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Page 1
Voir dans le PDF(s’ouvre dans une nouvelle fenêtre)Getting its
frombits
which govern the evolution of systems in
time, and are expected to be simple, and the
initial conditions, which mustbe given from
outside. The equations of classical physics
can be applied to any number of different
types of solar system, having different sizes
and shapes. There is nothing in Newton's
Frank Wiiczek
The inventor of the term ‘black hole’, John Wheeler, has a gift for
memorable phrases. ‘Getting its from bits’ Is another of his creations. It
refers not to an object, but to a vision of a world derived from pure logic
and mathematics. That vision has to a remarkable extent been embodied
In modern physics — here is a progress report.
he ‘its from bits’ programme’ has a
| venerable history, for perhaps the
first great quantitative generalization
in science was Pythagoras’ discovery of the
numerical patterns behind musical sounds.
When two strings of a lyre — of the same
material, and under equal tension — are
played together, they produce a pleasant harmony precisely when their lengths are a ratio
of small integers: 2 to 1 for an octave, 3 to 2
for a musical fifth, 4 to 3 for a fourth, and
so on. For the followers of Pythagoras, this
provided a satisfying example of a principle
they held to be completely general, the idea
that ‘all is number’.
A chain of thought extending over two
millennia links this idea to the inspirations
of Kepler. Kepler’s three laws of planetary
motion are enshrined in textbooks, and provided the foundation for Newton's celestial
mechanics. Less publicized is his erroneous
‘zeroth’ law, which was his version of Copernicanism, and the point of departure for his
©WILC.ZEK
original research. According to Kepler's
zeroth law, which would have pleased
Pythagoras, the orbits of the six planets are
great circles on spheres alternately inscribed
within and circumscribed about the five
regular solids. Of course, we now know that
there are more than six planets, and Kepler
himself was reluctantly forced, by Tycho
Brahe’s accurate observations, to abandon
circular orbits in favour of ellipses. According to modern views, the number of planets
laws of gravity and mechanics, nor for that
matter in the other pillar of classical physics,
Maxwell’s electrodynamics, that could serve
to fix a definite size. Symptomatic of this,
there is no way to forma characteristic length
from the parameters that govern these
theories, namely the gravitational coupling
G and the speed of light c. Classical physics
is profoundly anti-Pythagorean.
Modern Pythagorism
and the size of planetary orbits was deter-
The most successful theory of modern
physics, quantum mechanics, completely
changes the situation. Quantum mechanics
provides a unique ground-state configuration for each atom and molecule, thus relieving the indeterminacy in the analogous classical theory of solar systems, and making it
possible to understand why atoms and molemined more or less accidentally during the
complicated process whereby our Solar System condensed out of a gigantic interstellar
cules exhibit well-defined, universal chemistry. Ata yet deeper level, quantum field theory, which is the logical extension of quangas cloud. Solar systems around other stars,
tum mechanics to include special relativity,
which are now beginning to yield their
explains why the elementary constituents —
secrets to observation, are expected to be
very different.
electrons and nuclei — exist in myriads of
Indeed, classical physics teaches us that
the size ofplanctary orbits is not the sort of
thing we should aspire to predict. It makes
a sharp distinction between the basic laws,
single universal field. So, for example, quantum electrodynamics (QED) posits, in addition to the familiar electromagnetic field
identical copies, each being an excitation ofa
whose excitations represent the formation of
photons, an electron field whose excitations
Box 1: Afewwords
on dimensional analysis _
we sec as the creation of electrons.
Dimensional analysisis a time-honoured
When Planck introduced his quantum of
action, #, he immediately advertised the pos-
‘way to estimate the answer to a.
physical question without havingto
Solve: or even; perhaps, to fully
formulate the governing equations. The
24 \ AAA
main Ideais both trivial and profound. tt.
is that physical results mustbe .
independent of the. choice:of units:
Aclassic application of dimensional
‚analysis is to fluid:fiow, Suppose we :
‘are interested in
i flow of velocity pi
analysis leads to the vague, but
extremely useful, principle that
reasonably defined quantities should be
sibility of a new Pythagorism?. The inability
of classical physics to provide a definite scale
expressed in appropriate ‘natural units’.
of length had been relieved. For Planck
observed that from G, cand 4 one can form
Inthe system of natural units used in
the Planck length:
. numbers of the order unity when
+ ‘particle physics, quantities having
dimensions of mass, length and time
v2
ii [2 - 10 cm
-are:given the dimensions
of powers of. -
energy (usually in electronvolts), which
formisthe Reynolds number, Re = vL/v..
regard these as fundamental. units.
