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EINSTEIN COEFFICIENTS

  • Einstein coefficients
  • Quantities describing probability of absorption or emission of light

    the Einstein coefficients are quantities describing the probability of absorption or emission of a photon by an atom or molecule. The Einstein A coefficients

    Einstein coefficients

    Einstein coefficients

    Einstein_coefficients

  • Planck's law
  • Spectral density of light emitted by a black body

    above, can be expressed in terms of the Einstein coefficients. The relationships between the Einstein coefficients will yield the expression of Kirchhoff's

    Planck's law

    Planck's law

    Planck's_law

  • Stimulated emission
  • Release of a photon triggered by another

    introduced spontaneous and stimulated emission, as well as the Einstein coefficients. Einstein's theory of radiation was ahead of its time and prefigures the

    Stimulated emission

    Stimulated emission

    Stimulated_emission

  • Einstein Tower
  • Observatory

    The Einstein Tower (German: Einsteinturm) is an astrophysical observatory in the Albert Einstein Science Park in Potsdam, Germany. The Tower was built

    Einstein Tower

    Einstein Tower

    Einstein_Tower

  • List of things named after Albert Einstein
  • Einstein notation Einstein coefficients Einstein's cosmological constant Einstein relation (kinetic theory) Planck–Einstein relation Einstein–Brillouin–Keller

    List of things named after Albert Einstein

    List_of_things_named_after_Albert_Einstein

  • Einstein ring
  • Feature seen when light is gravitationally lensed by an object

    An Einstein ring, also known as an Einstein–Chwolson ring or Chwolson ring (named for Orest Chwolson), is created when light from a galaxy or star passes

    Einstein ring

    Einstein ring

    Einstein_ring

  • Albert Einstein
  • German-born theoretical physicist (1879–1955)

    Albert Einstein (14 March 1879 – 18 April 1955) was a German-born theoretical physicist best known for developing the theory of relativity. Einstein also

    Albert Einstein

    Albert Einstein

    Albert_Einstein

  • Einstein notation
  • Shorthand notation for tensor operations

    physics and differential geometry, Einstein notation (also known as the Einstein summation convention or Einstein summation notation) is a notational

    Einstein notation

    Einstein_notation

  • Albert Einstein Science Park
  • Research institute in Germany

    Albert Einstein Science Park is located on the Telegrafenberg hill in Potsdam, Germany. The park was named after the physicist Albert Einstein. The best

    Albert Einstein Science Park

    Albert Einstein Science Park

    Albert_Einstein_Science_Park

  • Outline of Albert Einstein
  • Theoretical physicist (1879–1955)

    outline is provided as an overview of and topical guide to Albert Einstein: Albert Einstein – German-born theoretical physicist. He developed the theory of

    Outline of Albert Einstein

    Outline_of_Albert_Einstein

  • Albert Einstein House
  • United States historic place

    The Albert Einstein House at 112 Mercer Street in Princeton, Mercer County, New Jersey, United States, was the home of Albert Einstein from 1935 until

    Albert Einstein House

    Albert Einstein House

    Albert_Einstein_House

  • List of scientific publications by Albert Einstein
  • In 1918, Einstein developed a general theory of the process by which atoms emit and absorb electromagnetic radiation (the Einstein coefficients), which

    List of scientific publications by Albert Einstein

    List of scientific publications by Albert Einstein

    List_of_scientific_publications_by_Albert_Einstein

  • Bose–Einstein statistics
  • Description of the behaviour of bosons

    In quantum statistics, Bose–Einstein statistics (B–E statistics) describes one of two possible ways in which a collection of non-interacting identical

    Bose–Einstein statistics

    Bose–Einstein statistics

    Bose–Einstein_statistics

  • Einstein relation (kinetic theory)
  • Equation in Brownian motion

    Einstein relation is a previously unexpected[clarification needed] connection revealed independently by William Sutherland in 1904, Albert Einstein in

    Einstein relation (kinetic theory)

    Einstein_relation_(kinetic_theory)

  • Spontaneous emission
  • Quantum mechanical state change

    the phenomenon of stimulated emission and introduced the Einstein Coefficients. Einstein's quantum theory of radiation anticipated ideas later expressed

    Spontaneous emission

    Spontaneous_emission

  • Oscillator strength
  • Dimensionless quantity in spectroscopy

    spectral line Sum rule in quantum mechanics Electronic band structure Einstein coefficients W. Demtröder (2003). Laser Spectroscopy: Basic Concepts and Instrumentation

