The laws	Math record of law	Formulation of the law
1) Newton’s law	$a = 0$	Anybody, as long as it remains isolated, retains its state of rest or uniform rectilinear motion (the acceleration of the body a is zero).
2) Newton’s law	$m a = F$	The product of the mass of a body by the acceleration it received from the action of the force A of another body, equal to the force A
3) Newton’s law	$F_{12} = - F_{21}$	There is always an equal and opposite reaction to action
Stefan-Boltzmann law of thermal radiation of solids	$q_{12} = \frac{φ_{12} ε_{1} С_{s} F_{1}}{F_{2}} х [{(\frac{Т_{1}}{100})}^{4} - {(\frac{Т_{2}}{100})}^{4}]$	The density of the flux of thermal radiation q₁₂ incident from body 1 to body 2 is directly proportional to the temperature difference of the bodies to the fourth degree.
Ohm’s law	$I = \frac{U}{R}$	The current flowing in the conductor is directly proportional to the voltage applied to it and inversely proportional to the resistance of the conductor.
Planck’s Law	$E_{0 λ} = c_{1} λ^{- 5} (e^{c_{2} / λ t} - 1)$	The density of the heat radiation flux in the blackbody is inversely proportional to the wavelength and directly proportional to the body temperature.
Wine Law	$λ_{М} T = 2879.8$	The wavelength at which the blackbody radiation density reaches its maximum value is inversely proportional to body temperature.
Einstein’s law for photoelectric effect	$h υ = A_{e} + \frac{m V^{2}}{2}$	The energy of a photon descending to the cathode, followed by the emission of an electron by the cathode, is equal to the exit energy and the kinetic energy of the electron.
Bohr’s Postulates	-	1) In a stationary state, the atom does not emit. 2) When an atom transfers from a state with a higher energy to a state with a lower energy, when an electron in an atom jumps from an orbit more remote from the nucleus, a quantum of electromagnetic, thermal radiation is emitted 3) In a stationary state, an electron moves in a certain orbit, a Coulomb force acts on an electron in an atom.