The Complete Physics Curriculum

Explore the fundamental laws that govern our universe, from classical mechanics to quantum physics, with historical context and real-world applications.

8
Core Topics
100+
Interactive Simulations
50+
Historical Figures

Classical Mechanics

Introduction

Classical mechanics, developed primarily in the 17th to 19th centuries, describes the motion of macroscopic objects under the influence of forces. It provides the foundation for understanding everything from the motion of planets to the design of modern machinery.

Newton's Laws

The fundamental principles governing motion and force

Work & Energy

Conservation principles and energy transformations

Momentum

Linear and angular momentum in systems

Rotational Motion

Dynamics of rotating objects and systems

Historical Context

Ancient Greece (400-300 BCE)

Aristotle's early theories on motion and gravity, though later disproven, laid the groundwork for systematic study of physics.

Renaissance (1500s)

Galileo's experiments challenged Aristotelian physics and established the scientific method.

Scientific Revolution (1600s)

Newton unified terrestrial and celestial mechanics with his laws of motion and universal gravitation.

Key Figures

Isaac Newton
Isaac Newton

Laws of Motion & Gravity

Galileo Galilei
Galileo Galilei

Experimental Method

Leonhard Euler
Leonhard Euler

Mathematical Physics

Modern Applications

Aerospace Engineering
  • • Aircraft design and flight dynamics
  • • Satellite orbital mechanics
  • • Rocket propulsion systems
Robotics & Automation
  • • Robot arm kinematics
  • • Autonomous vehicle control
  • • Industrial machinery

Key Concepts & Equations

Newton's Laws of Motion

First Law (Inertia)

An object remains at rest or in uniform motion unless acted upon by a net force.

ΣF = 0
Second Law (Force & Acceleration)

The acceleration of an object is directly proportional to the net force acting on it.

F = ma
Third Law (Action-Reaction)

For every action, there is an equal and opposite reaction.

F₁₂ = -F₂₁

Energy & Work

Work

The work done by a force is the product of the force and the displacement in its direction.

W = F·d
Kinetic Energy

The energy possessed by an object due to its motion.

KE = ½mv²
Potential Energy

The energy possessed by an object due to its position or configuration.

PE = mgh

Interactive Demonstrations

Waves & Oscillations

Understanding Wave Phenomena

Wave physics describes how energy propagates through space and matter. From sound waves to electromagnetic radiation, wave phenomena are fundamental to our understanding of nature and modern technology.

Simple Harmonic Motion

The mathematics of periodic motion

Wave Properties

Frequency, wavelength, and amplitude

Wave Interactions

Interference, diffraction, and resonance

Sound Waves

Mechanical waves in media

Historical Development

Pythagoras (6th century BCE)

Discovered the mathematical relationship between string length and musical pitch, laying the foundation for wave theory.

Christiaan Huygens (1678)

Proposed the wave theory of light, challenging Newton's particle theory.

Thomas Young (1801)

Demonstrated wave interference through the famous double-slit experiment.

Modern Applications

Medical Technology
  • • Ultrasound imaging
  • • Sound wave therapy
  • • Medical resonance imaging
Communications
  • • Radio transmission
  • • Fiber optic networks
  • • Acoustic engineering

Wave Mathematics & Equations

Wave Speed

The relationship between frequency and wavelength

v = fλ
Simple Harmonic Motion

Position as a function of time

x(t) = A cos(ωt + φ)
Wave Interference

Superposition of waves

y = y₁ + y₂

Wave Demonstrations

Relativity

Einstein's Revolution

Einstein's theories of special and general relativity fundamentally changed our understanding of space, time, gravity, and the universe itself. These theories predict phenomena that seem to defy common sense but have been repeatedly verified by experiments.

Special Relativity

Space-time and velocity effects

General Relativity

Gravity and curved spacetime

Relativistic Effects

Time dilation and length contraction

Cosmological Implications

Black holes and expanding universe

Historical Milestones

1905: Special Relativity

Einstein publishes "On the Electrodynamics of Moving Bodies," introducing special relativity.

