⚛️ Physics

The fundamental science of matter, energy, space, and time

Branches of Physics

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Classical Mechanics

Motion, forces, energy, and momentum. Newton's laws govern everyday objects at non-relativistic speeds.

F = ma
Newton's Second Law
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Thermodynamics

Heat, temperature, and energy transfer. The four laws govern all energy transformations.

ΔS ≥ 0
Second Law (entropy never decreases)

Electromagnetism

Electric and magnetic fields unified by Maxwell. Light is an electromagnetic wave.

c = 1/√(ε₀μ₀)
Speed of light from Maxwell
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Quantum Mechanics

Physics at atomic/subatomic scales. Wave-particle duality, superposition, entanglement.

ΔxΔp ≥ ℏ/2
Heisenberg Uncertainty Principle
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Special Relativity

Physics at high speeds. Time dilation, length contraction, mass-energy equivalence.

E = mc²
Mass-energy equivalence
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General Relativity

Gravity as spacetime curvature. Black holes, gravitational waves, the expanding universe.

Gμν = 8πG/c⁴ Tμν
Einstein Field Equations
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Particle Physics

The Standard Model of elementary particles — quarks, leptons, bosons, and the Higgs field.

17 fundamental particles
The Standard Model
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Wave & Optics

Light, sound, and wave behavior — reflection, refraction, diffraction, interference.

λf = v
Wave equation

Fundamental Constants

ConstantSymbolValueSignificance
Speed of Lightc2.998 × 10⁸ m/sMaximum speed in the universe
Planck's Constanth6.626 × 10⁻³⁴ J·sQuantum of action
Gravitational ConstantG6.674 × 10⁻¹¹ N·m²/kg²Strength of gravity
Elementary Chargee1.602 × 10⁻¹⁹ CCharge of a proton/electron
Boltzmann's Constantk_B1.381 × 10⁻²³ J/KLinks temperature to energy
Avogadro's NumberN_A6.022 × 10²³ mol⁻¹Particles per mole
Fine-Structure Constantα1/137.036Strength of electromagnetism
Electron Massm_e9.109 × 10⁻³¹ kgLightest charged lepton

Classical Mechanics

Newton's Laws of Motion

1st (Inertia): An object at rest stays at rest; an object in motion stays in motion, unless acted on by a net force.

2nd (F=ma): The net force on an object equals its mass times acceleration.

3rd (Action-Reaction): For every action, there is an equal and opposite reaction.

Key Equations

F = ma
Net force
W = Fd·cosθ
Work done
KE = ½mv²
Kinetic energy
PE = mgh
Gravitational potential energy

Kinematics

v = u + at
Velocity (uniform acceleration)
s = ut + ½at²
Displacement
v² = u² + 2as
Velocity from displacement

u = initial velocity, v = final velocity, a = acceleration, t = time, s = displacement

Momentum & Collisions

Momentum p = mv is conserved in all closed systems.

p₁ + p₂ = p₁' + p₂'
Conservation of momentum

In elastic collisions, kinetic energy is also conserved. In inelastic collisions, KE is converted to heat/deformation.

Circular Motion & Gravity

F_c = mv²/r
Centripetal force
F_g = Gm₁m₂/r²
Newton's Law of Gravitation

Orbital velocity: v = √(GM/r). Escape velocity: v_e = √(2GM/r)

Simple Harmonic Motion

x(t) = A·cos(ωt + φ)
Oscillation equation
T = 2π√(m/k)
Period of spring
T = 2π√(L/g)
Period of pendulum

k = spring constant, L = pendulum length, g = 9.81 m/s²

Thermodynamics

The Four Laws

Zeroth: If A is in thermal equilibrium with B, and B with C, then A is with C. (Defines temperature.)

First: Energy is conserved: ΔU = Q − W. Heat added minus work done.

Second: Entropy of an isolated system never decreases. ΔS ≥ 0.

