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Length used in relativistic quantum physics
The Compton wavelength is defined as the wavelength of a photon whose energy is the same as the rest energy of that particle. The wavelength sets the minimum
Compton_wavelength
Scattering of photons off charged particles
reduced, and thus its wavelength is increased. This trade-off between wavelength and energy in response to the collision is the Compton effect. Because of
Compton_scattering
American physicist (1892–1962)
the Compton wavelength of the electron; it is equal to 2.43×10−12 m. The wavelength shift λ′ − λ lies between zero (for θ = 0°) and twice the Compton wavelength
Arthur_Compton
Radius of the event horizon of a Schwarzschild black hole
center of the object); rs is the Schwarzschild radius. The reduced Compton wavelength, ℏ / M c {\displaystyle \hbar /Mc} , is a characteristic length
Schwarzschild_radius
Reference value of length
School of Physics "Enrico Fermi". pp. 142–143. ISBN 9781586031671. "Compton wavelength over 2 pi". The NIST Reference on Constants, Units, and Uncertainty
Unit_of_length
Verifying quantum electrodynamics by measuring the fine-structure constant
measured with high precision through a very precise measurement of its Compton wavelength. This is then combined with the value of the Rydberg constant to extract
Precision_tests_of_QED
Low energy photon scattering off charged particles
equivalently, if the wavelength of the light is much greater than the Compton wavelength of the particle (e.g., for electrons, longer wavelengths than hard x-rays)
Thomson_scattering
Quantum mechanical waves describing matter
basis of our theory." (This frequency is also known as Compton frequency.) To find the wavelength equivalent to a moving body, de Broglie set the total
Matter_wave
Physical constant providing length scale to interatomic interactions
two being the Bohr radius a 0 {\displaystyle a_{0}} and the reduced Compton wavelength of the electron λ ¯ e {\displaystyle \lambda \!\!\!{\bar {}}_{\text{e}}}
Classical_electron_radius
Particle effect
time, and an oscillation term with an amplitude equal to the reduced Compton wavelength. That oscillation term is the so-called Zitterbewegung. Another way
Zitterbewegung
Units defined only by physical constants
interpreted in various ways, such as considering a particle whose reduced Compton wavelength is comparable to its Schwarzschild radius, though whether those concepts
Planck_units
Physical constants of energy and wavenumber
is the Compton wavelength of the electron, f C = m e c 2 / h {\displaystyle f_{\text{C}}=m_{\text{e}}c^{2}/h} is the Compton frequency of the
Rydberg_constant
Electron-photon scattering cross section
where λ c = h / m e c {\displaystyle \lambda _{c}=h/m_{e}c} is the Compton wavelength of the electron (~2.42 pm). Notice that the scatter ratio λ ′ / λ
Klein–Nishina_formula
Elementary particle with negative charge
amount called the Compton shift. The maximum magnitude of this wavelength shift is h/mec, which is known as the Compton wavelength. For an electron, it
Electron
Condition in which spacetime itself breaks down
does not permit particles to inhabit a space smaller than their Compton wavelengths. Many theories in physics have mathematical singularities of one
Gravitational_singularity
Measure of the size of atomic nuclei
masses of the electron and the deuteron respectively while λC is the Compton wavelength of the electron. For the proton, the two radii are the same. The first
Charge_radius
Range of frequencies or wavelengths of electromagnetic radiation
the full range of electromagnetic radiation, organized by frequency or wavelength. The spectrum is divided into separate bands, with different names for
Electromagnetic_spectrum
Electromagnetic radiation humans can see
1923 Arthur Holly Compton showed that the wavelength shift seen when low intensity X-rays scattered from electrons (so called Compton scattering) could
Light
Hypothetical elementary particle that mediates gravity
yielded a new upper bound on the mass of gravitons. The graviton's Compton wavelength is at least 1.6×1016 m, or about 1.6 light-years, corresponding to
Graviton
Modified letter of the Greek alphabet
also called . In physics, it represents the reduced Compton wavelength, i.e. the Compton wavelength λ divided by 2π. It was first used in a phonetics context
Barred_lambda
Deviation of electrons from their original trajectories
