| Revision as of 21:29, 10 February 2003 editLooxix~enwiki (talk | contribs)6,016 editsm Add Coulomb's law← Previous edit | Revision as of 21:16, 11 February 2003 edit undoXJaM (talk | contribs)Extended confirmed users11,305 editsm typoNext edit → | ||
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| ** ] ''F''<sub>g</sub> = ''G'' ''m''<sub>1</sub> ''m''<sub>2</sub>/''r''<sup>2</sup> (universal ]) | ** ] ''F''<sub>g</sub> = ''G'' ''m''<sub>1</sub> ''m''<sub>2</sub>/''r''<sup>2</sup> (universal ]) | ||
| ** ] | ** ] | ||
| * ] (''F'' = ''q''<sub>1</sub>''q''<sub>2</sub>/4π&epsilon<sub>0</sub>''r''<sup>2</sup>) | * ] (''F'' = ''q''<sub>1</sub>''q''<sub>2</sub>/4πε<sub>0</sub>''r''<sup>2</sup>) | ||
| * ] (''V'' = ''I'' ''R'') | * ] (''V'' = ''I'' ''R'') | ||
| * ] (] and ] laws) | * ] (] and ] laws) | ||
Revision as of 21:16, 11 February 2003
This is a list of physical laws discovered by science. Some might say that the only true "laws" of science are those of the scientific method.
- Boyle's Law (pressure and volume of ideal gas)
- Charles & Gay-Lussac (gases expand equally with the same change of temperature)
- Dulong-Petit law cV = 3R/M (specific heat capacity at constant volume)
- Einstein
- Relativity E=mc (Energy=mass×speed of light)
- Laws of Kepler (planetary motion)
- Beer-Lambert (light absorption)
- Newton
- Newton's laws of motion (inertia, F=ma, action and reaction)
- General law of gravitation Fg = G m1 m2/r (universal gravitation force)
- Law of heat conduction
- Coulomb's law (F = q1q2/4πε0r)
- Ohm's Law (V = I R)
- Kirchhoff's Laws (current and voltage laws)
- Maxwell's equations (electric and magnetic fields: in vacuum File:Del.gif·E = 0, File:Del.gif·B = 0, File:Del.gif×E = -∂B/∂t, File:Del.gif×B = c∂E/∂t)
- Poiseuille's law ΦV = (π r/8 η)(Δp/l) (voluminal laminar stationary flow of incompressible uniform viscous liquid through a cylindrical tube with the constant circular cross-section)
- Radiation laws
- Planck's Law of Radiation (spectral density in a radiation of a blackbody)
- Stefan-Boltzmann law j = σ T (total radiation from a blackbody)
- Wien's law λ0 T = kW (wavelength of the peak of the emission of a blackbody)
- Thermodynamics
