Theoretical Physics

A friendly grand tour of the frameworks that make sense of the world — from falling apples to black holes, from light waves to quantum information. You’ll find long explanations written for curious students, with optional “go deeper” panels and links to full pages if you want even more.

A good theory is a small set of ideas that keeps its promises across many experiments.
QParadox

What is theoretical physics (and why it matters)

Theoretical physics is the practice of turning patterns into principles and principles into equations that make testable claims. It does not replace experiments — it guides them, explains them, and predicts new ones. You’ll see three layers over and over: principles, models, and calculations.

Getting started

How to read equations without fear

You don’t need to memorize everything. Focus on what a symbol means in words and what would change if you poked the system. If an equation has a derivative with respect to time, it’s about change. If you see a symmetry, expect a conserved quantity. If a result seems weird, try a limit: what happens when something is very small, very large, or zero?

habit stack: units checkorder-of-magnitudedraw a picturetest extremes

Read More • What is Theoretical?
Go deeper • Principles → Models → Calculations

Principle: light speed is the same for all inertial observers. Model: two spaceships exchanging signals. Calculation: derive time dilation and length contraction and compare to GPS corrections. You just did relativity logic.

Classical mechanics • motion, energy, and elegant shortcuts

Start with forces and motion (Newton), then learn the elegant re-writes (Lagrange & Hamilton) that make tough problems simple. Classical ideas still power engineering, spaceflight, and all “back-of-the-envelope” reasoning.

Newton → Lagrange

From pushes and pulls to a single action

Newton says $\mathbf{F}=m\mathbf{a}$. Lagrange says: choose a function $L=T-V$ and take the path that makes the action $S=\int L\,dt$ “stationary” (small wiggles don’t matter to first order). Same physics, cleaner math, easier coordinates.

Try it • Pendulum in one line

$L=\tfrac12 m \ell^2 \dot{\theta}^2 - mg\ell(1-\cos\theta) \Rightarrow \ddot{\theta} + \tfrac{g}{\ell}\sin\theta=0$. Small angles: $\sin\theta\approx \theta$ → simple harmonic motion.

Symmetry

Conservation laws you can feel

Time-shift symmetry → energy conserved. Space-shift symmetry → momentum conserved. Rotation symmetry → angular momentum conserved. When you spot a symmetry, you’ve found a constant of motion — a compass for problem solving.

Electromagnetism • fields, waves, and light

Maxwell’s equations unify electricity, magnetism, and light. They explain radios, rainbows, MRI scanners, and why lasers make fringes.

Field view

Why “fields” are worth the mindset shift

Instead of forces that jump across space, EM treats space itself as filled with fields ${\bf E}$ and ${\bf B}$ that carry energy and momentum. Changes ripple as waves at speed $c$. That’s light! A field picture also plays perfectly with relativity and later with quantum fields.

Go deeper • One-line wave equation

Combine Maxwell’s curl equations in empty space → $\\frac{1}{c^2}\\partial_t^2 \mathbf{E} - \nabla^2 \mathbf{E}=0$ (and same for $\mathbf{B}$). That’s a wave with speed $c$.

Tech

From theory to devices

Antennas, fiber optics, spectrometers — all are Maxwell made practical. Interference patterns are theory you can see.

Relativity • spacetime as geometry

Special relativity mixes space and time; general relativity says gravity is curvature. Clean ideas, big consequences: GPS, black holes, gravitational waves.

Special

Why time dilates (without pain)

If the speed of light is the same for everyone, moving clocks must tick differently so the math stays consistent. It’s not a trick — it’s how spacetime keeps laws universal.

General

Gravity isn’t a pull — it’s a path

Mass and energy curve spacetime; free objects follow the straightest possible paths (geodesics) in that curved geometry. Light bends near stars; time runs slower in stronger gravity.

Quantum mechanics • the rules of the small (and surprising)

Quantum theory is simple at heart: states are vectors, observables are operators, probabilities come from $|\text{amplitude}|^2$. The surprises (superposition, entanglement) are features, not bugs.

States

Superposition • adding possibilities

A system can be in a mix of options at once — and the phase matters. Two paths can add or cancel like waves. If you learn which path it took, the interference fades. Information changes the pattern.

Quick model • Two-path interference

Amplitudes $A$ and $B$. Total = $A+B$, probability = $|A+B|^2$. The cross term depends on their relative phase → fringes.

Limits

Uncertainty is about spreads, not clumsiness

For position $X$ and momentum $P$, spreads obey $\Delta X\,\Delta P \ge \hbar/2$. It’s a property of the state and the math, not “disturbance.” You can know a lot — just not everything at once.

