Author Archives: Michael Weiss

Set Theory Jottings 10. Axiomatic Set Theory

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“An Axiom, you know, is a thing that you accept without contradiction. For instance, if I were to say ‘Here we are!’ that would be accepted without any contradiction, and it’s a nice sort of remark to begin a conversation with. So it would be an Axiom. Or again, supposing I were to say, ‘Here we are not!’, that would be—”

“—a fib!” cried Bruno.

“that would be accepted, if people were civil”, continued the Professor; “so it would be another Axiom.”

“It might be an Axledum”, Bruno said: “but it wouldn’t be true!

—Lewis Carroll, Sylvie and Bruno Concluded

To get to the “good stuff” in math, you almost always need some set theory. Zermelo-Fraenkel set theory (ZF), plus the axiom of choice (AC; ZF+AC=ZFC) has become the standard first-order axiom system for set theory.

Before diving into the details, some generalities on axiom systems. Nowadays we’re pretty chill about them; you can take any collection you like (hopefully consistent) for a theory, and then you can start writing your thesis. Not, perhaps, an interesting thesis, but at any rate Bruno won’t complain that your axioms aren’t true!

For the Greeks, the axioms and postulates were true, in some sense. Idealized, sure, but descriptive of reality. This tie began to fray with the discovery of non-Euclidean geometries. Algebraic axiom systems, like those for groups and for fields, appear by the end of the 19th century.

For roughly two thousand years after Euclid, most math developed without axioms. Take calculus as an example. You have the rules of calculus, but you don’t see anything like the Euclidean treatment of geometry. This remained true even as people subjected its foundations to stricter and stricter scrutiny. Mathematical intuition reigned supreme.

Hilbert’s Grundlagen der Geometrie (Foundations of Geometry, 1899) pushed towards a more formalist attitude. A celebrated quote of his, from years earlier, sums it up nicely:

One must be able to say at all times, instead of points, lines, and planes: tables, chairs, and beer mugs.

At times Cantor seemed to endorse this perspective:

Mathematics is entirely free in its development, and its concepts are only bound by the necessity of being consistent, and being related to the concepts introduced previously by means of precise definitions.

Grundlagen einer allgemeinen Mannigfaltigkeitslehre (Foundations of a general theory of sets)

But he held strong opinions on what’s true in mathematics:

I entertain no doubts as to the truths of the tranfinites, which I recognized with God’s help and which, in their diversity, I have studied for more than twenty years; every year, and almost every day brings me further in this science.

—Letter from Cantor to Jeiler, quoted in Dauben (p.147).

On the other hand, he referred to the “Cholera-Bacillus of infinitesimals”, and called them “nothing but paper numbers!” (Dauben, p.131). The Continuum Hypothesis was for him a question of fact.

Two other themes run through this period: mathematics as a mental activity, and as logic.

Recall that Boole titled his famous treatise An Investigation of the Laws of Thought: on Which are Founded the Mathematical Theories of Logic and Probabilities. Cantor’s definition of “set” in his last major work reads

By a set we are to understand any collection into a whole M of definite and separate objects m of our intuition or our thought.

Here is the first sentence of Dedekind’s Was sind und sollen die Zahlen?: “In what follows I understand by thing every object of our thought.” His proof of the existence of an infinite set relies on this ontology:

Theorem: There exist infinite systems.

Proof: My own realm of thoughts, i.e., the totality S of all things which can be objects of my thought, is infinite. For if s signifies an element of S, then the thought s′, that s can be an element of my thought, is itself an element of S

[Dedekind then appeals to his definition of infinite as having a bijection with a proper subset.]

Frege severely criticized this injection of psychology into mathematics. Cantor’s “proof” of the Well-Ordering Theorem suffers from it, as it consists of successively choosing elements of the set to be well-ordered. If we take this literally, then the choices must take place at an increasing sequence of times t1<t2<…. This limits us to ordinals that are “realizable in ℝ’’, and thus to countable ordinals (see post 4). Yet Cantor claimed that every set can be well-ordered, in particular ℝ.

This is why Zermelo was at pains to say in his second proof of the Well-Ordering Theorem, “…the ‘general principle of choice’ can be reduced to the following axiom, whose purely objective character is immediately evident.” (My emphasis.)

