Y1: Electromagnetic Radiation and Quantum Phenomena Flashcards

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1
Q

What is the photoelectric effect

A

If you shine radiation of a high enough frequency onto the surface of a metal, it will emit electrons

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2
Q

What causes the photoelectric effect

A

Free electrons near the surface of the metal absorb energy from the oncoming radiation, causing them to vibrate. If enough energy is absorbed, the bond between the metal and the electron in overcome, releasing it as a photoelectron.

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3
Q

What are the conclusions from the photoelectric effect experiments

A
  • No photoelectrons can ever be emitted if the radiation freq. is below the threshold freq.
  • Photoelectrons are emitted with a variety of kinetic energies, with the max value increasing at higher frequencies (Ek not affected by radiation intensity)
  • The No. of photoelectrons emitted per second is proportional to the radiation intensity
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4
Q

What is the photon model of light

A

EM waves can only exist as discrete packets, carrying a certain energy (E=hf), and these photons have 1:1 interactions with the electrons as part of the photoelectric effect.

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5
Q

What would be the expected observation if the frequency of the radiation is below the threshold frequency, according to the wave theory.

A

If the light interacted with the electrons as a wave, it would take longer for the photoelectrons to be emitted with low freq. radiation, but they would eventually, as their energy would gradually increase

However, this is not observed

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6
Q

How does the threshold frequency support the photon model of light.

A

The energy of a photon is proportional to the freq. (E=hf), and each photon only contains a discrete quantity of energy. This means that if the freq. of the radiation is too low, the interaction with the electron will never cause it to be emitted, as there is not enough energy to overcome the bond with the metal.

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7
Q

What would be the expected observation if the intensity of the radiation increased, according to the wave theory.

A

If the light interacted with the electrons as a wave, higher intensity would increase the energy transferred to each electron, increasing their Kinetic energy

However, this is not observed

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8
Q

How does the kinetic energy of photoelectrons support the photon model of light.

A

Increasing the intensity of the radiation causes an increase in the number of photons, but doesn’t effect the energy of each one. This means that each interaction occurs with the same energy (proportional to freq.), so the electrons have the same Ek, but there are more interactions, so the total number of photoelectrons released increases.

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9
Q

What is the gold foil experiment for demonstrating the photoelectric effect.

A
  • A zinc plate is attached to the top of an electroscope (box containing a piece of metal with gold leaf attached).
  • The zinc plate is negatively charged, so the metal and the gold repel each other (gold foil lifts up)
  • UV light (high freq. - Red light wouldn’t work) is shone on the zinc plate
  • The energy of the photons causes electrons to be released (photoelectric effect)
  • This causes the zinc (and metal) to lose their charge, so the gold leaf is no longer repelled and falls back down.
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10
Q

What is the work function (ɸ)

A

The energy required to break the bond holding the electron to the metal

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11
Q

What is the equation for work function (ɸ)

A

In order for the photoelectric effect to occur

hf ≥ ɸ

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12
Q

What is the threshold frequency (fo)

A

The minimum frequency of a photon (radiation) needed for the photoelectric effect to occur

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13
Q

What is the equation for the threshold frequency (fo)

A

fo = ɸ/h

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14
Q

How do you calculate the maximum kinetic energy of a photoelectron (Ek)

A

hf = ɸ + Ek(max)

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15
Q

What is the stopping potential (Vs)

A

The potential difference required to stop the fastest (Ek max) moving electrons, as they lose their energy doing work against it.

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16
Q

What is the equation for stopping potential

A

eVs = Ek(max)

(e = 1.6x10^-19C)

17
Q

What is an electron volt (eV)

A

The kinetic energy carried by an electron after it has been accelerated from rest to a pd of 1V

18
Q

What is 1eV

A

1.6x10^-19J

19
Q

What is a ground state electron

A

An electron in the lowest energy level in an atom (n=1)

20
Q

How does an electron move up energy levels

A

If it absorbs a photon with the exact energy of the difference between the two levels, the electron is excited.

