Book: Ch. 7 Flashcards

1
Q

Define: electromagnetic radiation

A

Visible light, x-rays, radio waves, and microwaves are examples. Basically photons.

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2
Q

Define: frequency (ν)

A

Number of complete waves or cycles that pass a given point per second, usually expressed by the unit s⁻¹ or hertz (Hz)

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3
Q

Define: wavelength (λ)

A

Distance between any point on a wave and the corresponding point on the next crest or trough of the wave. The distance the wave travels during one cycle. Usually measured in nm.

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4
Q

Define: speed of light (c)

A

c = νλ = 3.00×10⁸ m/s

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5
Q

Define: amplitude

A

Height of the crest. For electromagnetic waves, this corresponds to the intensity of the radiation.

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6
Q

Define: electromagnetic spectrum

A

The types of electromagnetic radiation arranged in order of increasing wavelength.

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7
Q

Define: ultraviolet radiation (UV)

A

Spectrum of electromagnetic radiation to the left of visible light on the spectrum.

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8
Q

Define: infrared radiation (IR)

A

Spectrum of electromagnetic radiation to the right of visible light on the spectrum.

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9
Q

Define: refraction

A

When a wave passes from one medium to another, it refracts: it changes direction and the wave continues at a different angle.

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10
Q

Define: diffraction

A

When a wave strikes the edge of an object, it bends around it. This is diffraction.

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11
Q

What is the equation for the energy of a photon?

A

E = nhν, where n is a quantum number taking values of positive integers, and h is Planck’s constant.

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12
Q

Define: Planck’s constant

A

h = 6.626×10⁻³⁴ [J s]

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13
Q

What is the relationship between the change in energy of a photon and the properties of light is emits?

A

∆E atom = E emitted radiation = hν = hc/λ

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14
Q

Define: photoelectric effect

A

A phenomenon explained by Einstein with the introduction of the photon theory of light.

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15
Q

Define: photon

A

A single particle of light.

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16
Q

What is the energy of a photon?

A

E photon = hv = ∆E atom

17
Q

What is the Rydberg equation?

A

1/λ = R(1/n₁² - 1/n₂²)

18
Q

Define: stationary states

A

The H atom has only certain energy levels. Bohr called these the stationary states.

19
Q

How is the energy level between two different states of the H atom found?

A

∆E = -2.18×10⁻¹⁸ (1/n_f² - 1/n_i²)

20
Q

Define: de Broglie wavelength

A

Equation λ = h/mu, where u is speed of the object. Basically gives the wavelength of an object, under the assumption that matter behaves like a wave.

21
Q

Define: uncertainty principle

A

It is impossible to know simultaneously the position and momentum of a particle, so m∆x∆u ≥ h/4π

22
Q

Define: principal quantum number (n)

A

A positive integer giving the relative size of the orbital an electron has as well as its energy level.

23
Q

Define: angular momentum quantum number (l)

A

An integer from 0 to n - 1. n sets the limit on what values l can take. l is related to the shape of the orbital.

24
Q

Define: magnetic quantum number (m_l)

A

An integer from -l through 0 to l. Number of m_l values = 2l+1 = number of orbitals for a given l. Prescribes three-dimensional orientation of the orbital in the space around the nucleus.

25
Q

Define: levels and sublevels for atoms

A

Level: aka shells of an atom. Given by n value.
Sublevels: subshells. Given by the l value. l = 0 is s sublevel, 1 is p, 2 is d, 3 is f.