Quantum Physics in a Mirror Universe
PBS Space Time
September 18, 2026
PBS Member Stations rely on viewers like you. Check out the new Space Time Merch Store! When you look in mirror, and see what you think is a perfect reflection. You might be looking at universe whose laws are fundamentally different. Tweet at us! @pbsspacetime Email us!
Speakers Matt O'Dowd
TopicsAstronomyScienceEducation
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Matt O'Dowd (1:33)
Thanks to brilliant.org for supporting PBS Digital Studios. When you look in a mirror, you might think you see a perfect reflection, but you're actually looking at a universe whose laws are fundamentally different.
When we think about symmetry, the first thing that comes to mind is mirror symmetry. Butterflies, raw shark tests and classically attractive faces all look the same when flipped left to right.
In physics, a symmetry is when the laws of physics are unchanged due to some transformation of coordinates. We've seen examples where this holds. The universe is symmetric to coordinate shifts in space, time, and even the rather abstract phase of the wave function in quantum mechanics.
So it might be surprising to learn that with all the weird ways in which the universe is symmetric, it's not entirely symmetric under the most intuitive one. The laws of physics work differently in the universe of the mirror. Let's talk about the physics of entering the mirror universe. The technical name for such a reflection is a parity transformation. And when something remains identical under such a transformation, we say that the thing is parity symmetric, p-symmetric. Parity is a weird type of symmetry. In the case of those other symmetries I mentioned, the shift in position, time, or phase can be by any amount small or large. These are continuous symmetries. But there's no such thing as a partial reflection. You either reflect or you don't. Parity is a discrete symmetry.
Other types of discrete symmetries include charge conjugation, flipping the sign of the electric charge, and time reversal, sending in the clock, ticking backwards. We'll come back to both of these. They are going to save us in the end. Parity transformations involve the flipping of spatial axes. If we define the mirror to be in the XY plane, reflections send Z to minus Z and vice versa. Objects are turned back to front and front to back. And it looks like your right hand becomes your left and vice versa as though you had actually flipped in the X direction, not the Z.
Well, actually, a true X axis reflection would look like this.
Left still goes to right, but forward-facing stays the same. This is exactly the same as a Z axis reflection plus a rotation. In fact, a reflection on any single axis can be reproduced by a reflection on a different axis plus a rotation. A reflection on two axes then puts things back to normal, while reflection on all three axes gives the same left-right switch as a reflection on one axis. But formally, a full parity inversion means flipping all three axes. Now, when you reflect the universe, obviously it is different. All position vectors point in the opposite direction. Same with velocity slash momentum. Throw a ball at the mirror away from yourself and its reflection looks like it's coming towards you. In the language of parity, we call properties that flip sign odd functions. Properties that don't change under reflections are called even. Things like the energy of the ball, its mass, the time on its clock and, as we'll see, angular momentum don't change in the mirror universe. Now, even though some signs do get flipped, the laws of physics should be unaltered in that mirror world. Newton's laws will still give the ball's trajectory. Those laws work the same, no matter the direction of motion. In fact, if we rotate the whole mirror ball's trajectory by 180 degrees, it's identical to the original trajectory.
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