5 ms·
Think about 2D surfaces. Which ones are the most symmetric? A flat plane is a very nice space: every point is as good as any other (there’s nothing intrinsic to
by zachf 5y ago
Think about 2D surfaces. Which ones are the most symmetric? A flat plane is a very nice space: every point is as good as any other (there’s nothing intrinsic to any point to distinguish any point from any other, except arbitrarily), and no direction is particularly special either. A space like that has a lot of symmetries. A sphere also has a lot of symmetries, it also has no directions or points which are distinguished until you declare, “this is my North Pole” arbitrarily. (The earth isn’t a perfect sphere of course and we can use the imperfections as the way we define north and south.) The last type of symmetric space looks like a saddle (like on a horse). It bends one way in one direction and bends the other way in the other direction. An idealized saddle also has no distinguished directions or points.
The analogs of these things in higher dimensions, and where one of the directions is time, are important in general relativity. The analog of the plane is called “flat space” or “Minkowski space”. The analog of the sphere is “de Sitter space”. Finally, the analog of the saddle is “anti-de Sitter space” (usually abbreviated AdS, with a lowercase d). It’s a bit of an odd space in a lot of ways. When you look at what space looks like at any given time, it’s a bit like M.C. Escher’s “Angels and Devils”.
Surprisingly, Anti-de Sitter space is the easiest space to understand quantum aspects of gravity in. That’s because anti-de Sitter space is curved in such a way that the complicated stuff can be neatly separated from the easy stuff. You can start from something you understand well and turn on the complexity piece by piece. Roughly speaking it’s because the gravitational stuff becomes less important as you go farther and farther away from any matter you’re considering, in a way which is even faster than this happens in flat space or de Sitter space. It turns out that we can exactly understand everything in this gravitational theory by mapping the physics one-to-one to a nongravitational model which we understand really well. There’s a lot of evidence that the map works perfectly. This is called the AdS/CFT correspondence. A lot of work goes into testing the correspondence and attempting to prove it, and this is a big research area.
de Sitter space doesn’t have the same desirable properties. Nevertheless there has been great progress in understanding quantum properties of de Sitter in the last year [0]. These results would not have been possible without understanding AdS first.
Flat space quantum gravity remains challenging, although again some progress has been made recently too [1].
[0] arxiv:2110.14670
[1] arxiv:1905.09809 and many others
- verve_rat 5y agoThanks for the fantastic explanation. So there is flat space, de Sitter space, and Anti-de Sitter space, do we know which one most closely resembles the world we observe?
- zachf 5y agoStrictly speaking it’s none of them, because those are idealized perfectly symmetrical spaces with no matter in them, only dark energy, and our universe (happily) has matter in it :). But it’s very, very close to flat, except not quite perfectly flat, and the best observational evidence leads us to believe that if you neglect the matter and think only about the dark energy part, we’d actually be living in a de Sitter spacetime. The quantity that measures this is called the cosmological constant. It’s zero in flat space, positive in de Sitter and negative in anti-de Sitter. It turns out from measurements that our cosmological constant is positive but outrageously small, tiny compared to anything else we know about in physics. This is puzzling because we would love to relate it to something we understand already but it’s hard to arrive at a result so small working with quantities that are considerably larger. So there’s an interesting open question about why it is what it is.
- ramadis 5y agoJust to add to the reply, the AdS/CFT correspondence (aka Maldacena duality) was proposed by Juan Maldacena, one of the authors of this paper (Humanly traversable wormholes).
- ncmncm 5y agoSeems to me you can think of Minkowski space as an extremum of both AdS or dS, with zero curvature. I.e., if you can prove something in AdS or dS, it must also be true of almost-flat, barely-AdS or barely-S space.
- sdoering 5y agoThanks for the great explanation