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单词 ProofOfHausdorffParadox
释义

proof of Hausdorff paradox


We start by outlining the general ideas, followed by the strict proof.

General approach

The unit sphereMathworldPlanetmath S2 in the Euclidean space 3 isfinite in the sense that it is http://planetmath.org/node/4826bounded and has a finite volume:43π.

On the other hand, S2 is an infiniteMathworldPlanetmath point set. As everyone who hasever visited Hilbert’s Hotel knows, it is possible to split aninfinite set, such as the natural numbersMathworldPlanetmath, in pieces and all piecesare, in a sense, equal to the original set, for example if

3:={nn is divisible by 3},

then naïvely 3 has a third of the size of , andhalf of the size of 3. There exists,however, a bijectionMathworldPlanetmath from to 3, so3 has, again naïvely, both half and a third ofthe size of .

To do the same thing with S2, bijections won’t suffice, however: weneed isometriesMathworldPlanetmath to establish congruenceMathworldPlanetmathPlanetmathPlanetmathPlanetmath. We can almost reducethis problem to the case of bijections in the following way. The groupR of rotationsMathworldPlanetmath (rotations are isometries) in 3 acts onS2 (say, from the right). Given an countably infiniteMathworldPlanetmath subgroupMathworldPlanetmathPlanetmath Gof R which acts freely (or almost so) on S2, take a set of http://planetmath.org/node/1517orbitrepresentatives M of the action of G on S2 (this requires thehttp://planetmath.org/node/310axiom of choiceMathworldPlanetmath). Then a disjoint decompositionG1,Gn of G intocountable sets acting on M yields a disjoint decomposition ofS2. Doing similarMathworldPlanetmathPlanetmathPlanetmath juggling with G1,,Gn as we did with, 3 and 3 above shouldyield the result, if all the G1,Gn are related by fixedisometries, for example if G1=G2φ for some isometryφ, and similar relationsMathworldPlanetmathPlanetmath for the other pieces. This lastrestrictionPlanetmathPlanetmathPlanetmath will make the proof possible only in three or moredimensionsPlanetmathPlanetmathPlanetmath, and indeed, Banach and Tarski later showed in [BT]that analogous theorems on the line or in the plane do not hold.

The proof

Let G be the subgroup of rotations of 3 generated by ahalf rotation φ and a one third rotation ψ arounddifferent axes. We fix an orthonormal basis for the restof the proof, so we may identify φ and ψ with theirrotation matricesMathworldPlanetmath acting from the right on the row vectorsMathworldPlanetmath of3, such that without restriction

ψ=(λμ0-μλ0001),φ=(-cosϑ0sinϑ0-10sinϑ0cosϑ),

where λ=cos2π3=-12,μ=sin2π3=123 and ϑ isarbitrary for now.

Since φ2=1 and ψ3=1, there existsfor each element g from G other than the unity, ϕ, ψ or ψ2 apositive integer n and numbers mk{1,2}, 1kn,such that g can be written in one of the following ways:

  • (α)

    (k=1nφψmk),

  • (β)

    ψm1(k=2nφψmk)φ,

  • (γ)

    (k=1nφψmk)φ,

  • (δ)

    ψm1(k=2nφψmk)(n2).

To have completePlanetmathPlanetmathPlanetmathPlanetmathPlanetmathPlanetmath control over the structureMathworldPlanetmath of G, we fix ϑin such a way, that g can be written uniquely in one of theways (α)–(δ), with fixed n and mk. In other words: wefix ϑ such that the unity 1 cannot be written inone of the ways (α)–(δ).