    Oscillator strength

    Oscillator_strength

  • Friction
  • Force resisting sliding motion

    Encyclopædia Britannica. Vol. 11 (11th ed.). 1911. Coefficients of Friction – tables of coefficients, plus many links Physclips: Mechanics with animations

    Friction

    Friction

    Friction

  • Photon
  • Elementary particle or quantum of light

    the Einstein coefficients. Einstein could not fully justify his rate equations, but claimed that it should be possible to calculate the coefficients A i

    Photon

    Photon

  • Schwarzschild's equation for radiative transfer
  • Formula for radiative heat transfer

    the absorption and emission of radiation are controlled by the Einstein coefficients for absorption, emission and stimulated emission of a photon (B12

    Schwarzschild's equation for radiative transfer

    Schwarzschild's_equation_for_radiative_transfer

  • Wien approximation
  • Law of physics

    increases. Albert Einstein used this property in his 1917 quantum theory of radiation to establish a relationship between the coefficients that give the rates

    Wien approximation

    Wien approximation

    Wien_approximation

  • Spectral line ratios
  • l_{2}}A_{u_{2}\rightarrow l_{2}}}}} The transition frequencies and the Einstein coefficients of transitions are well known and listed in various tables as in

    Spectral line ratios

    Spectral_line_ratios

  • Pearson correlation coefficient
  • Measure of linear correlation

    without changing the correlation coefficient. (This holds for both the population and sample Pearson correlation coefficients.) More general linear transformations

    Pearson correlation coefficient

    Pearson correlation coefficient

    Pearson_correlation_coefficient

  • Laser
  • Device that emits light via optical amplification

    Planck's law of radiation, conceptually based upon probability coefficients (Einstein coefficients) for the absorption, spontaneous emission, and stimulated

    Laser

    Laser

    Laser

  • Fluorescence
  • Emission of light by a substance that has absorbed light

    "Franck–Condon Factors, r-Centroids, Electronic Transition Moments, and Einstein Coefficients for Many Nitrogen and Oxygen Band Systems". Journal of Physical

    Fluorescence

    Fluorescence

    Fluorescence

  • Detailed balance
  • Principle in kinetic systems

    Metropolis–Hastings algorithm Atomic spectral line (deduction of the Einstein coefficients) Random walks on graphs Boltzmann, L. (1964), Lectures on gas theory

    Detailed balance

    Detailed_balance

  • General relativity
  • Theory of gravitation as curved spacetime

    symbols (sometimes called the affine connection coefficients or Levi-Civita connection coefficients) which is symmetric in the two lower indices. Greek

    General relativity

    General relativity

    General_relativity

  • Albert Einstein: The Practical Bohemian
  • Play written by Ed Metzger

    Albert Einstein: The Practical Bohemian is a stage play that is the only show officially endorsed by the Einstein family. A quote from Albert Einstein's first

    Albert Einstein: The Practical Bohemian

    Albert_Einstein:_The_Practical_Bohemian

  • Luminiferous aether
  • Obsolete postulated medium for the propagation of light

    aether. This was further elaborated by Einstein in some semi-popular articles (1918, 1920, 1924, 1930). In 1918, Einstein publicly alluded to that new definition

    Luminiferous aether

    Luminiferous aether

    Luminiferous_aether

  • Cosmological constant
  • Value representing energy density of space

    letter lambda: Λ), alternatively called Einstein's cosmological constant, is a coefficient that Albert Einstein initially added to his field equations

    Cosmological constant

    Cosmological constant

    Cosmological_constant

  • Ambiguity
  • Type of uncertainty of meaning where several interpretations are possible

    their value (and sometimes even dimension, as in the case of the Einstein coefficients) depends on the system of notations. Many terms are ambiguous. Each

    Ambiguity

    Ambiguity

    Ambiguity

  • Absorption spectroscopy
  • Spectroscopic techniques that measure the absorption of radiation

    absorption spectrum can be calculated from the emission spectrum using Einstein coefficients. The scattering and reflection spectra of a material are influenced

    Absorption spectroscopy

    Absorption spectroscopy

    Absorption_spectroscopy

  • Einstein's constant
  • Topics referred to by the same term

    theory), diffusion coefficient Speed of light in vacuum This disambiguation page lists articles associated with the title Einstein's constant. If an internal