So, for example, we can use model
Planck proposed that
in a complete
More generally, by combining appropriate
powers of these parameters one can reproduce any unit of measurement needed in the
description of the physical world. On the
other hand, one cannot combine them to
produce a dimensionless pure number.
Thus G, ¢ and # provide an ideal, nonredundant system of physical units. From
this arises the modern Pythagoras-Planck
aircraft in a wind tunnel
to study the
formulation of physics, not yet attained,
programme:
flow around real aircraft, by
the only additional parameter.to appear
compensating with.a larger: v for a
smaller L. As long as Re stays the same,
would be Newton's gravitational
framework in which G, c and # are all
profoundly incorporated, and to calculate
within that framework all the constants of
the flows will differ only by trivial reconstants of nature, expressed in these
Planck units, would be calculable pure
numbers.
FW.
-a bodyof size L, in a fluid of viscosity _
“per. unit density. Vi‘Since: v.‘has
Pi
dimensions of.length? /time, while vof
effectively. makes Planck's constant of
action #andthe speed:of light, c, both
- equal to unity, Essentially all the
equations in particle physics contain
course has dimensions of lengih/time,
the speed of light:c and Planck’s:
the only dimensionless-quantity we can
constant of action. 4, soit is natural to
scalings.
In its abstract form, dimensional
NATURE | VOL 397| 28 JANUARY 1999 | www.nature.com
constant G. In such a theory, all other
$A
© 1999 Macmillan Magazines Ltd
to
formulate a
theoretical
nature, expressed in Planck’s units, as pure
numbers.
This is a tall order. A particular challenge
is that fundamental quantities such as the
Page 2
Voir dans le PDF(s’ouvre dans une nouvelle fenêtre)size of atoms or the mass of the proton turn
Strong insights
because it is able to give an accurate and
outto have outlandish values (about 10” and
The modern theory of the strong interaction,
107", respectively) when expressed in
Planck units. If the Pythagoras-Planck
which binds atomic nuclei together, is quantum chromodynamics (QCD). This theory
has notably advanced us towards getting ‘its
from bits, in three distinct ways. First, it
accounts, in principle, for those problematical nuclear masses. A full formulation of
QCD requires, on the face of it, seven parameters: a pure number a,, analogous to
the fine-structure constant, that governs the
strength of the strong interaction, plus the
masses of six different types of quarks, in
addition to # and c. The up, down, strange,
charm, bottom and top quarks are the particles that, together with the colour gluons,
carry the colour charges of QCD. Although
detailed account of high-energy processes,
where the calculations become much simprogramme is to succeed, then the standard
working assumption of dimensional analysis
(see Box 1), that naturally defined entities
should be of order unity in natural units,
must be profoundly subverted.
Asatomic physics developed, some of the
spirit of the Pythagoras-Planck programme
was realized, but major compromises were
required. For many purposes it is a very
good approximation to neglect the effects of
relativity, and to regard nuclei as infinitely
heavy compared with electrons. In this
approximation, the fundamental equations
of atomic and molecular physics can be formulated in a way that #, together with m,
and e, the mass and charge of the electron,
appear as the only parameters. From these
we can construct a unique unit oflength, the
Bohr radius:
a=
È
em
This does give the approximate size of atoms
— so in this case dimensional analysis is
vindicated.
In a more accurate treatment of atoms
and molecules (such as QED) one must
include relativistic effects, and the ability of
finite mass protons and nuclei to recoil. The
description of these effects brings c, and the
finite masses of the proton and other atomic
nuclei, into the equations. (Gravity is utterly
negligible here, so Gis not required.) Once c
is added to the parameters of atomic physics,
one can form the fine-structure constant, a,
a dimensionless quantity:
pler (see Fig. 1). There has also been impressive progress in calculating the masses and
properties of the mesons and baryons that
take part in strong interactions. These are
analogous to atoms formed of quarks, antiquarks and gluons, whereas nuclei — aside
from the proton itself — are analogous
to complicated molecules. Representative
results are shown in Fig. 2 (fora fuller discussion, see Box 2 and ref. 3). These results leave
little doubt that correct values of the nuclear
masses would emerge from more numerical
work, but definitive calculations are probably some years off.
even this would be reasonably economical,
Second, QCD brings to the fore a proconsidering the amount of data to be correfound property of quantum field theories,
what we might call the relativity of charge.
lated, that parameter count is grossly unfair
to QCD. The up and down quark masses are
very small, and they are the only two quarks
that are significant for nuclear physics. By
According to modern quantum physics the
vacuum, which evolution has selected us to
regard asan empty background, isin realitya
highly structured, responsive and dynamic
medium. Because of the uncertainty principle the ‘vacuum’ contains virtual particles
that can, like the molecules in an insulator,
arrange themselves to partially screen an
inserted charge. If that happens, the charge
one measures at smaller distances, inside the
screening cloud, or equivalently in higherenergy processes, will effectively increase.
