OpenStax Chapter 6 Key Term Flashcards

1
Q

wave

A

oscillation or periodic movement that can transport energy from one point in space to another

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2
Q

wavelength

A

distance from peak to peak or trough to trough

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3
Q

frequency

A

the number of wave cycles (one complete wavelength) that can pass a given point in space in a given amount of time s^-1

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4
Q

amplitude

A

maximum displacement from equilibrium

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5
Q

hertz

A

unit for frequency

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6
Q

electromagnetic spectrum

A

energy and frequency have a direct relationship
frequency and wavelength have a indirect relationship

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7
Q

standing waves

A

constrained within a region in space
play important role in understanding electronic structure of atoms
have an integer number, n, of half wavelengths between endpoints

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8
Q

quantization

A

only discrete values for a more general set of continuous values of some properties are observed

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9
Q

nodes

A

points between the two end points that are not in motion
n-1 nodes, where n is the number of half wavelengths
energy increases with the amount of nodes

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10
Q

blackbody radiation

A

sunlight consists of a range of broadly distributed wavelengths that form a continuous spectrum
blackbody - convenient, ideal emitter that approximates the behavior of many materials when heated

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11
Q

ultraviolet catastrophe

A

classical prediction that the intensity of the radiation radiated by a blackbody would increase as the wavelength decreased

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12
Q

photoelectric effect

A

electrons can be emitted from surface of metal when it is hit with light that has a frequency greater than the threshold
the kinetic energy of the emitted electron depends on the frequency of the light
even at lower intensity, light of the appropriate frequency can eject an electron

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13
Q

photoelectric effect (conc.)

A

light consists of radiation or quanta or packets of EM radiation with energy proportional to frequency of light
the greater the frequency of the photon, the greater the KE of the emitted electron
light has wave and particle nature

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14
Q

photon

A

particle of light

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15
Q

wave-particle duality

A

light has wave and particle behavior

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16
Q

line spectrum

A

heated solid, liquids, and condensed gases emit light of a range of frequencies to produce a continuous spectrum
heated gases emit light at discrete wavelengths; each emission line consists of a single wavelength

17
Q

Balmer

A

derived an equation that related the four visible lines in the hydrogen emission spectrum to whole numbers
n_f = 2

18
Q

Rydberg

A

developed an equation to reproduce all of the lines in the hydrogen spectrum

19
Q

Bohr’s model of the atom

A

assumed that electrons would not emit or absorb energy unless it moved from one level to another
energy emitted or absorbed would reflect the energy difference between levels
quantization of energy
rearranges the Rydberg equation/derived an equation for the energy of an electron in hydrogen-like atoms and ions

20
Q

ground state of the electron

A

lowest energy state of the electron

21
Q

excited state of the electron

A

higher energy states of the electrons

22
Q

deBroglie wavelength

A

extended the wave particle duality of light to material particles
wavelength = h/p
Bohr’s idea only applies if electrons are considered circular standing waves
2pir=nlambda

23
Q

Davisson and Germer

A

electrons can behave as waves

24
Q

Heisenberg Uncertainty Principle

A

it is impossible to determine simultaneously and exactly the momentum and the position of a particle

25
Q

Schrodinger

A

described electrons as wavefunctions
three-dimensional stationary waves
reproduced Bohr’s expression for energy and the Rydberg formula

26
Q

Max Born

A

electrons are still particles
waves are not physical waves but complex probability molecules
the square of the magnitude of a wavefunction describes the probability of a particle being near a location in space
wavefunctions can be used to determine the distribution of electron density with respect to the nucleus

27
Q

principal quantum number

A

the quantum number on which the energy of the electron principally depends on
determines the size of the shell and the distance from the nucleus

28
Q

angular momentum quantum number

A

specifies the subshell and the shape of the orbital
0 = s
1 = p
2 = d
3 = f

29
Q

magnetic quantum number

A

specifies the orbital’s orientation in space
adopts values: -l…0…+l

30
Q

spin quantum number

A

specifies the spin of the electron
ms = +1/2 or -1/2

31
Q

atomic radius

A

increases down a group (more energy levels)
decreases across a period (valence electrons being added to the same energy level while proton number increases makes nucleus pull electrons closer)

32
Q

ionization energy

A

energy that is required to remove an electron from an atom
decreases down a group (added energy levels makes electrons easier to remove since there is more shielding)
increases across a period (nucleus pulling electrons closer together makes it harder to remove them)

33
Q

electron affinity

A

energy change associated with added an electron to a gaseous atom
- = wants to accept an electron
+ = does not want to accept an electron

34
Q

B and O exceptions to IE

A

B: 2s subshell has a higher effective nuclear charge since there is a possibility of the electrons being found near the nucleus, so the 2p1 electron is easier to remove
O: half-filled subshell has some stability associated with it, pairing energy - energetic cost associated with adding an electron to a pre-existing orbital with an electron