    Einstein's constant

    Einstein's_constant

  • Christoffel symbols
  • Array of numbers describing a metric connection

    otherwise noted. Einstein summation convention is used in this article, with vectors indicated by bold font. The connection coefficients of the Levi-Civita

    Christoffel symbols

    Christoffel_symbols

  • Diatomic molecule
  • Molecule composed of any two atoms

    "Franck-Condon Factors, r-Centroids, Electronic Transition Moments, and Einstein Coefficients for Many Nitrogen and Oxygen Band Systems". Journal of Physical

    Diatomic molecule

    Diatomic molecule

    Diatomic_molecule

  • Special relativity
  • Theory of interwoven space and time by Albert Einstein

    scientific theory of the relationship between space and time. In Albert Einstein's 1905 paper, "On the Electrodynamics of Moving Bodies", the theory is presented

    Special relativity

    Special relativity

    Special_relativity

  • Emergency Committee of Atomic Scientists
  • Einstein's committee of atomic scientists

    Emergency Committee of Atomic Scientists (ECAS) was founded by Albert Einstein and Leó Szilárd in May, 1946, primarily as a fundraising and policy-making

    Emergency Committee of Atomic Scientists

    Emergency_Committee_of_Atomic_Scientists

  • Einstein's Gift
  • 2003 play by Vern Thiessen

    Einstein's Gift is a 2003 play written by Canadian playwright Vern Thiessen and published in 2003 by Playwrights Canada Press. Through the recollections

    Einstein's Gift

    Einstein's_Gift

  • Ensemble interpretation
  • Concept in Quantum mechanics

    phases are of real physical importance, and that in consequence the Einstein coefficients are inadequate to describe the phenomena except in special cases

    Ensemble interpretation

    Ensemble_interpretation

  • Diathermal wall
  • Barrier permeable to heat but not matter

    one-way radiation. These things are important for the study of the Einstein coefficients, which relies partly on the notion of thermodynamic equilibrium

    Diathermal wall

    Diathermal_wall

  • Mass diffusivity
  • Proportionality constant in some physical laws

    approximate dependence of the diffusion coefficient on temperature in liquids can often be found using Stokes–Einstein equation, which predicts that D T 1

    Mass diffusivity

    Mass_diffusivity

  • Emission spectrum
  • Frequencies of light emitted by atoms or chemical compounds

    monochromatic emission coefficient relating to its temperature and total power radiation. This is sometimes called the second Einstein coefficient, and can be deduced

    Emission spectrum

    Emission spectrum

    Emission_spectrum

  • Kaniadakis distribution
  • Continuous probability distribution

    Kamel; Tribeche, Mouloud (2014-06-24). "Planck radiation law and Einstein coefficients reexamined in Kaniadakis κ statistics". Physical Review E. 89 (6)

    Kaniadakis distribution

    Kaniadakis_distribution

  • Nonlinear theory of semiconductor lasers
  • Nontraditional laser theory of Fabry-Perot semiconductor lasers

    derivations have been made: Einstein’s spectral coefficient in a semiconductor laser and, accordingly, Einstein’s coefficient; formula for the saturation

    Nonlinear theory of semiconductor lasers

    Nonlinear_theory_of_semiconductor_lasers

  • Brownian motion
  • Random motion of particles suspended in a fluid

    expression to Einstein's formula for the diffusion coefficient was also found by Walther Nernst in 1888 in which he expressed the diffusion coefficient as the

    Brownian motion

    Brownian motion

    Brownian_motion

  • Newman–Penrose formalism
  • Notation in general relativity

    equations connecting spin coefficients, Weyl-NP and Ricci-NP scalars (recall that in an orthogonal tetrad, Ricci rotation coefficients would respect Cartan's

    Newman–Penrose formalism

    Newman–Penrose_formalism

  • Quantum noise
  • Quantum effect of uncertainty

    approximation, and semi-classical model of a two level atom). The Einstein coefficients and the laser rate equations are adequate if one is interested in

    Quantum noise

    Quantum_noise

  • Satyendra Nath Bose
  • Indian theoretical physicist (1894–1974)

    early 1920s, in developing the foundation for Bose–Einstein statistics, and the theory of the Bose–Einstein condensate. A Fellow of the Royal Society, he was

