Nature of Light Flashcards

1
Q

Describe the Corpuscular theory

A

Corpuscular theory - proposed by Newton - light made up of corpuscles (or tiny particles). He imagined the light particles to bounce off surfaces, like a ball bouncing off a wall, to explain reflection and suggested that the light particles changed speed when they moved from one material to another to explain refraction.

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2
Q

Describe the Wave theory

A

Wave theory - proposed by Huygens - light consists of waves

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3
Q

Define Photon and Quantum

A

Photon - a discrete bundle (quanta) of energy. One photon (if it has enough energy) will release one photo electron.

Quantum - a fixed indivisible amount.

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4
Q

Explain the Complimentary principle

A

The complimentary principle says that sometimes electrons have the properties of particles and sometimes the properties of waves, but never both.

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5
Q

Describe the Photoelectric effect and how it can be demonstrated

A

The photoelectric effect can be demonstrated by means of a negatively charged zinc plate. (If it was positive the transmitted photoelectrons would be immediately attracted back by the charge)
The ultraviolet light causes the gold leaf electroscope to discharge (leaf goes down). The uv light is absorbed and the energy is used to eject the electrons from the metal surface.

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6
Q

Define Photoelectrons

A

Photoelectrons - the electrons near the surface of zinc that gain enough energy to escape from the attraction of the positive charge on the nucleus

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7
Q

What is the formula (in words) that explains this effect?

A

Energy from UV light = Energy needed to remove electrons from metal surface + KE of photoelectrons

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8
Q

What is the condition necessary for photoelectrons to be emitted?

A

Electron would only be emitted if a single quantum of the light had enough energy for the electron to escape. This is because one photon will only release one photoelectron.

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9
Q

What are the observations from the photoelectricity experiment? (3)

A
  1. Using visible light we do not get any photoelectrons, even if the light is left on for a long time. This is in contradiction with the wave theory, as it suggests that eventually, enough energy should be given to an electron to remove it from the metal surface. This does not happen. No photoelectrons emitted from the surface.
  2. Increasing brightness (intensity) and hence the energy of the waves should produce photoelectrons, according to wave theory. Using a green laser (very bright) with the zinc does not produce any photoelectrons. Wave theory: Energy is proportional to share of intesity. This does not happen so this contradicts the wave theory.
  3. