Chapter 39 Quantum Physics Flashcards

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1
Q

The Photon

A
  • Photons are fundamental particles which make up all forms of electromagnetic radiation
  • A photon is a massless “packet” or a “quantum” of electromagnetic energy
  • Energy is not transferred continuously, but as discrete packets of energy
  • each photon carries a specific amount of energy, and transfers this energy all in one go
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2
Q

Calculating Photon Energy

A
  • The energy of a photon can be calculated using the formula:

E = hf

  • Using the wave equation, energy can also be equal to:
  • Where:
    • E = energy of the photon (J)
    • h = Planck’s constant (J s)
    • c = the speed of light (m s-1)
    • f = frequency in Hertz (Hz)
    • λ = wavelength (m)
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3
Q

This equation tells us what:

A
  • The higher the frequency of EM radiation, the higher the energy of the photon
  • The energy of a photon is inversely proportional to the wavelength
  • A long-wavelength photon of light has a lower energy than a shorter-wavelength photon
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4
Q

Photon Momentum

A
  • a photon travelling in a vacuum has momentum, despite it having no mass
  • The momentum (p) of a photon is related to its energy (E) by the equation and Where c is the speed of light:
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5
Q

The Electronvolt is derived from?

A
  • the definition of potential difference:
  • When an electron travels through a potential difference, energy is transferred between two points in a circuit, or electric field
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6
Q

electronvolt is defined as:

A

The energy gained by an electron travelling through a potential difference of one volt

1 eV = 1.6 × 10-19 J

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7
Q

(relation to kinetic energy) When a charged particle is accelerated through a potential difference, it

A
  • gains kinetic energy
  • If an electron accelerates from rest, an electronvolt is equal to the kinetic energy gained:

eV = ½ mv2

  • Rearranging the equation gives the speed of the electron:
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8
Q
  • To convert between eV and J:
A
  • eV → J: multiply by 1.6 × 10-19
  • J → eV: divide by 1.6 × 10-19
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9
Q

The photoelectric effect is the

A
  • phenomena in which electrons are emitted from the surface of a metal upon the absorption of electromagnetic radiation
  • Electrons removed from a metal known as photoelectrons
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10
Q

The photoelectric effect provides important evidence that light is

A

quantised, or carried in discrete packets

  • This is shown by the fact each electron can absorb only a single photon
  • This means only the frequencies of light above a threshold frequency will emit a photoelectron
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11
Q
  • The threshold frequency is defined as:
A

The minimum frequency of incident electromagnetic radiation required to remove a photoelectron from the surface of a metal

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12
Q

The threshold wavelength, related to

A
  • threshold frequency by the wave equation, is defined as:

The longest wavelength of incident electromagnetic radiation that would remove a photoelectron from the surface of a metal

  • Threshold frequency and wavelength are properties of a material, and vary from metal to metal
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13
Q

The Photoelectric Equation

A

E = hf = Φ + ½mv2max

  • Symbols:
    • h = Planck’s constant (J s)
    • f = the frequency of the incident radiation (Hz)
    • Φ = the work function of the material (J)
    • ½mv2max= the maximum kinetic energy of the photoelectrons (J)
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14
Q
  • Since energy is always conserved, the energy of an incident photon is equal to:
A

The threshold energy + the kinetic energy of the photoelectron

  • The energy within a photon is equal to hf
  • This energy is transferred to the electron to release it from a material (the work function) and gives the emitted photoelectron the remaining amount as kinetic energy
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15
Q

(E = hf = Φ + ½mv2max )This equation demonstrates

A
  • If the incident photons do not have a high enough frequency (f) and energy to overcome the work function (Φ)
  • >no electrons will be emitted
  • When hf0 = Φ, where f0 = threshold frequency, photoelectric emission only just occurs
  • Ekmax depends only on the frequency of the incident photon, and not the intensity of the radiation
  • The majority of photoelectrons will have kinetic energies less than Ekmax
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16
Q

Graphical Representation of Work Function

A
  • The photoelectric equation can be rearranged into the straight line equation:
  • y = mx + c
  • Comparing this to the photoelectric equation:
  • Ekmax = hf - Φ
  • A graph of maximum kinetic energy Ekmax against frequency f can be obtained
17
Q

The key elements of the graph:

A
  • The work function Φ is the y-intercept
  • The threshold frequency f0 is the x-intercept
  • The gradient is equal to Planck’s constant h
  • There are no electrons emitted below the threshold frequency f0
18
Q
  • The work function Φ, or threshold energy, of a material is defined as:
A

The minimum energy required to release a photoelectron from the surface of a material

19
Q

an electron can only escape the surface of the metal if

A

it absorbs a photon which has an energy equal to Φ or higher because the electrons in a metal as trapped inside an ‘energy well’ where the energy between the surface and the top of the well is equal to the work function Φ

A single electron absorbs one photon

20
Q
  • Different metals have different threshold frequencies, and hence different work functions
  • Using the well analogy:
A
  • A more tightly bound electron requires more energy to reach the top of the well
  • A less tightly bound electron requires less energy to reach the top of the well
21
Q

Alkali metals have threshold frequencies in the

A
  • such as sodium and potassium, have threshold frequencies in the visible light region
    • This is because the attractive forces between the surface electrons and positive metal ions are relatively weak
22
Q

Transition metals have threshold frequencies in the

A

such as manganese and iron, have threshold frequencies in the ultraviolet region

  • This is because the attractive forces between the surface electrons and positive metal ions are much stronger
23
Q

The maximum kinetic energy of the photoelectrons is

A
  • independent of the intensity of the incident radiation
  • This is because each electron can only absorb one photon
24
Q

The maximum kinetic energy of the photoelectrons is

A
  • independent of the intensity of the incident radiation
  • This is because each electron can only absorb one photon
25
Q

Kinetic energy is only dependent on the

A
  • frequency of the incident radiation
  • Intensity is a measure of the number of photons incident on the surface of the metal
  • So, increasing the number of electrons striking the metal will not increase the kinetic energy of the electrons, it will increase the number of photoelectrons emitted
26
Q

Photoelectric Current is

A

the number of photoelectrons emitted per second

27
Q

Photoelectric current is proportional

A
  • to the intensity of the radiation incident on the surface of the metal
  • This is because intensity is proportional to the number of photons striking the metal per second
28
Q

Photoelectric current is proportional

A
  • to the intensity of the radiation incident on the surface of the metal
  • This is because intensity is proportional to the number of photons striking the metal per second
29
Q

Kinetic energy of photoelectrons is independent of intensity, whereas the photoelectric current is proportional to intensity and independent of frequency

A
30
Q

Alkali metals have threshold frequencies in the

A
  • such as sodium and potassium, have threshold frequencies in the visible light region
    • This is because the attractive forces between the surface electrons and positive metal ions are relatively weak