The opposite behaviour, antiscreening or
putting their masses to zero, and ignoring
the other quarks, one obtains an excellent
approximate theory containing just one
dimensionless quantity, a,.
In practice it is very difficult to use QCD
to calculate nuclear masses, just as it is very
difficult to do self-contained calculations
of chemical processes beginning with the
Schrédinger equation of quantum mechanics. We have faith in the theory primarily
05 y
e?
as “lea 0.00735
ic
This parameterizes
the strength of the
electromagnetic attraction between protons
and electrons, or equivalently the size of the
quantum of electric charge. In the spirit of
a,(Q)
Planck and Pythagoras, one should not be
satisfied to have such a quantity appearing as
fundamental in the laws of physics. Rather,
one should aspire to calculate it.
The pioneers of atomic physics were
acutely aware of this challenge. Pauli was
fond of saying that the first question he
would ask the Almighty would be to explain
the value of the fine structure constant. (The
joke continues, that after hearing the explanation — from Satan — Pauli thought for a
moment, then snapped “Wrong!”.) Thechal-
|
lenge escalates when we consider the nuclear
masses. Indeed, by taking ratios of these
masses, ortheratioofany ofthemto theelec-
0.
—
1
_
-
Y A
Energy scale Q/(GeV)
100
tron mass, we can construct many more
dimensionless numbers, To satisfy Pythagoras and Planck, we would have to calculate
all these numbers, not just take them from
experiment.
304
Figure 1 The relativity of charge. Value of the strong coupling constant, a,, established by a variety of
experiments (data points) at different energy scales, and compared to the QCD theoretical prediction
for a, (solid line). See ref. 4 for detailed references to the experiments.
ZA
© 1999 Macmillan Magazines Ltd
NATURE
| 28 JANUARY 1999 | www.nature.com
Page 3
Voir dans le PDF(s’ouvre dans une nouvelle fenêtre)arithmically on the distance at which they
are measured. So, a small coupling will
evolve only very slowly. As an illustration,
the strong coupling a, is observed to change
from a value close to 1 at 107"? cm to about
1/8 at 107 cm, and is predicted to be about
1/25 at 10°” cm. So, whereas thestrong coupling might eventually merge with its weaker brethren, its approach is quite a drawnout affair. When we calculate where the unification takes place, we find a truly remarkable result. The strong, electromagnetic and
14
M(aGseV)
12
weak couplings, which are significantly dif-
À
ferent when measured at ‘practical’ distances, are calculated to become equal when
measured at distances about 17 orders of
magnitude smaller — near the Planck unit
ofdistance.
It is extraordinarily suggestive that the
0.8
Planck scale emerges here. To appreciate
why, we must consider extending the notion
of the relativity of charge to gravity. The sorts
of charges, strong, weak or electromagnetic,
0.6
to which the interactions of the Standard
Model of particle physics respond, change
only logarithmically with distance, owing
to subtle quantum mechanical effects. But
0.4
Figure 2 Comparison of masses of light hadrons (dotted lines) to various lattice simulations (data
gravity responds to energy directly, so that it
points). These calculations contain just one free parameter, the strange quark mass. Sources of error in
runs linearly with energy (or inverse disthe current lattice calculations, which are believed to be responsible for the small residual errors, are
tance) scale. From its much inferior strength
discussed in ref. 3.
at accessible energies, gravity ascends to
equality with the other interactions at
roughly the Planck scale. Thus we discover
asymptotic freedom, though less familiar,
with two massless quarks, provides a truly
is also possible. In either case, the value of
marvellous partial realization of the vision of
the charge, or coupling strength, is not an
Pythagoras and Planck. Using # and c as
units, and with no further inputs — except
absolute concept, but depends on how it is
measured. Antiscreening is calculated to
occur in QCD. The experimental evidence
for this behaviour is now quite firm", as you
can see in Fig, 1.
Because of the relativity of charge, the
QCD analogue of Pauli’s question — why is
the value of the fine structure constant what
the number of colour charges, of which there
are three (binary *11'), and the number of
quarks, of which there are two (binary ‘10°)
— it accurately accounts for all the ‘its’ of
nuclear physics, and much else besides. ‘Its
from bits, to be sure!
that all the coupling strengths become equal
simultaneously. Even in the absence of a
detailed theory, we find here a concrete,
semi-quantitative indication that all of the
basic forces arise from a common source.
