Topologically, of course, it has 1: it's homeomorphic to a punctured disk. But intuitively it has 2: one at the top and one at the bottom. And this answer lies at the heart of the most rigorous axiomatization of quantum field theory. (1/20)
In this intuitive picture, the two "holes" of the straw are 1-dimensional circles, and they're connected by a 2-dimensional cylinder (the straw itself). Mathematically, this relationship is called a "cobordism". Two n-dimensional manifolds are "cobordant" if they form... (2/20)
...the boundary of some n+1-dimensional manifold (like the two circles forming the boundary of the cylinder). And cobordisms give one a natural framework for thinking about time evolution in physics. Suppose we have two moments in time: t1 and t2, with t1 < t2. (3/20)
We can think of these moments as being 0-dimensional manifolds, and the interval [t1, t2] as being a 1-dimensional cobordism between them. We can call this collection of moments and intervals a "1-dimensional cobordism category" since it satisfies the axioms of a category. (4/20)
Namely, the composition/union of intervals is associative (since it doesn't matter in what order you take unions) and has an identity operation (the trivial interval [t, t] can act as a "do nothing" operation under composition). And in quantum mechanics, each moment... (5/20)
...of time t1 can be mapped to a vector space V1 (the "space of quantum states" at that time), and each time interval [t1, t2] can be mapped to a unitary operator U: V1 -> V2 (obtained from the Schrödinger equation, by exponentiating the time integral of the Hamiltonian). (6/20)
The union of intervals maps to a composition of unitary operators. The identity interval [t, t] maps to the identity operator. We call this map from the category of moments and intervals to the category of vector spaces and unitary operators a "cobordism functor"... (7/20)
...since it is a structure-preserving map (i.e. a functor) between cobordism categories. So time evolution in QM can be recast as a cobordism functor (there is a lot of other algebraic structure here that I'm neglecting, e.g. tensor products, duals, Hermitian adjoints). (8/20)
But this all seems a bit heavy-handed: why bother with cobordism categories when we're just dealing with 0-dimensional manifolds and 1-dimensional cobordisms? Well, in QM, we don't need to. But what happens when we try to make this description relativistically invariant? (9/20)
In relativity, we can't think in terms of single moments of time: we have to think in terms of *simultaneity surfaces* (i.e. spacelike hypersurfaces). So our cobordism category now consists of 3-dimensional spacelike hypersurfaces, joined by 4-dimensional spacetime... (10/20)
...volumes (in place of our previous 1-dimensional intervals). Our cobordism functor now maps each spacelike hypersurface to a space of quantum states, and each spacetime volume (or "foliation") to a unitary transformation. So this functor describes a covariant version... (11/20)
...of QM, i.e. a quantum field theory. Except... not quite. Because, unlike in the non-covariant case with 0-dimensional moments of time, in the covariant case there isn't just *one* foliation of spacetime connecting two spacelike hypersurfaces (i.e. a preferred frame). (12/20)
There exists an infinite family of spacetime foliations connecting any two spacelike hypersurfaces (all related by smooth gauge transformations), so our cobordism category must somehow contain an infinite family of cobordisms connecting any two 3-dimensional manifolds. (13/20)
So how do we include these gauge transformations? Well, a (linear) gauge transformation relating two 4-dimensional spacetime foliations can *itself* be formalized as a 5-dimensional cobordism between spacetimes. In other words, a cobordism between cobordisms. (14/20)
We've now entered the recursive world of higher category theory: cobordism 2-categories containing both cobordisms between manifolds *and* cobordisms between cobordisms, plus cobordism 2-functors relating those 2-categories together. But it doesn't stop there. (15/20)
We've so far only encoded the *linear* gauge transformations: for full covariance, we have to keep going, adding 6-dimensional cobordisms between the 5-dimensional ones, 7-dimensional ones between the 6-dimensional ones, etc. All the way up to infinity. (16/20)
So we finally reach a cobordism ∞-functor between cobordism ∞-categories: one encoding hypersurfaces and their spacetime transformations, the other encoding spaces of quantum states and their unitary transformations. In QFT, this functor is called the "path integral". (17/20)
This idea that QFT could be formalized in terms of cobordisms and ∞-categories goes back to Segal (for conformal field theory) and Atiyah (for topological field theory), through Baez and Dolan (the cobordism hypothesis), to Lurie, Grady and Pavlov in the present day. (18/20)
It has been the most successful program for formalizing QFT to date, generalizing earlier results such as Wightman's axioms and the Haag-Kastler axioms. But it still works only for very restricted cases: countable degrees of freedom (TQFT) or conformal symmetry (CFT). (19/20)
Could such a formalization work for the "real" QFTs that appear to be of relevance to our actual universe (i.e. Yang-Mills theories)? Nobody knows. But straws, cobordisms, and ∞-categories seem like a promising place to look. (20/20)
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The desiccated "Theorem, Lemma, Proof, Corollary,..." presentational style is staggeringly counterproductive, if one's objective is actually communicating the underlying mathematical intuitions and thought processes behind a result. In reality, the process is more like... (1/4)
"First, I tried <standard method>, but it failed for <enlightening reason>, so I investigated whether I could exploit this fact to find <counterexample> with <property>, but all objects obtained through this technique ended up having <interesting property> in common.... (2/4)
...So I tried relaxing <axiom> to see whether <related property> could be removed, and this led me to realize that <intermediate lemma> is actually crucial to the structure of <related object>..." Etc. You occasionally get these insights from (very good) mathematical talks. (3/4)
What's a gravitational wave? Anything that distorts the shape of spacetime, but preserves its volume.
