هذه قائمة بقوانين العلوم مقسمة حسب المجال.

Others, such as Roger Penrose in his 2004 book The Road to Reality (subtitled "A Complete Guide to the Laws of the Universe"), argue that there are a large number of established laws of science. Some laws, such as Descartes’ first law of nature, have become obsolete.^[] A rough outline of the basic laws in science is as follows:

قوانين الحفظ

Most significant laws in science are conservation laws:

• Conservation of mass law
• Conservation of energy law
• Conservation of momentum law
• Conservation of angular momentum law
• Charge conservation law

These fundamental laws follow from homogeneity of space, time and phase (see Emmy Noether theorem).

Gas laws

Other less significant (non fundamental) laws are the mathematical consequences of the above conservation laws for derivative physical quantities (mathematically defined as force, pressure, temperature, density, force fields, etc):

• Boyle's Law (pressure and volume of ideal gas)
• Charles & Gay-Lussac (gases expand equally with the same change of temperature)
• Ideal Gas Law ${\displaystyle PV=\ nRT$

Einstein's laws

• Energy of photons - Energy equals Planck's constant multiplied by the frequency of the light.

${\displaystyle E\ =hf$

Special Relativity

• Constancy of the speed of light
• Lorentz transformations - Transformations of Cartesian coordinates between relatively moving reference frames.

  ${\displaystyle x'=(x-vt)/{\sqrt {1-v^{2 /c^{2$

  ${\displaystyle y'=y$

  ${\displaystyle z'=z$

  ${\displaystyle t'=(t-vx/c^{2 )/{\sqrt {1-v^{2 /c^{2$

• Mass-energy equivalence

  ${\displaystyle E=m{c}^2}$

General Relativity

• Energy-momentum (including mass via E=mc²) curves spacetime.

  This is described by the Einstein field equations:

  ${\displaystyle R_{ab -{1 \over 2 R\,g_{ab ={8\pi G \over c^{4 T_{ab .$

  ${\displaystyle R_{ab}}$${\displaystyle R}$${\displaystyle g_{ab}}$${\displaystyle T_{ab}}$${\displaystyle \mathrm{\pi <!--\; \pi \; -->}}$${\displaystyle c}$${\displaystyle G}$

  ${\displaystyle \ E=mc^{2$ where ${\displaystyle m={\frac {m_{0 {\sqrt {1-{\frac {v^{2 {c^{2$

قوانين نيوتن

• Newton's laws of motion - Replaced by relativity

1. Law of Inertia
2. ${\displaystyle \ F=d({\vec {p )/dt$. Although it implies ${\displaystyle \ F=ma$, that is not necessarily true.
3. ${\displaystyle F_{ab}=-<!--\; -\; -->F_{ba}}$

• Law of heat conduction
• General law of gravitation - Gravitational force between two objects equals the gravitational constant times the product of the masses divided by the distance between them squared.

• ${\displaystyle F_{g =G{\frac {m_{1 m_{2 {r^{2$
• This law is really just the low limit solution of Einstein's field equations and is not accurate with modern high precision gravitational measurements.

Chemical laws

Chemical laws are those laws of nature relevant to chemistry. The most fundamental concept in chemistry is the law of conservation of mass, which states that there is no detectable change in the quantity of matter during an ordinary chemical reaction. Modern physics shows that it is actually energy that is conserved, and that energy and mass are related; a concept which becomes important in nuclear chemistry. Conservation of energy leads to the important concepts of equilibrium, thermodynamics, and kinetics.

Additional laws of chemistry elaborate on the law of conservation of mass. Joseph Proust's law of definite composition says that pure chemicals are composed of elements in a definite formulation; we now know that the structural arrangement of these elements is also important.

Dalton's law of multiple proportions says that these chemicals will present themselves in proportions that are small whole numbers (i.e. 1:2 O:H in water); although in many systems (notably biomacromolecules and minerals) the ratios tend to require large numbers, and are frequently represented as a fraction.

More modern laws of chemistry define the relationship between energy and transformations.

• In equilibrium, molecules exist in mixture defined by the transformations possible on the timescale of the equilibrium, and are in a ratio defined by the intrinsic energy of the molecules—the lower the intrinsic energy, the more abundant the molecule.
• Transforming one structure to another requires the input of energy to cross an energy barrier; this can come from the intrinsic energy of the molecules themselves, or from an external source which will generally accelerate transformations. The higher the energy barrier, the slower the transformation occurs.
• There is a hypothetical intermediate, or transition structure, that corresponds to the structure at the top of the energy barrier. The Hammond-Leffler Postulate states that this structure looks most similar to the product or starting material which has intrinsic energy closest to that of the energy barrier. Stabilizing this hypothetical intermediate through chemical interaction is one way to achieve catalysis.
• All chemical processes are reversible (law of microscopic reversibility) although some processes have such an energy bias, they are essentially irreversible.

قوانين الكهرومغناطيسية

• Coulomb's law - Force between any two charges is equal to the product of the charges divided by أربعة pi times the vacuum permittivity times the distance squared between the two charges.