known as the Compton wavelength, but is in fact a proportionality constant for the wavelength shift. The collision causes the photon wavelength to increase
Electron_scattering
Conjectured dark matter in cosmology
position of a particle is larger than its Compton wavelength (a particle with mass 10−22 eV has a Compton wavelength of 1.3 light years), and for some reasonable
Scalar_field_dark_matter
Topics referred to by the same term
Compton scattering, an effect observed when photons interact with electrons Compton wavelength, a quantum mechanical property of a particle Compton (surname)
Compton
Theory of gravity in which the graviton has nonzero mass
observations. Observations of gravitational waves have constrained the Compton wavelength of the graviton to be λg > 1.6×1016 m, which can be interpreted as
Massive_gravity
Quantum phenomena
particle, m c 2 {\displaystyle mc^{2}} , would need to occur over the Compton wavelength of the particle, ℏ / m c {\displaystyle \hbar /mc} , which works out
Klein_paradox
Hypothetical form of cold dark matter proposed to solve the cuspy halo problem
the order of ≈ 10 − 22 {\displaystyle \approx 10^{-22}} eV; so a Compton wavelength on the order of 1 light year. Fuzzy cold dark matter halos in dwarf
Fuzzy_cold_dark_matter
Energy driving the accelerated expansion of the universe
like matter, the field must be very light so that it has a large Compton wavelength. In the simplest scenarios, the quintessence field has a canonical
Dark_energy
Recoil force on accelerating charged particle
physics, and therefore may not be valid at distances of roughly the Compton wavelength or below. There are, however, two analogs of the formula that are
Abraham–Lorentz_force
Pictorial representation of the behavior of subatomic particles
to determine the position so that the uncertainty is less than the compton wavelength, the uncertainty in energy is large enough to produce more particles
Feynman_diagram
Comparison of a wide range of lengths
particle displacement in acoustics 2.4 pm – the Compton wavelength of an electron 5 pm – shorter X-ray wavelengths (approx.) To help compare different orders
Orders_of_magnitude_(length)
Unit of length about the size of a hydrogen atom
is one of a set of related lengths, the others being the reduced Compton wavelength of the electron ( λ ¯ e {\displaystyle \lambda \!\!\!{\bar {}}_{\mathrm
Bohr_radius
Method in physics used to deal with infinities
/ ( m e c ) {\displaystyle \hbar /(m_{\text{e}}c)} is the reduced Compton wavelength of the electron. The total effective mass of a spherical charged particle
Renormalization
Dimensionless number that quantifies the strength of the electromagnetic interaction
characteristic lengths: the classical electron radius re, the reduced Compton wavelength of the electron ƛe, and the Bohr radius a0: re = αƛe = α2a0. In quantum
Fine-structure_constant
Energy–frequency relation in quantum mechanics
.} This is a direct consequence of the Planck–Einstein relation. Compton wavelength French & Taylor (1978), pp. 24, 55. Cohen-Tannoudji, Diu & Laloë (1973/1977)
Planck_relation
Most basic type of physical force
{H}}\,c\,r/\hbar }} , with Higgs mass 125.18 GeV. Because the reduced Compton wavelength of the Higgs boson is so small (1.576×10−18 m, comparable to the W
Fundamental_interaction
Optical filter device
radiation passing through polarizer, λ {\displaystyle \lambda } – Compton wavelength of electron, c {\displaystyle c} – speed of light in vacuum. Circular
Polarizer
Speculative physics theory
transmitted by a light scalar field (i.e. a scalar field with a long Compton wavelength, which determines the range). This has prompted much recent interest
Fifth_force
Hypothetical invisible cosmic material
black holes through a process called superradiance. If the boson's Compton wavelength is comparable to the black hole's event horizon size, the particles
Dark_matter
Variety of resonant circuit
where λ 0 = h / m 0 c − {\displaystyle \lambda _{0}=h/m_{0}c-\ } Compton wavelength of electron. Thus, the wave quantum LC circuit has no charges in it
Quantum_LC_circuit
System of measurement
{\displaystyle \alpha ^{2}\,a_{0}\approx 0.0000532\,a_{0}} reduced Compton wavelength of the electron λ ¯ e = ℏ m e c {\displaystyle \lambda \!\!\!{\bar
Atomic_units
Model of the universe – alternative to the Big Bang model
hole whose Schwarzschild radius is approximately the same as its Compton wavelength; the evaporation of such a particle has been evoked as the source
