Branches of Physics

Domains of major fields of physics
Physics deals with the combination of matter and energy. It also deals with a wide variety of systems, about which theories have been developed that are used by physicists. In general, theories are experimentally tested numerous times before they are accepted as correct as a description of Nature (within a certain domain of validity). For instance, the theory of classical mechanics accurately describes the motion of objects, provided they are much larger than atoms and moving at much less than the speed of light. These theories continue to be areas of active research: for instance, a remarkable aspect of classical mechanics known as chaos was discovered in the 20th century, three centuries after the original formulation of classical mechanics by Isaac Newton (1642–1727). These "central theories" are important tools for research in more specialized topics, and any physicist, regardless of his or her specialization, is expected to be literate in them.

Classical mechanics[edit]

Classical mechanics is a model of the physics of forces acting upon bodies; includes sub-fields to describe the behaviours of solidsgases, and fluids. It is often referred to as "Newtonian mechanics" after Isaac Newton and his laws of motion. It also includes classical approach as given by Hamiltonian and Lagrange methods. It deals with motion of particles and general system of particles.
There are many branches of classical mechanics, such as: staticsdynamicskinematicscontinuum mechanics (which includes fluid mechanics), statistical mechanics, etc.
  • Mechanics: branch of physics in which we study about the object and properties of an object in form of motion under the action of force.

Thermodynamics and statistical mechanics[edit]

The first chapter of The Feynman Lectures on Physics is about the existence of atoms, which Feynman considered to be the most compact statement of physics, from which science could easily result even if all other knowledge was lost.[1] By modeling matter as collections of hard spheres, it is possible to describe the kinetic theory of gases, upon which classical thermodynamics is based.
Thermodynamics studies the effects of changes in temperaturepressure, and volume on physical systems on the macroscopic scale, and the transfer of energy as heat.[2][3]Historically, thermodynamics developed out of the desire to increase the efficiency of early steam engines.[4]
The starting point for most thermodynamic considerations is the laws of thermodynamics, which postulate that energy can be exchanged between physical systems as heat or work.[5] They also postulate the existence of a quantity named entropy, which can be defined for any system.[6] In thermodynamics, interactions between large ensembles of objects are studied and categorized. Central to this are the concepts of system and surroundings. A system is composed of particles, whose average motions define its properties, which in turn are related to one another through equations of state. Properties can be combined to express internal energy and thermodynamic potentials, which are useful for determining conditions for equilibrium and spontaneous process.
The table below lists the core theories along with many of the concepts they employ.
TheoryMajor subtopicsConcepts
Classical mechanicsNewton's laws of motionLagrangian mechanicsHamiltonian mechanicskinematicsstaticsdynamicschaos theoryacousticsfluid dynamicscontinuum mechanicsDensitydimensiongravityspacetimemotionlength, position, velocityaccelerationGalilean invariancemassmomentumimpulseforceenergyangular velocityangular momentummoment of inertiatorqueconservation lawharmonic oscillatorwaveworkpowerLagrangianHamiltonianTait–Bryan anglesEuler anglespneumatichydraulic
ElectromagnetismElectrostaticselectrodynamicselectricitymagnetismmagnetostaticsMaxwell's equationsopticsCapacitanceelectric chargecurrentelectrical conductivityelectric fieldelectric permittivityelectric potentialelectrical resistanceelectromagnetic fieldelectromagnetic inductionelectromagnetic radiationGaussian surfacemagnetic fieldmagnetic fluxmagnetic monopolemagnetic permeability
Thermodynamicsand statistical mechanicsHeat enginekinetic theoryBoltzmann's constantconjugate variablesenthalpyentropyequation of stateequipartition theoremthermodynamic free energyheatideal gas lawinternal energylaws of thermodynamicsMaxwell relationsirreversible processIsing modelmechanical actionpartition functionpressurereversible processspontaneous processstate functionstatistical ensembletemperaturethermodynamic equilibriumthermodynamic potentialthermodynamic processesthermodynamic statethermodynamic systemviscosityvolumeworkgranular material
Quantum mechanicsPath integral formulationscattering theorySchrödinger equationquantum field theoryquantum statistical mechanicsAdiabatic approximationblack-body radiationcorrespondence principlefree particleHamiltonianHilbert spaceidentical particlesmatrix mechanicsPlanck's constantobserver effectoperatorsquantaquantizationquantum entanglementquantum harmonic oscillatorquantum numberquantum tunnelingSchrödinger's catDirac equationspinwave functionwave mechanicswave–particle dualityzero-point energyPauli exclusion principleHeisenberg uncertainty principle
RelativitySpecial relativitygeneral relativityEinstein field equationsCovarianceEinstein manifoldequivalence principlefour-momentumfour-vectorgeneral principle of relativitygeodesic motiongravitygravitoelectromagnetisminertial frame of referenceinvariancelength contractionLorentzian manifoldLorentz transformationmass–energy equivalencemetricMinkowski diagramMinkowski spaceprinciple of relativityproper lengthproper timereference framerest energyrest massrelativity of simultaneityspacetimespecial principle of relativityspeed of lightstress–energy tensortime dilationtwin paradoxworld line

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