed to alternate
between exasperation and fascination.
As
the Princeton physicist John Wheeler later described it, “Space-time
tells matter how to move; matter tells space-time how to curve.” Easy to
say, but hard to compute. The stars might be actors on a stage set, but
every time they moved, the whole stage rearranged itself.
It wasn’t long before Einstein received his first comeuppance.
In
December 1915, he received a telegram from Karl Schwarzschild, a German
astrophysicist serving at the front in the war, who had solved
Einstein’s equation to describe the gravitational field around a
solitary star.
One strange feature of his work was that at a certain distance from the star — to be known forever as the Schwarzschild radius — the equations would go kerblooey.
“If this result were real, it would be a true disaster,” Einstein said. This was the beginning of black holes.
That
Einstein’s equations could be solved at all for a single star baffled
him. One of his guiding lights had been the Austrian physicist and
philosopher Ernst Mach,
who taught that everything in the universe was relative. Einstein took
Mach’s Principle, as he called it, to mean that it should be impossible
to solve his equations for the case of a solitary object.
“One
can express it as a joke,” he told Schwarzschild. “If all things were
to disappear from the world, then according to Newton Galilean inertial
space remains. According to my conception, however, nothing is left.”
And yet here was a star, according to his equations, bending space all by itself, a little universe in a nutshell.
Designing a Universe
Like
most of his colleagues at the time, Einstein considered the universe to
consist of a cloud of stars, the Milky Way, surrounded by vast space.
What was beyond? Was the universe infinite? And if so, what stopped a
star from drifting so far that it would have nothing to relate to?
To
avoid such problems, Einstein set out in 1917 to design a universe
without boundaries. In his model, space is bent around to meet itself,
like the side of a tin can.
“I
have committed another suggestion with respect to gravitation which
exposes me to the danger of being confined to the nut house,” he
confided to a friend.
This
got rid of the need for troublesome boundaries. But this universe was
unstable, and the cylinder would collapse if something didn’t hold its
sides apart.
That something was a fudge factor
added to the equations Einstein called the cosmological constant.
Physically, this new term, denoted by the Greek letter lambda,
represented a long-range repulsive force.
The
happy result, Einstein thought, was a static universe of the type
nearly everybody believed they lived in and in which geometry was
strictly determined by matter.
But it didn’t last. Willem de Sitter, a Dutch astronomer, came up with his own solution describing a universe that had no matter at all and was flying apart.
“It would be unsatisfactory, in my opinion,” Einstein grumbled, “if a world without matter were possible.”
And then Edwin Hubble discovered that the universe really was expanding.
If
the cosmological constant couldn’t keep the universe still, then forget
about it and Mach’s Principle, Einstein said. “It dates back to the
time in which one thought that the ‘ponderable bodies’ are the only
physically real entities,” he later wrote to the British cosmologist
Felix Pirani.
But it was too late. Quantum mechanics soon invested empty space with energy. In 1998 astronomers discovered that dark energy, acting just like the cosmological constant, seems to be blowing space-time apart, just as in de Sitter’s universe.
In
fact, most cosmologists agree today that not quite all motion is
relative and that space-time does have an existence independent of
matter, though it is anything but static and absolute. The best example
are gravitational waves, ripples of compression and stretching speeding
through empty space at the speed of light.
A Century Ago, Einstein’s Theory of Relativity Changed Everything
PRINCETON, N.J. — By the fall of 1915, Albert Einstein was a bit grumpy.
And
why not? Cheered on, to his disgust, by most of his Berlin colleagues,
Germany had started a ruinous world war. He had split up with his wife,
and she had decamped to Switzerland with his sons.
He
was living alone. A friend, Janos Plesch, once said, “He sleeps until
he is awakened; he stays awake until he is told to go to bed; he will go
hungry until he is given something to eat; and then he eats until he is
stopped.”
Worse,
he had discovered a fatal flaw in his new theory of gravity, propounded
with great fanfare only a couple of years before. And now he no longer
had the field to himself. The German mathematician David Hilbert was breathing down his neck.
So Einstein went back to the blackboard. And on Nov. 25, 1915, he set down the equation that rules the universe.
As compact and mysterious as a Viking rune, it describes space-time as a
kind of sagging mattress where matter and energy, like a heavy sleeper,
distort the geometry of the cosmos to produce the effect we call
gravity, obliging light beams as well as marbles and falling apples to
follow curved paths through space.
This
is the general theory of relativity. It’s a standard trope in science
writing to say that some theory or experiment transformed our
understanding of space and time. General relativity really did.
