Chemistry Final Exam Flashcards

1
Q

What are examples of electromagnetic radiation

A

Visible light, x- rays, radio waves, & microwaves

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2
Q

What are the properties of the wave nature of light?

A
  1. Frequency (v)
  2. Wavelength (lambda)
  3. Speed ( meters)
  4. Amplitude ( height of the crest of a wave)
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3
Q

electromagnetic spectrum:

A

a continuum of wavelengths of radiant energy

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4
Q

From lowest to highest frequency, what order are the different areas of the electromagnetic spectrum

A

Gamma ray, X-ray, Ultraviolet, Visible light, infrared, Microwave, Radio waves

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5
Q

Refraction definition

A

The phenomenon in which a wave changes its speed and therefore its direction as it passes through a phase boundary to a different medium

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6
Q

`Dispersion definition

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

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7
Q

Interference definition:

A

Constructive and destructive; constructive: amplitudes add together to form a brighter region, destructive: amplitudes cancel to form a darker region`

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8
Q

Blackbody radiation

A

When a solid is heated to about 1000K, it begins to emit visible light

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9
Q

Particle nature of light

A
  1. Blackbody radiation

2. quantum theory E= nhv

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10
Q

Planck’s constant:

A

6.626 x 10^-34 (J)(s)

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11
Q

Quantum

A

A packet of energy equal to hv. The smallest quantity of energy that can be emitted or absorbed

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12
Q

Photoelectric effect and the Photon theory of light

A

When monochromatic light of sufficient frequency shines on a metal plate, a current is produced

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13
Q

Threshold frequency

A

For current to flow, the light shining on the metal must have a minimum or threshold frequency

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14
Q

Absence of time lag:

A

Current flows the moment light of the minimum frequency shines on the metal regardless of the light’s intensity

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15
Q

Photon theory

A

Ephoton = hv = deltaEatom

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16
Q

Line spectrum definition

A

a series of fine lines at specific frequencies separated by black spaces

17
Q

Rydberg equation

A

1/lambda = R((1/n1^2)-(1/n2^2)

18
Q

Postulates of the Bohr model

A
  1. The H atom has only certain energy levels which Bohr called stationary states. Each state is associated with a fixed circular orbit around the nucleus. The higher the energy level, the farther it is from the nucleus
  2. The atom does NOT radiate energy while in one of its stationary states
  3. The atom changes to another stationary state (the electron moves to another orbit) only by emitting or absorbing a photon. The energy of the photon equals the energy of the two states
19
Q

Features of the Bohr’s model

A
  1. Quantum numbers and electron orbit (n is a positive integer)
  2. Ground state
  3. Excited States
  4. Absorption
  5. Emission
20
Q

Ground State definition

A

When the electron is in the 1st orbit (n=1), it is closest to the nucleus and the H atom is in its lowest energy level

21
Q

Excited states definition

A

Any other orbit than the ground state

22
Q

Absorption

A

If an atom absorbs a photon whose energy equals the difference between lower and higher energy levels, the electron moves to a higher energy orbit

23
Q

Emission definition

A

If an H atom in a higher energy level (electron in a farther orbit) returns to a lower energy level (electron in a closer orbit), the atom emits a photon whose energy equals the difference between the two levels

24
Q

How the model explains line spectra

A

Since an atom’s energy is not continuous, but rather has only certain states, an atomic spectrum is not continuous

25
Q

Limitations of Bohr’s model

A

failed to predict the spectra of any other atom; repulsion and additional electron reactions make the actions too complex for Bohr’s model

26
Q

λ=h/mu

A

De broglies equation

27
Q

Electron Affinity

A

the energy change when one mole of an electron is added to one mole of the gaseous atom or ion