Steady-state_model
Details in the emission spectrum of an atom
t\approx \hbar /mc=\lambda \!\!\!{\bar {}}_{\text{C}}} , their reduced Compton wavelength. The electrons of the atom interact with those pairs. This yields
Fine_structure
Effect in quantum electrodynamics
{\displaystyle k>\pi /a_{0}} . It is also valid only for wavelengths longer than the Compton wavelength, or equivalently k < m c / ℏ {\displaystyle k<mc/\hbar
Lamb_shift
Quantum physics terminology
g is the gauge coupling constant, and ƛi = ℏ/mic is the reduced Compton wavelength. A scalar boson produces a universally attractive potential, whereas
Bound_state
Gauge boson self-energy due to interactions with virtual particles
must be modified at extremely small distances less than the reduced Compton wavelength λ ¯ c {\displaystyle {\bar {\lambda }}_{\text{c}}} ( = ℏ m c = 3.86
Vacuum_polarization
Screened Coulomb potential which exponentially decays
where λ ¯ {\displaystyle \lambda \!\!\!{\bar {}}} is the reduced Compton wavelength of the meson. μ {\displaystyle \ \mu \ } can be estimated from
Yukawa_potential
2015 detection made by LIGO interferometers
observations to 2.1×10−58 kg, corresponding to 1.2×10−22 eV/c2 or a Compton wavelength (λg) of greater than 1013 km, roughly 1 light-year. Using the lowest
First observation of gravitational waves
First_observation_of_gravitational_waves
Hypothesis relating age of the universe to physical constants
universe's volume to the volume of a typical nucleon bounded by its Compton wavelength, and he identified this ratio with the sum of elementary events or
Dirac large numbers hypothesis
Dirac_large_numbers_hypothesis
Formula to approximate nuclear mass based on nucleon counts
25 femtometers. R P {\displaystyle R_{\text{P}}} is the proton reduced Compton wavelength, and m p {\displaystyle m_{\text{p}}} is the proton mass. This gives
Semi-empirical_mass_formula
Hypothetical elementary particle
pair discovered that the value would also explain the luminosity and wavelength of fast radio bursts, being a possible origin for both phenomena. In 2022
Axion
Electron diffraction using very short pulses
_{n}}{\sigma _{x}}},} where Δs is the reciprocal-space resolution, λe is the Compton wavelength of the electrons, ϵn is the normalized emittance of the electrons
Ultrafast electron diffraction
Ultrafast_electron_diffraction
NASA space observatory designed to detect X-rays and gamma rays (1991–2000)
The Compton Gamma Ray Observatory (CGRO) was a space observatory detecting photons with energies from 20 keV to 30 GeV, in Earth orbit from 1991 to 2000
Compton_Gamma_Ray_Observatory
Interpretation of quantum mechanics
Mukhopadhyay, P. (1986). "A correlation between the compton wavelength and the de Broglie wavelength". Physics Letters A. 114 (4): 179–182. Bibcode:1986PhLA
De_Broglie–Bohm_theory
Method used in mathematical physics
constant, and ℏ / m e c {\displaystyle \hbar /m_{\mathrm {e} }c} is the Compton wavelength of the electron. Regularization: Classical physics theory breaks down
Regularization_(physics)
Mechanism of beta decay proposed in 1933
{\displaystyle \phi _{\sigma }} are constant within the nucleus (i.e., their Compton wavelength is much larger than the size of the nucleus). This leads to H ρ =
Fermi's_interaction
Complex four-component spinor
{\textstyle {\frac {mc}{\hbar }}} (which is called the inverse reduced Compton wavelength) in ordinary units. The Dirac equation has the form ( − i α ⋅ ∇ +
Plane-wave solutions to the Dirac equation
Plane-wave_solutions_to_the_Dirac_equation
Elementary particle involved with rest mass
their masses have since been confirmed by measurement. (See also: Compton wavelength and static forces and virtual-particle exchange) By the 1960s, many
Higgs_boson
Overview of and topical guide to black holes
the properties of the electron including the magnetic moment and Compton wavelength. Stellar black hole – black hole formed by the gravitational collapse
Outline_of_black_holes
Gravitational-wave event
Compton wavelength is at least 1.6×1016 m, or about 1.6 light-years, corresponding to a graviton mass of no more than 7.7×10−23 eV/c2. This Compton wavelength
GW170104
Series of NASA satellites
Energy Solar Spectroscopic Imager (RHESSI), observed in some Compton and Chandra wavelengths between its February 2002 launch and April 2023 decommissioning
Great_Observatories_program
Form of electromagnetic radiation
