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Unformatted text preview: C OPYRIGHT 2003 SCIENTIFIC AMERICAN, INC. By Max Tegmark Parallel
Not just a staple
of science fiction,
other universes are
a direct implication
of cosmological observations ALFRED T. KAMAJIAN Is there a copy of you
reading this article? A person who is not you but who lives on
a planet called Earth, with misty mountains, fertile ﬁelds and
sprawling cities, in a solar system with eight other planets? The
life of this person has been identical to yours in every respect.
But perhaps he or she now decides to put down this article without ﬁnishing it, while you read on.
The idea of such an alter ego seems strange and implausible, but it looks as if we will just have to live with it, because it
is supported by astronomical observations. The simplest and
most popular cosmological model today predicts that you have
a twin in a galaxy about 10 to the 1028 meters from here. This
distance is so large that it is beyond astronomical, but that does
not make your doppelgänger any less real. The estimate is derived from elementary probability and does not even assume
speculative modern physics, merely that space is inﬁnite (or at
least sufﬁciently large) in size and almost uniformly ﬁlled with
matter, as observations indicate. In inﬁnite space, even the most
unlikely events must take place somewhere. There are inﬁnitely many other inhabited planets, including not just one but inﬁnitely many that have people with the same appearance, name
and memories as you, who play out every possible permutation
of your life choices. You will probably never see your other selves. The farthest
you can observe is the distance that light has been able to travel during the 14 billion years since the big bang expansion began. The most distant visible objects are now about 4 × 1026
meters away— a distance that deﬁnes our observable universe,
also called our Hubble volume, our horizon volume or simply
our universe. Likewise, the universes of your other selves are
spheres of the same size centered on their planets. They are the
most straightforward example of parallel universes. Each universe is merely a small part of a larger “multiverse.”
By this very deﬁnition of “universe,” one might expect the
notion of a multiverse to be forever in the domain of metaphysics. Yet the borderline between physics and metaphysics is
deﬁned by whether a theory is experimentally testable, not by
whether it is weird or involves unobservable entities. The frontiers of physics have gradually expanded to incorporate ever
more abstract (and once metaphysical) concepts such as a round
Earth, invisible electromagnetic ﬁelds, time slowdown at high
speeds, quantum superpositions, curved space, and black holes.
Over the past several years the concept of a multiverse has joined
this list. It is grounded in well-tested theories such as relativity
and quantum mechanics, and it fulﬁlls both of the basic criteria w ww.sciam.com SCIENTIFIC AMERICAN COPYRIGHT 2003 SCIENTIFIC AMERICAN, INC. 41 Level I: Beyond Our Cosmic Horizon
T H E P A R A L L E L U N I V E R S E S of your alter egos constitute the
Level I multiverse. It is the least controversial type. We all accept the existence of things that we cannot see but could see if
we moved to a different vantage point or merely waited, like
people watching for ships to come over the horizon. Objects
beyond the cosmic horizon have a similar status. The observable universe grows by a light-year every year as light from farther away has time to reach us. An inﬁnity lies out there, waiting to be seen. You will probably die long before your alter egos
come into view, but in principle, and if cosmic expansion cooperates, your descendants could observe them through a sufﬁciently powerful telescope.
If anything, the Level I multiverse sounds trivially obvious.
How could space not be inﬁnite? Is there a sign somewhere saying “Space Ends Here— Mind the Gap”? If so, what lies beyond
it? In fact, Einstein’s theory of gravity calls this intuition into
question. Space could be ﬁnite if it has a convex curvature or
an unusual topology (that is, interconnectedness). A spherical,
doughnut-shaped or pretzel-shaped universe would have a limited volume and no edges. The cosmic microwave background
radiation allows sensitive tests of such scenarios [see “Is Space
Finite?” by Jean-Pierre Luminet, Glenn D. Starkman and Jeffrey R. Weeks; Scientiﬁc American, April 1999]. So far,
however, the evidence is against them. Inﬁnite models ﬁt the
data, and strong limits have been placed on the alternatives.
Another possibility is that space is inﬁnite but matter is conﬁned to a ﬁnite region around us— the historically popular “island universe” model. In a variant on this model, matter thins
out on large scales in a fractal pattern. In both cases, almost Overview/ Multiverses
One of the many implications of recent cosmological
observations is that the concept of parallel universes is
no mere metaphor. Space appears to be infinite in size. If
so, then somewhere out there, everything that is possible
becomes real, no matter how improbable it is. Beyond the
range of our telescopes are other regions of space that
are identical to ours. Those regions are a type of parallel
universe. Scientists can even calculate how distant these
universes are, on average.
■ And that is fairly solid physics. When cosmologists consider
theories that are less well established, they conclude that
other universes can have entirely different properties and
laws of physics. The presence of those universes would
explain various strange aspects of our own. It could even
answer fundamental questions about the nature of time
and the comprehensibility of the physical world.
■ 42 all universes in the Level I multiverse would be empty and dead.
But recent observations of the three-dimensional galaxy distribution and the microwave background have shown that the
arrangement of matter gives way to dull uniformity on large
scales, with no coherent structures larger than about 1024 meters. Assuming that this pattern continues, space beyond our
observable universe teems with galaxies, stars and planets.
