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70 Cards in this Set
- Front
- Back
electronic structure
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the description of how electrons are arranged around the nucleus of an atom
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classical mechanics
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the laws of motion proposed by Newton in the seventeenth century
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quantum mechanics
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the description of matter that takes into account the wave-particle duality of mater and the fact that the energy of an object may be changed only in discrete steps
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spectroscopy
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the analysis of the electromagnetic radiation emitted or absorbed by substancesd
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electromagnetic radiation
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a wave of oscillating electric and magnetic fields; includes light, x-rays, and _ rays
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cycles
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complete reversals or direction away from and back to the initial strength and direction
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frequency (of radiation)
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the number of cycles per second
unit: hertz (Hz) |
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amplitude
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the height of the wave above the center line
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intensity
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brightness of the radiation, determined by the square of the amplitude
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wavelength
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(lambda _) the peak-to-peak distance
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visible light
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electromagnetic radiation that can be detected by the human eye, with wavelengths ranging from 700nm to 400nm
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ultraviolet radiation
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radiation at higher frequency than violet light; wavelength less than 400nm
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infrared radiation
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radiation we experience as heat, with a lower frequency and longer wavelength than red light; wavelength greater than 800nm
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incandescence
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light emitted by a hot body
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black body
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an object that absorbs and emits all frequencies of radiation without favor
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black-body radiation
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the radiation emitted at different wavelengths by a heated black body
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Stefan-Boltzmann law
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the total intensity of radiation emitted by a heated black body is proportional to the fourth power of the absolute temperature
e |
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Wien's law
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the wavelength corresponding to the maximum in the radiation emitted by a heated black body is inversely proportional to the absolute temperature
e |
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second radiation constant
(c2) |
the proportionality constant in Wein's law
e |
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ultraviolet catastrophe
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the classical prediction that any black body at any temperature should emit intense ultraviolet radiation
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quanta
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packets of energy
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Planck's constant
(h) |
A fundamental constant of nature with the value
e |
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photoelectric effect
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the ejection of electrons from a metal when its surface is exposed to ultraviolet radiation
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photons
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A particle-like packet of electromagnetic radiation. the energy of a photon of frequency v is E=hv
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work function
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the energy required to remove an electron from metal
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diffraction
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the pattern of high and low intensities generated by an object in the path of a ray of light
the deflection of waves and the resulting interference caused by an object in their path |
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constructive interference
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interference that results in an increased amplitude of a wave
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destructive interference
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interference that results in a reduced amplitude of a wave
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wave-particle duality
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the combined wavelike and particle-like character of both radiation and matter
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linear momentum
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(p)
the product of mass and velocity |
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de Broglie relation
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the proposal that every particle has wavelike properties and that its wavelength
e |
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trajectory
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path on which location and linear momentum are specified at each instant
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complementarity
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the impossibility of knowing the position of a particle with arbitrarily great precision if its linear momentum is known precisely
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Heisenberg uncertainty principle
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e
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wavefunction
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e
a solution og the Schrodinger equation; the probability amplitude |
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Born interpretation
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e
the interpretation of the square of the wavefunction, _, of a particle as the probability density for finding the particle in a region of space |
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probability density (of a particle)
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A function that, when multiplied by the volume of the region, gives the probability that the particle will be found in that region of space
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node
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A point or surface on which and electron will not be found
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Schrodinger equation
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An equation for calculating the wavefunction of a particle, especially for an electron in an atom or molecule
e |
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hamiltonian
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The operator H in the Schrodinger equation,
e |
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particle in a box
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A particle confined between rigid walls
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quantum number
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An integer (sometimes, a half-integer) that labels a wavefunction and specifies the value of a property
Ex. principle quantum number, n. |
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boundary conditions
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Constraints on the values of the wavefunction iof a particle
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zero-point energy
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The lowest possible energy of a system
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transition
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A change of quantum state
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Bohr frequency condition
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The relation between the change in energy of an atom or molecule and the frequency of radiation emitted or absorbed:
e |
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Balmer series
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(R)
The constant in the formula for the frequencies of the lines in the spectrum of atomic hydrogen; e |
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Lyman series
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A series of lines in the spectrum of atomic hydrogen in which the transitions are to orbitals with n = 1
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principal quantum number
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(n) The quantum number that specifies the energy of an electron in a hydrogen atom and labels the shells of the atom
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ground state
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The state of lowest energy
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ionization
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Conversion into ions by the transfer of electrons
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atomic orbitals
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A region of space in which there is a high probability of finding and electron in an atom. And s-orbital is a spherical region; a p-orbital has two lobes, on opposite dsides of the nucleus; a d-orbital typically has four lobes, with the nucleus at its center; and f-orbital has a more complicated arrangement of lobes
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spherical polar coordinates
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The coordinates of a point expressed in the terms of radius r, the colatitude _, and the azimuth _.
e |
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radial wavefunction
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(R(r))
The radial part of a wavefunction, particularly the radial component of the wavefunctions of the hydrogen atom; the probability amplitude of and electron as a function of distance from the nucleus |
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angular wavefunction
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ee
The angular part of a wavefunction, particularly the angular component of the wavefunctions of the hydrogen atom; the probability amplitude of an electron as a function of orientation around the nucleus |
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Bohr radius
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e
In an early model of the hydrogen atom, the radius of the lowest energy orbit; now a specific combination of fundamental constants |
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orbital angular momentum number
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(l)
The quantum number that specifies the subshell of a given shell in an atom and determines the shapes of the orbitals in the subshell; l = 0,1,2,...,n-1 |
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subshells
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All the atomic orbitals of a given shell of an atom that have the same value of the quantum number l.
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s-orbitals
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orbitals with l = 0
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p-orbitals
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orbitals with l = 1
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d-orbitals
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orbitals with l = 2
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f-orbitals
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orbitals with l = 3
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orbital angular momentum
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a measure of the rate at which the electron circulates round the nucleus
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degenerate
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having the same energy
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s-orbitals
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orbitals with l = 0
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p-orbitals
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orbitals with l = 1
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d-orbitals
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orbitals with l = 2
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f-orbitals
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orbitals with l = 3
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orbital angular momentum
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a measure of the rate at which the electron circulates round the nucleus
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degenerate
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having the same energy
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