radiation with a wavelength shorter than those of ultraviolet rays and longer than those of gamma rays. Roughly, X-rays have a wavelength ranging from 10 nanometers
X-ray
Physical property of allowing light
macroscopic scale (one in which the dimensions are much larger than the wavelengths of the photons in question), the photons can be said to follow Snell's
Transparency_and_translucency
derivation of the Compton frequency f for a stationary massive particle, equal to mc2/h. De Broglie also proposed that the wavelength λ for a moving particle
Matter_wave_clock
Force on an electromagnet when its magnetic moment changes
no longer be trusted at distances of the order of (or below) the Compton wavelength…Only when all distances involved are in the classical domain is classical
Magnetic radiation reaction force
Magnetic_radiation_reaction_force
Hypothesis that inertial and gravitational masses are equivalent
principle because they contain many light scalar fields with long Compton wavelengths, which should generate fifth forces and variation of the fundamental
Equivalence_principle
Physical model of propagating energy
a broad spectrum, classified by frequency (inversely proportional to wavelength), ranging from radio waves, microwaves, infrared, visible light, ultraviolet
Electromagnetic_radiation
Penetrating form of electromagnetic radiation
Andrade measured the wavelengths of gamma rays from radium, and found they were similar to X-rays, but with shorter wavelengths and thus, higher frequency
Gamma_ray
Background galaxy containing a quasar
direct collapse of gas clouds. Due to the agreement between the multi-wavelength properties of UHZ1 and the theoretical model template predictions, some
UHZ1
Lunar hotspot
The Compton–Belkovich Thorium Anomaly is a volcanic complex on the far side of the Moon. It was found by a gamma-ray spectrometer in 1998 and is an area
Compton–Belkovich Thorium Anomaly
Compton–Belkovich_Thorium_Anomaly
Elastic interaction of x-rays with electrons
the wavelength was much larger than the spacing between the resonators. Von Laue realized that electromagnetic radiation of a shorter wavelength was needed
X-ray_diffraction
Massive fermion wave equation in Kerr spacetime
particle's rest mass (measured in units so that it is the inverse of the Compton wavelength), and L n = d d θ + ( m csc θ − a ω sin θ ) + n cot θ , {\displaystyle
Chandrasekhar–Page_equations
Particle collisions conserving kinetic energy
low-energy limit of Compton scattering). In Rayleigh scattering a medium composed of particles whose sizes are much smaller than the wavelength scatters light
Elastic_scattering
Compression (physical) Compression lift Compton Gamma Ray Observatory Compton scattering Compton wavelength Compton–Getting effect Computational Materials
Index_of_physics_articles_(C)
Gradual loss of flux intensity through a medium
the longest wavelengths. Thus, red, orange, and yellow wavelengths are totally absorbed at shallower depths, while blue and violet wavelengths reach deeper
Attenuation
large wavelengths (or, equivalently, low frequencies), but strongly disagrees at short wavelengths (or high frequencies). In fact, at short wavelengths, classical
History_of_quantum_mechanics
Property of light sources related to black-body radiation
lower ("warmer") color temperature due to increased scattering of shorter-wavelength sunlight by atmospheric particulates – an optical phenomenon called the
Color_temperature
Range of physical processes in physics
scattering (small particle compared to wavelength of light); α ≈ 1: Mie scattering (particle about the same size as wavelength of light, valid only for spheres);
Scattering
Earth scientist and academic
Compton Tucker is an Earth scientist and academic. He is a Senior Earth Scientist in the Laboratory for Hydrospheric and Biospheric Sciences at NASA Goddard
Compton_Tucker
Light or sound absorption in a substance
coefficient in frequency and spectral hemispherical attenuation coefficient in wavelength of a volume, denoted μν and μλ respectively, are defined as: μ ν = − 1
Attenuation_coefficient
Material which glows when excited by ionizing radiation
phosphorescence. The correspondence depends on the type of transition and hence the wavelength of the emitted optical photon. A scintillation detector or scintillation
Scintillator
English musician and songwriter (1944–2024)
lineup as the lead guitarist and a vocalist in March 1978, to record the Wavelength album. Tench was recommended to Morrison by drummer Peter Van Hooke, after