Observers living in Level I parallel universes experience the
same laws of physics as we do but with different initial conditions. According to current theories, processes early in the big
bang spread matter around with a degree of randomness, generating all possible arrangements with nonzero probability. Cosmologists assume that our universe, with an almost uniform distribution of matter and initial density ﬂuctuations of one part in
100,000, is a fairly typical one (at least among those that contain observers). That assumption underlies the estimate that
your closest identical copy is 10 to the 1028 meters away. About
10 to the 1092 meters away, there should be a sphere of radius
100 light-years identical to the one centered here, so all perceptions that we have during the next century will be identical to
those of our counterparts over there. About 10 to the 10118 meters away should be an entire Hubble volume identical to ours.
These are extremely conservative estimates, derived simply
by counting all possible quantum states that a Hubble volume
can have if it is no hotter than 108 kelvins. One way to do the
calculation is to ask how many protons could be packed into
a Hubble volume at that temperature. The answer is 10118 protons. Each of those particles may or may not, in fact, be present,
which makes for 2 to the 10118 possible arrangements of protons. A box containing that many Hubble volumes exhausts all
the possibilities. If you round off the numbers, such a box is
about 10 to the 10118 meters across. Beyond that box, universes— including ours— must repeat. Roughly the same number
could be derived by using thermodynamic or quantum-gravitational estimates of the total information content of the universe.
Your nearest doppelgänger is most likely to be much closer than these numbers suggest, given the processes of planet formation and biological evolution that tip the odds in your favor.
Astronomers suspect that our Hubble volume has at least 1020
habitable planets; some might well look like Earth.
The Level I multiverse framework is used routinely to evaluate theories in modern cosmology, although this procedure is
rarely spelled out explicitly. For instance, consider how cosmologists used the microwave background to rule out a ﬁnite
spherical geometry. Hot and cold spots in microwave background maps have a characteristic size that depends on the curvature of space, and the observed spots appear too small to be
consistent with a spherical shape. But it is important to be statistically rigorous. The average spot size varies randomly from
one Hubble volume to another, so it is possible that our universe
is fooling us— it could be spherical but happen to have abnormally small spots. When cosmologists say they have ruled out
the spherical model with 99.9 percent conﬁdence, they really
mean that if this model were true, fewer than one in 1,000 Hubble volumes would show spots as small as those we observe. SCIENTIFIC AMERICAN MAY 2003 COPYRIGHT 2003 SCIENTIFIC AMERICAN, INC. ALFRED T. KAMAJIAN ( background ); SARA CHEN ( inset ) of an empirical science: it makes predictions, and it can be falsiﬁed. Scientists have discussed as many as four distinct types
of parallel universes. The key question is not whether the multiverse exists but rather how many levels it has. LEVEL I MULTIVERSE
THE SIMPLEST TYPE of parallel universe is simply a region of space
that is too far away for us to have seen yet. The farthest that we
can observe is currently about 4 × 10 26 meters, or 42 billion lightyears— the distance that light has been able to travel since the big bang began. (The distance is greater than 14 billion light-years
because cosmic expansion has lengthened distances.) Each of the
Level I parallel universes is basically the same as ours. All the
differences stem from variations in the initial arrangement of matter. LIMIT OF
OBSERVATION 4 × 1026 METERS
PARALLEL UNIVERSE OUR UNIVERSE How Far Away Is a Duplicate Universe?
E XAMPLE UNIVERSE Imagine a two-dimensional universe with space for four particles.
Such a universe has 24, or 16, possible arrangements of matter.
If more than 16 of these universes exist, they must begin to
repeat. In this example, the distance to the nearest duplicate is
roughly four times the diameter of each universe.
DISTANCE TO REPEAT 12
34 PARALLEL UNIVERSE 1010 118 METERS 4 particles
OUR UNIVERSE ALL 16 POSSIBILITIES The same argument applies to our universe, which has space
for about 10118 subatomic particles. The number of possible
arrangements is therefore 2 to the 10118, or approximately
10 to the 10118. Multiplying by the diameter of the universe
gives an average distance to the nearest duplicate of 10 to
the 10118 meters.
2 × 10–13 METER 10118 particles
8 × 1026 meters IDENTICAL
UNIVERSE COPYRIGHT 2003 SCIENTIFIC AMERICAN, INC. 70
20 521 0.5 0.2 Angular Scale (degrees) 1023
10 19 1017
10 15 1013
107 GA X
LA YS UR Y
VE 108 TA
DENSITY 109 Size of Universe Temperature Fluctuation (microkelvins) 1025 Mass within Sphere (solar masses) 1 2 4 8 16 80 8 Radius of Space (billions of light-years) 1010 1011 Sphere Radius (light-years) or infinite (center). (One caveat: some cosmologists speculate that the
discrepant point on the left of the graph is evidence for a finite volume.) In
addition, WMAP and the 2dF Galaxy Redshift Survey have found that space
on large scales is filled with matter uniformly (right), meaning that other
universes should look basically like ours. The lesson is that the multiverse theory can be tested and
falsiﬁed even though we cannot see the other universes. The key
is to predict what the ensemble of parallel universes is and to
specify a probability distribution, or what mathematicians call
a “measure,” over that ensemble. Our universe should emerge
as one of the most probable. If not— if, according to the multiverse theory, we live in an improbable universe— then the theory is in trouble. As I will discuss later, this measure problem
can become quite challenging. tween our bubble and its neighbors is expanding faster than you
could travel through it. Your descendants will never see their
doppelgängers elsewhere in Level II. For the same reason, if cosmic expansion is accelerating, as observations now suggest,
they might not see their alter egos even in Level I.
