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70 Cards in this Set

  • Front
  • Back
electronic structure
the description of how electrons are arranged around the nucleus of an atom
classical mechanics
the laws of motion proposed by Newton in the seventeenth century
quantum mechanics
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
spectroscopy
the analysis of the electromagnetic radiation emitted or absorbed by substancesd
electromagnetic radiation
a wave of oscillating electric and magnetic fields; includes light, x-rays, and _ rays
cycles
complete reversals or direction away from and back to the initial strength and direction
frequency (of radiation)
the number of cycles per second

unit: hertz (Hz)
amplitude
the height of the wave above the center line
intensity
brightness of the radiation, determined by the square of the amplitude
wavelength
(lambda _) the peak-to-peak distance
visible light
electromagnetic radiation that can be detected by the human eye, with wavelengths ranging from 700nm to 400nm
ultraviolet radiation
radiation at higher frequency than violet light; wavelength less than 400nm
infrared radiation
radiation we experience as heat, with a lower frequency and longer wavelength than red light; wavelength greater than 800nm
incandescence
light emitted by a hot body
black body
an object that absorbs and emits all frequencies of radiation without favor
black-body radiation
the radiation emitted at different wavelengths by a heated black body
Stefan-Boltzmann law
the total intensity of radiation emitted by a heated black body is proportional to the fourth power of the absolute temperature

e
Wien's law
the wavelength corresponding to the maximum in the radiation emitted by a heated black body is inversely proportional to the absolute temperature

e
second radiation constant

(c2)
the proportionality constant in Wein's law

e
ultraviolet catastrophe
the classical prediction that any black body at any temperature should emit intense ultraviolet radiation
quanta
packets of energy
Planck's constant

(h)
A fundamental constant of nature with the value

e
photoelectric effect
the ejection of electrons from a metal when its surface is exposed to ultraviolet radiation
photons
A particle-like packet of electromagnetic radiation. the energy of a photon of frequency v is E=hv
work function
the energy required to remove an electron from metal
diffraction
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
constructive interference
interference that results in an increased amplitude of a wave
destructive interference
interference that results in a reduced amplitude of a wave
wave-particle duality
the combined wavelike and particle-like character of both radiation and matter
linear momentum
(p)

the product of mass and velocity
de Broglie relation
the proposal that every particle has wavelike properties and that its wavelength

e
trajectory
path on which location and linear momentum are specified at each instant
complementarity
the impossibility of knowing the position of a particle with arbitrarily great precision if its linear momentum is known precisely
Heisenberg uncertainty principle
e
wavefunction
e

a solution og the Schrodinger equation; the probability amplitude
Born interpretation
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
probability density (of a particle)
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
node
A point or surface on which and electron will not be found
Schrodinger equation
An equation for calculating the wavefunction of a particle, especially for an electron in an atom or molecule

e
hamiltonian
The operator H in the Schrodinger equation,

e
particle in a box
A particle confined between rigid walls
quantum number
An integer (sometimes, a half-integer) that labels a wavefunction and specifies the value of a property

Ex. principle quantum number, n.
boundary conditions
Constraints on the values of the wavefunction iof a particle
zero-point energy
The lowest possible energy of a system
transition
A change of quantum state
Bohr frequency condition
The relation between the change in energy of an atom or molecule and the frequency of radiation emitted or absorbed:

e
Balmer series
(R)

The constant in the formula for the frequencies of the lines in the spectrum of atomic hydrogen;

e
Lyman series
A series of lines in the spectrum of atomic hydrogen in which the transitions are to orbitals with n = 1
principal quantum number
(n) The quantum number that specifies the energy of an electron in a hydrogen atom and labels the shells of the atom
ground state
The state of lowest energy
ionization
Conversion into ions by the transfer of electrons
atomic orbitals
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
spherical polar coordinates
The coordinates of a point expressed in the terms of radius r, the colatitude _, and the azimuth _.

e
radial wavefunction
(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
angular wavefunction
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
Bohr radius
e

In an early model of the hydrogen atom, the radius of the lowest energy orbit; now a specific combination of fundamental constants
orbital angular momentum number
(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
subshells
All the atomic orbitals of a given shell of an atom that have the same value of the quantum number l.
s-orbitals
orbitals with l = 0
p-orbitals
orbitals with l = 1
d-orbitals
orbitals with l = 2
f-orbitals
orbitals with l = 3
orbital angular momentum
a measure of the rate at which the electron circulates round the nucleus
degenerate
having the same energy
s-orbitals
orbitals with l = 0
p-orbitals
orbitals with l = 1
d-orbitals
orbitals with l = 2
f-orbitals
orbitals with l = 3
orbital angular momentum
a measure of the rate at which the electron circulates round the nucleus
degenerate
having the same energy