Constants
A constant in physics is a quantity with a fixed value that does not change regardless of the conditions or the variables in a given situation. Constants serve as fundamental benchmarks in various equations and theories, providing consistency and predictability in scientific calculations. Examples include the speed of light in a vacuum (c), Planck’s constant (h), and the gravitational constant (G). These constants are crucial for formulating physical laws and principles, enabling scientists to describe and understand the natural world accurately.
What are Constants?
In physics, constants refer to quantities with fixed values that do not change regardless of the conditions or context in which they are measured. These values remain unchanged over time and space, serving as fundamental reference points in scientific calculations and theories.
List of Constants in Physics
Constant | Symbol | Value | Units |
---|---|---|---|
Speed of Light | c | 2.998Γ10βΈ | meters per second (m/s) |
Gravitational Constant | G | 6.674Γ10β»ΒΉΒΉ | mΒ³kgΒΉsΒ² |
Planck’s Constant | h | 6.626Γ10β34 | Joule seconds (Js) |
Reduced Planck’s Constant | β | 1.055Γ10β34 | Joule seconds (Js) |
Elementary Charge | e | 1.602Γ10β19 | Coulombs (C) |
Avogadro’s Number | NA | 6.022Γ1023 | molβ1 |
Boltzmann Constant | kB | 1.381Γ10β23 | Joules per kelvin (J/K) |
Gas Constant | R | 8.314 | J β molβ1 β Kβ1 |
Permittivity of Free Space | Ξ΅0 | 8.854Γ10β12 | Fβ mβ1 |
Permeability of Free Space | ΞΌ0 | 4ΟΓ10β7 | Nβ Aβ2 |
Electron Mass | me | 9.109Γ10β31 | Kilograms (kg) |
Proton Mass | mp | 1.673Γ10β27 | Kilograms (kg) |
Neutron Mass | mn | 1.675Γ10β27 | Kilograms (kg) |
Fine-Structure Constant | Ξ± | 7.297Γ10β3 | Dimensionless |
Stefan-Boltzmann Constant | Ο | 5.670Γ10β8 | Wβ mβ2β Kβ4 |
Rydberg Constant | Rβ | 1.097Γ107 | mβ1 |
Faraday Constant | F | 9.649Γ104 | Coulombs per mole (C/mol) |
Atomic Mass Unit | u | 1.661Γ10β27 | Kilograms (kg) |
Bohr Radius | a0 | 5.292Γ10β11 | Meters (m) |
Coulomb’s Constant | ke | 8.988Γ109 | Nβ m2β Cβ2 |
Universal Gas Constant | R | 8.314 | Jβ molβ1β Kβ1 |
Planck Length | βP | 1.616Γ10β35 | Meters (m) |
Planck Time | tP | 5.391Γ10β44 | Seconds (s) |
Planck Mass | mPβ | 2.176Γ10β8 | Kilograms (kg) |
Planck Temperature | TP | 1.416Γ1032 | Kelvin (K) |
Wien’s Displacement Constant | b | 2.898Γ10β3 | mβ K |
Bohr Magneton | ΞΌB | 9.274Γ10β24 | Joules per Tesla (J/T) |
Nuclear Magneton | ΞΌN | 5.051Γ10β27 | Joules per Tesla (J/T) |
Magnetic Flux Quantum | Ξ¦0 | 2.068Γ10β15 | Weber (Wb) |
Conductance Quantum | G0 | 7.748Γ10β5 | Siemens (S) |
Von Klitzing Constant | RK | 2.581Γ104 | Ohms (Ξ©) |
Josephson Constant | KJ | 4.835Γ1014 | Hzβ Vβ1 |
Compton Wavelength | Ξ»C | 2.426Γ10β12 | Meters (m) |
Electron Volt | eV | 1.602Γ10β19 | Joules (J) |
Hartree Energy | Eh | 4.360Γ10β18 | Joules (J) |
Atomic Unit of Charge | e | 1.602Γ10β19 | Coulombs (C) |
Atomic Unit of Mass | me | 9.109Γ10β31 | Kilograms (kg) |
Atomic Unit of Length | a0 | 5.292Γ10β11 | Meters (m) |
Atomic Unit of Time | t0 | 2.418Γ10β17 | Seconds (s) |
Fermi Coupling Constant | GF | 1.166Γ10β5 | GeVβ2 |
Weak Mixing Angle | sinβ‘2ΞΈW | 0.2229 | Dimensionless |
Solar Mass | Mβ | 1.989Γ1030 | Kilograms (kg) |
Astronomical Unit | AU | 1.496Γ1011 | Meters (m) |
Light Year | ly | 9.461Γ1015 | Meters (m) |
Parsec | pc | 3.086Γ1016 | Meters (m) |
Hubble Constant | H0 | 67.4 | kmβ sβ1β Mpcβ1 |
Chandrasekhar Limit | MChβ | 1.4 | Solar Masses (M_\odot) |
Electron Magnetic Moment | ΞΌeβ | β9.284Γ10β24 | Joules per Tesla (J/T) |
Speed of Light (c)
The speed of light in a vacuum, denoted as c, is approximately 2.998Γ10βΈ meters per second. This constant is fundamental in physics because it sets the maximum speed at which all energy, matter, and information in the universe can travel. It plays a crucial role in Einstein’s theory of relativity, which shows how space and time are interwoven.
