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Emmy Noether was born on March 23, 1882. A German mathematician who made many important contributions to abstract algebra. She discovered Noether's theorem, which is fundamental in mathematical physics. She was described by Pavel Alexandrov, Albert Einstein, Jean Dieudonné, Hermann Weyl and Norbert Wiener as the most important woman in the history of mathematics. As one of the leading mathematicians of her time, she developed some theories of rings, fields, and algebras. In physics, Noether's theorem explains the connection between symmetry and conservation laws.
Noether’s Theorem - A Quick Explanation
Noether's Theorem is super rad. The theorem is, colloquially,
>> Continuous symmetries imply conserved quantities. <<
Let’s dig into the origin of this powerful theorem and list a couple of examples. I’ll restrict my attention to a subclass of symmetries for the sake of space, buuuut if there’s interest, I could do a more general post in the future. (Heads up: because this post is written using LaTeX, it's probably easiest to read directly from my blog.)
• Defining the Lingo: A Lagrangian is a function that (after some manipulation) yields the physical evolution of a system. A generic Lagrangian $L$ can be a real continuous function of...
$m$ real parameters $t_j$, where $j=1,\cdots,m$, and
$n$ pairs of paths, which we label $q_i(t_1,\cdots,t_m)$ and $\tilde{q}_i(t_1,\cdots,t_m)$, where $i=1,\cdots,n$ and a path means “a real continuous function of the aforementioned parameters”
In this exceedingly general case, we might write
$$L = L(q_1,\cdots,q_n,\tilde{q}_1,\cdots,\tilde{q}_n,t_1,\cdots, t_m)$$
However, for the sake of clarity, let's restrict ourselves to one parameter $t$ and one function pair $(q,\tilde{q})$. Let's further suppose $L$ depends on its parameter only through the function pair, aka let us write $L = L(q,\tilde{q})$ (as opposed to $L = L(q,\tilde{q},t)$). This is the case relevant to a classical particle confined to a friction-free line, wherein $q(t)$ is the particle’s position along the line and $t$ records the time.
While $L$ is constructed to be a function of position $q(t)$ and some other path $\tilde{q}(t)$, we always intend to eventually set $\tilde{q}(t)$ equal to the velocity $\dot{q}\equiv dq/dt$. Furthermore, of the many combinations $(q(t),\tilde{q}(t))$ equaling $(q(t),\dot{q}(t))$, nature chooses the pair satisfying the Euler-Lagrange equation:
$$\left.\frac{\partial L}{\partial q} \right|_{\tilde{q} = \dot{q}} = \frac{dp}{dt}$$
where
$$p\equiv \left. \frac{\partial L}{\partial \tilde{q}}\right|_{\tilde{q} = \dot{q}}$$
The differential equation we get from plugging a specific $L$ into the Euler-Lagrange equation is called the equation of motion of the system, and $p$ is the momentum conjugate to $q$.
• The Main Idea: No matter the specific form of $L$, we can plot it over $(q,\tilde{q})$ space. (To be clear: this is the space of values to which the paths $q(t)$ and $\tilde{q}(t)$ are mapping, so essentially the real plane.) The resulting plot will look something like the left plot in the following image:
I've made a point to highlight contours of constant $L$ in orange. The right plot projects those contours onto the $(q,\tilde{q})$ plane. These contours lie at the heart of Noether's Theorem: imagine we slide the coordinates $(q,\tilde{q})$ around in the plane so that each point moves continuously along a contour of constant $L$. Usually the shape of $L$ is changed when we distort the $(q,\tilde{q})$ plane below it, but by forcing each $(q,\tilde{q})$ to flow along a contour, $L$ is unaffected! A continuous transformation that leaves $L$ unchanged is called a continuous symmetry of the Lagrangian.
We can make this whole business quantitative by parameterizing the sliding operation with a real variable $\alpha$. Let's choose $\alpha$ so that $\alpha=0$ corresponds our initial unchanged $(q,\tilde{q})$ plane. Then the statement “$\alpha$ parameterizes contours of constant $L$” is mathematically expressible as
$$\left.\frac{dL}{d\alpha}\right|_{\alpha =0} =0$$
which equals, by the chain rule of differentiation,
$$\frac{\partial L}{\partial q}\hspace{3 pt}\left.\frac{dq}{d\alpha}\right|_{\alpha =0} + \frac{\partial L}{\partial \tilde{q}} \hspace{3 pt} \left.\frac{d\tilde{q}}{d\alpha}\right|_{\alpha =0} = 0$$
Now, this equation holds true across all of $(q,\tilde{q})$ space, including along the physical path solving the equations of motion. For that path, we may use the Euler-Lagrange equation, the definition of conjugate momentum $p\equiv \partial L/\partial\tilde{q}$, and the fact that $\partial \dot{q}/\partial \alpha = d/dt(\partial q/\partial \alpha)$ to write,
$$\frac{dp}{dt} \hspace{3 pt} \frac{\partial q}{\partial\alpha} + p \hspace{3 pt} \frac{d}{dt}\left[\frac{\partial q}{\partial \alpha}\right] = 0$$
aka, according to the product rule of differentiation,
$$ \frac{d}{dt}\left[p \hspace{3 pt} \frac{\partial q}{\partial \alpha}\right] =0 $$
In other words, the value of $p \hspace{3 pt} (\partial q/\partial \alpha)$ doesn’t change in time--it’s a conserved quantity! This is a special case of Noether's Theorem.
