Professor Quillibrace had placed three sheets of paper on the table. Mr Blottisham regarded them with the suspicion usually reserved for documents requiring a signature.
Blottisham: I have been thinking about our last discussion. I believe I can now settle the matter.
Quillibrace: How gratifying. Which matter?
Blottisham: Scientific anomalies. When a theory encounters a difficulty, we adjust the theory. We introduce a new variable, refine a measurement, discover a previously neglected mechanism. There is no need to abandon the framework. Give sufficiently ingenious scientists sufficient time, and they will find a way through.
Elowen: And if the way through changes what counts as a possible explanation?
Blottisham: Then we shall have adjusted the framework rather more extensively than usual.
Quillibrace: You appear to be treating adjustment and reorganisation as differences of degree.
Blottisham: What else could they be? Science advances by correcting its mistakes.
Quillibrace: Sometimes. But consider the distinction between correcting an answer and discovering that the question has been framed too narrowly.
Blottisham: If the question is badly framed, we reframe it. That is still scientific progress.
Elowen: Certainly. But it may alter more than the question. It may alter the space of answers we can recognise as possible.
Blottisham reached for a biscuit.
Blottisham: I suspect we are about to make a great deal of fuss over a perfectly ordinary activity.
Quillibrace: Then let us examine an ordinary case.
He pushed the first sheet across the table.
Quillibrace: The rotation curve of the Milky Way. Astronomers estimate how the Galaxy's circular speed varies with distance from its centre. For a long time, the possibility of a relatively flat outer rotation curve was an important part of the case for a substantial dark matter halo. More recent analyses have renewed debate about whether the curve declines more steeply at large radii, perhaps approaching the Keplerian decline expected when most of the enclosed mass lies within the region being measured.
Blottisham: And if it does, the familiar halo models face difficulties. So we improve the models.
Quillibrace: That is one possibility.
Blottisham: One possibility? It is the obvious one.
Elowen: It may be. But notice what we have already done. We have not simply observed the Galaxy. We have inferred a curve from observations, using assumptions about stellar motions, the distribution of matter, the Galaxy's structure and the effects of disturbances. The curve itself is an achievement of scientific inference.
Blottisham: Are you suggesting the Galaxy might not have a rotation curve?
Elowen: I am suggesting that the curve we infer is not identical to the observations from which we infer it. That does not make it arbitrary. It makes the inferential process part of what we need to understand.
Quillibrace: Quite. And the debate is not settled by the steep decline alone. Other constraints support a more substantial Galactic halo than some radical interpretations would permit. The question is how the different lines of evidence fit together.
Blottisham: Which is precisely why we need better models. We reconcile the evidence, perhaps by revising the halo profile or accounting for systematic errors.
Quillibrace: And perhaps we shall. But let us ask what would count as success. Suppose an increasingly elaborate model could accommodate every new result by introducing another adjustment. Would that, by itself, establish that we understood the Galaxy?
Blottisham: If it made accurate predictions, certainly.
Elowen: Even if each success depended on a new assumption whose only purpose was to protect the previous ones?
Blottisham: Scientists are perfectly capable of distinguishing a productive refinement from an ad hoc rescue.
Quillibrace: They are. The distinction, however, is not always immediately apparent. A modification that initially looks like a rescue may lead to new predictions. An elegant explanation may eventually fail. We cannot decide the matter merely by inspecting how comfortably a proposal fits the existing framework.
Blottisham: Then we test it.
Quillibrace: Yes. But what if the difficulty concerns not just a particular proposal, but the relations among the assumptions that make certain proposals seem natural in the first place?
Blottisham paused.
Blottisham: I take it that is the question you have been waiting to ask.
Elowen: Consider how the problem appears from within the established framework. We have observations, a gravitational theory, models of visible matter, and a range of possible distributions of dark matter. When the inferred motion does not fit our expectations, we ask which part of the model needs adjustment.
Blottisham: A sensible procedure.
Elowen: Indeed. But the procedure also organises our possibilities. It directs attention towards certain explanations and away from others. What we regard as a missing quantity, a measurement error, a physical mechanism or a failure of the framework depends partly on how the problem has been organised.
Blottisham: You make that sound suspicious. Every investigation requires assumptions. We cannot begin from nowhere.
Quillibrace: Nor need we. The question is whether those assumptions remain open to revision when the evidence warrants it. A framework is indispensable to inquiry, but indispensability is not immunity.
Blottisham: I have never claimed immunity. I claim that science can revise its assumptions without requiring us to treat every anomaly as a revolution.