21
Q

How does an electron move down energy levels

A

If it emits a photon with the exact energy of the difference between the two energy levels

22
Q

Why are the energies of the different energy levels in an atom negative

A

The electrons within this level are bound to the atom (like a ball in a pit with -GPE), and at infinity, the energy is 0J, so levels closer to the atom have negative values.

23
Q

What is the ionisation energy

A

The energy required to remove and electron from an atom, beginning at ground state.

24
Q

How do you work out the ionisation energy of an atom

A

The energy of an electron must reach 0J to escape the atom, so the ionisation energy is the positive value of the energy at ground state (eg. Hydrogen = 13.6eV)

25
Q

How are photons (visible light) emitted by fluorescent tubes

A
  • Tube contain mercury vapour, with a high voltage supplied across it.
  • This accelerates free electrons, ionising some mercury atoms to produce more free electrons
  • Free electrons collide with electrons in mercury atoms, exciting them to higher energy levels.
  • As the electrons return to ground state, they emit high energy photons (UV).
  • These photons are absorbed by phosphor coating on the inside of the tube, exciting it’s electrons
  • When these electrons move down energy levels, they emit many lower energy photons of visible light.
26
Q

What is line emission spectra

A

When photons (light) are emitted from an atom as it’s electrons de-excite, the light can be diffracted to separate out the wavelengths.
This will show a black screen with several coloured lines corresponding to the wavelengths of the photons emitted.

27
Q

What is line absorption spectra

A

When white light passes through a cool gas, certain wavelengths of photons are absorbed as the electrons are excited.
The remaining light that passes through can be diffracted to give a colour spectrum, with several dark lines corresponding to the wavelengths of photons that were absorbed.

28
Q

Why must the light pass through a cool gas for line absorption spectra

A

At low temperatures, most of the electrons will be at ground state, so all possible photons that can be absorbed, will be.

29
Q

How can line emission/absorption spectra be used to determine the elements within a gas/object in deep space.

A

The lines on the spectra correspond with the wavelengths of photons emitted/absorbed by the atoms, and as E∝λ (E=cf/λ), the wavelengths correspond to the energies of the photons, which is exactly equal to the difference in the energy levels of the atoms. This means that the line emission/absorption spectra is unique for each element.

30
Q

When does light have wave-like properties

A

Diffraction: When a beam of light passes through a narrow gap, it spreads out, which can only be explained if light acts as a wave.

31
Q

When does light have particle like properties

A

Photoelectric effect: When photons hit a metal, electrons are released, and increasing the light intensity only increases the number of electrons (not the Ek of each), which can only be explained is light is considered as particle-like photons.

32
Q

What is the wave-particle duality theory

A

If ‘wave-like’ light shows particle properties (photons), particles such as electrons should show ‘wave-like’ properties.

33
Q

What is the de Broglie wavelength equation

A

λ = h/mv

Links a ‘wave-like’ property (λ) with a particle property (momentum)

34
Q

How does electron diffraction occur

A

Electrons are accelerated to high velocities in a diffraction tube, then passed through a graphite crystal.
This produces a diffraction pattern of rings (of the probability of where an electron will end up).

35
Q

How does changing the speed of the electrons in the diffraction tube effect the diffraction pattern

A

λ ∝ diffraction spacing (just like in light),
and as λ=h/mv: Diffraction spacing ∝ 1/v

So, slower electrons form widely spaced rings, and vice versa

36
Q

How does changing the mass of the particles in the diffraction tube (eg. neutrons instead of electrons) effect the diffraction pattern

A

λ ∝ diffraction spacing (just like in light),
and as λ=h/mv: Diffraction spacing ∝ 1/m

So, heavier particles form more tightly spaced rings, and vice versa

37
Q

What must the size of the lattice spacing be in a crystalline structure for diffraction to occur through it

A

The lattice spacing must be similar to the wavelength of the incident radiation in order for diffraction to occur through a crystalline structure.