    Satyendra Nath Bose

    Satyendra Nath Bose

    Satyendra_Nath_Bose

  • Diffusion
  • Transport of dissolved species from the highest to the lowest concentration region

    multicomponent diffusion must be non-linear. The Einstein relation (kinetic theory) connects the diffusion coefficient and the mobility (the ratio of the particle's

    Diffusion

    Diffusion

    Diffusion

  • Quantum error correction
  • Process in quantum computing

    control, it remains coupled to its environment through nonzero Einstein coefficients. When the environment is cooled to its vacuum state, this coupling

    Quantum error correction

    Quantum_error_correction

  • Curvilinear coordinates
  • Coordinate system whose directions vary in space

    all points where the derivatives are well-defined, we define the Lamé coefficients (after Gabriel Lamé) by h 1 = | h 1 | ; h 2 = | h 2 | ; h 3 = | h 3 |

    Curvilinear coordinates

    Curvilinear coordinates

    Curvilinear_coordinates

  • Polylogarithm
  • Special mathematical function

    Fermi–Dirac distribution and the Bose–Einstein distribution, and is also known as the Fermi–Dirac integral or the Bose–Einstein integral. In quantum electrodynamics

    Polylogarithm

    Polylogarithm

    Polylogarithm

  • Transport coefficient
  • transport coefficient γ {\displaystyle \gamma } measures how rapidly a perturbed system returns to equilibrium. The transport coefficients occur in transport

    Transport coefficient

    Transport_coefficient

  • Green–Kubo relations
  • Equation relating transport coefficients to correlation functions

    transport coefficients which is valid for systems of arbitrary temperature T, and density. They proved that linear transport coefficients are exactly

    Green–Kubo relations

    Green–Kubo_relations

  • Zurich Notebook
  • Notebook of Albert Einstein

    Albert Einstein's notebooks, from his time in Zürich. It contains much of Einstein's foundational work on general relativity. John D. Norton. "Einstein's Zurich

    Zurich Notebook

    Zurich_Notebook

  • Taylor series
  • Mathematical approximation of a function

    }}\right)x^{4}+\cdots \end{aligned}}} Comparing the coefficients of g(x) cos x with the coefficients of ex, c 0 = 1 ,     c 1 = 1 ,     c 2 − 1 2 c 0 =

    Taylor series

    Taylor series

    Taylor_series

  • Structure constants
  • Coefficients of an algebra over a field

    mathematics, the structure constants or structure coefficients of an algebra over a field are the coefficients of the basis expansion (into linear combination

    Structure constants

    Structure constants

    Structure_constants

  • Curved spacetime
  • Mathematical theory of the geometry of space and time

    appearance of the metric coefficients alone does not determine whether a space is intrinsically curved. Complicated coefficients may arise merely from the

    Curved spacetime

    Curved spacetime

    Curved_spacetime

  • Fudge factor
  • Ad hoc element introduced into a calculation

    misleadingly good match to experimental data. In theoretical physics, when Albert Einstein originally tried to produce a general theory of relativity, he found that

    Fudge factor

    Fudge_factor

  • Optical decay
  • just spontaneous emission, and its rate is determined with the Einstein Coefficients. For the most of laser systems, the effects of decoherence determine

    Optical decay

    Optical_decay

  • Virial expansion
  • Series expansion of the equation of state for a many-particle system

    Kamerlingh Onnes. The terms A, B, and C represent the virial coefficients. The leading coefficient A is defined as the constant value of 1, which ensures that

    Virial expansion

    Virial_expansion

  • Fizeau experiment
  • Experiment measuring the speed of light in moving water

    measurement was developed with the advent of Albert Einstein's theory of special relativity. Einstein later pointed out the importance of the experiment

    Fizeau experiment

    Fizeau experiment

    Fizeau_experiment

  • Gravitational constant
  • Physical constant for the strength of gravity induced by a mass

    effects in Isaac Newton's law of universal gravitation and in Albert Einstein's theory of general relativity. It is also known as the universal gravitational

    Gravitational constant

    Gravitational constant

    Gravitational_constant

  • Spacetime
  • Mathematical model combining space and time

    further development of general relativity, Einstein fully incorporated the spacetime formalism. When Einstein published in 1905, another of his competitors

    Spacetime

    Spacetime

    Spacetime

  • Metric tensor (general relativity)
  • Tensor that describes the 4D geometry of spacetime

    constant G {\displaystyle G} will be kept explicit. This article employs the Einstein summation convention, where repeated indices are automatically summed over