The Level II multiverse is far more diverse than the Level I
multiverse. The bubbles vary not only in their initial conditions
but also in seemingly immutable aspects of nature. The prevailing view in physics today is that the dimensionality of spacetime,
the qualities of elementary particles and many of the so-called
physical constants are not built into physical laws but are the
outcome of processes known as symmetry breaking. For instance, theorists think that the space in our universe once had
nine dimensions, all on an equal footing. Early in cosmic history, three of them partook in the cosmic expansion and became
the three dimensions we now observe. The other six are now unobservable, either because they have stayed microscopic with a
doughnutlike topology or because all matter is conﬁned to a
three-dimensional surface (a membrane, or simply “brane”) in
the nine-dimensional space.
Thus, the original symmetry among the dimensions broke.
The quantum ﬂuctuations that drive chaotic inﬂation could
cause different symmetry breaking in different bubbles. Some
might become four-dimensional, others could contain only two
rather than three generations of quarks, and still others might
have a stronger cosmological constant than our universe does.
Another way to produce a Level II multiverse might be
through a cycle of birth and destruction of universes. In a scientiﬁc context, this idea was introduced by physicist Richard C.
Tolman in the 1930s and recently elaborated on by Paul J. Steinhardt of Princeton University and Neil Turok of the University
of Cambridge. The Steinhardt and Turok proposal and related
models involve a second three-dimensional brane that is quite
literally parallel to ours, merely offset in a higher dimension [see
“Been There, Done That,” by George Musser; News Scan, Scientiﬁc American, March 2002]. This parallel universe is not Level II: Other Postinflation Bubbles
was hard to stomach, try
imagining an inﬁnite set of distinct Level I multiverses, some
perhaps with different spacetime dimensionality and different
physical constants. Those other multiverses— which constitute
a Level II multiverse— are predicted by the currently popular
theory of chaotic eternal inﬂation.
Inﬂation is an extension of the big bang theory and ties up
many of the loose ends of that theory, such as why the universe
is so big, so uniform and so ﬂat. A rapid stretching of space long
ago can explain all these and other attributes in one fell swoop
[see “The Inﬂationary Universe,” by Alan H. Guth and Paul J.
Steinhard; Scientiﬁc American, May 1984; and “The Self-Reproducing Inﬂationary Universe,” by Andrei Linde, November
1994]. Such stretching is predicted by a wide class of theories
of elementary particles, and all available evidence bears it out.
The phrase “chaotic eternal” refers to what happens on the very
largest scales. Space as a whole is stretching and will continue
doing so forever, but some regions of space stop stretching and
form distinct bubbles, like gas pockets in a loaf of rising bread.
Inﬁnitely many such bubbles emerge. Each is an embryonic Level I multiverse: inﬁnite in size and ﬁlled with matter deposited by
the energy ﬁeld that drove inﬂation.
Those bubbles are more than inﬁnitely far away from Earth,
in the sense that you would never get there even if you traveled
at the speed of light forever. The reason is that the space beIF THE LEVEL I MULTIVERSE 44 SCIENTIFIC AMERICAN MAY 2003 COPYRIGHT 2003 SCIENTIFIC AMERICAN, INC. MAX TEGMARK ( sphere ); SARA CHEN ( graphs ) COSMOLOGICAL DATA support the idea that space continues beyond the
confines of our observable universe. The WMAP satellite recently
measured the fluctuations in the microwave background (left). The
strongest fluctuations are just over half a degree across, which
indicates— after applying the rules of geometry— that space is very large LEVEL II MULTIVERSE
volume. Other bubbles exist out there, disconnected from ours.
They nucleate like raindrops in a cloud. During nucleation,
variations in quantum fields endow each bubble with properties
that distinguish it from other bubbles. A SOMEWHAT MORE ELABORATE type of parallel universe emerges from the theory of cosmological inflation. The idea is that our Level I
multiverse— namely, our universe and contiguous regions of
space— is a bubble embedded in an even vaster but mostly empty EMPTY
MULTIVERSE OUR LEVEL I
MULTIVERSE Bubble Nucleation P ARALLEL
MULTIVERSE POSITION ∞ of Level II parallel universes by
scrutinizing the properties of our
universe. These properties, including
the strength of the forces of nature
( right) and the number of observable
space and time dimensions
( far right), were established by
random processes during the birth
of our universe. Yet they have
exactly the values that sustain life.
That suggests the existence of other
universes with other values. 5 GRAVITY DOMINATES COSMOLOGISTS INFER the presence Number of Large Time Dimensions Evidence FIELD
STRENGTH causes space to expand rapidly. In the bulk of
space, random fluctuations prevent the field
from decaying away. But in certain regions,
the field loses its strength and the expansion
slows down. Those regions become bubbles. Strength of Strong Nuclear Force ALFRED
CREDIT T. KAMAJIAN ( background ); CORNELIA BLIK ( top inset ); SARA CHEN ( bottom inset ) A Q UANTUM FIELD known as the inflaton PREDICTED BY GRAND UNIFIED THEORY 10
EXPLODE 1 ALL ATOMS ARE
RADIOACTIVE WE ARE
HERE 10–1 CARBON IS UNSTABLE DEUTERIUM IS UNSTABLE 0
0 10–1 1 10 ∞ Strength of Electromagnetism www.sciam.com ATOMS
UNSTABLE 4 FIELDS
UNSTABLE 3 EVENTS ARE
CANNOT EXIST 1 WE ARE ATOMS ARE
HERE UNSTABLE EVENTS ARE COMPLETELY
0 1 2 3 4 Number of Large Spatial Dimensions SCIENTIFIC AMERICAN COPYRIGHT 2003 SCIENTIFIC AMERICAN, INC. 45 46 ues of the physical constants [see “Exploring Our Universe and
Others,” by Martin Rees; Scientiﬁc American, December
1999]. The Level II multiverse theory predicts that physicists
will never be able to determine the values of these constants
from ﬁrst principles. They will merely compute probability distributions for what they should expect to ﬁnd, taking selection
effects into account. The result should be as generic as is consistent with our existence. Level III: Quantum Many Worlds
T H E L E V E L I A N D L E V E L I I multiverses involve parallel
worlds that are far away, beyond the domain even of astronomers. But the next level of multiverse is right around you.