Time
Space
it is? — receives a startling answer: “It’s anything you like, at some distance or other”. We
can simply declare it to be, say, 1/10, thereby
defining the distance where it is 1/10. This is
the phenomenon of dimensional transmu-
Getting it all — or hitting a wall?
tation’. A dimensionless measure of the
quantum of charge, the coupling ‘constant’
has been transmuted into a unit of distance.
ras-Planck programme? This brings me to
my third and final point. The relativity of
charge, which plays such a central role in
The approximate QCD theory with two
QCD, applies as well to the other interactions
massless quarks appears, naively, to bea famof the Standard Model of modern physics —
ily of theories, each with a different value of
the coupling, and none defining a scale of
distance. But because of dimensional transthe weak and electromagnetic interactions
Although QCD accounts admirably for
the strongest forces in nature, it is certainly
not a Theory of Everything. What, if anything, does it portend for the full Pythago-
Electron
Photon
DIDI
Da
FA
Quark
ba
units they use to measure length. This differ-
(although for them it is a much smaller
effect). This brings up the possibility that all
the couplings — that is the quanta of each of
the strong, weak and electromagnetic charges
— might have a common value when meaence in units matters for comparison of
sured at exceedingly small distance scales (or
purely QCD quantities to non-QCD quantiequivalently at high energies), despite their
disparate values at currently accessible scales,
There are several other pieces of evidence
contributing to electron-electron scattering in
pointing
QED, by exchange ofa
mutation, it turns out to be a family of perfectly identical theories that differ only in the
ties, such as the ratio of the diameter of the
proton to the Bohr radius, but it does not
affect dimensionless quantities within QCD
itself, such as ratios of nuclear sizes or
nuclear masses.
So QCD, in its slightly idealized version
NATURE | VOL 397 | 28 JANUARY 1999 | www.nature.com
toward
this
possibility,
as
I
Giuon
Figure 3 Feynman graphs. a, The simplest graph
virtual photon. Ina more
described in these pages last year“.
accurate calculation, b, one must allow for
For our present discussion, what is crucial is that the inverse couplings depend logmultiple exchanges. c, A typical contribution to
FA
© 1999 Macmillan Magazines Ltd
the interaction of quarks in QCD.
Page 4
Voir dans le PDF(s’ouvre dans une nouvelle fenêtre)This example of how vastly different
scales emerge, provides critical insight for
antiscreening) is small. An outstanding
the vexing problem, fundamental for the
its quantum size (Compton wavelength)
But this is related, by the relativity of charge,
to the exponentially smaller distance where
unification takes place. Putting this idea into
Pythagoras-Planck programme, of how to
generate extremely large (or extremely
small) dimensionless numbers. Any dynamical effect due to a large coupling automatically generates an exponentially
large ratio of
defined by 41 m,),....,¢ According to QCD, the
an equation, we find:
scales, if the fundamental coupling (before
That occurs when a, is measured to be unity.
example is the proton mass, or equivalently
proton’s Compton wavelength is essentially
determined by the dimensionally transmuted length where the strong interaction
becomes strong and holds in the quarks.
Box 2:Bit proliferation- crunching thenumbers
Mproton a exp( kl unifica) Mptanck
for the proton mass in Planck units. Here,
Mpiande = (Ae1 G)'?= 10" porn is the Planck
mass unit, Q, ,i¢eq = 1/25 is the common value
of the strong, electromagnetic and weak cou-
È are always violent, but dome
plings when they unify, and k= 11/2 risacalculable numerical factor that characterizes
extremely complex. outputs, there:
and short-lived, quantum fluctuations:
“must be a lot of logical processing inin the colour version of electric and
the antiscreening. This formula works
remarkably well. Suddenly one sees ‘out-
If simple input parameters are to.give.
between. Here! describe the
14
computationalmachinery that processes
“and ‘01’ into: tables.of nuclear
2 magnetic
fields, even in:what evolution
has designed us to regard as ‘empty’
space (for otherwise we'd always be
landish’ numbers like 10% from the perspective of exp( — 1/a) — which is actually considerably bigger — and they no longer
distracted), ..i
appear quite so daunting.
and calculatein quantum:field theories
waytoa ld these all up. The only really
Although all of these developments justify optimism, it remains conceivable that the
properties.
|
The traditional way to visualize
is by means:of Feynman:graphs,
successful approach has been to
‘its from bits’ programme will hit a wall. A
which follow the tracks of particles
crunch the numbers (see ref. 3 for
particularly serious possibility is that we will
in.space and time.
a review): To do that, one first replaces
continuous:Space-time by a lattice,
converge on a unique set of basic equations
for physics — many physicists believe that
and restrictsattention to:a finite box.