    Metric tensor (general relativity)

    Metric_tensor_(general_relativity)

  • Hamilton–Jacobi–Einstein equation
  • Reformulation of general relativity

    In general relativity, the Hamilton–Jacobi–Einstein equation (HJEE) or Einstein–Hamilton–Jacobi equation (EHJE) is an equation in the Hamiltonian formulation

    Hamilton–Jacobi–Einstein equation

    Hamilton–Jacobi–Einstein_equation

  • Quantum mechanics
  • Description of physical properties at the atomic and subatomic scale

    Einstein's long-running exchanges with Bohr about the meaning and status of quantum mechanics are now known as the Bohr–Einstein debates. Einstein believed

    Quantum mechanics

    Quantum mechanics

    Quantum_mechanics

  • Fluid solution
  • Class of exact solutions to Einstein's field equations

    Newton's identities, the traces of the powers of the Einstein tensor are related to these coefficients as follows: G a a = t 1 = a 1 {\displaystyle

    Fluid solution

    Fluid_solution

  • Mathematics of general relativity
  • connection coefficients are not the components of a tensor. Generally speaking, there are D 3 {\displaystyle D^{3}} independent connection coefficients at each

    Mathematics of general relativity

    Mathematics_of_general_relativity

  • Kaniadakis exponential distribution
  • Probability distribution

    Ourabah, Kamel; Tribeche, Mouloud (2014). "Planck radiation law and Einstein coefficients reexamined in Kaniadakis κ statistics". Physical Review E. 89 (6)

    Kaniadakis exponential distribution

    Kaniadakis_exponential_distribution

  • Quantum superposition
  • Principle of quantum mechanics

    {\displaystyle \Psi =c_{1}\Psi _{1}+c_{2}\Psi _{2}} for arbitrary complex coefficients c 1 {\displaystyle c_{1}} and c 2 {\displaystyle c_{2}} . If the wave

    Quantum superposition

    Quantum superposition

    Quantum_superposition

  • Einstein Prize for Laser Science
  • 3-inch brass medal including Einstein's image and a depiction of a two-level transition including the A and B coefficients. Recipients of the prize include:

    Einstein Prize for Laser Science

    Einstein Prize for Laser Science

    Einstein_Prize_for_Laser_Science

  • Aether theories
  • Set of theories

    John Stachel argue, Einstein's views on the "new aether" are not in conflict with his abandonment of the aether in 1905. As Einstein himself pointed out

    Aether theories

    Aether_theories

  • Convection–diffusion equation
  • Combination of the diffusion and convection (advection) equations

    variable coefficients in the variable c(x): y ′ ( x ) = f ( x ) y ( x ) + g ( x ) . {\displaystyle y'(x)=f(x)y(x)+g(x).} where the coefficients are: f (

    Convection–diffusion equation

    Convection–diffusion_equation

  • Absolute zero
  • Lowest theoretical temperature

    mechanical phenomena such as superconductivity, superfluidity, and Bose–Einstein condensation. The particles still exhibit zero-point energy motion, as

    Absolute zero

    Absolute zero

    Absolute_zero

  • Tensor
  • Algebraic object with geometric applications

    the rightmost expression the summation sign was suppressed: this is the Einstein summation convention, which will be used throughout this article. The components

    Tensor

    Tensor

    Tensor

  • Aether drag hypothesis
  • Early attempt to explain constant speed of light

    own aether theory, which banished any form of aether dragging. Albert Einstein's special theory of relativity (1905) excludes aether as a mechanical medium

    Aether drag hypothesis

    Aether_drag_hypothesis

  • Fick's laws of diffusion
  • Mathematical descriptions of molecular diffusion

    particles according to the Stokes–Einstein relation. The modeling and prediction of Fick's diffusion coefficients is difficult. They can be estimated

    Fick's laws of diffusion

    Fick's laws of diffusion

    Fick's_laws_of_diffusion

  • Emmy Noether
  • German mathematician (1882–1935)

    mathematical physics. Noether was described by Pavel Alexandrov, Albert Einstein, Jean Dieudonné, Hermann Weyl, and Norbert Wiener as the most important

    Emmy Noether

    Emmy Noether

    Emmy_Noether

  • Debye model
  • Method in physics

    vibrations of the atomic lattice (heat) as phonons in a box in contrast to the Einstein solid model, which treats the solid as many individual, non-interacting