It arises from the famous, and famously controversial, manyworlds interpretation of quantum mechanics— the idea that
random quantum processes cause the universe to branch into
multiple copies, one for each possible outcome.
In the early 20th century the theory of quantum mechanics
revolutionized physics by explaining the atomic realm, which
does not abide by the classical rules of Newtonian mechanics.
Despite the obvious successes of the theory, a heated debate
rages about what it really means. The theory speciﬁes the state
of the universe not in classical terms, such as the positions and
velocities of all particles, but in terms of a mathematical object called a wave function. According to the Schrödinger equation, this state evolves over time in a fashion that mathematicians term “unitary,” meaning that the wave function rotates
in an abstract inﬁnite-dimensional space called Hilbert space.
Although quantum mechanics is often described as inherently
random and uncertain, the wave function evolves in a deterministic way. There is nothing random or uncertain about it.
The sticky part is how to connect this wave function with
what we observe. Many legitimate wave functions correspond
to counterintuitive situations, such as a cat being dead and alive
at the same time in a so-called superposition. In the 1920s
physicists explained away this weirdness by postulating that the
wave function “collapsed” into some deﬁnite classical outcome
whenever someone made an observation. This add-on had the
virtue of explaining observations, but it turned an elegant, unitary theory into a kludgy, nonunitary one. The intrinsic randomness commonly ascribed to quantum mechanics is the result of this postulate.
Over the years many physicists have abandoned this view
in favor of one developed in 1957 by Princeton graduate student Hugh Everett III. He showed that the collapse postulate
is unnecessary. Unadulterated quantum theory does not, in fact,
pose any contradictions. Although it predicts that one classical reality gradually splits into superpositions of many such realities, observers subjectively experience this splitting merely as
a slight randomness, with probabilities in exact agreement with
those from the old collapse postulate. This superposition of
classical worlds is the Level III multiverse.
Everett’s many-worlds interpretation has been boggling
minds inside and outside physics for more than four decades.
But the theory becomes easier to grasp when one distinguishes SCIENTIFIC AMERICAN MAY 2003 COPYRIGHT 2003 SCIENTIFIC AMERICAN, INC. ALFRED T. KAMAJIAN really a separate universe, because it interacts with ours. But the
ensemble of universes— past, present and future— that these
branes create would form a multiverse, arguably with a diversity similar to that produced by chaotic inﬂation. An idea proposed by physicist Lee Smolin of the Perimeter Institute in Waterloo, Ontario, involves yet another multiverse comparable in
diversity to that of Level II but mutating and sprouting new universes through black holes rather than through brane physics.
Although we cannot interact with other Level II parallel universes, cosmologists can infer their presence indirectly, because
their existence can account for unexplained coincidences in our
universe. To give an analogy, suppose you check into a hotel,
are assigned room 1967 and note that this is the year you were
born. What a coincidence, you say. After a moment of reﬂection, however, you conclude that this is not so surprising after all.
The hotel has hundreds of rooms, and you would not have been
having these thoughts in the ﬁrst place if you had been assigned
one with a number that meant nothing to you. The lesson is that
even if you knew nothing about hotels, you could infer the existence of other hotel rooms to explain the coincidence.
As a more pertinent example, consider the mass of the sun.
The mass of a star determines its luminosity, and using basic
physics, one can compute that life as we know it on Earth is
possible only if the sun’s mass falls into the narrow range between 1.6 × 1030 and 2.4 × 1030 kilograms. Otherwise Earth’s
climate would be colder than that of present-day Mars or hotter than that of present-day Venus. The measured solar mass
is 2.0 × 1030 kilograms. At ﬁrst glance, this apparent coincidence of the habitable and observed mass values appears to be
a wild stroke of luck. Stellar masses run from 1029 to 1032 kilograms, so if the sun acquired its mass at random, it had only a
small chance of falling into the habitable range. But just as in
the hotel example, one can explain this apparent coincidence
by postulating an ensemble (in this case, a number of planetary
systems) and a selection effect (the fact that we must ﬁnd ourselves living on a habitable planet). Such observer-related selection effects are referred to as “anthropic,” and although the
“A-word” is notorious for triggering controversy, physicists
broadly agree that these selection effects cannot be neglected
when testing fundamental theories.
What applies to hotel rooms and planetary systems applies
to parallel universes. Most, if not all, of the attributes set by
symmetry breaking appear to be ﬁne-tuned. Changing their values by modest amounts would have resulted in a qualitatively
different universe— one in which we probably would not exist. If protons were 0.2 percent heavier, they could decay into
neutrons, destabilizing atoms. If the electromagnetic force were
4 percent weaker, there would be no hydrogen and no normal
stars. If the weak interaction were much weaker, hydrogen
would not exist; if it were much stronger, supernovae would
fail to seed interstellar space with heavy elements. If the cosmological constant were much larger, the universe would have
blown itself apart before galaxies could form.