Thedetailsare very intricate-and
such equations will emerge from investigations into superstring theory — but that
the scattering of particles, by
Clever, but one must check that the
these equations will contain consistent solupinto kl:all'the
‘approximations involved in discretizing
tions describing many basically different
‘and ‘boxingare: not too severe.In
possible worlds. There might, for example,
be valid solutions describing worlds with different electron/proton mass ratios, or different numbers of quarks. Twenty years ago,
Particles that are
not observed - those that are neither
in the:initial nor final state- are virtual
‘particles. Feynman graphs describe
ssible ways:
practice; about 10° points are used,
to ensure accuracy at.thé few per
quantum:electrodyn:
cent level. Sums over so many variables
s (QED). itis.
almost always agoo approximation:
in-QED to use only the simplest possible.
graph to describe:the: interaction, and
are employed. Heroes working on
numerical QCD have pushedthe’
an excellentapproximation to.use
only a few. In quantum:chromodynamics sl ©
(QCD), ón the.other hand,theprobability
that more:‘complicatedgraphs such.
frontierofhigh-speed parallel
processing, often designing and.
constructing their own computi ng
When
floating point multiplications per
become impractic =
An entirely different.approach is
calculates the masses of observed:
hadrons;mesons, baryons or; in
ences of the sorts mentioned above. Many
principle; Nuclei and ‘gluebalis’
particulars of what we commonly regard as
the most basic features of the world would
then hinge on an accident of history (that is,
necessary: The particle picture,
epitomized. by Fey man: graphs;is
an easy-to-calculate approximation
for limited purposes, but the:
gluons). by. dropping appropriate
(bound states made purely of colour
fundamental equationis:of QCD are.
mixtures ofquarks, antiquarks and
formulatedinterms offields fillinggluons into the roiling medium of
d the simplest,:
which amplified patch we emerged from).
Attempts to calculate the electron mass from
first principles might be as futile as attempts
fields at one space-time point, and
and perhaps the most profound, way:
together, and how fast theymove.
to calculate the shape of the Solar System, or
the anatomy of frogs. Still, wemusttry.
O
The particles we see are the resonant
Frank Wilczek is at the Institute for Advanced Study,
modes, which can persist as coherent
School of Natural Sciences, Olden Lane, Princeton,
‚measuring how long they hang
to state the theoryis to give the rule
which:governs the probability
amplitudes for different configurations
of the fields. This:tuletis easily stated:
mathematically,
is verysymmetrical,
entities fora reasonable amount of
and relates only:th fields at nearby::
- of hadrons are found, quite titerally,.
space-time points (thatis,it is local).
asthe: frequencies one can sound on
The difficultyis that when.one applies.
an exoticgong, constructed to purely
New Jersey 08450, USA.
time. In these calculations, the masses
the rule, one finds that many different
“
configurations «occur with substantial
result
that would surely have pleased
probably They:reflect thatthere
“Pythagoras.
Hes
which posits that the entire observable Universe expanded from a small patch early on,
has made it plausible that the known Universe is homogeneous not for any fundamental reason, but just because we are only
sampling a small patch of reality. With this in
mind, we need only travel sufficiently far, or
wait sufficiently long, to encounter differ-
Second),
Within this framework, one
Substantial:cont
space.and time,
Universe is a very big place (volume ~10' in
Planck units), But inflationary cosmology’,
machines. At the moment, two different
teraflop machines are devoted full
time to QCD calculations (1 teraflop=10”
as Fig. 3ccontribute to the interaction
is notparticular! sm
many complic
one might have objected, against this possibility, that if there were other solutions, we
should have seen regions of the known Universe where they are realized. After all, the
-cahnot:be done analytically, so
Monte Carlo sampling techniques
e-mail: wilezek@sns.ias.edu
1. Misner,C., Thorne, K. & Wheeler, |, in Gravitation Ch, 44
(Freeman, New York, 1973).
2. Planck, M, S.-B, Pruss, Akad, Wiss, 440-480 (1899),
3. Burkhalter, R. http://xxx.lanl.gov/abs/hcp-12/9810043
mathematical specifications. It is a
4. Schmelling, M. httphoolunl.govf«bs/hep-<x/9701002
5. Coleman, $. & Weinberg, E. Phys. Rev. D7, 1888-1910 (1973).
FW.
6. Wilczek, F. Nature 394, 13-15 (1998).
7. Linde, A. Inflation and Quantum Cosmology (Academic, San
Diego, 1990).
$A © 1999 Macmillan Magazines Ltd
NATURE | VOL 397 | 28 JANUARY 1999 | www.nature.com