Bobby_Tench
Particle accelerator designed to produce intense x-ray beams
the only viable luminous source of wide-band radiation in far infrared wavelength range for some applications, such as far-infrared absorption spectrometry
Synchrotron_light_source
Branch of physics that studies light
increasing wavelength, which is seen in most transparent materials. This is called "normal dispersion". It occurs in all dielectric materials, in wavelength ranges
Optics
Property of materials
μ/ρi are functions of wavelength. If there are N solutes or solvents, this procedure requires at least N measured wavelengths to create a solvable system
Mass_attenuation_coefficient
Light passing through successive filters
through microscopic "stacks" of partially absorbing media, allowing some wavelengths of light to reach the eye and not others. It is also a concept seen in
Subtractive_color
Harmful high-frequency radiation
excitation. At 38 nanometers wavelength for electromagnetic radiation, 33 eV is close to the energy at the conventional 10 nm wavelength transition between extreme
Ionizing_radiation
Branch of biology that studies cells
to label a specific component of the cell. Afterwards, a certain light wavelength is used to excite the fluorescent marker which can then be visualized
Cell_biology
Centineo, Becky Ann Baker, Avan Jogia She Dances EKKL Entertainment / Wavelength Rick Gomez (director/screenplay); Steve Zahn (screenplay); Steve Zahn
List of American films of 2026
List_of_American_films_of_2026
NASA/ESA space telescope launched in 1990
an accuracy of 10 nanometers, or about 1/65 of the wavelength of red light. On the long wavelength end, the OTA was not designed with optimum infrared
Hubble_Space_Telescope
Instrument that makes distant objects appear magnified
ground-based telescopes as these have to be observed from orbit. Even if a wavelength is observable from the ground, it might still be advantageous to place
Telescope
Study involving matter and electromagnetic radiation
radiation and the matter that shifts the wavelength of the scattered radiation. These include Raman and Compton scattering. Coherent or resonance spectroscopy
Spectroscopy
Emission of electrons when electromagnetic radiation hits a material
requires a few electron-volt (eV) light quanta, corresponding to short-wavelength visible or ultraviolet light. In extreme cases, emissions are induced
Photoelectric_effect
NASA satellite of the Explorer program
study of gamma-ray bursts, Swift now functions as a general-purpose multi-wavelength observatory, particularly for the rapid follow-up and characterization
Neil Gehrels Swift Observatory
Neil_Gehrels_Swift_Observatory
Subfield of astronomy
laboratory research closely allied to astronomical physics, including wavelength determinations of metallic and gaseous spectra and experiments on radiation
Astrophysics
Elementary particle or quantum of light
can be written with angular frequency ( ω {\displaystyle \omega } ) or wavelength (λ): E = ℏ ω = h c λ {\displaystyle E=\hbar \,\omega ={\frac {\,h\,c\
Photon
Reflection which reverses the direction of a wave, particle, or signal
experiments (neutron backscattering, X-ray backscattering spectroscopy); Compton scattering, used in Backscatter X-ray imaging. Stimulated backscatter,
Backscatter
Technique to characterize materials using X-ray radiation
previously gained by excitation is emitted as a photon of one of the wavelengths uniquely characteristic of the element. Analysis of the X-ray emission
X-ray_spectroscopy
Scientific study of celestial objects
shortest wavelengths (highest energy) of the electromagnetic spectrum. Gamma rays may be observed directly by satellites such as the Compton Gamma Ray
Astronomy
Galaxy in the constellation Perseus
18 September 1828. In 2016, astronomers confirmed NGC 1106 contains a Compton-thick active galactic nucleus, after extensive analysis of the galaxy's
NGC_1106
Mmeasures the probability of an absorption process
section is the ability of a molecule to absorb a photon of a particular wavelength and polarization. Analogously, in the context of nuclear engineering,
Absorption_cross_section
COMPTON WAVELENGTH
COMPTON WAVELENGTH
Surname or Lastname
English (of Norman origin) and French
English (of Norman origin) and French : status name for a professional champion (see Champion, Kemp), from the Norman French form campion.