Although the degree of ﬁne-tuning is still debated, these examples suggest the existence of parallel universes with other val- LEVEL III MULTIVERSE
Q UANTUM MECHANICS PREDICTS a vast number of parallel
universes by broadening the concept of “elsewhere.” These
universes are located elsewhere, not in ordinary space but in an
abstract realm of all possible states. Every conceivable way that the world could be (within the scope of quantum mechanics)
corresponds to a different universe. The parallel universes make
their presence felt in laboratory experiments, such as wave
interference and quantum computation. Quantum Dice
IMAGINE AN IDEAL DIE whose randomness is purely quantum. When you roll it, the
die appears to land on a certain value at
random. Quantum mechanics, however,
predicts that it lands on all values at
once. One way to reconcile these
contradictory views is to conclude that
the die lands on different values in
different universes. In one sixth of the
universes, it lands on 1; in one sixth, on 2,
and so on. Trapped within one universe,
we can perceive only a fraction of the full
quantum reality. Ergodicity The Nature of Time A CCORDING TO THE PRINCIPLE of ergodicity, quantum parallel
universes are equivalent to more prosaic types of parallel universes.
A quantum universe splits over time into multiple universes ( left ).
Yet those new universes are no different from parallel universes that
already exist somewhere else in space— in, for example, other Level I
universes ( right ). The key idea is that parallel universes, of whatever
type, embody different ways that events could have unfolded. M OST PEOPLE THINK of time as a way to describe change. At one moment, matter has a certain
arrangement; a moment later, it has another
( left). The concept of multiverses suggests an
alternative view. If parallel universes contain all
possible arrangements of matter ( right), then
time is simply a way to put those universes into a
sequence. The universes themselves are static;
change is an illusion, albeit an interesting one. = = www.sciam.com SCIENTIFIC AMERICAN COPYRIGHT 2003 SCIENTIFIC AMERICAN, INC. 47 THE AUTHOR between two ways of viewing a physical theory: the outside
view of a physicist studying its mathematical equations, like a
bird surveying a landscape from high above it, and the inside
view of an observer living in the world described by the equations, like a frog living in the landscape surveyed by the bird.
From the bird perspective, the Level III multiverse is simple.
There is only one wave function. It evolves smoothly and deterministically over time without any kind of splitting or parallelism. The abstract quantum world described by this evolving wave function contains within it a vast number of parallel
classical story lines, continuously splitting and merging, as well
as a number of quantum phenomena that lack a classical description. From their frog perspective, observers perceive only
a tiny fraction of this full reality. They can view their own Level I universe, but a process called decoherence— which mimics
wave function collapse while preserving unitarity— prevents
them from seeing Level III parallel copies of themselves.
Whenever observers are asked a question, make a snap decision and give an answer, quantum effects in their brains lead to
a superposition of outcomes, such as “Continue reading the article” and “Put down the article.” From the bird perspective, the
act of making a decision causes a person to split into multiple
copies: one who keeps on reading and one who doesn’t. From
their frog perspective, however, each of these alter egos is unaware of the others and notices the branching merely as a slight
randomness: a certain probability of continuing to read or not.
As strange as this may sound, the exact same situation occurs even in the Level I multiverse. You have evidently decided
to keep on reading the article, but one of your alter egos in a
distant galaxy put down the magazine after the ﬁrst paragraph.
The only difference between Level I and Level III is where your
doppelgängers reside. In Level I they live elsewhere in good old
three-dimensional space. In Level III they live on another quantum branch in inﬁnite-dimensional Hilbert space.
The existence of Level III depends on one crucial assumption: that the time evolution of the wave function is unitary. So
far experimenters have encountered no departures from unitarity. In the past few decades they have conﬁrmed unitarity for
ever larger systems, including carbon 60 buckyball molecules
and kilometer-long optical ﬁbers. On the theoretical side, the
case for unitarity has been bolstered by the discovery of decoherence [see “100 Years of Quantum Mysteries,” by Max 48 MAX TEGMARK wrote a four-dimensional version of the computer
game Tetris while in college. In another universe, he went on to become a highly paid software developer. In our universe, however,
he wound up as professor of physics and astronomy at the University of Pennsylvania. Tegmark is an expert in analyzing the
cosmic microwave background and galaxy clustering. Much of his
work bears on the concept of parallel universes: evaluating evidence for infinite space and cosmological inflation; developing insights into quantum decoherence; and studying the possibility
that the amplitude of microwave background fluctuations, the dimensionality of spacetime and the fundamental laws of physics
can vary from place to place. Tegmark and John Archibald Wheeler; Scientiﬁc American,
February 2001]. Some theorists who work on quantum gravity
have questioned unitarity; one concern is that evaporating black
holes might destroy information, which would be a nonunitary
process. But a recent breakthrough in string theory known as
AdS/CFT correspondence suggests that even quantum gravity is
unitary. If so, black holes do not destroy information but merely transmit it elsewhere. [Editors’ note: An upcoming article will
discuss this correspondence in greater detail.]
If physics is unitary, then the standard picture of how quantum ﬂuctuations operated early in the big bang must change.
These ﬂuctuations did not generate initial conditions at random. Rather they generated a quantum superposition of all
possible initial conditions, which coexisted simultaneously. Decoherence then caused these initial conditions to behave classically in separate quantum branches. Here is the crucial point:
the distribution of outcomes on different quantum branches
in a given Hubble volume (Level III) is identical to the distribution of outcomes in different Hubble volumes within a single
quantum branch (Level I). This property of the quantum ﬂuctuations is known in statistical mechanics as ergodicity.
The same reasoning applies to Level II. The process of symmetry breaking did not produce a unique outcome but rather
a superposition of all outcomes, which rapidly went their separate ways. So if physical constants, spacetime dimensionality
and so on can vary among parallel quantum branches at Level
III, then they will also vary among parallel universes at Level II.
In other words, the Level III multiverse adds nothing new
beyond Level I and Level II, just more indistinguishable copies
of the same universes— the same old story lines playing out
again and again in other quantum branches. The passionate debate about Everett’s theory therefore seems to be ending in a
grand anticlimax, with the discovery of less controversial multiverses (Levels I and II) that are equally large.
Needless to say, the implications are profound, and physicists are only beginning to explore them. For instance, consider the ramiﬁcations of the answer to a long-standing question:
Does the number of universes exponentially increase over time?
The surprising answer is no. From the bird perspective, there is
of course only one quantum universe. From the frog perspective,
what matters is the number of universes that are distinguishable
at a given instant— that is, the number of noticeably different
Hubble volumes. Imagine moving planets to random new locations, imagine having married someone else, and so on. At the
quantum level, there are 10 to the 10118 universes with temperatures below 108 kelvins. That is a vast number, but a ﬁnite one.
From the frog perspective, the evolution of the wave function corresponds to a never-ending sliding from one of these 10
to the 10118 states to another. Now you are in universe A, the
one in which you are reading this sentence. Now you are in universe B, the one in which you are reading this other sentence.
Put differently, universe B has an observer identical to one in
universe A, except with an extra instant of memories. All possible states exist at every instant, so the passage of time may be
in the eye of the beholder— an idea explored in Greg Egan’s SCIENTIFIC AMERICAN MAY 2003 COPYRIGHT 2003 SCIENTIFIC AMERICAN, INC. The Mystery of Probability: What Are the Odds?
AS MULTIVERSE THEORIES gain credence, the sticky issue of how to compute probabilities in physics is growing from a minor nuisance
into a major embarrassment. If there are indeed many identical
copies of you, the traditional notion of determinism evaporates.
You could not compute your own future even if you had complete
knowledge of the entire state of the multiverse, because there is no
way for you to determine which of these copies is you (they all feel
they are). All you can predict, therefore, are probabilities for what
you would observe. If an outcome has a probability of, say, 50
percent, it means that half the observers observe that outcome.
Unfortunately, it is not an easy task to compute what fraction
of the infinitely many observers perceive what. The answer
depends on the order in which you count them. By analogy, the
fraction of the integers that are even is 50 percent if you order
them numerically (1, 2, 3, 4, ...) but approaches 100 percent if you
sort them digit by digit, the way your word processor would (1, 10,
100, 1,000, ...). When observers reside in disconnected universes,
there is no obviously natural way in which to order them. Instead
one must sample from the different universes with some statistical
weights referred to by mathematicians as a “measure.”
This problem crops up in a mild and treatable manner at Level I, 1994 science-ﬁction novel Permutation City and developed by
physicist David Deutsch of the University of Oxford, independent physicist Julian Barbour, and others. The multiverse
framework may thus prove essential to understanding the nature of time. SARA CHEN Level IV: Other Mathematical Structures
T H E I N I T I A L C O N D I T I O N S and physical constants in the
Level I, Level II and Level III multiverses can vary, but the
fundamental laws that govern nature remain the same. Why
stop there? Why not allow the laws themselves to vary? How
about a universe that obeys the laws of classical physics, with
no quantum effects? How about time that comes in discrete
steps, as for computers, instead of being continuous? How
about a universe that is simply an empty dodecahedron? In the
Level IV multiverse, all these alternative realities actually exist.
A hint that such a multiverse might not be just some beerfueled speculation is the tight correspondence between the
worlds of abstract reasoning and of observed reality. Equations
and, more generally, mathematical structures such as numbers,
vectors and geometric objects describe the world with remarkable verisimilitude. In a famous 1959 lecture, physicist Eugene
P. Wigner argued that “the enormous usefulness of mathematics in the natural sciences is something bordering on the mysterious.” Conversely, mathematical structures have an eerily
real feel to them. They satisfy a central criterion of objective existence: they are the same no matter who studies them. A theorem is true regardless of whether it is proved by a human, a
computer or an intelligent dolphin. Contemplative alien civilizations would ﬁnd the same mathematical structures as we becomes severe at Level II, has caused much debate at Level III,
and is horrendous at Level IV. At Level II, for instance, Alexander
Vilenkin of Tufts University and others have published predictions
for the probability distributions of various cosmological
parameters. They have argued that different parallel universes that
have inflated by different amounts should be given statistical
weights proportional to their volume. On the other hand, any
mathematician will tell you that 2 × ∞ = ∞, so there is no objective
sense in which an infinite universe that has expanded by a factor of
two has gotten larger. Moreover, a finite universe with the topology
of a torus is equivalent to a perfectly periodic universe with infinite
volume, both from the mathematical bird perspective and from the
frog perspective of an observer within it. So why should its infinitely
smaller volume give it zero statistical weight? After all, even in the
Level I multiverse, Hubble volumes start repeating (albeit in a
random order, not periodically) after about 10 to the 10 118 meters.
