Week 1 - Intro Quantum I Flashcards

1
Q

Light is _______

A

Electromagnetic Radiation

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2
Q

As you move from UV to infrared, does wavelength increase or decrease?

A

Increase

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3
Q

(1) What is wavelength, (2) what symbolizes it, and (3) what units is it measured in?

A

(1) The distance a wave travels in one cycle, (2) λ, and (3) nanometres (nm)

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4
Q

(1) what is frequency, (2) what symbolizes it, and (3) what units is it measured in?

A

(1) The number of cycles a wave undergoes per second, (2) ν, and (3) Hertz (Hz), aka s^-1

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5
Q

What is amplitude?

A

1/2 the height of a wave from peak to trough

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6
Q

Relationship between wavelength and frequency?

A

Inversely proportional

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7
Q

How are waves and particles different? (moving from one medium to another)

A

waves undergo refraction; particles slow down and follow a curved path

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8
Q

How are waves and particles different? (interaction with an object)

A

waves bend around an object, may result in diffraction; particles have a binary response, they are either obstructed or not

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9
Q

Interference of waves can be…

A

constructive or destructive

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10
Q

Classical definitions of matter and light could not describe what three major observations?

A
  1. Blackbody Radiation
  2. Photoelectric Effect
  3. Atomic Spectra
    Attempting to understand these led to the Quantum Theory that describes matter and light as having both particle- and wave-like properties
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11
Q

What is a blackbody?

A

A theoretical (ideal) model that absorbs all radiation falling on it – A “perfect” absorber or emitter. To stay in thermal equilibrium, it must emit radiation at the same rate as it absorbs it so a blackbody also radiates well.

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12
Q

What is blackbody radiation?

A

Everything at a temperature emits radiation with the same shape curve, just ‘shifted’ to shorter wavelength as things get warmer (visible if hot)

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13
Q

What is Ultraviolet catastrophe?

A

(Related to blackbody radiation) the predicted results from classical theory deviated from the observed data, especially at shorter wavelength - showed intensity becoming infinitely large as the wavelengths became smaller

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14
Q

What was the theory behind the mathematical expression to describe the phenomenon of blackbody radiation, and what was the expression developed?

A

Theory: that energy only assumes certain values (is quantized), E = nhv (or E = hv for n=1; Hydrogen). E = energy of the radiation, n = quantization factor (element number), h = Planck’s constant, v = frequency

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15
Q

What is photoelectric effect?

A

When reflecting light off metal surfaces, it was observed that light sources above a threshold frequency could eject electrons from the surface. However, light sources below that threshold would never eject electrons even when the brightness was increased.

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16
Q

Why could photoelectric effect not be explained with classical mechanics? What do we know now that we did not back then?

A

According to classical mechanics, there was no relation between the kinetic energy and the frequency of light. Now, we know that KE increases with frequency.

17
Q

What is the work function (required to remove an electron) dependent on? How is work function represented?

A

Threshold frequency; work function of metal = Φ

18
Q

How is the kinetic energy of an electron (reflecting off a metal surface) determined?

A

The excess energy (h*v) over the threshold freq/work function

19
Q

What did einstein discover (related to photoelectric effect)?

A

Light comes in packets - photons

20
Q

How is velocity represented?

A

u

21
Q

In the equation (hν = ½mu^2 + hv0), what does each part mean?

A

h = Planck’s constant
v = frequency
- h*v = Energy of photon
m = mass of electron (constant)
u = velocity
- ½mu^2 = kinetic energy of electron
hv0 = threshold frequency = Φ (work function)

22
Q

Classical vs. observed idea: relationship between frequency of light and kinetic energy of electron

A

Classical: no relationship
Observed: once threshold is passed, as frequency increases KE increases as well

23
Q

Classical vs. observed idea: relationship between number of electrons and kinetic energy of electron

A

Classical: as frequency increases, so does number of electrons
Observed: no relationship after threshold passed

24
Q

Graphically, how were Einstein’s explanations of photoelectric effect proved?

A

JJ Thompson; y-intercept is equal to negative work function

25
Q

Spectra is…

A

unique to and characteristic of each element (colour lines like we saw in the lab)

26
Q

What was Rutherford’s atomic model and what were the two major problems with it?

A

Model: nucleus at centre, positively charged, surrounded by electrons
Problems: orbiting electrons should spiral into the nucleus, emission spectrum from such an atom should be continuous
Phenomenon: what keeps the electrons away from the nucleus and the atom stable?

27
Q

In Rydberg’s equation (1/𝜆 = R (( Z^2 / n1^2 ) - ( Z^2 / n2^2 ), what does each term mean?

A

𝜆 is the wavelength; 1/𝜆 is called the wave number
R is Rydberg’s constant
Z is atomic number (H=1, He=2, Li=3…)
n1 and n2 are positive whole numbers, where n2 > n1. They represent the movement between energy levels.