Example: Light from the Sun takes about 8 minutes and 20 seconds to reach Earth, traveling at this constant speed.
Gravitational Constant (G)
The gravitational constant, G, is 6.674Γ10β»ΒΉΒΉ mΒ³kgΒΉsΒ². It is a key quantity in Newton’s law of universal gravitation, which describes the gravitational attraction between two masses. This constant helps us understand the strength of the gravitational force in the universe.
Example: The gravitational force between two 1 kg masses separated by 1 meter is 6.674Γ10β11 Newtons.
Planck’s Constant (h)
Planck’s constant, h, is 6.626Γ10β34 Joule seconds. It is a fundamental constant in quantum mechanics, reflecting the quantization of energy levels in atomic and subatomic systems. It is central to the Heisenberg uncertainty principle and the Planck-Einstein relation E=hΞ½, linking energy and frequency.
Example: The energy of a photon with a frequency of 5Γ1014 Hz is 3.313Γ10β19 Joules, calculated using E=hΞ½.
Reduced Planck’s Constant (β)
The reduced Planck’s constant, β, is 1.055Γ10β34 Joule seconds. It is used frequently in quantum mechanics and is equal to Planck’s constant divided by 2Ο. It is pivotal in defining the scales at which quantum effects become significant.
Example: The angular momentum of an electron in the ground state of a hydrogen atom is β.
Elementary Charge (e)
The elementary charge, e, is 1.602Γ10β19 Coulombs. This constant represents the electric charge carried by a single proton or the magnitude of the charge of a single electron, crucial for understanding electromagnetic interactions.
Example: The charge of an electron is β1.602Γ10β19 Coulombs.
Avogadro’s Number (NAβ)
Avogadro’s number, NβA, is 6.022Γ10 23 per mole. It defines the number of atoms, ions, or molecules in one mole of a substance, forming a bridge between the macroscopic and atomic worlds in chemistry and physics.
Example: One mole of water molecules contains 6.022Γ1023 water molecules.
Boltzmann Constant (kBβ)
The Boltzmann constant, kBβ, is 1.381Γ10β23 Joules per Kelvin. It relates the average kinetic energy of particles in a gas with the temperature of the gas, playing a crucial role in statistical mechanics and thermodynamics.
Example: At room temperature (300 K), the average kinetic energy of a gas molecule is 4.143Γ10β21
Joules.
Gas Constant (R)
The gas constant, R, is 8.314 Jβ molβ1β Kβ1. It is the constant of proportionality in the ideal gas law PV=nRT, linking pressure, volume, temperature, and the amount of gas.
Example: The pressure of 1 mole of an ideal gas at 1 liter and 300 K is 24.942 atm.
Permittivity of Free Space (Ξ΅0β)
The permittivity of free space, Ξ΅0β, is 8.854Γ10β12 Fβ mβ1. It is a measure of the ability of the vacuum to permit electric field lines, essential for understanding electrostatics and capacitance.
Example: The capacitance of a parallel-plate capacitor with a vacuum between the plates, an area of 1m2, and a separation of 1m is 8.854Γ10β9 Farads.
Permeability of Free Space (ΞΌ0β)
The permeability of free space, ΞΌ0β, is 4ΟΓ10β7. This constant measures the ability of the vacuum to support magnetic field lines, important in the study of magnetostatics and electromagnetic theory.
Example: The magnetic field around a long straight wire carrying a current of 1 A is 2Γ10β7 Tesla at a distance of 1 meter.
Electron Mass (meβ)
The electron mass, meβ, is 9.109Γ10β31 kilograms. This is the mass of a single electron at rest and is a fundamental constant in both atomic physics and quantum mechanics.
Example: The rest energy of an electron is 8.187Γ10β14 Joules, calculated using E=mc2
Proton Mass (mpβ)
The proton mass, mpβ, is 1.673Γ10β27 kilograms. It represents the mass of a single proton, fundamental in nuclear physics and chemistry, as protons are a primary constituent of atomic nuclei.
Example: The rest energy of a proton is 1.503Γ10β10 Joules.