If you think that is bad, consider the problem of assigning
statistical weights to different mathematical structures at Level IV.
The fact that our universe seems relatively simple has led many
people to suggest that the correct measure somehow involves
complexity. have. Accordingly, mathematicians commonly say that they
discover mathematical structures rather than create them.
There are two tenable but diametrically opposed paradigms
for understanding the correspondence between mathematics
and physics, a dichotomy that arguably goes as far back as Plato and Aristotle. According to the Aristotelian paradigm, physical reality is fundamental and mathematical language is merely a useful approximation. According to the Platonic paradigm,
the mathematical structure is the true reality and observers perceive it imperfectly. In other words, the two paradigms disagree
on which is more basic, the frog perspective of the observer or
the bird perspective of the physical laws. The Aristotelian paradigm prefers the frog perspective, whereas the Platonic paradigm prefers the bird perspective.
As children, long before we had even heard of mathematics, we were all indoctrinated with the Aristotelian paradigm.
The Platonic view is an acquired taste. Modern theoretical
physicists tend to be Platonists, suspecting that mathematics describes the universe so well because the universe is inherently
mathematical. Then all of physics is ultimately a mathematics
problem: a mathematician with unlimited intelligence and resources could in principle compute the frog perspective— that
is, compute what self-aware observers the universe contains,
what they perceive, and what languages they invent to describe
their perceptions to one another.
A mathematical structure is an abstract, immutable entity
existing outside of space and time. If history were a movie, the
structure would correspond not to a single frame of it but to the
entire videotape. Consider, for example, a world made up of
pointlike particles moving around in three-dimensional space. www.sciam.com SCIENTIFIC AMERICAN COPYRIGHT 2003 SCIENTIFIC AMERICAN, INC. 49 LEVEL IV MULTIVERSE
T HE ULTIMATE TYPE of parallel universe opens up the full realm of
possibility. Universes can differ not just in location, cosmological
properties or quantum state but also in the laws of physics. Existing
outside of space and time, they are almost impossible to visualize; the
best one can do is to think of them abstractly, as static sculptures
that represent the mathematical structure of the physical laws that govern them. For example, consider a simple universe: Earth, moon
and sun, obeying Newton’s laws. To an objective observer, this
universe looks like a circular ring (Earth’s orbit smeared out in time)
wrapped in a braid (the moon’s orbit around Earth). Other shapes
embody other laws of physics (a, b, c, d). This paradigm solves various
problems concerning the foundations of physics. a d
do not reside in the same space but exist outside of space and
time. Most of them are probably devoid of observers. This hypothesis can be viewed as a form of radical Platonism, asserting that the mathematical structures in Plato’s realm of ideas or
the “mindscape” of mathematician Rudy Rucker of San Jose
State University exist in a physical sense. It is akin to what cosmologist John D. Barrow of the University of Cambridge refers
to as “π in the sky,” what the late Harvard University philosopher Robert Nozick called the principle of fecundity and what
the late Princeton philosopher David K. Lewis called modal realism. Level IV brings closure to the hierarchy of multiverses, because any self-consistent fundamental physical theory can be
phrased as some kind of mathematical structure.
The Level IV multiverse hypothesis makes testable predictions. As with Level II, it involves an ensemble (in this case, the
full range of mathematical structures) and selection effects. As
mathematicians continue to categorize mathematical structures, they should ﬁnd that the structure describing our world
is the most generic one consistent with our observations. Similarly, our future observations should be the most generic ones
that are consistent with our past observations, and our past observations should be the most generic ones that are consistent
with our existence.
Quantifying what “generic” means is a severe problem, and
this investigation is only now beginning. But one striking and SCIENTIFIC AMERICAN MAY 2003 COPYRIGHT 2003 SCIENTIFIC AMERICAN, INC. CREDIT CHRISTIE DESIGN ( left ); ALFRED T. KAMAJIAN ( a–d )
B RYAN SUN In four-dimensional spacetime— the bird perspective— these
particle trajectories resemble a tangle of spaghetti. If the frog
sees a particle moving with constant velocity, the bird sees a
straight strand of uncooked spaghetti. If the frog sees a pair of
orbiting particles, the bird sees two spaghetti strands intertwined like a double helix. To the frog, the world is described
by Newton’s laws of motion and gravitation. To the bird, it is
described by the geometry of the pasta— a mathematical structure. The frog itself is merely a thick bundle of pasta, whose
highly complex intertwining corresponds to a cluster of particles that store and process information. Our universe is far
more complicated than this example, and scientists do not yet
know to what, if any, mathematical structure it corresponds.
The Platonic paradigm raises the question of why the universe is the way it is. To an Aristotelian, this is a meaningless
question: the universe just is. But a Platonist cannot help but
wonder why it could not have been different. If the universe is
inherently mathematical, then why was only one of the many
mathematical structures singled out to describe a universe? A
fundamental asymmetry appears to be built into the very heart
As a way out of this conundrum, I have suggested that complete mathematical symmetry holds: that all mathematical structures exist physically as well. Every mathematical structure corresponds to a parallel universe. The elements of this multiverse 50 b c EARTH’S
ORBIT encouraging feature of mathematical structures is that the symmetry and invariance properties that are responsible for the
simplicity and orderliness of our universe tend to be generic,
more the rule than the exception. Mathematical structures tend
to have them by default, and complicated additional axioms
must be added to make them go away. What Says Occam?
