Let
us consider the type of work done by theoretical cosmologists. One of
the main activities of such people is to create theories about the
universe, and theories about the origin of the universe. Quite
typically, such theories are mainly speculations which have little
basis in fact.
An example is the family of speculations known as cosmic inflation theory, which speculates about a sudden surge in the expansion rate of the universe at a time about a trillionth of a trillionth of a trillionth of a second after the universe's beginning (a surge which then suddenly ended after a fraction of a second). The facts we have about the universe do not directly support such an idea, but merely the much simpler idea that the farther you go back in time, the hotter and more dense the universe was (which leads you back to a point, apparently, of infinite density at the very beginning of cosmic history). Another example of a speculative cosmological theory is Paul Steinhardt's ekpyrotic theory, an attempt to replace the speculative cosmic inflation theory with an arguably even more speculative theory involving unobserved cosmic cycles. Another speculative cosmological theory is the theory of cosmological natural selection, which also involves many cosmic cycles. Then there is the “string landscape theory” involving a multiverse of more than 1,000,000,000,000,000,000 universes.
An example is the family of speculations known as cosmic inflation theory, which speculates about a sudden surge in the expansion rate of the universe at a time about a trillionth of a trillionth of a trillionth of a second after the universe's beginning (a surge which then suddenly ended after a fraction of a second). The facts we have about the universe do not directly support such an idea, but merely the much simpler idea that the farther you go back in time, the hotter and more dense the universe was (which leads you back to a point, apparently, of infinite density at the very beginning of cosmic history). Another example of a speculative cosmological theory is Paul Steinhardt's ekpyrotic theory, an attempt to replace the speculative cosmic inflation theory with an arguably even more speculative theory involving unobserved cosmic cycles. Another speculative cosmological theory is the theory of cosmological natural selection, which also involves many cosmic cycles. Then there is the “string landscape theory” involving a multiverse of more than 1,000,000,000,000,000,000 universes.
The
job of the theoretical cosmologist is in some ways very similar to
the job of a novelist or screenwriter who is trying to dream up a
plot for his next novel or screenplay. Just as a writer of a novel
or screenplay set in modern America or ancient Rome or renaissance
Florence will often try to keep his imaginative creations consistent
with known facts, a theoretical cosmologist will often present an
imaginative scenario which he attempts to keep consistent with known
facts about the universe. But there is one big difference. Rather
than selling his imaginative creations to a publishing house or a
movie studio, a theoretical cosmologist must pitch his imaginative
creations to a scientific journal. The theoretical cosmologist must
therefore wrap up his speculations in a kind of scientific garb,
making such imaginative creations sound like examples of science.
How does he do that?
In
his scientific paper our theoretical cosmologist will never refer to
his speculative ideas as speculations. Instead he will typically
describe his theory as a “model.” But it is often misleading to
use such a term when referring to cosmological speculations. In
science a model is an attempt to represent known reality by
presenting a simplified description that accounts for certain
features of that reality, or represents that known reality in a
mathematical way.
A
very simple example of a model is the Bohr model of the atom, which
represented the electrons in an atom as being like planets rotating
around the sun, with the nucleus of the atom being like the sun.
This model was later found to be too simple, but at least it shows
the idea of a model: a mental representation we can use to help us
understand a much more complicated reality.
Bohr model of the atom
Another
example of a model is the “solid particle” model of subatomic
particles. This simply involves depicting things such as electrons
as hard, solid particles. This is a simplification, because it turns
out electrons can act like either waves or particles, and the
position of an electron should more realistically be represented as a
kind of “smeared out” probability cloud. Another example of a
model is the plate tectonics model. The physical surface of our
planet involves countless details, but we can more simply describe it
as being a set of about 12 big plates that generate earthquakes when
they collide with each other.
Why
is it inappropriate to use the term “model” to refer to
speculative cosmological theories such as the cosmic inflation
theory, the ekpyrotic theory, the theory of eternal inflation, and
the theory of cosmological natural selection? It's because such
theories are not simplifications, but are typically the opposite of
simplifications. Speculative cosmological theories involve assuming
the existence of events or physical realities that have not been
observed. Such theories don't involve a mental representation in
which things are simpler (as we have with models), but instead
involve depictions of nature in which things are more complicated.
Theories of such a type are not rightfully called models (although
some of them are so ornate that we might rightfully call them
extravaganzas).
Another
way in which speculative cosmologists hide their speculations and
guesswork is to avoid candid phrases such as “we guess” and “we
speculate,” replacing them with phrases such as “let us start
with,” “we assume,” “we take,” “we model” and “we
describe.”
Here
is an example from this scientific paper. The
authors begin by saying, “Let us start with a model of slow
roll-inflation,” and then describe a very specific version of this
theory. They've immediately journeyed far into the airy dreamland of
cosmological speculation, since “slow-roll inflation” is a highly
speculative theory to begin with. The authors then say “we model
this by adding a field,” and then describe a further highly
speculative complication needed so that some thing “is anchored at
the bottom of the inflationary valley.” Mentioning two fields, both
of which are speculative, the authors say “we also assume that the
fields ...interact via a higher-order operator,” adding another
layer of complication to the speculative spider web they are
spinning. They later say “we take the representative central
value” to have a numerical value of 55, making an arbitrary guess.
They then say, “We
assume that inflation ends abruptly after the
critical point,” making yet another speculative assumption. They
mention “we can adjust the inflationary scale” in some particular
way, and apparently do that also – still another piece of
speculative guesswork.
Do
you get the picture on what is going on here? Speculations heaped
upon speculations. Wild guesses piled upon wild guesses. Picking
numerical values out of a hat. But the reader might not be aware of
that, because the authors don't use candid language to describe their
guesswork.
If a paper such as this were to be written candidly, it might be written something like this:
We will begin our speculations by starting off with the wildly speculative blah-blah-blah theory already advanced by previous cosmologists fond of guesswork. We add to this some further speculations involving blah-blah-blah and blah-blah-blah. But to accomplish our imaginative task, we must further guess that blah-blah-blah-blah-blah. We must also arbitrarily guess that blah-blah-blah has a numerical value of 130. When we further speculate that the blah-blah-blah theoretical construct has the very specific shape of blah-blah-blah and that the imagined blah-blah-blah effect has some weird characteristics that we will imaginatively describe, our speculative extravaganza (not to be confused with a scientific model) is finished.
If a paper such as this were to be written candidly, it might be written something like this:
We will begin our speculations by starting off with the wildly speculative blah-blah-blah theory already advanced by previous cosmologists fond of guesswork. We add to this some further speculations involving blah-blah-blah and blah-blah-blah. But to accomplish our imaginative task, we must further guess that blah-blah-blah-blah-blah. We must also arbitrarily guess that blah-blah-blah has a numerical value of 130. When we further speculate that the blah-blah-blah theoretical construct has the very specific shape of blah-blah-blah and that the imagined blah-blah-blah effect has some weird characteristics that we will imaginatively describe, our speculative extravaganza (not to be confused with a scientific model) is finished.
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