Chapter 2: The Quantum-Mechanical Model of the Atom Flashcards

1
Q

Define quantum-mechanical model.

A

A model that explains the behavior of absolutely small particles such as electrons and photons.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
2
Q

Define electromagnetic radiation.

A

A form of energy embodied in oscillating, perpendicular electric and magnetic fields.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
3
Q

How can we characterize a wave?

A

By its amplitude, wavelength, and frequency

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
4
Q

Define amplitude.

A

The vertical height of a crest (or depth of a trough) of a wave; a measure of wave intensity.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
5
Q

What does amplitude determine in light?

A

The light’s intensity or brightness - the greater the amplitude, the greater the intensity.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
6
Q

Define wavelength.

A

The distance between adjacent crests of a wave (or any two analogous points).

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
7
Q

What does wavelength determine in light?

A

The light’s color

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
8
Q

Define frequency.

A

For waves, the number of cycles (or complete wavelengths) that pass through a stationary point in one second. Directly proportional to the speed at which the wave is traveling.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
9
Q

Define hertz (Hz).

A

1 cycle/s; 1/s; s^-1

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
10
Q

Formula relationship between frequency and wavelength.

A

c = λ * ν

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
11
Q

What is the speed of light (c)?

A

c = 3.00 x 10^8 m/s

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
12
Q

Visible light from longest wavelength to shortest wavelength.

A

ROYGBIV

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

Visible light from lowest frequency to highest frequency.

A

ROYGBIV

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
14
Q

Why do objects appear a certain color?

A

Objects reflect the colors in which they appear and absorb most other colors.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
15
Q

Define electromagnetic spectrum.

A

The range of the wavelengths of all possible electromagnetic radiation.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
16
Q

Electromagnetic spectrum from low energy to high energy.

A

Radio, Microwave, Infrared, Visible Light (ROYGBIV), Ultraviolent, X-ray, Gamma-ray

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
17
Q

Define interference.

A

The superposition of two or more waves overlapping in space, resulting in either an increase in amplitude (constructive interference) or a decrease in amplitude (destructive interference).

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
18
Q

Define constructive interference.

A

The interaction of waves from two sources that align with overlapping crests, resulting in a wave of greater amplitude.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
19
Q

Define destructive interference.

A

The interaction of waves from two sources that are aligned so that the crest of one overlaps the trough of the other, resulting in cancellation.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
20
Q

Define diffraction.

A

The phenomena by which a wave emerging from an aperture spreads out to form a new wave front.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
21
Q

What happens when light passes through two slits separated by a distance comparable to the wavelength of the light?

A

The diffraction of light through the slits results in an interference pattern. Each slit acts as a new wave source, and the two new waves interfere with each other. The resulting pattern is a series of bright and dark lines. At the center, the two waves travel equal distances and interfere constructively. At the point where the difference in distance is one-half on one wavelength, the interference is destructive and a dark line appears. Constructive again at one whole wavelength away.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
22
Q

Define photoelectric effect.

A

The observation that many metals emit electrons when light falls upon the metal.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
23
Q

Define binding energy.

A

Energy with which an electron is bound to the metal.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
24
Q

Define threshold frequency.

A

The frequency at which the energy of a photon exceeds the energy with which an electron is held to the metal, thus ejecting an electron from the metal.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
25
Q

What did Albert Einstein propose for the explanation of the photoelectric effect?

A

Light energy must come in packets, with the amount of energy (E) in a light packet depending on its frequency. The emission of electrons from the metal depends on whether or not a single photon has sufficient energy to dislodge a single electron. For an electron bound to the metal with binding energy Φ, the threshold frequency is reached when the energy of the photon is equal to Φ.

26
Q

Formula Energy relationship to frequency.

A

E = h * ν

27
Q

Define Planck’s constant (h).

A

h = 6.626 x 10^-34 J*s

28
Q

Define photon.

A

(quantum) The smallest possible packet of electromagnetic radiation with an energy = h*v.