Surname or Lastname
English
English : habitational name from any of the numerous places throughout England (but especially in the south) named Compton, from Old English cumb ‘short, straight valley’ + tūn ‘enclosure’, ‘settlement’.
Surname or Lastname
English
English : variant of Crumpton.
Surname or Lastname
English
English : habitational name from places in Hertfordshire and Hampshire, both named from the Old English personal name C̄ma + Old English tūn ‘settlement’.English : variant of Kempton.
Boy/Male
American, British, English
From the Winding Farm
Surname or Lastname
English
English : see Cumpston.
Surname or Lastname
English
English : from a Middle English personal name, Colstan, which is probably from Old Norse Kolsteinn, composed of the elements kol ‘charcoal’ + steinn ‘stone’.English : habitational name from Colston Basset in Nottinghamshire, or the nearby Car Colston, both of which seem to have originally been named from the Old Norse personal name Kolr + Old English tūn ‘settlement’. The first syllable of Car Colson was originally the defining prefix kirk ‘church’.English : habitational name from Coulston in Wiltshire, which is named with the genitive case of an Old English personal name Cufel (diminutive of Cufa) + Old English tūn ‘enclosure’, ‘settlement’.
Surname or Lastname
English and Scottish
English and Scottish : habitational name from any of the numerous places called Hampton, including the cities of Southampton and Northampton (both of which were originally simply Hamtun). These all share the final Old English element tÅ«n ‘enclosure’, ‘settlement’, but the first is variously hÄm ‘homestead’, hamm ‘water meadow’, or hÄ“an, weak dative case (originally used after a preposition and article) of hÄ“ah ‘high’. This name is also established in Ireland, having first been taken there in the medieval period.The descendants of the clergyman Thomas Hampton, resident at Jamestown, VA, in 1630, lived in VA through three generations, multiplying their homesteads as the colony expanded and then branched into SC.
Surname or Lastname
English
English : variant of Compton.
Surname or Lastname
English
English : habitational name from Campton in Bedfordshire, named in Old English as ‘settlement (Old English tūn) by the Camel river’ (a lost river-name of Celtic origin).
Surname or Lastname
English
English : habitational name from either of two places named Rampton, in Cambridgeshire and Nottinghamshire; the first, and probably also the second, is named Old English ramm ‘ram’ + tūn ‘settlement’. However, the modern surname is concentrated in Hampshire, suggesting perhaps that another, unidentified source could be involved.
Surname or Lastname
English
English : habitational name from a place called Kempton in Shropshire, named from an Old English personal name Cempa (or the Old English vocabulary word cempa ‘warrior’) + tūn ‘farmstead’, ‘settlement’.English : variant of Kimpton.
Surname or Lastname
English
English : habitational name from any of various places, for example in Essex, Suffolk, and Warwickshire, named Clopton from Old English clopp(a) ‘rock’, ‘hill’ + tūn ‘settlement’.
Surname or Lastname
English and Scottish
English and Scottish : habitational name from any of various places called Colton in England, perhaps also Colton House in Scotland. Examples in Norfolk, Staffordshire, and North Yorkshire are from the Old English personal name Cola (or the cognate Old Norse Koli; see Cole 2) + Old English tūn ‘enclosure’, ‘settlement’. The place so named in Somerset has as its first element the Old English personal name Cūla (of uncertain origin). The one in Cumbria has a river name apparently derived from a Celtic word meaning ‘hazel’.