Both Frege and Russell held that the truths of mathematics are logical facts. Thus we find debates on whether Zermelo’s axiom of choice is logically valid. Not surprising, historically. Aristotle’s logic dealt with propositions. From “proposition” we obtain “propositional function”, that is, a proposition with a free variable, like “x is mortal”. It becomes a proposition if we assign a value to the variable (“Socrates is mortal”), or quantify over it (“All men are mortal”). The class of all things satisfying a propositional function went by the name, “extension of a concept”.

Zooming out from these specifics, logic and mathematics both lay claim to necessary truth. This is elaborated in Kantian philosophy. Kant classified mathematical facts as synthetic a priori: necessary truths that go beyond analytic truth, which are true by definition. Poincaré classified the Axiom of Choice as a synthetic a priori judgment, just like the principle of induction.

The rise of formal logic and axiomatic set theory resulted in a sharply drawn boundary between logic and set theory. We have the axioms and rules of inference of first-order logic; then we have the axioms of ZFC or similar systems, which are particular first-order theories. Things weren’t so clear at the dawn of the 20th century.

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From Kepler to Ptolemy 16

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Kepler

Kepler wrote five major astronomical works. Chronologically:

the Mysterium cosmographicum (1596)

the Astronomia nova (1609)

the Epitome astronomiae Copernicanae (1618–1622)

the Harmonice mundi (1619)

and the Tabulae Rudolphinae (1627).

The Mysterium cosmographicum (Cosmographical Mystery) expresses Kepler’s youthful enthusiasm and sounds the leading notes to themes that would persist throughout his career. Kepler’s elliptical orbits and the area speed law make their debut in the Astronomia nova (New Astronomy). (Although at this point Kepler regarded the area law as just an approximation to the inverse speed law.) The Epitome astronomiae Copernicanae (Epitome of Copernican Astronomy) completes and refines his theory. The Harmonice mundi (Harmonies of the World) contains the statement of Kepler’s 3rd law, its main scientific claim to fame. The Tabulae Rudolphinae (Rudolphine Tables) ultimately led to the widespread acceptance of Keplerian astronomy.

He also wrote several lesser astronomical works, and treatises on optics, on computing volumes, on the philosophy of science, a pamplet on snowflakes… The critical edition of his collected works runs to 22 volumes. I will focus just on the Mysterium cosmographicum and the Astronomia nova.

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Set Theory Jottings 9. Cantor Normal Form

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Suppose β>1, and let ζ>0 be arbitrary. Then ζ has a unique representation in so-called Cantor normal form:

ζ α1 χ1+···+βαk χk
α1>···>αk, 1≤χi<β for all i
(1)

Stillwell gives an illustration, close to a proof, in §2.6 (pp.46–47)1, for the most important special case: β=ω and ζ<ε0. (The Cantor normal form for ε0 is just ωε0, not helpful.)

Here’s a more formal proof of the full theorem. First generalize division to all ordinals. If β>1, then any ζ has a unique representation in the form

ζ= βχ+ρ,   ρ<β

Proof: since β>1, β(ζ+1)≥ζ+1, and so there is a least χ′ such that βχ′>ζ. Furthermore χ′ cannot be a limit ordinal: if βξ≤ζ for all ξ<λ, then βλ≤ζ by continuity of multiplication. Set χ=χ′−1, so

βχ≤ζ<β(χ+1)

Now write (by equation (7) of post 8)

ζ=βχ+(−βχ+ζ)=βχ+ρ

setting ρ=−βχ+ζ. We cannot have ρ≥β, otherwise

ζ=βχ+ρ≥βχ+β=β(χ+1)>ζ

Uniqueness needs to be done just right, since ordinal addition has cancellation on the left but not on the right. Suppose

βχ11=βχ22,    ρ12

If χ12 then χ21+γ for some γ>0. So

βχ11=β(χ1+γ)+ρ2=βχ1+βγ+ρ2

Cancelling on the left,

ρ1=βγ+ρ2≥βγ≥β

contradicting the definition of ρ1. So χ12=χ (say), and we can cancel βχ on the left to get ρ12.

The proof of Cantor normal form starts out in a similar fashion. First prove by induction that βα≥α for all α. Since βζ+1>ζ, it follows that there is a least α with βα>ζ. Furthermore α cannot be a limit ordinal by continuity of exponentiation (in the exponent). Set α1=α−1. So

βα1≤ζ<βα1+1

Now we divide ζ by βα1:

ζ=βα1χ11,    ρ1α1

We cannot have χ1≥β, otherwise

ζ=βα1χ11≥βα1β=βα1+1

Repeat with ρ1:

ρ1α2χ22,   χ2<β,   ρ2α2

We must have α21 because βα2≤ρ1α1. Continuing we get a descending sequence of αi’s which must terminate in finitely many steps, because ordinals. This establishes (1).