29
Q

Formula Energy relationship to wavelength.

A

E = (h*c) / λ

30
Q

Formula threshold frequency.

A

h * v = Φ

31
Q

Formula kinetic energy of ejected electron.

A

KE = (h * v) - Φ

32
Q

Define wave-particle duality of light.

A

Sometimes light appears to behave like a wave, at other times like a particle. The behavior we observe depends on the particular experiment.

33
Q

Define emission spectrum.

A

The range of wavelengths emitted by a particular element; used to identify the element.

34
Q

Why does the emission spectrum of an atom consist of discrete lines?

A

Because the stationary states exist only at specific, fixed energies. The energy of the photon emitted when an electron makes a transition from one stationary state to another is the energy difference between the two stationary states.

35
Q

Relationship between stationary states and energy.

A

Transitions between stationary states that are closer together produce light of lower energy than transitions between stationary states that are farther apart.

36
Q

Define absorption spectrum.

A

A plot of the absorption of light of a sample of matter as a function of wavelength.

37
Q

Define de Broglie relation.

A

The observation that the wavelength of a particle is inversely proportional to its momentum.

38
Q

Formula de Broglie relation.

A

λ = h / (m*v)

39
Q

Define complementary properties.

A

Properties that exclude one another; that is, the more you know about one, the less you know about the other. For example, the wave nature and particle nature of the electron are complementary.

40
Q

Define Heisenberg’s uncertainty principle.

A

The principle stating that due to the wave-particle duality, it is fundamentally impossible to precisely determine both the position and velocity of a particle at a given moment in time.

41
Q

Define deterministic.

A

A characteristic of the classical laws of motion, which imply that present circumstances determine future events.

42
Q

What is a probability distribution map for an electron?

A

It is a statistical map that shows where an electron is likely to be found under a given set of conditions.

43
Q

Define indeterminacy.

A

The principle stating that present circumstances do not necessarily determine future events in the quantum-mechanical realm.

44
Q

Define orbital.

A

A probability distribution map, based on the quantum-mechanical model of the atom, used to describe the likely position of an electron in an atom; also an allowed energy state for an electron.

45
Q

Define quantum number.

A

One of the four interrelated numbers that determine the shape and energy of orbitals, as specified by the solution of the Schrodinger equation.

46
Q

Define principal quantum number (n).

A

An integer that specifies the overall size and energy of an orbital; the higher the quantum number n, the greater the average distance between the electron and the nucleus and the higher its energy. (n = 1, 2, 3, …)

47
Q

Define angular momentum quantum number (l).

A

An integer that determines the shape of an orbital. (l = 0, 1, …, n-1)

48
Q

Define magnetic quantum number (m>l).

A

An integer that specifies the orientation of an orbital. (m>l = -l, …, 0, …, +l)

49
Q

What is the letter designation of an orbital according to l?

A

l=0 : s
l=1 : p
l=2 : d
l=3 : f
l=4 : g
l=5 : h

50
Q

Define spin quantum number (m>s).

A

Specifies the orientation of the spin of the electron. (m>s = -1/2, +1/2)

51
Q

Define electron spin.

A

A fundamental property of electrons; spin can have a value of +1/2 or -1/2.

52
Q

Value of spin up?

A

+1/2

53
Q

Value of spin down?

A

-1/2

54
Q

Define principal level (shell).

A

The group of orbitals with the same value of n.

55
Q

Define sublevel (subshell).

A

Those orbitals in the same principle level with the same value of n and l.

56
Q

Formula number of orbitals in any sublevel.

A

2l + 1

57
Q

Formula number of orbitals in a level.

A

n^2

58
Q

Shape of s orbital (l=0).

A

Spherical, nodes within the sphere at which the probability is 0

59
Q

Shape of p orbital (l=1).

A

Dumbbell, node located at the nucleus. The three p orbitals differ only in their orientation and are orthogonal to each other.

60
Q

Shape of d orbitals (l=2).

A

Four have a clover leaf, one has a dumbbell with a donut around the center.