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Reduction and Elimination in Philosophy and the Sciences

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<strong>Reduction</strong> <strong>and</strong> <strong>Reduction</strong>ism <strong>in</strong> Physics<br />

Rico Gutschmidt, Bonn, Germany<br />

The good old st<strong>and</strong>ard def<strong>in</strong>ition of reduction is penned by<br />

(Nagel 1961) <strong>and</strong> dem<strong>and</strong>s for a <strong>the</strong>ory to be reduced to<br />

ano<strong>the</strong>r that <strong>the</strong> laws of <strong>the</strong> first one can be logically<br />

deduced by <strong>the</strong> laws of <strong>the</strong> latter with <strong>the</strong> help of bridge<br />

laws connect<strong>in</strong>g <strong>the</strong> different languages of <strong>the</strong> <strong>the</strong>ories. A<br />

<strong>the</strong>ory reduced <strong>in</strong> this way should <strong>the</strong>n be <strong>in</strong> pr<strong>in</strong>ciple<br />

superfluous - if all <strong>the</strong>ir laws are, given <strong>the</strong> bridge laws,<br />

logically conta<strong>in</strong>ed <strong>in</strong> <strong>the</strong> reduc<strong>in</strong>g <strong>the</strong>ory, it is <strong>in</strong> a strict<br />

sense not required anymore <strong>in</strong> our physical description of<br />

<strong>the</strong> world.<br />

But th<strong>in</strong>gs are not that easy. As (Feyerabend 1962)<br />

has shown, this concept is somewhat naïve <strong>and</strong> <strong>the</strong>re are<br />

no <strong>in</strong>terest<strong>in</strong>g examples of reduction <strong>in</strong> <strong>the</strong> Nagelian<br />

sense. Feyerabend’s po<strong>in</strong>t is based ma<strong>in</strong>ly on two<br />

objections. First, <strong>the</strong> l<strong>in</strong>ks between physical <strong>the</strong>ories are<br />

mostly an approximate derivation of laws ra<strong>the</strong>r than <strong>the</strong>ir<br />

deduction - <strong>and</strong> <strong>the</strong>re is a great <strong>and</strong> <strong>in</strong> <strong>the</strong> debate of<br />

reduction largely overlooked difference between derivation<br />

<strong>and</strong> deduction. And second, <strong>the</strong> conception of <strong>the</strong> bridge<br />

laws is ra<strong>the</strong>r vague: Feyerabend argues that <strong>the</strong> terms of<br />

different <strong>the</strong>ories satisfy not only no identity relation, which<br />

could be expressed <strong>in</strong> bridge laws, but are actually<br />

<strong>in</strong>commensurable <strong>and</strong> not comparable whatsoever.<br />

Let us take a closer look on <strong>the</strong>se two assertions.<br />

First, <strong>the</strong>re is <strong>the</strong> ma<strong>the</strong>matical problem of approximate<br />

derivation: With<strong>in</strong> physics it seems to be a well established<br />

practise to derive laws “only” approximately. But what does<br />

this mean <strong>in</strong> <strong>the</strong> context of <strong>in</strong>ter<strong>the</strong>oretic relations? To take<br />

an example from <strong>the</strong> context of gravitation, accord<strong>in</strong>g to<br />

Newton’s law of gravitation Galileo’s law of fall<strong>in</strong>g bodies is<br />

strictly speak<strong>in</strong>g false: The acceleration <strong>in</strong>creases <strong>in</strong>stead<br />

of be<strong>in</strong>g constant. Hence <strong>the</strong>se <strong>the</strong>ories contradict each<br />

o<strong>the</strong>r, <strong>and</strong> <strong>the</strong>refore a deduction is simply impossible <strong>and</strong><br />

any “derivation” of Galileo’s law from Newton’s law of<br />

gravitation must thus conta<strong>in</strong> some contra-to-fact<br />

assumptions. Such assumptions can <strong>in</strong> this case be <strong>and</strong><br />

are widely <strong>in</strong> physical derivations hidden <strong>in</strong> limit<strong>in</strong>g<br />

processes where some parameter, which is not zero or<br />

<strong>in</strong>f<strong>in</strong>ite with<strong>in</strong> <strong>the</strong> law to be derived, is taken to be zero or<br />

