Week 1 - Intro Quantum I Flashcards

(27 cards)

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?

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
Spectra is...
unique to and characteristic of each element (colour lines like we saw in the lab)
26
What was Rutherford's atomic model and what were the two major problems with it?
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
In Rydberg's equation (1/𝜆 = R (( Z^2 / n1^2 ) - ( Z^2 / n2^2 ), what does each term mean?
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.