    Debye model

    Debye model

    Debye_model

  • Paul Dirac
  • British physicist (1902–1984)

    change through emission and absorption, and derived the correct Einstein A and B coefficients. Dirac's quantum electrodynamics (QED) included terms with infinite

    Paul Dirac

    Paul Dirac

    Paul_Dirac

  • Gradient
  • Multivariate derivative (mathematics)

    {\hat {\mathbf {e} }}^{i}} , using the scale factors (also known as Lamé coefficients) h i = ‖ e i ‖ = g i i = 1 / ‖ e i ‖ {\displaystyle h_{i}=\lVert \mathbf

    Gradient

    Gradient

    Gradient

  • Curl (mathematics)
  • Circulation density in a vector field

    with one function as coefficient: a 123 d x ∧ d y ∧ d z . {\displaystyle a_{123}\,dx\wedge dy\wedge dz.} (Here the a-coefficients are real functions of

    Curl (mathematics)

    Curl (mathematics)

    Curl_(mathematics)

  • Gödel metric
  • Solution of Einstein field equations

    Gödel universe, is an exact solution, found in 1949 by Kurt Gödel, of the Einstein field equations in which the stress–energy tensor contains two terms: the

    Gödel metric

    Gödel_metric

  • Basis (linear algebra)
  • Set of vectors used to define coordinates

    the coefficients, one loses the correspondence between coefficients and basis elements, and several vectors may have the same set of coefficients. For

    Basis (linear algebra)

    Basis (linear algebra)

    Basis_(linear_algebra)

  • Ezra T. Newman
  • American physicist (1929–2021)

    emeritus at the University of Pittsburgh. Newman was awarded the 2011 Einstein Prize from the American Physical Society. Newman was born in the Bronx

    Ezra T. Newman

    Ezra T. Newman

    Ezra_T._Newman

  • Kerr metric
  • Exact solution for the Einstein field equations

    quasispherical event horizon. The Kerr metric is an exact solution of the Einstein field equations of general relativity; these equations are highly non-linear

    Kerr metric

    Kerr metric

    Kerr_metric

  • Hall effect
  • Electromagnetic effect in physics

    Sakaguchi, Isao; Adachi, Yutaka; Haneda, Hajime (2008). "Positive Hall coefficients obtained from contact misplacement on evident n-type ZnO films and crystals"

    Hall effect

    Hall effect

    Hall_effect

  • History of Lorentz transformations
  • Development of linear transformations forming the Lorentz group

    other frame the same event has coordinates x′,y′,z′ and t′. Using the coefficients of a symmetric matrix g, the associated bilinear form, and a linear transformations

    History of Lorentz transformations

    History_of_Lorentz_transformations

  • Alternatives to general relativity
  • Proposed theories of gravity

    attempt to describe the phenomenon of gravitation in competition with Einstein's theory of general relativity. There have been many different attempts

    Alternatives to general relativity

    Alternatives_to_general_relativity

  • Volatility (finance)
  • Degree of variation of a trading price series over time

    uncover the hidden principles underpinning the world around us, as Albert Einstein did with his theory of relativity", we should remember that "models are

    Volatility (finance)

    Volatility (finance)

    Volatility_(finance)

  • Michelson–Morley experiment
  • 1887 investigation of the speed of light

    which rules out motion against an aether. Of this experiment, Albert Einstein wrote, "If the Michelson–Morley experiment had not brought us into serious

    Michelson–Morley experiment

    Michelson–Morley experiment

    Michelson–Morley_experiment

  • WKB approximation
  • Solution method for linear differential equations

    approximate solutions to linear differential equations with spatially varying coefficients. It is typically used for a semiclassical calculation in quantum mechanics

    WKB approximation

    WKB_approximation

  • One-way speed of light
  • Concept in relativity theory

    reflection) and back again to the detector. Albert Einstein chose a synchronization convention (see Einstein synchronization) that made the one-way speed equal

    One-way speed of light

    One-way_speed_of_light

  • Free fall
  • Motion of a body subject only to gravity

    1885). It is the basis of the equivalence principle, from which basis Einstein's theory of general relativity initially took off. Dynamical time scale

    Free fall

    Free_fall

  • Kähler manifold
  • Manifold with Riemannian, complex and symplectic structure

    as Hermitian Yang–Mills connections, or special metrics such as Kähler–Einstein metrics. Every smooth complex projective variety is a Kähler manifold.