What's matter/energy/momentum? Anything that distorts the volume of spacetime, but preserves its shape.
A 🧵 on the Ricci decomposition theorem, as applied to gravity. (1/13)
Classical gravity is a manifestation of the Riemann curvature of spacetime, which describes how your coordinate system distorts as you move from point to point. More precisely, the *connection* describes how the coordinate system distorts, and the Riemann curvature... (2/13)
...describes how the connection distorts. So the Riemann curvature is effectively a second derivative of your coordinate system. The Ricci decomposition theorem then says that the Riemann curvature can be decomposed into two pieces: a "trace" part and a "trace-free" part. (3/13)
Calling c the "speed of light" completely misses the point. Rather, c is the "spacetime exchange rate": how many units of space you can exchange for one unit of time.
In actuality, everything travels at the "speed of light", just not necessarily through space alone... (1/4)
Rather, everything travels through both space *and* time, simultaneously, with a speed of c. If you're standing still, then all of your velocity is focused in the time direction (with none in the space directions), so you move through time with a speed of c. (2/4)
If you start moving, then now a little bit of your velocity vector points in one of the space directions, so a little bit less must point in the time direction. So you move through time slightly slower than c, such that your overall speed through space *and* time remains c. (3/4)
Consider a rotating disk. What does it mean to say that the disk has angular momentum? Well, imagine assigning a momentum vector to every point on the surface of the disk, and then slicing through the middle of the disk with a flat surface. (1/14)
The "net flux” of momentum vectors through the surface is zero, since every momentum vector poking through the surface in one direction is counteracted by a momentum vector poking through in the opposite direction. In other words, the disk has no *linear* momentum. (2/14)
But the "total flux" of momentum vectors (i.e. the total amount of momentum intersecting the surface, irrespective of direction) is clearly non-zero, because the disk is rotating. This discrepancy between the total flux vs. the net flux is what we call "angular momentum". (3/14)
Birkhoff's theorem tells us that the spacetime around a non-rotating black hole is indistinguishable from that around any other non-rotating compact object, like a neutron star.
But what if it's rotating? Turns out, the differences can be *huge*. (1/4)
Link:
Though the spacetime around an uncharged black hole depends on two parameters (mass and spin) by the no-hair theorem(s), objects like neutron stars have "hair" in the form of many other multipole moments: mass quadrupole, spin octupole, etc. (2/4)arxiv.org/abs/2505.05299
Most calculations and simulations of neutron stars assume that such moments don't matter (i.e. that the geometry is well-described by the Kerr metric of a spinning black hole). We show that this isn't true, for physically realistic neutron stars spinning at moderate speeds. (3/4)
My recent "dunk" about encoding functions and the algorithmic/Kolmogorov complexity of the laws of physics may have seemed flippant, but it actually goes back to an old 17th century philosophical conundrum: the dichotomy between idealism and materialism.
When attempting to model the world computationally, there are typically *three* computations that one needs to consider: the computation that the system itself (e.g. the universe) performs, the computation that the observer performs, and the "encoding function". (2/14)
The encoding function is the computation that maps between states of the system and states of the observer. You might think that the system's computation is the only one that matters, but science is full of examples where the state of "the observer" matters too. (3/14)