Physics: A Complete Map of the Physical World
Linas JuozėnasShare
Start here · Series introduction
Physics: A Complete Map of the Physical World
A carefully structured library guiding the reader from first measurements and classical motion to quantum fields, living systems, Earth, and the universe.
Physics is the attempt to discover the most general patterns in nature. It asks how objects move, why matter holds together, how heat and light travel, what space and time are, how stars are born, and how the same basic laws can describe phenomena separated by more than forty orders of magnitude. This project is designed as one connected home for those ideas.
This project is designed as one connected home for those ideas. Over time, around 300–400 in-depth articles will be written to cover physics as fully as possible for us all — from the beginner taking the first steps into understanding, to the curious mind reaching toward the borders of what is known, and even to scientists looking for a wider, connected overview.
New interactive home · Under development
Explore the Physics Learning Map
A new possible home for this project is taking shape inside the Global Knowledge Ark. The learning map is still unfinished and under active development, so some sections may be incomplete or change as new material is added. You are warmly invited to explore it now, try the available paths, and return as the project continues to grow.
Open the Physics Learning Map →1. What physics is
Physics begins with observation. A stone falls. A pendulum swings. A metal wire carries current. A prism separates white light into colors. The night sky contains stars whose light has crossed space for years, centuries, or billions of years before reaching us. Physics tries to turn observations such as these into explanations that are precise, testable, and widely applicable.
A physical explanation is more than a description. It identifies measurable quantities, proposes a model, derives consequences, and compares those consequences with experiment. When a model succeeds, it allows us to predict events we have not yet observed. When it fails, the failure reveals where its assumptions or range of validity break down.
The power of physics comes from compression. An enormous variety of motions can be understood through a small set of mechanical principles. Electricity, magnetism, and light can be described within one electromagnetic theory. The behavior of atoms and materials emerges from quantum mechanics. The motion of planets, the structure of stars, and the expansion of the universe can be linked to the same laws tested in laboratories on Earth.
2. Why physics needs one connected map
Physics is often taught as a sequence of separate subjects: mechanics, heat, electricity, optics, relativity, quantum mechanics, and perhaps nuclear or particle physics. That division is useful for teaching, but nature itself is not divided in this way. A star is simultaneously a gravitational, thermodynamic, nuclear, electromagnetic, plasma, and quantum system. A smartphone depends on mechanics, semiconductor physics, electromagnetism, optics, information theory, materials science, and relativity. The climate is shaped by radiation, fluid dynamics, thermodynamics, phase transitions, chemistry, and planetary motion.
A complete course therefore needs more than a list of definitions and equations. It needs a structure that shows how ideas depend on one another. It must explain why energy appears in almost every field, how symmetry leads to conservation laws, why waves arise in mechanical, electromagnetic, quantum, and gravitational systems, and how simple microscopic rules can produce complex macroscopic behavior.
This series is built as that map. It begins with the language and methods of physics, develops the major theories in a logical order, and then applies them to matter, technology, Earth, life, and the universe. Earlier articles provide foundations for later ones, while links between fields allow readers to follow a concept wherever it appears.
3. How the series is organized
Rather than forcing the subject into a rigid article count, the library is arranged into broad parts and carefully sequenced topic groups. Additional deep dives can explore longer derivations, specialized applications, historical episodes, experiments, computational projects, and active research without disturbing the main learning path.
Part I — Foundations and tools
What physical theories are, how quantities are measured, which mathematical tools are needed, and how experiments, statistics, and computation turn observations into reliable knowledge.
Part II — Mechanics, waves, and continua
Motion, forces, energy, momentum, rotation, oscillations, chaos, elasticity, fluids, and the behavior of systems whose properties vary continuously through space and time.
Part III — Heat, fields, light, and plasma
Thermodynamics, statistical physics, electricity, magnetism, circuits, signals, optics, photonics, ionized matter, and fusion.
Part IV — Spacetime and quantum theory
Special and general relativity, quantum states, uncertainty, measurement, entanglement, quantum information, and the theories that replace classical intuition at extreme speeds, gravities, and scales.