    Kähler manifold

    Kähler_manifold

  • Regge calculus
  • Formalism in general relativity

    producing simplicial approximations of spacetimes that are solutions to the Einstein field equation. The calculus was introduced by the Italian theoretician

    Regge calculus

    Regge_calculus

  • Asymptotic safety
  • Attempt to find a consistent theory of quantum gravity

    renormalizable according to the old point of view. (In order to render the Einstein–Hilbert action 1 16 π G ∫ d 2 x g R {\displaystyle \textstyle {1 \over

    Asymptotic safety

    Asymptotic safety

    Asymptotic_safety

  • Viscosity
  • Resistance of a fluid to shear deformation

    Enskog theory for Mie fluids: Prediction of diffusion coefficients, thermal diffusion coefficients, viscosities, and thermal conductivities". The Journal

    Viscosity

    Viscosity

    Viscosity

  • Stern–Volmer relationship
  • Relationship describing the kinetics of intermolecular photochemical deactivation

    the viscosity of the solution. This formula is derived from the Stokes–Einstein relation and is only useful in this form in the case of two spherical particles

    Stern–Volmer relationship

    Stern–Volmer relationship

    Stern–Volmer_relationship

  • Stokes radius
  • Parameter of solute diffusion

    The Stokes radius or Stokes–Einstein radius of a solute is the radius of a hard sphere that diffuses at the same rate as that solute. Named after George

    Stokes radius

    Stokes_radius

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  • Amber
  • Surname or Lastname

    English

    Amber

    English : unexplained.Possibly an Americanized spelling of French Imbert or a translation of German and Jewish Bernstein, which means ‘amber’.Muslim (widespread throughout the Muslim world) : from the Arabic personal name ‛Anbar, literally ‘perfume’, ‘ambergris’, figuratively ‘good’, ‘pleasant’, ‘agreeable’.

    Amber

  • Geirstein
  • Boy/Male

    Norse

    Geirstein

    Rock or hard spear.

    Geirstein

  • Eystein
  • Boy/Male

    Norse

    Eystein

    Lucky.

    Eystein

  • Winston
  • Surname or Lastname

    English

    Winston

    English : from an Old English personal name composed of the elements wynn ‘joy’ + stān ‘stone’.English : habitational name from any of various places called Winston or Winstone, from various Old English personal names + Old English tūn ‘enclosure’, ‘settlement’, or, in the case of Winstone in Gloucestershire, Old English stān ‘stone’.Americanized form of Jewish Weinstein.

    Winston

  • Burston
  • Surname or Lastname

    English

    Burston

    English : habitational name from any of various places called Burston, in Buckinghamshire, Norfolk, and Staffordshire, which have different origins. The Buckinghamshire place name is from an Old English personal name Briddel + Old English þorn ‘thorn tree’; the place in Norfolk is named with Old English byrst ‘rough ground’, ‘landslip’ + tūn ‘farmstead’; the Staffordshire place name has the same second element, the first being an Old English personal name Burgwine or Burgwulf.English : possibly from an unrecorded Old English personal name, Burgstān.Jewish (American) : Americanized spelling of Burstein (see Bernstein).

    Burston

  • Eistein
  • Boy/Male

    Norse

    Eistein

    Lucky.

    Eistein

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  • Potential
  • n.

    In the theory of gravitation, or of other forces acting in space, a function of the rectangular coordinates which determine the position of a point, such that its differential coefficients with respect to the coordinates are equal to the components of the force at the point considered; -- also called potential function, or force function. It is called also Newtonian potential when the force is directed to a fixed center and is inversely as the square of the distance from the center.

  • Osculatrix
  • n.

    A curve whose contact with a given curve, at a given point, is of a higher order (or involves the equality of a greater number of successive differential coefficients of the ordinates of the curves taken at that point) than that of any other curve of the same kind.

  • Coefficient
  • n.

    A number or letter put before a letter or quantity, known or unknown, to show how many times the latter is to be taken; as, 6x; bx; here 6 and b are coefficients of x.

  • Covariant
  • n.

    A function involving the coefficients and the variables of a quantic, and such that when the quantic is lineally transformed the same function of the new variables and coefficients shall be equal to the old function multiplied by a factor. An invariant is a like function involving only the coefficients of the quantic.

  • Invariant
  • n.

    An invariable quantity; specifically, a function of the coefficients of one or more forms, which remains unaltered, when these undergo suitable linear transformations.