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Theories

Theory, from the Greek word for viewing or contemplation, has played a significant role in the understanding of science since the early 19th century but was not considered central before then. Instead, philosophers and scientists spoke more often of (Natural) Law and of hypothesis, defined by Mill as “any supposition which we make (either without actual evidence, or on evidence avowedly insufficient)in order to endeavor to deduce from it conclusions in accordance with facts which are known to be real.” As philosophical interpretation became more language based and conceptually analytical, however, theory became more important in the analytical tradition of science, and in the Marxist tradition, theory (theoria) was often contrasted with practice (praxis), following Marx in the Theses on Feuerbach.

In the period following Einstein and Darwin, however, “theory” became a term that applied to a set of laws and hypotheses that were well-attested, coherent, precise, and covered all of the explanatory domain in question. Hence, Einstein's general theory of relativity is understood to cover all dynamics previously covered by Newtonian physics, with the added benefits of improved accuracy and precision and increased coverage of phenomena that Newtonian physics could not explain. Theories replaced earlier theories, it was held, in particular by the philosophical school known as the Logical Positivists, or the Vienna Circle, on rational grounds, and this replacement was absolute progress.

Popper's Account and Theories as Explanations

Theories were thought at this time to be constructed on the basis of evidence through logical induction—generalizing from observed instances to formulate universal claims. This set up the Problem of Induction, which David Hume had first formulated in the latter part of the 18th century, and Karl Popper revived as a problem in 1934,in his Logik der Forschung (“the logic of research,” unfortunately titled The Logic of Scientific Discovery when published in English). Popper observed, as Hume had, that a universal claim cannot be derived from any finite number of observations and so cannot be rationally justified or verified, as the positivists had sought to do. He defined theories as “universal statements…nets cast to catch what we call ‘the world’: to rationalize, to explain, and to master it.” Theories explained events by giving a deduction from their universal laws and singular initial conditions that described the event to be explained. Carl Hempel generalized this as the nomological-deductive model of explanation. Variations for law-like generalizations that were not exceptionless universal statements, and for stochastic and probabilistic inferences, were also developed by Hempel and others. In particular, a historical form of explanation worked, so to speak, in reverse: if you could produce a law-like generalization from which, together with some initial and boundary terms, you could deduce (or induce or infer in some manner) the events that were recorded, then you had offered an explanation of the events—the so-called covering law model. If there were more than one generalization that covered the event, then the best theory was the one that covered the most events or cases. Prediction was not possible in historical science, of course, but retrodiction or the “prediction” of already known events from the covering law explanation was considered to be equivalent logically to prediction in the experimental and present sciences.

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