T H E S C I E N T I F I C T H E O R I E S of parallel universes, therefore,
form a four-level hierarchy, in which universes become progressively more different from ours. They might have different
initial conditions (Level I); different physical constants and particles (Level II); or different physical laws (Level IV). It is ironic that Level III is the one that has drawn the most ﬁre in the
past decades, because it is the only one that adds no qualitatively new types of universes.
In the coming decade, dramatically improved cosmological
measurements of the microwave background and the largescale matter distribution will support or refute Level I by further pinning down the curvature and topology of space. These
measurements will also probe Level II by testing the theory of
chaotic eternal inﬂation. Progress in both astrophysics and
high-energy physics should also clarify the extent to which
physical constants are ﬁne-tuned, thereby weakening or
strengthening the case for Level II.
If current efforts to build quantum computers succeed, they
will provide further evidence for Level III, as they would, in
essence, be exploiting the parallelism of the Level III multiverse
for parallel computation. Experimenters are also looking for
evidence of unitarity violation, which would rule out Level III.
Finally, success or failure in the grand challenge of modern
physics— unifying general relativity and quantum ﬁeld theory—
will sway opinions on Level IV. Either we will ﬁnd a mathematical structure that exactly matches our universe, or we will
bump up against a limit to the unreasonable effectiveness of
mathematics and have to abandon that level.
So should you believe in parallel universes? The principal
arguments against them are that they are wasteful and that they
are weird. The ﬁrst argument is that multiverse theories are vulnerable to Occam’s razor because they postulate the existence
of other worlds that we can never observe. Why should nature
be so wasteful and indulge in such opulence as an inﬁnity of different worlds? Yet this argument can be turned around to argue for a multiverse. What precisely would nature be wasting?
Certainly not space, mass or atoms— the uncontroversial Level I multiverse already contains an inﬁnite amount of all three,
so who cares if nature wastes some more? The real issue here
is the apparent reduction in simplicity. A skeptic worries about
all the information necessary to specify all those unseen worlds.
But an entire ensemble is often much simpler than one of its
members. This principle can be stated more formally using the
notion of algorithmic information content. The algorithmic information content in a number is, roughly speaking, the length
of the shortest computer program that will produce that number as output. For example, consider the set of all integers. Which is simpler, the whole set or just one number? Naively,
you might think that a single number is simpler, but the entire
set can be generated by quite a trivial computer program,
whereas a single number can be hugely long. Therefore, the
whole set is actually simpler.
Similarly, the set of all solutions to Einstein’s ﬁeld equations
is simpler than a speciﬁc solution. The former is described by
a few equations, whereas the latter requires the speciﬁcation of
vast amounts of initial data on some hypersurface. The lesson
is that complexity increases when we restrict our attention to
one particular element in an ensemble, thereby losing the symmetry and simplicity that were inherent in the totality of all the
elements taken together.
In this sense, the higher-level multiverses are simpler. Going from our universe to the Level I multiverse eliminates the
need to specify initial conditions, upgrading to Level II eliminates the need to specify physical constants, and the Level IV
multiverse eliminates the need to specify anything at all. The
opulence of complexity is all in the subjective perceptions of observers— the frog perspective. From the bird perspective, the
multiverse could hardly be any simpler.
The complaint about weirdness is aesthetic rather than scientiﬁc, and it really makes sense only in the Aristotelian worldview. Yet what did we expect? When we ask a profound question about the nature of reality, do we not expect an answer
that sounds strange? Evolution provided us with intuition for
the everyday physics that had survival value for our distant ancestors, so whenever we venture beyond the everyday world,
we should expect it to seem bizarre.
A common feature of all four multiverse levels is that the
simplest and arguably most elegant theory involves parallel universes by default. To deny the existence of those universes, one
needs to complicate the theory by adding experimentally unsupported processes and ad hoc postulates: ﬁnite space, wave
function collapse and ontological asymmetry. Our judgment
therefore comes down to which we ﬁnd more wasteful and inelegant: many worlds or many words. Perhaps we will gradually get used to the weird ways of our cosmos and ﬁnd its
strangeness to be part of its charm. MORE TO E XPLORE
Why Is the CMB Fluctuation Level 10 –5? Max Tegmark and Martin Rees in
Astrophysical Journal, Vol. 499, No. 2, pages 526–532; June 1, 1998.
Available online at arXiv.org/abs/astro-ph/9709058
Is “The Theory of Everything” Merely the Ultimate Ensemble Theory?
Max Tegmark in Annals of Physics, Vol. 270, No.1, pages 1–51;
November 20, 1998. Available online at arXiv.org/abs/gr-qc/9704009
Many Worlds in One. Jaume Garriga and Alexander Vilenkin in Physical
Review, Vol. D64, No. 043511; July 26, 2001. Available online at
Our Cosmic Habitat. Martin Rees. Princeton University Press, 2001.
Inflation, Quantum Cosmology and the Anthropic Principle. Andrei Linde
in Science and Ultimate Reality: From Quantum to Cosmos. Edited by J. D.
Barrow, P.C.W. Davies and C. L. Harper. Cambridge University Press, 2003.
Available online at arXiv.org/abs/hep-th/0211048
The author’s Web site has more information at
www.hep.upenn.edu/~max/multiverse.html www.sciam.com SCIENTIFIC AMERICAN COPYRIGHT 2003 SCIENTIFIC AMERICAN, INC. 51 ...
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