Since
the dawn of the scientific revolution and the days of Isaac Newton, the
discoverer of gravity, scientists and philosophers had thought of
space-time as a kind of stage on which we actors, matter and energy,
strode and strutted.
With
general relativity, the stage itself sprang into action. Space-time
could curve, fold, wrap itself up around a dead star and disappear into a
black hole. It could jiggle like Santa Claus’s belly, radiating waves
of gravitational compression, or whirl like dough in a Mixmaster. It
could even rip or tear. It could stretch and grow, or it could collapse
into a speck of infinite density at the end or beginning of time.
Scientists have been lighting birthday candles for general relativity all year, including here at the Institute for Advanced Study,
where Einstein spent the last 22 years of his life, and where they
gathered in November to review a century of gravity and to attend
performances by Brian Greene, the Columbia University physicist and World Science Festival
impresario, and the violinist Joshua Bell. Even nature, it seems, has
been doing its bit. Last spring, astronomers said they had discovered an
“Einstein cross,”
in which the gravity of a distant cluster of galaxies had split the
light from a supernova beyond them into separate beams in which
telescopes could watch the star exploding again and again, in a cosmic
version of the movie “Groundhog Day.”
Graphic
What Is General Relativity?
Einstein presented his general theory of relativity 100 years ago this month.
Hardly
anybody would be more surprised by all this than Einstein himself. The
space-time he conjured turned out to be far more frisky than he had
bargained for back in 1907.
It
was then — perhaps tilting too far back in his chair at the patent
office in Bern, Switzerland — that he had the revelation that a falling
body would feel weightless. That insight led him to try to extend his
new relativity theory from slip-siding trains to the universe.
According
to that foundational theory, now known as special relativity, the laws
of physics don’t care how fast you are going — the laws of physics and
the speed of light are the same. Einstein figured that the laws of
physics should look the same no matter how you were moving — falling,
spinning, tumbling or being pressed into the seat of an accelerating
car.
One
consequence, Einstein quickly realized, was that even light beams would
bend downward and time would slow in a gravitational field. Gravity was
not a force transmitted across space-time like magnetism; it was the
geometry of that space-time itself that kept the planets in their orbits
and apples falling.
It
would take him another eight difficult years to figure out just how
this elastic space-time would work, during which he went from Bern to
Prague to Zurich and then to a prestigious post in Berlin.
In
1913, he and his old classmate Marcel Grossmann published with great
fanfare an outline of a gravity theory that was less relative than they
had hoped. But it did predict light bending, and Erwin Freundlich, an
astronomer at the Berlin Observatory, set off to measure the deflection
of starlight during a solar eclipse in the Crimea.
When
World War I started, Freundlich and others on his expedition were
arrested as spies. Then Einstein discovered a flaw in his calculations.
“There are two ways that a theoretician goes astray,” he wrote to the physicist Hendrik Lorentz.
“1) The devil leads him around by the nose with a false hypothesis (for
this he deserves pity) 2) His arguments are erroneous and ridiculous
(for this he deserves a beating).”
And
so the stage was set for a series of lectures to the Prussian Academy
that would constitute the final countdown on his quest to grasp gravity.
A Breakthrough Moment
Midway
through the month, he used the emerging theory to calculate a puzzling
anomaly in the motion of Mercury; its egg-shaped orbit changes by 43
seconds of arc per century. The answer was spot on, and Einstein had
heart palpitations.
The
equation that Einstein wrote out a week later was identical to one that
he had written in his notebook two years before but had abandoned.
On
one side of the equal sign was the distribution of matter and energy in
space. On the other side was the geometry of the space, the so-called
metric, which was a prescription for how to compute the distance between
two points.
Albert Einstein and Relativity in the Pages of The Times
When Albert Einstein and his work first became known to
the broader public, articles in The Times often seemed to alternate
between exasperation and fascination.
As
the Princeton physicist John Wheeler later described it, “Space-time
tells matter how to move; matter tells space-time how to curve.” Easy to
say, but hard to compute. The stars might be actors on a stage set, but
every time they moved, the whole stage rearranged itself.
It wasn’t long before Einstein received his first comeuppance.
In
December 1915, he received a telegram from Karl Schwarzschild, a German
astrophysicist serving at the front in the war, who had solved
Einstein’s equation to describe the gravitational field around a
solitary star.
One strange feature of his work was that at a certain distance from the star — to be known forever as the Schwarzschild radius — the equations would go kerblooey.
“If this result were real, it would be a true disaster,” Einstein said. This was the beginning of black holes.