Part V — Matter and fundamental interactions
Atoms, molecules, solids, soft matter, quantum fields, nuclei, elementary particles, accelerators, radiation, detectors, and the technologies used to study the smallest known structures.
Part VI — Universe, Earth, and life
Stars, galaxies, cosmology, planets, atmosphere, oceans, climate, living systems, medical imaging, radiation therapy, and the application of physical ideas to complex natural systems.
This order is intentional. Measurement and mathematics come before advanced theory. Mechanics introduces motion, forces, energy, and conservation. Waves prepare the way for sound, light, quantum mechanics, and field theory. Thermodynamics and statistics explain how large-scale behavior emerges from enormous numbers of microscopic constituents. Electromagnetism leads naturally to relativity and optics. Quantum mechanics becomes the foundation for atomic, molecular, condensed-matter, nuclear, and particle physics. The final part brings all of those tools together in systems of extraordinary scale and complexity.
4. How to read the series
There is no single correct route through physics. A reader’s route should depend on existing knowledge, goals, and available time. The series therefore supports several levels of engagement.
The overview route
Read the overview article for each major topic. This route gives a broad map of physics without requiring every derivation. It is suitable for readers who want to understand what each field studies, how the fields connect, and which questions remain open.
The foundational route
Begin with units, vectors, graphs, elementary calculus, measurement, Newtonian mechanics, oscillations, thermodynamics, electromagnetism, special relativity, and introductory quantum mechanics. This route supplies the conceptual spine needed for most later subjects.
The complete route
Follow the articles in their recommended order. Definitions, notation, and prerequisites will be introduced before they are used. Later articles will link back to earlier explanations instead of repeating them without context.
The specialist route
Enter through a subject of interest—such as astrophysics, electronics, climate physics, or quantum information—and follow the prerequisite links backward when necessary. Cross-topic tags will connect each application to the underlying theories.
You do not need to understand all of physics before beginning. The purpose of the map is to show where you are, what comes next, and which earlier ideas will help you move forward.
5. What each article will contain
Every core article will use a consistent structure. This makes the series easier to navigate and prevents mathematical detail from becoming detached from physical meaning.
- A central question that identifies the phenomenon or problem being explained.
- Prerequisites and links to the earlier ideas required for the discussion.
- A concrete observation, experiment, or application that gives the topic a physical setting.
- Definitions and notation introduced before equations are used.
- Qualitative intuition explaining the mechanism in ordinary language.
- Assumptions and idealizations showing how the real system is simplified.
- Mathematical development with the main results derived rather than merely stated.
- Worked examples ranging from simple checks to realistic calculations.
- Experimental evidence and an account of how the relevant quantities are measured.
- Limitations and common misconceptions identifying where intuition or equations can fail.
- Applications and cross-links connecting the subject to other areas of physics.
- Exercises or computational projects that turn reading into active understanding.
Advanced details can appear in expandable sections or separate deep-dive articles. This keeps the main explanation readable while preserving a path to rigorous derivations and specialized material.
6. Ideas that connect every field
Although the series is divided into subjects, a smaller set of ideas will recur throughout it. Learning to recognize these patterns is one of the main goals of a serious physics education.
Symmetry reveals what does not change when a system is transformed. In many theories, these invariances are directly connected to conserved quantities such as energy, momentum, and charge. Fields describe quantities distributed through space and time, from temperature and fluid velocity to electric fields and spacetime geometry. Waves describe the propagation of disturbances and information. Statistical reasoning connects uncertain microscopic events to stable macroscopic laws. Scale determines which description is useful: a gas may be a collection of molecules at one level and a continuous fluid at another.
Theories themselves are layered. Newtonian mechanics remains extraordinarily useful even though relativity and quantum mechanics are more fundamental in certain regimes. Thermodynamics can describe heat engines without following every molecule. Fluid dynamics can model air without tracking every atom. A less fundamental theory is not necessarily less valuable; it may be the clearest and most efficient description at the scale of interest.