${\displaystyle F={\frac {\left|q_{1 q_{2 \right| {4\pi \epsilon _{0 r^{2$

• Ohm's Law

${\displaystyle V=I\cdot R$

• Kirchhoff's circuit laws (current and voltage laws)
• Kirchhoff's law of thermal radiation
• Maxwell's equations (electric and magnetic fields):

الاسم الشكل التفاضلي الجزئي قانون گوس : ${\displaystyle \nabla \cdot \mathbf {D =\rho$ قانون گوس للمغناطيسية: ${\displaystyle \nabla \cdot \mathbf {B =0$ قانون فاراداي في التحريض: ${\displaystyle \nabla \times \mathbf {E =-{\frac {\partial \mathbf {B {\partial t$ Ampère's law + Maxwell's extension: ${\displaystyle \nabla \times \mathbf {H =\mathbf {J +{\frac {\partial \mathbf {D {\partial t$

قوانين الديناميكا الحرارية

ديناميكا حرارية

• Zeroth law of thermodynamics

  If two systems are in thermal equilibrium with a third system, then they are in thermal equilibrium with one another.

• First law of thermodynamics

  The change in energy dU in a system is accounted for entirely by the heat δQ absorbed by the system and the work δW done by the system:

  ${\displaystyle \mathrm {d U=\delta Q-\delta W\,$

• Second law of thermodynamics

  ${\displaystyle \int {\frac {\delta Q {T \geq 0$

• Third law of thermodynamics

  As the temperature T of a system approaches absolute zero, the entropy S approaches a minimum value C: as T → 0, S → C.

• Onsager reciprocal relations - sometimes called the Fourth Law of Thermodynamics

  ${\displaystyle \mathbf {J _{u =L_{uu \,\nabla (1/T)-L_{ur \,\nabla (m/T)\!$;

  ${\displaystyle \mathbf {J _{r =L_{ru \,\nabla (1/T)-L_{rr \,\nabla (m/T)\!$.

قوانين الكم

ميكانيكا الكم

• Heisenberg Uncertainty Principle - Uncertainty in position multiplied by uncertainty in momentum is equal to or greater than the reduced Planck constant divided by 2.

  ${\displaystyle \Delta x\Delta p\geq {\frac {\hbar {2$

• Matter wavelength - Laid the foundations of particle-wave duality and was the key idea in the Schrödinger equation.

  ${\displaystyle \lambda ={\frac {hc {mc^{2 ={\frac {h {mc ={\frac {h {p$

• Schrödinger equation - Describes the time dependence of a quantum mechanical system.

  ${\displaystyle H(t)\left|\psi (t)\right\rangle =i\hbar {\partial \over \partial t \left|\psi (t)\right\rangle$

  The Hamiltonian H(t) is a self-adjoint operator acting on the state space, ${\displaystyle \mathrm{\psi <!--\; \psi \; -->}(t)}$] at time t, i is the unit imaginary number, ${\displaystyle \mathrm{\hslash <!--\; \hslash \; -->}}$

It is thought that the successful integration of Einstein's field equations with the uncertainty principle and Schrödinger equation, something no one has achieved so far with a testable theory, will lead to a theory of quantum gravity, the most basic physical law sought after today.

قوانين أخرى

• معادلات ناڤييه-ستوكس لميكانيكا الموائع

${\displaystyle -\nabla p+\mu \left(\nabla ^{2 \mathbf {u +{1 \over 3 \nabla (\nabla \cdot \mathbf {u )\right)+\rho \mathbf {u =\rho \left({\partial \mathbf {u \over \partial t +\mathbf {u \cdot \nabla \mathbf {u \right)$

• Poiseuille's law (voluminal laminar stationary flow of incompressible uniform viscous liquid through a cylindrical tube with the constant circular cross-section)

${\displaystyle \Phi _{V ={\pi r^{4 \over 8\eta {\triangle p^{\star \over l$

• Radiation laws

• قانون پلانك في إشعاع الجسم الأسود (الكثافة الطيفية في إشعاع الجسم الأسود)
• قانون ڤين (طول موجة قمة إشعاع جسم أسود) :λ₀T = k_w
• Stefan-Boltzmann law (total radiation from a black body)

  ${\displaystyle j^{\star =\sigma T^{4$

• قوانين كپلر (حركة الكواكب)
• قانون أڤوگادرو(الأحجام المتساوية من الغازات المثالية، عند نفس درجة الحرارة والضغط، يحتوون على نفس العدد من الجسيمات، أوالجزيئات.)
• بير-لامبير (امتصاص الضوء)
• قانون دولونگ-پتيت (سعة الحرارة النوعية عند حجم ثابت)

  ${\displaystyle c_{V ={\frac {3R {M$

قانون بايز-بالوت (الرياح تنتقل بعكس عقارب الساعة نظام منخفض الضغط في نصف الكرة الشمالي)

انظر أيضا

• قانون فيزيائي - ويتضمن مناقشة ما يشكل القانون
• قوانين علوم على اسم شخص

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