To see how to do that, let us see to where the vector (0,0,1) istransported by a transformationMathworldPlanetmath of type (α). It is easilyverified that

φψ=(-λcosϑ-μcosϑsinϑμ-λ0λsinϑμsinϑcosϑ) and φψ2=(λcosϑ-μcosϑsinϑμλ0-λsinϑμsinϑcosϑ),

so that(0,0,1)φψ=(λsinϑ,μsinϑ,cosϑ)and(0,0,1)φψ2=(-λsinϑ,μsinϑ,cosϑ).More generally, let n be a positive integer, p1,p2 polynomialsof degree n-1 and p3 a polynomial of degree n, then

(p1(cosϑ)sinϑ,p2(cosϑ)sinϑ,p3(cosϑ))φψ=((λp3(cosϑ)+μp2(cosϑ)-λcosϑp1(cosϑ))sinϑ,(μp3(cosϑ)-λp2(cosϑ)-μcosϑp1(cosϑ))sinϑ,(1-cos2ϑ)p1(cosϑ)+p3(cosϑ)),
(p1(cosϑ)sinϑ,p2(cosϑ)sinϑ,p3(cosϑ))φψ2=((-λp3(cosϑ)+μp2(cosϑ)+λcosϑp1(cosϑ))sinϑ,(μp3(cosϑ)+λp2(cosϑ)-μcosϑp1(cosϑ))sinϑ,(1-cos2ϑ)p1(cosϑ)+p3(cosϑ)).

By inductionMathworldPlanetmath, it follows that (0,0,1) is transported by atransformation of type (α) to a vector whose third componentMathworldPlanetmathPlanetmathPlanetmath isa nonconstant polynomial p in cosϑ. If we restrict ϑ such that0ϑπ, there are only finitely many values forϑ such that p(cosϑ)=1. Given all possiblecombinationsMathworldPlanetmathPlanetmath of n and mk, 1kn, there are in totalonly countably many problematic values for ϑ, so we caneasily fix hereby an unproblematic one. Now that the case (α)has been dealt with, so have been the others automatically. For assumeone could write a 1 of type (γ), one could convert it to type(δ) by 1=φ1φ, and from type δ to type(α) or type (β) by 1=ψ3-m11ψm1, andlastly from type (β) to type (α) by 1=φ1φ,completing the contradictionMathworldPlanetmathPlanetmath.

Now that we know the structure of G, how does it act on S2?Certainly not freely, since every rotation other than the unity hasits axis as fixed pointPlanetmathPlanetmathPlanetmath set, which in case of the sphere makes twofixed points per rotation. The productPlanetmathPlanetmath of two rotations is again arotation. Furthermore G is finitely generatedMathworldPlanetmath and so iscountableMathworldPlanetmath. So there are only countably many points of S2 where theaction of G fails to be free. Denote the set of these points by D,so that G acts freely on E:=S2D. The action creates apartitionMathworldPlanetmathPlanetmath on E into orbits. The allows us to choosea set M, such that M meets any orbit in precisely one element. Wehave then the disjoint unionMathworldPlanetmath

E=gGMg,

where Mg is the image of M under the action of the group elementg. We now define three sets A, B, C to be the smallest sets satisfying:

  • M1=MA;

  • if Mg is a subset of A, B or C, then Mgφ is asubset of B, A or A, respectively;

  • if Mg is a subset of A, B or C, then Mgψ is asubset of B, C or A, respectively;

  • if Mg is a subset of A, B or C, then Mgψ2 is asubset of C, A or B, respectively.

The sets A, B and C are well-defined because we ensured theuniqueness of the representations (α)–(δ) above.

The sets A, B, C and BC are all congruentMathworldPlanetmath by virtue of

Aψ=B,Aψ2=CandAφ=BC.

Since S2=ABCD, a disjoint union, and D iscountable, the theorem is proven.

References

  • BT St. Banach, A. Tarski, Sur la décompositionMathworldPlanetmathPlanetmathdes ensembles de points en parties respectivement congruentes,Fund. math. 6, 244–277, (1924).
  • H F. Hausdorff, Bemerkung über den Inhalt vonPunktmengen, Math. Ann. 75, 428–433, (1915).
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更新时间:2025/5/24 21:06:54