<strong>in</strong>f<strong>in</strong>ite. In our case <strong>the</strong> distance to earth of <strong>the</strong> fall<strong>in</strong>g body<br />

compared to <strong>the</strong> earth’s radius is taken to be zero - but <strong>the</strong><br />

law derived under this assumption is strictly speak<strong>in</strong>g only<br />

valid for bodies lay<strong>in</strong>g down on <strong>the</strong> earth’s surface, while<br />

Galileo’s law is about fall<strong>in</strong>g bodies. Thus <strong>the</strong> common<br />

mode of speak<strong>in</strong>g that this derivation delivers approximate<br />

validity only for small distances covers <strong>the</strong> fact that we<br />

haven’t deduced Galileo’s law but ra<strong>the</strong>r established a<br />

comparison between <strong>the</strong> two <strong>the</strong>ories under certa<strong>in</strong><br />

circumstances: This is all we can say about “approximate<br />

derivations” here <strong>and</strong> similarly elsewhere.<br />

Never<strong>the</strong>less, Galileo’s law is superfluous, not<br />

because of be<strong>in</strong>g deduced, but ra<strong>the</strong>r because Newtonian<br />

physics can also describe fall<strong>in</strong>g bodies, <strong>in</strong> a similar<br />

manner as Galileo’s law as shown <strong>in</strong> <strong>the</strong> comparative<br />

limit<strong>in</strong>g process. But if “reduc<strong>in</strong>g” <strong>the</strong>ories are more<br />

complex it is far from certa<strong>in</strong> that <strong>the</strong>y are able to<br />

reproduce any statement of a <strong>the</strong>ory to be reduced.<br />

Comparisons between <strong>the</strong>ories <strong>in</strong> <strong>the</strong> sense of<br />

approximate derivation seem to be just comparisons of<br />

ma<strong>the</strong>matical structure <strong>and</strong> not of concrete explanations of<br />

phenomena - <strong>and</strong> <strong>the</strong> possibility to compare ma<strong>the</strong>matical<br />

structure does not <strong>in</strong>clude that <strong>the</strong> “reduc<strong>in</strong>g” <strong>the</strong>ory is able<br />

128<br />

at all to deal with <strong>the</strong> phenomena expla<strong>in</strong>ed by <strong>the</strong> <strong>the</strong>ory<br />

to be reduced as it is <strong>the</strong> case <strong>in</strong> our simple example. If we<br />

are able to deduce <strong>the</strong> laws of a <strong>the</strong>ory we are<br />

automatically able to expla<strong>in</strong> <strong>the</strong>ir phenomena but we can’t<br />

expect to be able to do that by virtue of comparisons<br />

between ma<strong>the</strong>matical structures as we will see <strong>in</strong> <strong>the</strong><br />

clos<strong>in</strong>g part of this presentation, which discusses <strong>the</strong> case<br />

of general relativity <strong>in</strong> this respect.<br />

This po<strong>in</strong>t doesn’t catch one’s eye if one considers<br />

simple cases like that of Galileo’s law <strong>and</strong> has <strong>the</strong>refore<br />

widely been overlooked with<strong>in</strong> <strong>the</strong> debate of reduction. But<br />

<strong>in</strong>ter<strong>the</strong>oretic relations <strong>in</strong> physics actually are <strong>in</strong> many<br />

cases noth<strong>in</strong>g but comparisons between ma<strong>the</strong>matical<br />

structures: A look at <strong>the</strong> details shows, that e.g. <strong>in</strong> <strong>the</strong> case<br />

of <strong>the</strong> Newtonian <strong>the</strong>ory of gravitation <strong>and</strong> general relativity<br />