1915: General Relativity

Einstein completes general relativity, explaining gravity as curved spacetime.

1919: Experimental Confirmation

Eddington's expedition observes light bending during solar eclipse, confirming general relativity.

Key Contributors

Albert Einstein
Albert Einstein

Theory Development

Hermann Minkowski
Hermann Minkowski

Spacetime Geometry

Karl Schwarzschild
Karl Schwarzschild

Black Hole Solution

Modern Applications

Technology
  • • GPS satellite corrections
  • • Particle accelerators
  • • Nuclear energy calculations
Astronomy
  • • Black hole detection
  • • Gravitational wave astronomy
  • • Cosmological models

Fundamental Principles

Special Relativity Postulates

First Postulate

The laws of physics are the same in all inertial reference frames.

Second Postulate

The speed of light in vacuum is constant for all observers.

Special Relativity Equations

Lorentz Factor

Relativistic correction factor

γ = 1/√(1-v²/c²)
Time Dilation

Moving clock runs slower

Δt = γΔt₀
Length Contraction

Moving objects appear shorter

L = L₀/γ
Mass-Energy Equivalence

Einstein's most famous equation

E = mc²

General Relativity Principles

Equivalence Principle

Gravitational and inertial mass are equivalent. The effects of gravity are indistinguishable from acceleration.

Curved Spacetime

Mass and energy curve spacetime; curved spacetime tells matter how to move.

Einstein Field Equations

Relating matter to spacetime curvature

Gμν = 8πG/c⁴ Tμν

Experimental Evidence

Light Bending

Starlight bends around the Sun during eclipses, confirming spacetime curvature.

Gravitational Time Dilation

GPS satellites must account for both special and general relativistic time effects.

Gravitational Waves

LIGO's detection of gravitational waves from merging black holes.

Interactive Demonstrations

Engineering Applications

Physics in Engineering

Physics principles are fundamental to all branches of engineering, from mechanical systems to electronic devices.

Mechanical Engineering

  • • Stress and strain analysis
  • • Fluid dynamics
  • • Thermodynamic systems
  • • Structural mechanics

Electrical Engineering

  • • Circuit design
  • • Electromagnetic devices
  • • Power generation
  • • Signal processing

Medical Physics

Physics in Medicine

Modern medicine relies heavily on physics principles for both diagnostics and treatment.

Imaging Technologies

  • • X-ray and CT scanning
  • • MRI technology
  • • Ultrasound imaging
  • • PET scanning

Treatment Applications

  • • Radiation therapy
  • • Laser surgery
  • • Ultrasound therapy
  • • Nuclear medicine

Astronomy

Physics in Space

Physics helps us understand the cosmos, from planetary motion to the life cycles of stars.

Observational Tools

  • • Telescopes and optics
  • • Radio astronomy
  • • Spectroscopy
  • • Gravitational wave detection

Space Phenomena

  • • Black holes
  • • Stellar evolution
  • • Galactic dynamics
  • • Cosmic microwave background

Technology

Modern Applications

Physics principles drive technological innovation across all sectors of modern life.

Computing & Electronics

  • • Semiconductor devices
  • • Quantum computing
  • • Photonics
  • • Data storage

Energy Technology

  • • Solar cells
  • • Nuclear power
  • • Battery technology
  • • Smart grid systems

Ancient Physics

The Foundations

The earliest systematic study of nature began in ancient civilizations, laying the groundwork for modern physics.

Ancient Greece (600-300 BCE)

Key Figures
  • • Thales of Miletus
  • • Aristotle
  • • Archimedes
  • • Pythagoras
Major Contributions
  • • Theory of four elements
  • • Geometry foundations
  • • Basic mechanics
  • • Buoyancy principles

Ancient China

Developments
  • • Magnetism discovery
  • • Astronomical observations
  • • Acoustic principles
  • • Early optics
Applications
  • • Compass navigation
  • • Calendar systems
  • • Military technology
  • • Agricultural tools

Renaissance

The Scientific Revolution

The Renaissance period marked a dramatic shift from ancient to modern physics, establishing the scientific method.

