Chapter 7 - Quantum Theory and Atomic Structure Flashcards

(21 cards)

1
Q

Speed of light (c)

A

3.00 x 108 m/s

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2
Q

Frequency (v)

A

Number of complete waves or cycles that pass a given point per second expressed as a Hertz; cycles/second

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3
Q

Wavelength (λ)

A

Distance a wave travels in 1 cycle

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4
Q

Visible light spectrum

A

400 (violet) - 750 nm (red) wavelength range

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5
Q

Electromagnetic spectrum

A

Wavelength and frequency have an inversely proportional relationship: the longer the wavelength, the lower the frequency, the shorter the wavelength, the higher the frequency; in increasing wavelength order:

gamma < x-ray < ultraviolet < visible light < infrared < microwave < radio waves

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6
Q

Planck’s constant (h)

A

h = 6.626 x 10-34 J*s

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7
Q

Refraction

A

A phenomenon in which a wave changes its speed and therefore its direction as it passes through a phase boundary into a different medium; waves refract, particles do not refract

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8
Q

Dispersion

A

A type of refraction where white light disperses into its component colors when it passes through a prism (or any refracting object) because each incoming wave is refracted at a slightly different angle

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9
Q

Diffraction

A

The phenomenon in which a wave striking the edge of an object bends around it; a wave passing through a slit as wide as its wavelength forms a circular wave; only works with waves

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10
Q

Destructive interference

A

When waves of light pass through 2 adjacent slits, the nearby circular waves interact through the process of interference; the crests coincide with troughs and the amplitudes cancel to form a darker region

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11
Q

Constructive interference

A

When waves of light pass through 2 adjacent slits, the nearby circular waves interact through the process of interference; crests of the waves coincide in phase and the amplitudes add together to form a brighter region

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12
Q

Blackbody radiation

A

Solid object emits visible light when it is heated to about 1000K; changes in intensity and wavelength of emitted light as an object is heated is characteristic of blackbody radiation; ie. at a temperature of about 2000K, an object emits bright white light

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13
Q

Quantum theory

A

Since the hot objects emits only certain quantities of energy, and the energy must be emitted by the object’s atoms, each atom emits only certain quantities of energy; the energy of the an atom is quantized: it occurs in fixed quantities rather than being continuous

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14
Q

Quantum of energy equation

A
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15
Q

Photoelectric effect

A

Explains the flow of current when light strikes a metal; for a current to flow, the light shining on the metal must have a minimum frequency and different metals have different minimum frequencies; current flows the moment light of the minimum frequency shines on the metal, regardless of the light’s intensity

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16
Q

Photon theory

A

He proposed that light itself is particulate, quantized into tiny “bundles” of energy called photons; each atom changes its energy by an amount of (delta)E when it absorbs or emits one photon, one “particle” of light, whose energy is related to its frequency and not its amplitude (or intensity)

17
Q

Line spectrum

A

When light from electrically excited gaseous atoms passed through a slit and is refracted by a prism, it creates a line spectrum: a series of fine lines at specific wavelengths (specific frequencies) separated by black spaces; not a continuum of the entire spectrum

18
Q

Rydberg equation

A

n = arbitrary whole integer, R = Rydberg constant

R = 1.0967 x 107 m-1

19
Q

Bohr model of the Hydrogen atom

A

The H atom has only certain energy levels, which Bohr called stationary states (one circular orbit); the atom changes to another stationary state (electron moves to another orbit) only by absorbing or emitting a photon; the H atom absorbs a photon when an electron moves to an outer (higher energy) orbit; the H atom emits a photon when an electron moves to a lower energy orbit (closer to the nucleus)

20
Q

de Broglie wavelength

A

Matter behaves as though it moves in a wave; an object’s wavelength is inversely proportional to its mass so heavy objects such as planets and baseballs have wavelengths many orders of magnitude smaller than the object themselves, too small to be detected

h = Planck’s constant, u = speed of object, m = mass of object

21
Q

Heisenberg’s uncertainty principle

A

Werner Heisenberg postulated that it is impossible to know simultaneously the position and momentum (mass x speed) of a particle

(delta) x = uncertainty in position, (delta) u = uncertainty in speed