<strong>the</strong> <strong>in</strong>ter<strong>the</strong>oretic relation is much more complicated than a<br />

limit<strong>in</strong>g process <strong>and</strong> far from be<strong>in</strong>g well established. A<br />

ma<strong>the</strong>matical relation <strong>in</strong> a precise manner between <strong>the</strong>se<br />

<strong>the</strong>ories is given e.g. <strong>in</strong> (Scheibe 1999) <strong>in</strong> terms of a<br />

topological comparison between sets of models of <strong>the</strong>se<br />

<strong>the</strong>ories formulated axiomatically (cf. p. 59-108 for <strong>the</strong><br />

case of general relativity). And while <strong>the</strong>re are only s<strong>in</strong>gle<br />

cases <strong>in</strong> which explanations of concrete phenomena can<br />

be compared (e.g. <strong>the</strong> planet’s orbits, cf. p. 89-101),<br />

Scheibe’s “reduction” of <strong>the</strong> whole Newtonian <strong>the</strong>ory of<br />

gravitation is not completely worked out <strong>and</strong> can ei<strong>the</strong>r<br />

way be no deduction but noth<strong>in</strong>g but a very subtle<br />

comparison between ma<strong>the</strong>matical structure.<br />

The second of Feyerabend’s objections concerns<br />

language <strong>and</strong> <strong>the</strong> <strong>in</strong>commensurability of <strong>the</strong> vocabulary of<br />

different <strong>the</strong>ories. In our context, <strong>the</strong> equation of motion<br />

with<strong>in</strong> general relativity is <strong>the</strong> geodesic equation for neutral<br />

test particles whereas Newton’s law of gravitation<br />

describes a force between two masses. We thus are<br />

concerned with two entirely different concepts <strong>and</strong> <strong>the</strong><br />

identification of <strong>the</strong> Newtonian gravitational potential with<br />

Christoffel Symbols, which can be found <strong>in</strong> physics<br />

textbooks (cf. e.g. (Misner et al. 1973), chapter 12), is a<br />

“component manipulation” (l.c., p. 290) ra<strong>the</strong>r than a basis<br />

for a deduction. Even more concrete, <strong>in</strong> <strong>the</strong> example of <strong>the</strong><br />

planet’s orbits <strong>the</strong>ir description with<strong>in</strong> <strong>the</strong> Schwarzschild<br />

solution deals with test particles without <strong>in</strong>fluence to <strong>the</strong><br />

overall curvature <strong>and</strong> thus without gravitational masses<br />

whereas <strong>the</strong>ir Newtonian description is based on forces<br />

between just <strong>the</strong>se masses. Therefore, <strong>the</strong>se concepts<br />

cannot be related by any simple identification <strong>and</strong> we have<br />

to concede that we cannot establish reductions via logical<br />

deduction with <strong>the</strong> help of bridge laws.<br />

But never<strong>the</strong>less <strong>the</strong>ories need not to be<br />

<strong>in</strong>commensurable – we can of course compare <strong>the</strong><br />

concepts of different <strong>the</strong>ories. But this is <strong>in</strong> general a<br />

difficult <strong>and</strong> not straight forward comparison process far<br />

from be<strong>in</strong>g able to establish bridge laws suit<strong>in</strong>g for a<br />

logical deduction. We can relate <strong>the</strong> terms of two <strong>the</strong>ories<br />

with <strong>the</strong> help of special case studies <strong>and</strong> prove that e.g.<br />

<strong>the</strong> Newtonian potential is somehow related to <strong>the</strong><br />

Christoffel symbols, but such case studies are no selfevident<br />

processes <strong>and</strong> aga<strong>in</strong> lead to a compar<strong>in</strong>g relation<br />

ra<strong>the</strong>r than a deduction, <strong>and</strong> such a comparison on its own<br />

doesn’t make any <strong>the</strong>ory superfluous.

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