Axiom Wang

From Noether theorem to Thermodynamics

How the symmetries of the universe dictate the laws of motion and give birth to the First Law of Thermodynamics.

1. The Premise

In basic physics, you learned the First Law of Thermodynamics: Energy cannot be created or destroyed (). You also learned that Momentum and Angular Momentum are conserved.

But why are they conserved? In 1915, mathematician Emmy Noether proved a mind-bending theorem: Every continuous symmetry in the universe corresponds to a mathematically conserved quantity.

Today, we will use basic calculus to prove that Time, Space, and Rotational symmetries give us Energy, Momentum, and Angular Momentum. Then, we will scale this up to show how these mechanics form Thermodynamics.

2. Vectors vs. Scalars (The Lagrangian)

In classical mechanics, tracking particles using Newton's is exhausting because vectors constantly change directions. Joseph-Louis Lagrange realized we can solve mechanics using entirely scalars (numbers with no direction).

He defined the Lagrangian () as Kinetic Energy () minus Potential Energy ():

Nature inherently obeys the Principle of Least Action. Out of all possible paths a particle could take, it chooses the path that minimizes the accumulation of over time. Just like setting a derivative to zero in calculus finds a minimum, we use the Euler-Lagrange Equation to find this path:

The Euler-Lagrange Equation
Interactive: The Principle of Least Action
Instead of tracking vectors, nature calculates a single scalar number called Action (S) for the entire path. The true physical path is the one where the Action is minimized.
Slide to explore different paths. Notice how the Action (S) changes.

3. Spatial Symmetry → Momentum

Let's look at Spatial Translation Symmetry. This means the laws of physics don't care where you are. Empty space is uniform. An experiment done at coordinate yields the exact same results at .

Mathematically, if the environment is uniform, the Potential Energy doesn't depend on your absolute position . Therefore, the Lagrangian does not depend on . The partial derivative is zero:

Now, plug this zero into the Euler-Lagrange equation:

In calculus, if the time derivative of a quantity is zero, that quantity is a constant. We call this conserved quantity Momentum ()!

(Since , taking the derivative with respect to literally gives )

Spatial Symmetry (Momentum Conservation)
Colliding blocks at x=100 behave identically to blocks at x=400 because space is uniform. Their total momentum never changes.

4. Rotational Symmetry → Angular Momentum

What if we use polar coordinates? Rotational Symmetry means empty space is isotropic—it has no "up" or "down". The laws of physics don't care which angle you face.

If a system is rotationally symmetric (like a planet orbiting a star), the Lagrangian doesn't depend on the absolute angle .

The resulting constant is Angular Momentum (). For a mass spinning at radius with angular velocity , the angular momentum is . Because is constant, if the radius decreases, the rotation speed must increase to compensate!

Rotational Symmetry (Angular Momentum)
Pull the mass inward. Notice how the rotation accelerates to keep the scalar quantity J = mr²ω perfectly constant!
Radius (r): 120
Velocity (ω): 0.020
Angular Momentum (J): 0 (Constant)

5. Time Symmetry → Energy

Finally, Time Translation Symmetry. The background rules of physics don't have a clock. Gravity doesn't fade over time. Therefore, has no explicit time dependence: .

Taking the total derivative of with the chain rule, and substituting the Euler-Lagrange equation, Noether proved that the following quantity perfectly drops out as a constant:

This constant is Energy. (If you plug in , you get ).

The Noether Master Key:
  • Space is uniform → Momentum is conserved.
  • Space is isotropic → Angular Momentum is conserved.
  • Time is uniform → Energy is conserved.

6. Scaling up to Thermodynamics

We proved a single particle conserves energy over time. But for a gas made of particles, we group the energy into two macroscopic categories:

  1. Macroscopic Energy: The kinetic energy of the entire box moving (Momentum).
  2. Internal Energy (): The invisible, random kinetic jiggling of the trillions of particles inside.
Visualizing Heat and Work
Particles turn red as their microscopic scalar energy increases. Work is organized macroscopic pushing; Heat is random microscopic jiggling.
Internal Energy (U): 0 J

7. The First Law

According to Noether's theorem, total energy is strictly conserved ().

If our gas box is sitting still, its macroscopic momentum is zero. Any change to its Internal Energy () must come from energy crossing its boundaries. There are only two methods:

  • Heat (): Energy transferred through random microscopic collisions.
  • Work (): Energy transferred through macroscopic, organized force (a piston).

Because Noether mathematically guarantees total energy is constant, the change in the internal energy must equal the heat added plus the work done on the system.

Conclusion: The First Law of Thermodynamics is not a separate rule of nature. It is the direct macroscopic manifestation of Time Translation Symmetry operating on a microscopic scale!