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Physics constants and reference tables

Quantitative physics depends on a shared set of constants, units and tabulated material properties. Physical constants are quantities that, as far as can be measured, do not change with time or place. Familiar examples include the speed of light in vacuum, the gravitational constant, the elementary charge, the Planck constant and the Boltzmann constant. Their accepted values are determined by international metrology bodies and revised as measurement precision improves.

Constants are meaningful only alongside a consistent system of units. The International System of Units (SI) defines base units such as the metre, kilogram, second, ampere, kelvin, mole and candela, from which all other units are derived. Reference tables list conversion factors between SI and older or specialised units, and collect the scientific and technical acronyms, symbols and abbreviations used in equations and on instruments.

A large part of physical reference data describes the properties of materials and atoms. Tables of electrical conductivity and resistivity rank materials from good conductors to insulators, while acoustic data give the speed of sound and impedance in different media. Atomic physics contributes atomic weights and spectroscopic data: the characteristic wavelengths of light that each element emits or absorbs, which allow substances to be identified by their spectra. Data on condensed matter cover densities, melting and boiling points, and thermal and mechanical behaviour of solids and liquids. Gathered into handbooks and databases, these values let scientists and engineers carry out calculations, design experiments and compare measurements against established standards.

Frequently asked questions

What is a physical constant?
A physical constant is a measured quantity, such as the speed of light or the elementary charge, that is believed to have the same value everywhere and at all times.
Why are SI units important?
SI units give scientists a single agreed system for expressing measurements, so that results and constants can be compared and combined consistently worldwide.
What is atomic spectroscopic data used for?
It records the specific wavelengths of light that each element emits or absorbs, which lets researchers identify elements and study the structure of atoms.





Atomic and nuclear physics constants - tables 
Arrangement of electrons in atoms In the following table the electrons in an atom are shown arranged in shells and sub-shells
Chart interface to nuclear data
Ionization potentials The ionization potential is the least energy, expressed in electron volts, which is necessary to remove an electron from a free unexcited neutral atom (or additional electron from an ionized atom). It can be determined either directly from the speed of the slowest electrons which will ionize the atom by collision, or more accurately from the limit of a spectroscopic series
Nuclear structure and decay data Nuclear structure and decay data, NuBase with the Q-value calculator
Chart of the Nuclides Interactive Chart of Nuclides
Chart of the Nuclides Interactive Chart of Nuclei, Chart of the Nuclides
Neutrinos mass Laboratory measurements and limits for neutrino properties
Nuclides map nuclides map, map of the Nuclides
Nuclides: Table of nuclides
Nuclides chart of the nuclides
Nuclides: chart of the nuclides pdf file
Radioactive sources
SPECTRES d'emission Tous les atomes emettent dans certaines conditions des rayonnements formés d'un ensemble de radiations monochromatiques. Chaque atome possède un spectre qui lui est propre, en Français
Table of Isotopes pdf file
X-ray photoemission spectroscopy

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