Neutron Mass (mnβ)
The neutron mass, mnβ, is 1.675Γ10β27 kilograms. Neutrons, along with protons, make up the atomic nucleus, and their mass is crucial for calculations involving nuclear reactions and stability.
Fine-Structure Constant (Ξ±)
The fine-structure constant, Ξ±, is 7.297Γ10β3. This dimensionless constant characterizes the strength of the electromagnetic interaction between elementary charged particles, fundamental in quantum electrodynamics.
Stefan-Boltzmann Constant (Ο)
The Stefan-Boltzmann constant, Ο is 5.670Γ10β8 Wβ mβ2β Kβ4. It relates the total energy radiated per unit surface area of a black body to the fourth power of its temperature, crucial in thermodynamics and astrophysics.
Rydberg Constant (Rβ)
The Rydberg constant, Rββ, is 1.097Γ107 mβ1. It is used in atomic physics to describe the wavelengths of spectral lines of many chemical elements.
Faraday Constant (F)
The Faraday constant, F, is 9.649Γ104 Coulombs per mole. It represents the charge of one mole of electrons, linking electrochemistry to the amount of substance.
Atomic Mass Unit (u)
The atomic mass unit, u, is 1.661Γ10β27 kilograms. It is used to express atomic and molecular masses, providing a convenient scale for comparison of different atoms and molecules.
Bohr Radius (a0β)
The Bohr radius, a0β, is 5.292Γ10β11 meters. It represents the average distance between the nucleus and the electron in a hydrogen atom in its ground state, fundamental in atomic physics.
Coulomb’s Constant (keβ)
Coulomb’s constant, keβ, is 8.988Γ109 Nβ m2β Cβ2. It is the proportionality constant in Coulomb’s law, describing the force between two point charges.
Universal Gas Constant (R)
The universal gas constant, R, is 8.3148.3148.314 Jβ molβ1β Kβ1\text{J} \cdot \text{mol}^{-1} \cdot \text{K}^{-1}Jβ molβ1β Kβ1. It appears in the ideal gas law and other equations of state, relating the macroscopic properties of gases.
Planck Length (βP)
The Planck length, βPβ, is 1.616Γ10β35 meters. It is a fundamental scale in quantum mechanics, representing the smallest meaningful length, where classical ideas about gravity and space-time cease to be valid.
Planck Time (tPβ)
The Planck time, tPβ, is 1.416Γ1032 seconds. It is the time it takes for light to travel one Planck length, significant in quantum gravity and cosmology.
Planck Mass (mP)
The Planck mass, mPβ, is 2.176Γ10β8 kilograms. It is a fundamental mass scale in quantum mechanics, marking the transition between classical and quantum descriptions of gravity.
Planck Temperature (TPβ)
The Planck temperature, TPβ, is 1.416Γ1032 Kelvin. It is the highest theoretically possible temperature, beyond which the laws of physics as currently understood cease to be useful.
Wien’s Displacement Constant (b)
Wien’s displacement constant, b, is 2.898Γ10β3 m.k. It relates the temperature of a black body to the wavelength at which it emits radiation most strongly, used in thermal radiation studies.
Bohr Magneton (ΞΌBβ)
The Bohr magneton, ΞΌBβ, is 9.274Γ10β24 Joules per Tesla. It is a physical constant related to the magnetic moment of an electron due to its orbital or spin motion, important in quantum mechanics and magnetism.
Nuclear Magneton (ΞΌNβ)
The nuclear magneton, ΞΌNβ, is 5.051Γ10β27 Joules per Tesla. It is similar to the Bohr magneton but smaller, used to describe the magnetic moment of nucleons and nuclei.
Magnetic Flux Quantum (Ξ¦0β)
The magnetic flux quantum, Ξ¦0β, is 2.068Γ10β15 Weber. It is the quantum of magnetic flux, fundamental in the study of superconductivity and quantum Hall effects.
Conductance Quantum (G0)
The conductance quantum, G0β, is 7.748Γ10β5 Siemens. It represents the quantized unit of electrical conductance, crucial in the study of quantum transport.
Von Klitzing Constant (RKβ)
The von Klitzing constant, RK, is 2.581Γ104 Ohms. It is used in the quantum Hall effect to define the resistance quantum, providing a standard for electrical resistance.
Josephson Constant (KJβ)
The Josephson constant, KJβ, is 4.835Γ1014 Hzβ Vβ1. It relates the voltage across a Josephson junction to the frequency of the resulting AC current, important in superconductivity.
Compton Wavelength (Ξ»Cβ)
The Compton wavelength, Ξ»Cβ, is 2.426Γ10β12 meters. It represents a quantum mechanical limit to the localization of particles, significant in quantum field theory.