Surname or Lastname
English (Lancashire)
English (Lancashire) : habitational name from a place in North Yorkshire named Coulton, probably from Old English col ‘(char)coal’ + tūn ‘enclosure’, ‘settlement’.
Surname or Lastname
English
English : variant of Crumpton.
Surname or Lastname
English
English : habitational name from any of numerous places named from Old English cotum (dative plural of cot) ‘at the cottages or huts’ (or sometimes possibly from a Middle English plural, coten). Examples include Coton (Cambridgeshire, Northamptonshire, Staffordshire), Cottam (East Yorkshire, Lancashire, Nottinghamshire), and Cotham (Nottinghamshire).French : from a diminutive of Old French cot(t)e ‘coat (of mail)’ (see Cott).John Cotton (1584–1652) was a noted Puritan preacher, who landed at Boston, MA, from London in 1633 and became leader of the Congregationalists in America.
Surname or Lastname
English
English : habitational name from Crompton in Lancashire, named with an Old English crumbe ‘river bend’ + tūn ‘enclosure’, ‘settlement’.
Surname or Lastname
English
English : habitational name from Lampton in Greater London (formerly Middlesex) or Lambton in County Durham, named in Old English as ‘farm or settlement where lambs were reared’, from lamb ‘lamb’ + tūn ‘farmstead’, ‘settlement’.
Surname or Lastname
English
English : patronymic from Tom, a short form of the personal name Thomas.
COMPTON WAVELENGTH
COMPTON WAVELENGTH
Boy/Male
Hindu, Indian, Kannada, Marathi, Telugu
Fierce; Strong
Girl/Female
Australian, French, German, Italian, Latin, Portuguese
From Germany
Girl/Female
Indian, Telugu
Earth; Beautiful
Girl/Female
Hindu, Indian
Nakul's Wife
Girl/Female
Indian, Sanskrit
Lord Krishna
Boy/Male
English
Black-haired.
Boy/Male
Hindu
God of victory
Girl/Female
Arabic, Muslim
A Deponent; One who Bears Witness
Girl/Female
Arabic, Muslim
The Moon of the World
Boy/Male
Egyptian
Humble.
COMPTON WAVELENGTH
COMPTON WAVELENGTH
COMPTON WAVELENGTH
COMPTON WAVELENGTH
COMPTON WAVELENGTH
v. i.
To have a joint right with others in common ground.
n.
The right of taking a profit in the land of another, in common either with the owner or with other persons; -- so called from the community of interest which arises between the claimant of the right and the owner of the soil, or between the claimants and other commoners entitled to the same right.
n.
See Pumpion.
n.
The cotton plant. See Cotten plant, below.
n.
A soft, downy substance, resembling fine wool, consisting of the unicellular twisted hairs which grow on the seeds of the cotton plant. Long-staple cotton has a fiber sometimes almost two inches long; short-staple, from two thirds of an inch to an inch and a half.
a.
See Compony.
v. i.
To board together; to eat at a table in common.
n.
Cloth made of cotton.
n.
A preparation of fruit in sirup in such a manner as to preserve its form, either whole, halved, or quartered; as, a compote of pears.
n.
A plug in a flute or an organ pipe, to modulate the tone.
a.
See Compony.
n.
A stopper of a cannon or a musket. See Tampion.
v.
Belonging or relating equally, or similarly, to more than one; as, you and I have a common interest in the property.
v. i.
To take a liking to; to stick to one as cotton; -- used with to.
n.
The iron bottom to which grapeshot are fixed.
a.
Divided into squares of alternate tinctures in a single row; -- said of any bearing; or, in the case of a bearing having curved lines, divided into patches of alternate colors following the curve. If there are two rows it is called counter-compony.
a.
Alt. of Compone
v.
Belonging to or shared by, affecting or serving, all the members of a class, considered together; general; public; as, properties common to all plants; the common schools; the Book of Common Prayer.