If we repeat the above calculation with $n$ paths $q_i(t)$, we instead derive
$$\text{*}\hspace{25 pt}\frac{d}{dt}\left[\vec{p}\cdot \frac{d\vec{q}}{d\alpha}\right] =0 \hspace{25 pt}\text{*}$$
where $\vec{q} \equiv (q_1,\cdots,q_n)$ and $\vec{p} \equiv (p_1,\cdots, p_n)$, and we find that
>> Momentum along a continuous symmetry direction is conserved. <<
This powerful statement allows us to identify conserved quantities from symmetries alone. For example...
• 1. Coordinate Translation Symmetry: Suppose $L$ doesn't depend on the coordinate $q_i$ for some value of $i$. Then the translation $q_i\mapsto q_i+\alpha$ is a continuous symmetry transformation. Because $dq_k/d\alpha$ is nonzero only for the coordinate we’re transforming ($k=i$), the associated conserved quantity is...
$$\vec{p}\cdot \frac{d \vec{q}}{d\alpha} = p_i$$
which is the $i$th conjugate momentum. And so, coordinate translation invariance necessarily implies conservation of the corresponding momentum.
• 2. Rotational Symmetry: Suppose $L$ depends on the coordinates $(x,y,z)$ and is invariant under the rotation of $x$ and $y$ into one-another:
$$ x\mapsto (\cos\alpha)x + (\sin\alpha)y\hspace{50 pt}y\mapsto (\cos\alpha)y -(\sin\alpha)x$$
Then we may calculate,
$$\left.\frac{d x}{d\alpha}\right|_{\alpha =0} = y\hspace{50 pt} \left.\frac{d y}{d\alpha}\right|_{\alpha =0} = -x$$
from which Noether's Theorem implies conservation of...
$$\vec{p}\cdot \frac{d\vec{q}}{dt} = p_x y - p_y x = - L_z$$
where $L_z$ is the angular momentum in the $z$-direction. Rotational invariance necessarily implies angular momentum conservation.
• Closing Comment: Note how we didn't need an explicit form for $L$ to make these arguments. Noether's Theorem tells us that conserved quantities naturally emerge not as coincidences, but from the presence of symmetries. Consequently, if I experimentally observe a conserved quantity (like electric charge, or color charge, or even things like lepton number) then I can make my model consistent with that observation by encoding certain symmetries into my Lagrangian. In this way, Noether’s Theorem is impressive in both its elegance and practical power.
Thanks for the ask, anonymous! I hope this helped. Although I didn't have space to discuss it here, Noether's Theorem also extends to Lagrangians with explicit parameter dependence, systems with multiple evolution parameters (like QFT), instances where $(q,\tilde{q})$ transformations change $L$ by a total derivative, and more. One extension allows us to demonstrate how time translation invariance yields energy conservation.
Have a physics question you think I might be able to help answer? Send me an ask. Until then, have a great day! Best wishes, my friend!
Emmy Noether was born on March 23, 1882. A German mathematician who made many important contributions to abstract algebra. She discovered Noether's Theorem, which is fundamental in mathematical physics. She was described by Pavel Alexandrov, Albert Einstein, Jean Dieudonné, Hermann Weyl and Norbert Wiener as the most important woman in the history of mathematics. As one of the leading mathematicians of her time, she developed some theories of rings, fields, and algebras. In physics, Noether's theorem explains the connection between symmetry and conservation laws.
So I've been watching lots of vids on Noether's Theorem and I'm like, what if someone, like a scientist or a mathematician in a science-fictional or magical universe, who's been quietly collecting data on stuff that appears to be violating the laws of physics, and uses Noether's Theorem to find out what's being conserved
and hey, for the first few hundred examples, they can map the conserved values to magic or psionics or w/e, but then there are still anomalies, and they dig deeper and cross of different potential conserved values, from super-science to magic to belief…
and then they hit the last value and it's “narrative”
and they look at the camera past the fourth wall and whisper:
“You motherfuckers.”

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A friend showed me this video today. Noether’s theorem of symmetries and conservation laws is one of my top 5 or so favorite ideas in physics, and this is a really good explanation of it, aimed at a high school level I think.
Noether's Theorem: Symmetry & Conservation Laws
Social barriers aside, Noether immediately grasped the problem with Einstein's theory. Over the course of three years, she not only solved it, but in doing so she proved a theorem that simultaneously reached back to the dawn of physics and pushed forward to the physics of today. Noether’s Theorem, as it is now called, lies at the heart of modern physics, unifying everything from the orbits of planets to the theories of elementary particles. The full statement of Noether’s Theorem involves a good amount of advanced mathematics, far beyond the scope of this article. But it has a clear and intuitive physical meaning: the theorem uncovers a hidden relationship between symmetry and conservation, and that relationship is what came to unify all of physics.
Ars Technica’s write-up of the work of Amalie Emmy Noether, The female mathematician who changed the course of physics—but couldn’t get a job