Electron Volt (eV)
An electron volt, eV, is 1.602Γ10β19 Joules. It is a unit of energy commonly used in atomic, nuclear, and particle physics, representing the energy gained by an electron when accelerated through a potential difference of one volt.
Hartree Energy (Ehβ)
The Hartree energy, Ehβ, is 4.360Γ10β18 Joules. It is a unit of energy used in atomic physics and quantum chemistry, representing the electrostatic potential energy of the hydrogen atom in its ground state.
Atomic Unit of Charge (e)
The atomic unit of charge, e, is 1.602Γ10β19 Coulombs. It is used as a convenient unit of electric charge in atomic physics and quantum chemistry.
Atomic Unit of Mass (meβ)
The atomic unit of mass, meβ, is 9.109Γ10β31 kilograms. It provides a convenient scale for comparing the masses of different particles in atomic and molecular systems.
Atomic Unit of Length (a0β)
The atomic unit of length, a0β, is 5.292Γ10β11 meters. It is the Bohr radius, representing the typical size of atoms and providing a natural length scale in atomic physics.
Atomic Unit of Time (t0β)
The atomic unit of time, t0β, is 2.418Γ10β17 seconds. It provides a natural time scale in atomic and molecular physics, corresponding to the period of an electron orbiting a hydrogen nucleus.
Fermi Coupling Constant (GFβ)
The Fermi coupling constant, GF, is 1.166Γ10β5 GeVβ2. It characterizes the strength of the weak force, one of the four fundamental forces in the universe, crucial in particle physics.
Weak Mixing Angle (sinβ‘2ΞΈWβ)
The weak mixing angle, sinβ‘2ΞΈWβ, is 0.2229. It quantifies the mixing of the electromagnetic and weak forces in the electroweak interaction, fundamental in the Standard Model of particle physics.
Solar Mass (Mββ)
The solar mass, Mββ, is 1.989Γ1030 kilograms. It is the mass of the Sun, used as a standard unit for expressing the masses of other stars and galaxies in astrophysics.
Astronomical Unit (AU)
The astronomical unit, AU, is 1.496Γ1011 meters. It represents the average distance between the Earth and the Sun, providing a useful scale for measuring distances within the solar system.
Light Year (ly)
A light year, ly, is 9.461Γ1015 meters. It represents the distance that light travels in a vacuum in one year, used to express astronomical distances.
Parsec (pc)
A parsec, pc, is 3.086Γ1016 meters. It is a unit of distance used in astronomy, equal to about 3.26 light years, representing the distance at which one astronomical unit subtends an angle of one arcsecond.
Hubble Constant (H0β)
The Hubble constant, H0β, is 67.4 kmβ sβ1β Mpcβ1. It measures the rate of expansion of the universe, fundamental in cosmology.
Chandrasekhar Limit (MChβ)
The Chandrasekhar limit, MChβ, is 1.4 solar masses. It is the maximum mass of a stable white dwarf star, beyond which it will collapse into a neutron star or black hole, significant in stellar evolution.
Electron Magnetic Moment (ΞΌeβ)
The electron magnetic moment, ΞΌeβ, is β9.284Γ10β24 Joules per Tesla. It represents the intrinsic magnetic moment of an electron due to its spin, fundamental in quantum mechanics and magnetism.
FAQ’s
Why are constants important in physics?
Constants provide a foundation for developing theories and equations, ensuring consistency and accuracy in scientific measurements and predictions.
What is the Coulomb constant?
The Coulomb constant (ke) is 8.987551787Γ109 NΒ·mΒ²/CΒ², used in electrostatics to describe the force between two point charges.
What is the proton mass?
he proton mass (ππ) is 1.67262192369Γ10β27 kilograms, a fundamental constant in particle physics.
What is the neutron mass?
The mass of a neutron is approximately 1.674927498Γ10β27atomic mass units (amu).
What is the Hartree energy?
The Hartree energy (Ehβ) is 4.359Γ10-18 joules, a unit of energy used in atomic physics and quantum chemistry.
What is the Compton wavelength?
The Compton wavelength (ππΆ) is2.426Γ10β12 meters, representing the wavelength increase of a photon when scattered by a particle.
What is the Faraday constant?
The Faraday constant (πΉ) is 96485.33212 C/mol, the total electric charge carried by one mole of electrons.
What is the Wien displacement constant?
The Wien displacement constant (b) is 2.897771955Γ10β3 mΒ·K, describing the relationship between the temperature of a blackbody and the wavelength at which it emits most strongly.
What is the universal gas constant?
The universal gas constant (π ) is 8.3144621 J/molΒ·K, the constant in the equation of state of an ideal gas, relating energy scale to temperature scale.
What is the Rydberg constant?
The Rydberg constant (π β) is1.097373Γ107mβ1, used in atomic physics to describe the wavelengths of spectral lines.