Third: Entropy approaches zero as temperature approaches absolute zero.

Key Equations

ΔU = Q − W
First Law
S = k_B · ln(Ω)
Boltzmann entropy
PV = nRT
Ideal gas law
η = 1 − T_c/T_h
Carnot efficiency

Thermodynamic Processes

ProcessConstant
IsothermalTemperature (T)
IsobaricPressure (P)
IsochoricVolume (V)
AdiabaticNo heat exchange (Q=0)

Entropy & Arrow of Time

Entropy is a measure of disorder or the number of microstates a system can occupy. The Second Law explains why time appears to flow in one direction — systems naturally evolve from ordered to disordered states.

The heat death of the universe is a state of maximum entropy where no more work can be extracted.

Heat Transfer

Conduction: Q/t = kA(ΔT/d) — heat flows through a material.

Convection: Heat transferred by fluid motion. Drives weather and ocean currents.

Radiation: P = εσAT⁴ (Stefan-Boltzmann). All objects emit electromagnetic radiation.

Phase Transitions

Matter changes state at constant temperature by absorbing or releasing latent heat.

TransitionEnergy
Solid → Liquid (melting)Absorbs
Liquid → Gas (boiling)Absorbs
Gas → Liquid (condensation)Releases
Liquid → Solid (freezing)Releases

Electromagnetism

Maxwell's Equations

∇·E = ρ/ε₀
Gauss's Law (electric)
∇·B = 0
Gauss's Law (magnetic — no monopoles)
∇×E = −∂B/∂t
Faraday's Law
∇×B = μ₀J + μ₀ε₀∂E/∂t
Ampère-Maxwell Law

Electrostatics

F = kq₁q₂/r²
Coulomb's Law
E = F/q = kQ/r²
Electric field
V = kQ/r
Electric potential

k = 8.99×10⁹ N·m²/C² (Coulomb's constant)

Circuits

V = IR
Ohm's Law
P = IV = I²R = V²/R
Power dissipation

Series: R_total = R₁ + R₂ + …

Parallel: 1/R = 1/R₁ + 1/R₂ + …

Kirchhoff's Laws: current at junctions sums to zero; voltages around a loop sum to zero.

Magnetism

F = qv×B
Lorentz force
B = μ₀I/2πr
Magnetic field from wire

Moving charges create magnetic fields. Changing magnetic fields induce electric fields (Faraday's Law). This interplay produces electromagnetic waves — light.

Electromagnetic Spectrum

TypeWavelength
Radio> 1 mm
Microwave1 mm – 1 m (approx)
Infrared700 nm – 1 mm
Visible400 – 700 nm
Ultraviolet10 – 400 nm
X-ray0.01 – 10 nm
Gamma< 0.01 nm

Induction & AC

EMF = −dΦ_B/dt
Faraday's Law of Induction

Lenz's Law: induced current opposes the change that caused it.

Transformers step voltage up or down: V₁/V₂ = N₁/N₂. AC power generation and transmission depend entirely on electromagnetic induction.

Quantum Mechanics

Core Principles

Wave-Particle Duality: All matter and energy exhibits both wave and particle properties depending on how it is observed.

Superposition: A quantum system exists in all possible states until measured.

Entanglement: Two particles can be correlated such that measuring one instantly determines the state of the other, regardless of distance.

Uncertainty: Certain pairs of properties (position/momentum, energy/time) cannot both be known precisely.

Key Equations

E = hf = hc/λ
Photon energy (Planck)
λ = h/mv
de Broglie wavelength
iℏ ∂ψ/∂t = Ĥψ
Schrödinger Equation
ΔxΔp ≥ ℏ/2
Heisenberg Uncertainty

The Double-Slit Experiment

When electrons are fired at a barrier with two slits, they create an interference pattern — behaving as waves. But when you detect which slit each electron passes through, the pattern vanishes and they behave as particles.

Observation fundamentally changes the outcome. This is the measurement problem at the heart of quantum mechanics.