Revolutionary Thinkers

Galileo
Galileo Galilei

Scientific Method

Copernicus
Nicolaus Copernicus

Heliocentrism

Kepler
Johannes Kepler

Planetary Motion

Major Developments

Scientific Methods
  • • Empirical observation
  • • Mathematical description
  • • Controlled experiments
  • • Systematic documentation
Key Discoveries
  • • Laws of motion
  • • Planetary orbits
  • • Telescope improvements
  • • Basic calculus

Modern Era

The Classical Period

The modern era saw the development of comprehensive physical theories that unified various phenomena.

Key Developments

1687
Newton's Principia published
1800s
Electromagnetism unified by Maxwell
1895
X-rays discovered by Röntgen
1897
Electron discovered by Thomson

Major Theories

Classical Mechanics
  • • Newton's laws
  • • Conservation laws
  • • Gravitation
  • • Wave mechanics
Field Theory
  • • Electromagnetism
  • • Maxwell's equations
  • • Light theory
  • • Field concepts

Contemporary Physics

Current Frontiers

Contemporary physics pushes the boundaries of our understanding, from the smallest particles to the entire cosmos.

Active Research Areas

Particle Physics
  • • Standard Model
  • • Higgs boson
  • • Quantum chromodynamics
  • • Neutrino physics
Cosmology
  • • Dark matter
  • • Dark energy
  • • Early universe
  • • Gravitational waves

Future Frontiers

Emerging Fields
  • • Quantum computing
  • • String theory
  • • Quantum gravity
  • • Plasma physics
Applications
  • • Quantum technologies
  • • Advanced materials
  • • Clean energy
  • • Space exploration

Thermodynamics

Heat and Energy

Thermodynamics studies the relationships between heat, energy, and work, governing everything from engines to phase transitions in matter.

Laws of Thermodynamics

Energy conservation and entropy

Heat Transfer

Conduction, convection, radiation

Phase Transitions

States of matter and changes

Thermal Properties

Temperature, pressure, volume relations

Historical Development

Sadi Carnot (1824)

Established the foundations of thermodynamics through analysis of heat engines.

Rudolf Clausius (1850)

Introduced the concept of entropy and formulated the Second Law.

Ludwig Boltzmann (1870s)

Developed statistical mechanics, linking thermodynamics to atomic theory.

Laws of Thermodynamics

Zeroth Law

Transitivity of thermal equilibrium

If A = B and B = C, then A = C
First Law

Energy conservation

ΔU = Q - W
Second Law

Entropy always increases

ΔS ≥ 0
Third Law

Absolute zero temperature

S → 0 as T → 0

Modern Applications

Engineering
  • • Heat engines
  • • Refrigeration
  • • Power generation
  • • Climate control
Research
  • • Phase transitions
  • • Materials science
  • • Chemical processes
  • • Environmental systems

Interactive Demonstrations

Electromagnetism

Electric and Magnetic Fields

The unified theory of electricity and magnetism underlies modern technology and explains fundamental forces of nature.

Electric Fields

Coulomb's law and electric potential

Magnetic Fields

Magnetic forces and induction

Maxwell's Equations

Unified electromagnetic theory

EM Waves

Electromagnetic radiation

Historical Breakthroughs

Faraday (1831)

Discovered electromagnetic induction.

Maxwell (1865)

United electricity and magnetism mathematically.

Hertz (1887)

Demonstrated existence of electromagnetic waves.

