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Constants in Physics are fundamental values that remain unchanged across different contexts and experiments. These constants are universal in nature and are independent of the unit system used. They are essential for verifying the accuracy of theories and enabling practical applications based on those theories.
Some common constants are the Speed of Light in Vacuum (c), Planck's Constant (h), Boltzmann Constant (k), Elementary Charge (e), etc. In this article, we will provide a comprehensive list of all important constants in physics.
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Physical constants are fundamental quantities that cannot be explained by a theory and must be measured experimentally.
All physical constants are represented by some alphabet and have some value associated with them. The numerical values of dimensional physical constants depend on the unit system used to express them, but the physical constants themselves are independent of the unit system.
Some of the universal physical constants are:
Speed of Light in Vacuum is represented by "c" and has a value of 299,792.46 Km/sec. In other units, the speed of light is given as:
Units | Speed of Light in Vacuum |
|---|---|
Meters per second (m/s) | 299,792,458 |
Miles per second (mi/s) | 186,282.397 |
Astronomical Units per day (AU/day) | 173.1446 |
Light-years per year (ly/yr) | 9.461×1012 |
The Planck constant, symbolized as 'h', is a fundamental constant in physics, approximately equal to 6.626 x 10-34 joule seconds (J·s). It describes the relationship between energy and frequency in quantum mechanics.
The gravitational constant, denoted as 'G', has a value of approximately 6.674 × 10-11 Newton meters squared per kilogram square (N.m2/kg2). It quantifies the strength of the gravitational force between two objects with mass.
The Boltzmann constant, represented by 'k', has a value of approximately 1.381 × 10-23 joules per kelvin (J/K). The Boltzmann constant helps quantify the average energy per particle in a system at a given temperature.
The Rydberg constant, denoted as 'R∞', is approximately equal to 1.097 × 107 per meter (m-1). The Rydberg constant relates to the wavelengths of spectral lines emitted or absorbed by these atoms.
| Constant | Symbol | Value | Units |
|---|---|---|---|
| Speed of Light in Vacuum | c | 299,792,458 | meters per second (m/s) |
| Planck Constant | h | 6.62607015×10−34 | joule seconds (J⋅s) |
| Gravitational Constant | G | 6.67430×10−11 | cubic meters per kilogram per second squared (m3/kg/s2) |
| Boltzmann Constant | kB | 1.380649×10−23 | joules per kelvin (J/K) |
| Rydberg Constant | R∞ | 10,973,731.568527 | per meter (1/m) |
Some other universal physical constants are:
Constant | Symbol | Value | Units |
|---|---|---|---|
Elementary Charge | e | 1.602176634×10−19 | coulombs (C) |
Avogadro's Number | NA | 6.022×1023 | per mole |
Permeability of Free Space | μ0 | 4π×10−7 | newton per ampere squared (N/A2) |
Permittivity of Free Space | ε0 | 8.854187817×10−12 | farads per meter (F/m) |
Fine-structure Constant | α | 7.2973525693×10−3 | dimensionless |
In quantum mechanics, several fundamental constants play pivotal roles in describing the behaviour of particles at the smallest scales. These constants include Planck's constant (h), the reduced Planck constant (ħ), the elementary charge (e), the electron rest mass (mₑ), and the speed of light in a vacuum (c).
As we've already discussed Planck's Constant and Speed of light in vacuum, we'll discuss the rest constants in quantum mechanics.
Constants | Symbol | Value | Units |
|---|---|---|---|
Electron Rest Mass | mₑ | 9.109 × 10-31 | kilograms (kg) |
Reduced Planck's Constant | ħ | 1.054 × 10-34 | Joule Seconds (J·s) |
Bohr Magneton | ?B | 9.274 × 10-24 | Joule per Tesla (J/T) |
The reduced Planck constant, denoted as ħ (pronounced "h-bar"), is a fundamental constant in quantum mechanics, defined as ħ = h / (2π), where h is Planck's constant. Its value is approximately 1.054 × 10-34 joule seconds (J·s).
The Bohr magneton, denoted as μB, is a fundamental constant in quantum mechanics, approximately equal to 9.274 × 10-24 joule per tesla (J/T). It represents the magnetic moment of an electron due to its orbital angular momentum in a hydrogen atom.