Entanglement

Correlations that outsmart classical guesses

Some joint states can’t be described as “part A is this, part B is that.” Bell tests show the pattern beats any local hidden-variable plan. No faster-than-light messages, just different logic for joint outcomes.

Measurement

So… what “collapses”?

The math has smooth evolution and sharp outcomes. Interpretations explain that gap in different ways (Copenhagen, Many-Worlds, pilot-wave). You can do great physics without picking a side — but knowing the options helps.

Quantum Field Theory • particles as ripples of fields

QFT says fields are the main characters; “particles” are their excitations. Symmetry organizes interactions; renormalization tells you what matters at each scale.

Sum over paths

Feynman’s idea in friendly terms

The amplitude for a process is a sum of contributions from many possible histories, each with a phase that depends on the action. Nearby histories line up; wildly different ones cancel. Diagrams are smart bookkeeping for this math.

Taming infinities

Renormalization • scale honesty

Parameters “run” with energy scale. That’s not cheating — it’s acknowledging that a theory describes nature up to a certain resolution. Different systems can show the same big-scale behavior (universality).

Go deeper • Symmetry breaking & Higgs (plain words)

Sometimes the equations have a symmetry but the lowest-energy state picks a direction. In a gauge theory, the “wiggle” that would have been a massless mode gets absorbed, giving mass to force carriers. That’s the Higgs mechanism in one breath.

Read More • Quantum Field Theory

Statistical Mechanics • order from crowds

From many microscopic possibilities, you get simple macroscopic rules. Entropy counts options; temperature measures how energy is shared.

Big picture

Why averages beat chaos

You don’t track every molecule. You track distributions. The partition function $Z=\sum e^{-E_i/k_BT}$ is a master key: it builds averages and fluctuations without following each particle.

Arrow of time

Why eggs break but don’t unbreak

Microscopic laws are reversible, but we start the universe in a low-entropy condition. From there, typical evolution increases entropy. That’s your everyday arrow of time.

Cosmology • the universe as a dataset

Expansion, relic light, and the growth of structure tell a consistent story. A small set of parameters fits a huge set of measurements.

Inflation

Stretch tiny jitters into galaxies

A brief burst of accelerated expansion magnifies quantum fluctuations into the seeds of cosmic structure. The exact engine is debated; the general picture matches the sky remarkably well.

Dark sector

What we really know (and don’t)

We see gravity’s effects that point to dark matter and dark energy. We name them honestly and keep testing — separating measurement from guess.

Beyond the Textbook • beautiful corners you should know

These ideas impress professors because they matter in research but rarely show up in first courses — explained here in calm English.

Geometry

Berry phase • a phase from the path

Slowly loop a system’s settings and the state can pick up a geometric phase that depends on the loop’s shape, not the speed. Shows up in polarization and solid-state physics.

Topology

Topological phases • edges that won’t quit

Some materials have edge states protected by topology (not by energy barriers). That’s why their responses are quantized and robust to messiness.

Foundations

Decoherence-free subspaces

Store quantum information in subspaces the dominant noise can’t touch. This is a real strategy for quantum devices, not sci-fi.

Go deeper • Holography, anomalies, retrocausality (safe, short takes)

Holography: sometimes the physics in a volume equals a theory on its boundary. It links geometry and entanglement in stunning ways.

Anomalies: symmetries that work classically but fail quantum mechanically. If they don’t cancel, the theory is inconsistent — dealbreaker level.

Retrocausality: a minority view that future choices can constrain past hidden variables. Interesting, controversial, not mainstream.

Read More • Beyond the Textbook

Physics & Philosophy • meaning without hand-waving

When equations touch ideas like reality, time, and causation, philosophy helps keep our words sharp and our claims honest.

Observers

Wigner’s friend (plainly)

Inside the lab, the friend sees one outcome. From outside, Wigner treats the whole lab as a quantum system. The lesson: be explicit about information — who has which record — and many “paradoxes” calm down.

Probabilities

QBism, relational views, and superdeterminism

Different ways to connect math and meaning. You don’t have to swear loyalty — but knowing the menu keeps you from reading more into equations than they say.

Crossroads • where to go next

Start

Return to the map

Skim the other learning routes and pick a new doorway.

Back to Start Here
Compute

See code bring ideas to life

Short, readable notebooks that turn equations into pictures.

Computational wing
Measure

How labs test theories

Instruments, noise, and honest uncertainty bars.

Experimental wing