Maxwell's Equations

Gauss's Law (Electric)

Electric flux through closed surface

∮E·dA = Q/ε₀
Gauss's Law (Magnetic)

No magnetic monopoles

∮B·dA = 0
Faraday's Law

Electromagnetic induction

∮E·dl = -dΦB/dt
Ampère's Law

Magnetic fields from currents

∮B·dl = μ₀I + μ₀ε₀dΦE/dt

Modern Applications

Power & Energy
  • • Electric generators
  • • Power transmission
  • • Motors
  • • Transformers
Communications
  • • Radio waves
  • • Mobile networks
  • • Fiber optics
  • • Antenna design

Interactive Demonstrations

Optics

The Science of Light

Optics explores the behavior and properties of light, from simple reflection and refraction to complex phenomena like interference and polarization.

Geometric Optics

Ray tracing and image formation

Wave Optics

Interference and diffraction

Modern Optics

Lasers and optical devices

Optical Instruments

Microscopes and telescopes

Historical Development

Ibn al-Haytham (1021)

Published "Book of Optics," establishing scientific method in optics.

Newton & Huygens (1670s)

Debated particle vs wave nature of light.

Young & Fresnel (1800s)

Established wave theory through interference experiments.

Fundamental Laws & Equations

Law of Reflection

Angle of incidence equals angle of reflection

θᵢ = θᵣ
Snell's Law

Refraction at interfaces

n₁sinθ₁ = n₂sinθ₂
Lens Equation

Image formation by lenses

1/f = 1/u + 1/v

Modern Applications

Medical Applications
  • • Laser surgery
  • • Endoscopy
  • • Microscopy
  • • Optical imaging
Technology
  • • Fiber optics
  • • Digital cameras
  • • Display screens
  • • Optical computing

Interactive Demonstrations

Modern Physics

The Revolution in Physics

Modern physics emerged when classical theories failed to explain new phenomena, leading to revolutionary theories that changed our understanding of nature.

Special Relativity

Space, time, and mass-energy

Quantum Theory

Wave-particle duality

Nuclear Physics

Atomic nuclei and radioactivity

Particle Physics

Fundamental particles and forces

Key Discoveries

Planck (1900)

Discovered quantum nature of energy with blackbody radiation.

Einstein (1905)

Published special relativity and explained photoelectric effect.

Rutherford (1911)

Discovered the atomic nucleus through scattering experiments.

Fundamental Theories

Mass-Energy Equivalence

Einstein's famous equation

E = mc²
Time Dilation

Time slows at high speeds

t = t₀/√(1-v²/c²)
Length Contraction

Objects shorten along motion

L = L₀√(1-v²/c²)

Modern Applications

Nuclear Technology
  • • Nuclear power
  • • Medical imaging
  • • Radiation therapy
  • • Nuclear dating
Particle Physics
  • • Particle accelerators
  • • Detector technology
  • • Antimatter studies
  • • Cosmological research

Quantum Mechanics

The Quantum World

Quantum mechanics describes nature at its most fundamental level, revealing a world where particles behave like waves, measurements affect outcomes, and certainty gives way to probability.

Wave Functions

Quantum states and probability

Uncertainty Principle

Fundamental limitations

Quantum Systems

Particles and potentials

Quantum Effects

Tunneling and entanglement

Historical Development

Schrödinger (1925)

Developed wave mechanics and his famous equation.

Heisenberg (1925)

Introduced matrix mechanics and uncertainty principle.

Dirac (1928)

United quantum mechanics with special relativity.

Fundamental Principles

Schrödinger Equation

Evolution of quantum states

iℏ∂ψ/∂t = Ĥψ
Uncertainty Principle

Position-momentum uncertainty

ΔxΔp ≥ ℏ/2
Energy Levels

Quantized energy states

En = -13.6eV/n²

Modern Applications

Quantum Technology
  • • Quantum computers
  • • Quantum cryptography
  • • Quantum sensors
  • • Quantum teleportation
Research Applications
  • • Materials science
  • • Chemical modeling
  • • Quantum optics
  • • Molecular design

Interactive Demonstrations