7. The role of mathematics
Mathematics is the language in which physical relationships become precise. An equation can express how a quantity changes, which combinations remain constant, how one measurement depends on another, and what a theory predicts under conditions that have never been tested before.
Yet equations should not be treated as decorations or commands to memorize. Every important equation in this series will be accompanied by an explanation of its symbols, assumptions, units, interpretation, and range of validity. Whenever possible, results will be checked through dimensions, limiting cases, estimates, numerical examples, and comparison with experiment.
The mathematical level will increase gradually. Early articles rely mainly on algebra, geometry, graphs, and trigonometry. Calculus enters when we need to describe continuous change. Differential equations arise when physical laws determine how a system evolves. Linear algebra becomes essential for coupled systems, normal modes, relativity, and quantum mechanics. More advanced areas introduce probability theory, Fourier analysis, tensors, group theory, differential geometry, complex analysis, and variational methods.
8. Evidence, experiments, and computation
Physics is not established by elegance alone. A theory must make contact with observation. For that reason, the series will treat experiments as part of the argument rather than as historical footnotes. Readers will see how quantities are operationally defined, how instruments convert physical effects into data, how noise and uncertainty are handled, and how competing explanations are distinguished.
Some experiments can be reproduced with household objects, simple electronics, or freely available software. Others require telescopes, accelerators, cryogenic systems, spacecraft, gravitational-wave observatories, or detectors buried deep underground. Even when an experiment cannot be repeated at home, its logic can still be explained: what was measured, which prediction was tested, what alternative possibilities existed, and why the result changed our understanding.
Computation provides a third partner alongside theory and experiment. Many systems cannot be solved exactly. Numerical methods allow us to calculate planetary trajectories, fluid flow, quantum states, material properties, climate behavior, galaxy formation, and detector responses. Code, simulation, visualization, and data analysis will therefore appear throughout the project rather than being confined to a single topic.
9. What “complete” means
No finite collection can contain every calculation, material, device, astronomical object, biological mechanism, or research paper related to physics. The subject is too large, and it continues to develop. Here, “complete” has a more useful meaning: the project aims to provide a coherent route through every major branch of physics, the central ideas and equations of each branch, the evidence supporting them, their important applications, and clear paths toward more specialized study.
A few hundred well-developed core articles will form a finishable first edition. They give the project a clear boundary while still allowing indefinite expansion beneath a stable structure. A core article on quantum tunnelling, for example, can later link to separate pieces on alpha decay, scanning tunnelling microscopy, semiconductor devices, fusion, instantons, and the WKB approximation without disrupting the map.
Completeness also requires honesty about uncertainty. Some theories are extraordinarily well tested within known limits. Some models are useful approximations. Some measurements remain difficult to reconcile. Some questions—such as the nature of dark matter, the quantum description of gravity, and the origin of several observed constants—remain open. The series will distinguish established results from plausible models, active hypotheses, and unresolved problems.
10. Where the journey begins
We will begin before forces, atoms, or equations. The first task is to understand what physicists are trying to do when they describe nature. What counts as a physical quantity? How does an observation become a measurement? What is the difference between a model, a law, and a theory? Why are idealizations useful, and how do we know when they have been pushed too far?
From there, the journey will move outward and inward at the same time: from simple measurements to universal principles, from everyday motion to curved spacetime, from visible objects to quantum fields, and from local experiments to the history of the cosmos. Each article will add a piece to the map. Just as importantly, each will show how that piece connects to the rest.
Physics is often presented as a completed monument built by exceptional people in the past. It is better understood as an ongoing method of inquiry. Its equations preserve hard-won knowledge, but its deepest value lies in the habits behind them: define clearly, measure carefully, reason from assumptions, test predictions, quantify uncertainty, and revise the model when nature disagrees.
This series is an invitation to learn that method and use it—to see the physical world not as a collection of disconnected facts, but as a network of patterns that can be observed, modeled, calculated, challenged, and understood.
Part of the complete physics article series · Foundations to frontiers