In electromagnetism, several fundamental constants characterize the behavior of electric and magnetic fields. These constants include the permittivity of free space (ε₀), the permeability of free space (μ₀), and the speed of light in a vacuum (c).
Constant | Symbol | Value | Units |
|---|---|---|---|
Permittivity of free space | ε₀ | 8.854 × 10-12 | farads per meter (F/m) |
Permeability of free space | μ₀ | 4π×10−7 | Newton per Ampere squared (N/A2) |
Gravitational and cosmological constants are fundamental parameters in physics and cosmology that play crucial roles in understanding the structure, evolution, and behavior of the universe.
Constant | Symbol | Value | Units |
|---|---|---|---|
Gravitational Constant | G | 6.674 × 10-11 | Newton meters squared per kilogram squared (N.m2/kg2) |
Cosmological Constant | Λ | 1.1056 × 10-52 | Per square meter (1/m2) |
The terms "gravitational constant" and "Newtonian gravitational constant" are often used interchangeably to refer to the same fundamental constant, denoted as G.
Cosmological constants, often denoted by Λ (lambda), are parameters that arise in cosmological models, such as the Lambda-CDM (Lambda cold dark matter) model, which describes the large-scale structure and evolution of the universe.
Thermodynamic constants are fundamental parameters in thermodynamics, the branch of physics that deals with heat, energy, and work. These constants play essential roles in describing the behaviour of matter and energy in various physical systems, providing foundational principles for understanding and predicting thermodynamic processes.
Some of the key thermodynamic constants include:
Let's discuss these constant in detail.
This constant, denoted by R, represents the universal gas constant and is fundamental in the ideal gas law. Its value is 8.3145 in joules per mole per kelvin (J/mol/K) or in other appropriate units depending on the context.
Avogadro's number, denoted by N_A, represents the number of atoms, molecules, or particles in one mole of a substance. Its value is approximately 6.022 × 1023 per mole (mol-1), and it plays a crucial role in converting between macroscopic and microscopic scales in thermodynamics.
The Stefan-Boltzmann constant, denoted by σ, relates the total energy radiated by a blackbody to its temperature. It has a value of approximately 5.670 × 10-8 watts per square meter per kelvin to the fourth power (W/m2/K4) and is essential for understanding radiative heat transfer in thermodynamic systems.
All the important constants in thermodynamics are listed in the following table:
Constants | Symbol | Value | Units |
|---|---|---|---|
Gas Constant | R | 8.3145 | Joules per Mole per Kelvin (J/mol/K) |
Avogadro Number | NA | 6.022 × 1023 | Per Mole (mol-1) |
σ | 5.670 × 10-8 | Watts per Square Meter per Kelvin to the fourth power (W/m2/K4) | |
Faraday Constant | F | 96,485.33289 | Coulombs per mole (L/mol) |
Molar Volume of Ideal Gas at STP | Vm | 22.414 | Liters per Mole (L/mol) |
Constants in atomic and nuclear physics are fundamental parameters that describe various aspects of atomic and nuclear systems. These constants play crucial roles in understanding the behavior of atoms, nuclei, and their interactions. Some important constants in atomic and nuclear physics include:
| Constant | Symbol | Value | Units |
|---|---|---|---|
| Fine-Structure Constant | α | 0.0072973525693 | Dimensionless |
| Proton Rest Mass | mp | 1.6726219 × 10−27 | Kilograms (kg) |
| Neutron Rest Mass | mn | 1.674927471 × 10−27 | Kilograms (kg) |
Proton-to-Electron Mass Ratio | mp/me | 1836.15267389 | Dimensionless |
| Bohr Radius | a0 | 5.29177210903 × 10−11 | Meters (m) |
| Unified Atomic Mass Unit (u) | u | 1.66053906660 × 10−27 | Kilograms (kg) |
| Nuclear Magneton | μN | 5.0507837461 × 10−27 | Joules per tesla (J/T) |
In summary, physical constants, dimensionless constants, and universal constants are foundational to physics, spanning quantum mechanics to nuclear physics. These constants, such as Planck's constant and the speed of light, offer fixed numerical values crucial for understanding natural laws. They serve as fundamental pillars guiding theoretical models and experimental inquiries, illuminating the mysteries of the universe and driving scientific progress.
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