12.3 Quantum Gravity, String Theory, and Extra Dimensions 171
energy. First we recall the implication of the value of the Higgs field in the minimum
of the potential energy in the Standard Model: the masses of the W
±
and Z bosons,
as well as the masses of the quarks and charged leptons, are proportional to this
value. A generalization of this phenomenon would take place in every minimum of
the potential energy, which would correspond to a different solution (value) for a
constant Higgs field: in each minimum, the particles would have different masses. In
addition, coupling constants (fine structure constants, Yukawa couplings, and even
the gravitational coupling) may depend on fields, and would correspondingly possess
different values in different “solutions”. Finally, even the cosmological constant (the
value of the potential energy in the corresponding minimum) would be different in
each solution—this means that the Universe, the existing particles, and interactions
would differ dramatically in each different solution.
Hence, why is our known Universe—corresponding to the Standard Model of
particle physics and the corresponding values of its parameters, the gravitational
and cosmological constant—the one realized in nature? Such a question has been
asked before in one form or another, and a possible answer is the so-called anthropic
principle [60]: this principle states that the properties of the fundamental laws of
nature have to be such that intelligent life is possible—otherwise nobody would be
there to ask the question.
The necessary conditions on the parameters of the Standard Model of particle
physics, including gravity, for the development of intelligent life, at least in the form
known to us, is the subject of current discussions; among other things, the following
considerations play a role in this context:
(a) In order that the relatively complex carbon nuclei
12
6
C can be generated in nuclear
reactions (and remain stable) in the interior of stars, the electromagnetic and
strong forces (between baryons) have to assume their actual values with a preci-
sion of about 1%.
(b) In order that massive stars with their planetary systems can be formed, the
gravitational force between atoms and nuclei must be much smaller than all the
other interactions.
(c) In order that enough time for the formation of stars, planets, and life is available
(and the Universe neither collapses nor dilutes too much before), the value of
the cosmological constant must not be too large [61].
However, the anthropic principle alone is not a complete answer to the question about
the origin of the fundamental parameters; a complete answer based on the anthropic
principle requires that we have the choice among many different parameters, i.e.,
that correspondingly many different Universes were or are realized.
On one hand, the (speculative!) idea of the “landscape” furnishes a possible model
for this idea [62]: at the beginning, the fields of superstring theory could sit in
differentminima of the potential energy in diff erent regions of the Universe. Since the
gravitational and cosmological constants are typically very different in these different
regions, the cosmological development proceeds differently. This way, 10
500
–10
1500
different Universes come into being (we also talk about a multiverse), most of which
collapse or dilute infinitely within fractions of a second, however; we just happen to