COSMOLOGY,PHYSICAL ASPECTS
— 172—
masses move along geodesics, curves describing
the shortest possible path in space-time. Their mo-
tion, in turn, alters the curvature of space-time,
thus giving the field equations of the General The-
ory of Relativity their complicated nonlinear form.
Shortly after the discovery of the General The-
ory of Relativity, solutions to Einstein’s equations
were developed for two distinct classes of prob-
lems: (1) point masses, which when applied to the
solar system led to several key tests of the theory
and their eventual confirmation (including the de-
flection of starlight by the sun and the precession
in the perihelion of the orbit of Mercury); and (2)
dust, which when eventually applied to the distri-
bution of galaxies and galactic clusters described
the universe as expanding in time. Beginning in
the 1920s, telescopic observations by Edwin Hub-
ble showed that galaxies were indeed receding
from us and at a velocity proportional to their dis-
tance. In essence, the expansion of the universe
had been discovered.
There are in fact three standard types of ex-
pansion possible. In the so-called closed model,
the universe has the shape of a three-dimensional
sphere of finite size. It expands up to a maximum
size, approximately one hundred to five hundred
billion years from now, then contracts, eventually
collapsing to vanishing size with infinite tempera-
tures and densities. The so-called open model has
two variations, one in which the universe is flat,
and one in which it is saddle-shaped. In both ver-
sions of the open model, the universe is infinite in
size. In both cases the universe will expand forever
and cool towards absolute zero. The future of
these three models is often used to characterize
them as “freeze” (open) or “fry” (closed).
All three models came to be called Big Bang
models because they describe the universe as hav-
ing a finite past life of twelve to fifteen billion
years and as beginning in a singularity, an event of
infinite temperature, infinite density, and zero vol-
ume in which the laws of physics as we know
them break down. Since the age of the universe t
is calculated as starting here, it is convenient to
label the singularity “t = 0”; technically this event is
referred to as an essential singularity. In the 1960s,
Stephen Hawking, Roger Penrose, and Robert Ge-
roch proved key theorems demonstrating that the
existence of an essential singularity such as t = 0,
given Einstein’s General Theory of Relativity, was
unavoidable.
The relevance of t = 0 to creation ex nihilo
To what extent is t = 0 relevant to the doctrine of
creation ex nihilo? Responses have ranged widely
from direct relevance to complete irrelevance.
Direct relevance. For some scholars, the scien-
tific discovery of an absolute beginning of all
things (including time) provides empirical confir-
mation, perhaps even proof, of divine creation.
This was the position taken by Pope Pius XII in
1951 in an address to the Pontifical Academy of
Sciences. In 1978 Robert Jastrow, then head of
NASA’s Goddard Institute for Space Studies, spoke
metaphorically about scientists who, after climbing
the arduous mountain of cosmology, came to the
summit only to find theologians there already. The
idea that t = 0 provides strong, even convincing,
support for belief in God is frequently advanced by
conservative and evangelical Christians such as
Hugh Ross. Early in the debate, Lutheran theolo-
gian Ted Peters advanced a more nuanced argu-
ment elucidating the theological importance of a
beginning to the universe in terms of “consonance”
between theology and Big Bang cosmology. A so-
phisticated argument for the temporal finitude of
the universe based on t = 0, as well as on an argu-
ment that rejects the possibility that the universe is
also actually infinite in size, has been developed
by philosopher William Craig, partially through an
explicit debate with atheist Quentin Smith. More
recently, philosopher Phil Clayton has suggested
that contemporary cosmology affords a clear case
of divine activity.
t = 0 also has served indirectly to inspire the
construction of an alternative, and quite successful,
cosmology. In the 1940s, Fred Hoyle, an outspo-
ken atheist, together with colleagues Hermann
Bondi and Thomas Gold, constructed a cosmology
that would have no temporal beginning or end.
Their “steady state cosmology” depicted the uni-
verse as eternally old and expanding exponentially
forever. For two decades, the Big Bang and the
steady state models seemed equally viable given
the empirical evidence then available. By the mid-
1960s, however, the Big Bang model was vindi-
cated, at least in most scientists’ minds, by the dis-
covery of the microwave background radiation, the
successful prediction of the cosmological abun-
dances of hydrogen and helium, and other effects.
What is important here, however, is Hoyle’s moti-
vation in developing the steady state cosmology.
One reason, although probably only secondary,