Atomic Models

ModelYearDescription
Thomson1897Plum pudding (electrons in positive mass)
Rutherford1911Nucleus with orbiting electrons
Bohr1913Quantized electron orbits
Quantum1926Probability clouds (orbitals)

Quantum Numbers

Each electron is described by four quantum numbers:

n (principal): energy level (1, 2, 3…)

l (angular momentum): orbital shape (0 to n−1)

m_l (magnetic): orientation (−l to +l)

m_s (spin): ±½ (up or down)

Pauli Exclusion: no two electrons in an atom share all four quantum numbers.

Quantum Technologies

Lasers: Stimulated emission of photons — light amplification by quantum transitions.

Transistors: Quantum tunneling and band structure underpin all modern electronics.

MRI: Nuclear spin alignment in magnetic fields.

Quantum Computing: Qubits exploit superposition and entanglement for exponential parallelism.

Quantum Cryptography: Eavesdropping is physically detectable via wavefunction collapse.

Relativity

Special Relativity (1905)

Einstein's two postulates: the laws of physics are the same in all inertial frames, and the speed of light c is constant in all frames.

E² = (pc)² + (mc²)²
Energy-momentum relation
E = mc²
Rest energy (p=0)
E = γmc²
Total energy (moving)

Time Dilation & Length Contraction

Δt' = γΔt
Time dilation (moving clocks run slow)
L' = L/γ
Length contraction
γ = 1/√(1−v²/c²)
Lorentz factor

At v = 0.87c, γ ≈ 2 (clocks run at half speed). At v = 0.9999c, γ ≈ 70.

General Relativity (1915)

Gravity is not a force but the curvature of spacetime caused by mass and energy. Objects follow geodesics (shortest paths) through curved spacetime.

Gμν + Λgμν = 8πG/c⁴ · Tμν
Einstein Field Equations

Gμν = curvature, Tμν = mass-energy, Λ = cosmological constant

Predictions of GR

✓ Gravitational lensing — light bends around massive objects (confirmed 1919)

✓ Gravitational time dilation — GPS must correct for it

✓ Gravitational waves — ripples in spacetime (LIGO detected 2015)

✓ Black holes — regions where spacetime curvature becomes infinite

✓ Expanding universe — GR predicts cosmic expansion (Hubble, 1929)

Black Holes

r_s = 2GM/c²
Schwarzschild radius (event horizon)

At the event horizon, escape velocity equals c. For the Sun: r_s ≈ 3 km. For Earth: r_s ≈ 9 mm.

Hawking radiation: quantum effects cause black holes to slowly radiate. A black hole with mass M will evaporate in time t ≈ 5120πG²M³/(ℏc⁴).

Twin Paradox

One twin travels at near-light speed to a star and returns. Due to time dilation, they age less than the stay-at-home twin. This is real — astronauts returning from the ISS are slightly younger than they would have been on Earth.

GPS satellites: time runs faster in weaker gravity (+45 μs/day) but slower due to orbital speed (−7 μs/day). Net correction: +38 μs/day, or GPS would drift by 10 km/day without it.

Particle Physics — The Standard Model

Quarks

Elementary particles that make up protons and neutrons. Never found in isolation (confinement). Carry fractional electric charge.

QuarkChargeMass (approx)
Up (u)+2/32.2 MeV
Down (d)−1/34.7 MeV
Charm (c)+2/31.28 GeV
Strange (s)−1/396 MeV
Top (t)+2/3173 GeV
Bottom (b)−1/34.18 GeV

Leptons

LeptonChargeMass
Electron (e⁻)−10.511 MeV
Muon (μ)−1105.7 MeV
Tau (τ)−11,777 MeV
Electron neutrino (νe)0< 1.1 eV
Muon neutrino (νμ)0< 0.17 MeV
Tau neutrino (ντ)0< 18.2 MeV

Bosons (Force Carriers)