That
Einstein’s equations could be solved at all for a single star baffled
him. One of his guiding lights had been the Austrian physicist and
philosopher Ernst Mach,
who taught that everything in the universe was relative. Einstein took
Mach’s Principle, as he called it, to mean that it should be impossible
to solve his equations for the case of a solitary object.
“One
can express it as a joke,” he told Schwarzschild. “If all things were
to disappear from the world, then according to Newton Galilean inertial
space remains. According to my conception, however, nothing is left.”
And yet here was a star, according to his equations, bending space all by itself, a little universe in a nutshell.
Designing a Universe
Like
most of his colleagues at the time, Einstein considered the universe to
consist of a cloud of stars, the Milky Way, surrounded by vast space.
What was beyond? Was the universe infinite? And if so, what stopped a
star from drifting so far that it would have nothing to relate to?
To
avoid such problems, Einstein set out in 1917 to design a universe
without boundaries. In his model, space is bent around to meet itself,
like the side of a tin can.
“I
have committed another suggestion with respect to gravitation which
exposes me to the danger of being confined to the nut house,” he
confided to a friend.
This
got rid of the need for troublesome boundaries. But this universe was
unstable, and the cylinder would collapse if something didn’t hold its
sides apart.
That something was a fudge factor
added to the equations Einstein called the cosmological constant.
Physically, this new term, denoted by the Greek letter lambda,
represented a long-range repulsive force.
The
happy result, Einstein thought, was a static universe of the type
nearly everybody believed they lived in and in which geometry was
strictly determined by matter.
But it didn’t last. Willem de Sitter, a Dutch astronomer, came up with his own solution describing a universe that had no matter at all and was flying apart.
“It would be unsatisfactory, in my opinion,” Einstein grumbled, “if a world without matter were possible.”
And then Edwin Hubble discovered that the universe really was expanding.
If
the cosmological constant couldn’t keep the universe still, then forget
about it and Mach’s Principle, Einstein said. “It dates back to the
time in which one thought that the ‘ponderable bodies’ are the only
physically real entities,” he later wrote to the British cosmologist
Felix Pirani.
But it was too late. Quantum mechanics soon invested empty space with energy. In 1998 astronomers discovered that dark energy, acting just like the cosmological constant, seems to be blowing space-time apart, just as in de Sitter’s universe.
In
fact, most cosmologists agree today that not quite all motion is
relative and that space-time does have an existence independent of
matter, though it is anything but static and absolute. The best example
are gravitational waves, ripples of compression and stretching speeding
through empty space at the speed of light.
Einstein
was back and forth on this. In 1916, he told Schwarzschild they did not
exist, then published a paper saying they did. In 1936, he and his
assistant did the same flip-flop again.
Nobody said this was easy, even for Einstein.
He set out to do one thing, namely make all motion relative, Michel Janssen,
a science historian at the University of Minnesota, told a Princeton
gathering this month. He failed, but in the process succeeded in doing
something very interesting, unifying the effects of acceleration and
gravity.
The
story goes to show, he said, that Bob Dylan was right when he sang
“there’s no success like failure,” but wrong that “failure is no success
at all.”
Einstein’s
greatest success came in 1919, when Arthur Eddington did the experiment
that Freundlich had set out to do, and ascertained that lights in the
heavens were all askew during an eclipse, bent by the sun’s dark
gravity, just as Einstein had predicted.
Asked
what he would have done if general relativity had failed, Einstein
said, “Then I would have been sorry for the dear Lord. The theory is
correct.”
And still the champ.
Einstein
was back and forth on this. In 1916, he told Schwarzschild they did not
exist, then published a paper saying they did. In 1936, he and his
assistant did the same flip-flop again.
Nobody said this was easy, even for Einstein.
He set out to do one thing, namely make all motion relative, Michel Janssen,
a science historian at the University of Minnesota, told a Princeton
gathering this month. He failed, but in the process succeeded in doing
something very interesting, unifying the effects of acceleration and
gravity.
The
story goes to show, he said, that Bob Dylan was right when he sang
“there’s no success like failure,” but wrong that “failure is no success
at all.”
Einstein’s
greatest success came in 1919, when Arthur Eddington did the experiment
that Freundlich had set out to do, and ascertained that lights in the
heavens were all askew during an eclipse, bent by the sun’s dark
gravity, just as Einstein had predicted.
Asked
what he would have done if general relativity had failed, Einstein
said, “Then I would have been sorry for the dear Lord. The theory is
correct.”
And still the champ.
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