Quillibrace: A reasonable claim. And one we should preserve. Not every anomaly calls for a new framework. Sometimes the measurements are wrong; sometimes a familiar model needs refinement; sometimes an apparently profound problem disappears under closer investigation.
Elowen: But sometimes the available explanations keep multiplying while the difficulty remains. Then the problem may not be that we have yet to find the right answer within the existing arrangement. It may be that the arrangement itself needs reconsideration.
Blottisham: That sounds like an invitation to abandon a successful theory whenever someone finds it inconvenient.
Elowen: No. It is an invitation to distinguish a theory's success from the assumption that its present form exhausts the possibilities.
Quillibrace: We should also distinguish two claims that are often confused. One is that a scientific concept has not yet been conclusively established as referring to a particular kind of entity. The other is that the concept refers to nothing at all. Neither follows automatically from an anomaly.
Blottisham: So we are not declaring dark matter imaginary.
Quillibrace: Certainly not. The evidence relevant to dark matter extends far beyond the Milky Way's rotation curve, including gravitational lensing, the cosmic microwave background and the formation of large-scale structure. Any alternative account must address that wider body of evidence.
Elowen: The point is not to decide in advance whether dark matter exists. It is to recognise that its place in scientific thought has a history. An observation made a problem possible; a concept organised a set of explanations; successful applications strengthened that concept; and the concept then helped determine how later problems were posed.
Blottisham: A circle, then. We use the concept to interpret the evidence, and the interpreted evidence strengthens the concept.
Quillibrace: A circle can be vicious, but it need not be. The crucial question is whether the process exposes the concept to independent constraint. A framework that generates risky predictions, unifies different observations and survives serious attempts at falsification earns a different standing from one protected by adjustments that explain nothing beyond the data that prompted them.
Elowen: And even a well-supported framework remains capable of change. Its success does not make every assumption within it equally secure.
Blottisham looked again at the papers.
Blottisham: I see the distinction you are pursuing. I began by assuming that every anomaly could be accommodated if we were sufficiently ingenious. But ingenuity is not the same as explanation.
Quillibrace: An encouraging beginning.
Blottisham: Do not look so pleased, Professor. I have not conceded that a radical reorganisation is ever necessary in this particular case.
Elowen: Nor should you. The evidence has not settled that question. But perhaps we can agree that the possibility must remain open.
Blottisham: Provided that any proposed reorganisation does more than rename the difficulty.
Quillibrace: Agreed. A new way of thinking earns its place by explaining what the old one could not, while accounting for what the old one explained successfully.
Elowen: Which brings us to the word reality in our title. Reality does not rearrange itself to accommodate our theories, nor does it hand us a new conceptual framework when the old one falters. What changes is our relation to what we encounter. Evidence resists some possibilities, supports others, and may eventually force us to recognise possibilities we had not previously considered.
Blottisham: So reality reorganises our possibilities by refusing to cooperate with our expectations?
Quillibrace: A rather less mystical formulation than some I have heard.
Elowen: And a more demanding one. We cannot simply invent a new possibility because we prefer it. The world constrains what can be sustained. But neither can we assume that the possibilities already familiar to us are the only ones the world permits.
For a moment, nobody spoke. Blottisham broke the silence.
Blottisham: I still believe that scientific ingenuity will solve most of our problems.
Quillibrace: So do I.
Blottisham: You might have said so earlier.
Quillibrace: You had not yet distinguished ingenuity from the obligation to reconsider its premises.
Elowen smiled.
Elowen: Perhaps that is where our three conversations have brought us. First, scientific inference creates and revises an ecology of possibilities. Then, within that ecology, some concepts acquire the standing of entities. Finally, the evidence may alter not merely which explanation we favour, but the relations that make explanations possible.
Blottisham: And if it does not?
Elowen: Then a better answer within the existing framework may be exactly what we need.
Quillibrace: We have no general rule that tells us in advance which situation we face. That, I suspect, is why the question remains scientific rather than merely philosophical.
Blottisham raised his cup.
Blottisham: To the possibility that our possibilities are mistaken.
Quillibrace: More precisely, to the possibility that some of them are.
Elowen: And to noticing when the evidence asks us to think differently, rather than merely to think harder.
They drank.
Outside, the Galaxy continued its rotation, indifferent to the state of the Senior Common Room's deliberations. Whether its outer reaches would ultimately confirm a familiar account, require a more subtle one, or help open a different space of explanation remained a question for observation, inference and time.
The question was not whether science could change its mind. It plainly could.
It was whether we could recognise the moment when changing an answer was no longer enough.