The proof of uniqueness provides a bonus: a criterion for which of two normal forms is larger. It’s what you’d expect from decimal notation. Suppose

ζ α1 χ1+···+βαk χk
ζ′ = βα1 χ1′+···+ βαm χm

are two unequal normal forms. Because cancellation on the left holds for addition, we can remove any equal terms on the left, and assume either α11′ or α11′ and χ11′ (for the reverse inequalities, just flip things around). Then ζ<ζ′. I will call this the first difference criterion for the ordering of Cantor normal forms.

The proof resembles a decimal computation. To show that 999<1000 (for example), we add 1 and do the carries. Here, we begin by combining the last two terms of ζ, using the facts that χk<β and αk−1k:

βαk-1 χk-1αk χk αk-1 χk-1αk+1
≤βαk-1 χk-1αk-1
αk-1k-1+1)

Next we combine with the previous term, using the fact that χk−1+1≤β and αk−2k−1:

βαk-2 χk-2αk-1k-1+1) ≤βαk-2 χk-2αk-1+1
≤βαk-2k-2+1)

We keep going, until eventually we have

ζ<βα11+1)

If α11′ and χ11′, then we have βα11+1)≤βα1 χ1′. Thus ζ is less than the first term of ζ′. If α11′ then we use the fact that χ1+1≤β, concluding that βα11+1)≤βα1+1≤βα1, and hence ζ is again less than the first term of ζ′. A fortiori, ζ<ζ′.

Uniqueness follows. These ordering criteria are needed for the Goodstein and Hydra theorems.

[1] However, Stillwell messes up at the end of the example. In the last bullet he says, “This means that α is a term in the following sequence with limit ωω2·7+ω·4+11+ω= ωω2·7+ω·4+12.” This equation is incorrect; the last “+ω’’ should be “·ω’’. The sequence on the next line should have “·1’’, “·2’’, etc., instead of “+1’’, “+2’’, etc. So he has many more steps to go.

Another point. When he says that α “falls between” two terms in a sequence, he’s not entitled to assume it falls strictly between. He should say instead that there are two consecutive terms with α greater than or equal to the first and less than the second.

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Set Theory Jottings 8. Ordinal Arithmetic

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Usually one defines the ordinal operations via transfinite induction:

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From Kepler to Ptolemy 15

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The Planetary Hypotheses

In the Planetary Hypotheses, Ptolemy lays out his cosmology: that is, the structure and arrangement of the universe. This work answers the question, did Ptolemy believe in the physical truth of the Almagest’s celestial geometry?—with an unambiguous Yes. Contrary to an opinion often expressed by earlier historians, he did not regard it just as a calculational scheme for predicting planetary positions.

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Set Theory Jottings 7. The (Cantor-Dedekind-Schröder)-Bernstein Theorem

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The trichotomy of cardinals says that for any 𝔪 and 𝔫, exactly one of these holds: 𝔪<𝔫, 𝔪=𝔫, or 𝔪>𝔫. It’s equivalent to the conjunction of these two propositions, for any two cardinals 𝔪 and 𝔫:

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From Kepler to Ptolemy 14

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Cycle Counts

You may have heard that Ptolemaic systems grew to have 80 spheres or cycles, while the Copernican system had only 34. This is a myth.

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Set Theory Jottings 6. Zorn’s Lemma

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Zermelo’s 1904 proof of the well-ordering theorem got a lot of blowback, as we’ve seen. On the other hand, the very next year Hamel used it to prove the existence of a so-called Hamel basis. In 1910, Steinitz made numerous applications in the theory of fields. He wrote:

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From Kepler to Ptolemy 13

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Latitudes

First thing to note about Ptolemy’s latitude theory: its decoupling from the longitude theory. For longitudes, one projects the orbits into the ecliptic plane. The actual speeds will differ from the projected speeds. However, the effect is small because the inclinations are fairly small (see the table below), and Ptolemy’s longitude computations ignore it. The latitude algorithms use the longitude as an input.

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From Kepler to Ptolemy 12

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Mercury

Mercury refused to cooperate with Ptolemy’s basic paradigm. You might guess that the fault lies with Mercury’s larger eccentricity, but studies show that bad data bears most of the blame. Mercury hugs the Sun, only appearing near the horizon close to sunrise or sunset, hardly ideal observation conditions.

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