BosonForceMass
Photon (γ)Electromagnetic0
W⁺ / W⁻Weak nuclear80.4 GeV
Z⁰Weak nuclear91.2 GeV
Gluon (g)Strong nuclear0
Higgs (H)Mass field125.1 GeV
Graviton (?)Gravity0 (theoretical)

The Four Fundamental Forces

ForceRangeRelative Strength
Strong nuclear~10⁻¹⁵ m1
ElectromagneticInfinite10⁻²
Weak nuclear~10⁻¹⁸ m10⁻⁶
GravityInfinite10⁻³⁸

The Standard Model unifies electromagnetic, weak, and strong forces. Gravity remains separate — the great unresolved challenge of physics.

Antimatter

Every particle has a corresponding antiparticle with opposite charge. When a particle meets its antiparticle, they annihilate, releasing energy as photons.

The Big Bang produced equal amounts of matter and antimatter. Why there is more matter than antimatter today — baryogenesis — is one of physics' great unsolved mysteries.

Beyond the Standard Model

Dark Matter: ~27% of the universe's energy density. Does not interact electromagnetically — invisible but gravitationally detected.

Dark Energy: ~68% of energy density. Causes accelerating expansion of the universe.

String Theory: Proposes fundamental strings vibrating at different frequencies instead of point particles.

Supersymmetry: Predicts partner particles for all Standard Model particles (not yet observed).

Legendary Physicists

Isaac Newton
1643 – 1727
Laws of motion and universal gravitation. Invented calculus. Optics and the theory of light. Principia Mathematica (1687) — arguably the greatest scientific work ever written.
Albert Einstein
1879 – 1955
Special and general relativity. E=mc². Photoelectric effect (Nobel 1921). Brownian motion. His 1905 "Annus Mirabilis" papers transformed physics forever.
Richard Feynman
1918 – 1988
Quantum electrodynamics (Nobel 1965). Feynman diagrams. Manhattan Project. Known for brilliant teaching, deep curiosity, and making quantum physics accessible.
Niels Bohr
1885 – 1962
Atomic model with quantized orbits. Copenhagen interpretation of QM. Nobel 1922. Founded the Copenhagen school of quantum physics, debated Einstein for decades.
Marie Curie
1867 – 1934
Discovered polonium and radium. First person to win two Nobel Prizes (Physics 1903, Chemistry 1911). Pioneered radiation research. First woman to earn a physics doctorate in France.
Erwin Schrödinger
1887 – 1961
Wave mechanics and the Schrödinger equation. Nobel 1933. His famous cat thought experiment illustrates quantum superposition and the measurement problem.
Werner Heisenberg
1901 – 1976
Uncertainty principle. Matrix mechanics formulation of QM. Nobel 1932. His uncertainty relations show that nature has irreducible indeterminism at the quantum level.
Max Planck
1858 – 1947
Quantum theory. Planck's constant h. Nobel 1918. Solved the ultraviolet catastrophe by proposing energy comes in discrete quanta — inadvertently launching quantum mechanics.
James Clerk Maxwell
1831 – 1879
Unified electricity and magnetism. Maxwell's equations. Predicted electromagnetic waves and the speed of light. Often ranked the third greatest physicist after Newton and Einstein.
Paul Dirac
1902 – 1984
Dirac equation unifying QM and special relativity. Predicted antimatter (Nobel 1933). Quantum field theory foundations. Known for extraordinary mathematical elegance.
Stephen Hawking
1942 – 2018
Hawking radiation (black holes emit radiation). Singularity theorems with Penrose. A Brief History of Time — one of the best-selling science books ever. Defied ALS for 55 years.
Enrico Fermi
1901 – 1954
First nuclear reactor (Chicago Pile-1, 1942). Fermi-Dirac statistics. Nobel 1938. Manhattan Project. Legendary for Fermi estimation — back-of-envelope calculations with surprising accuracy.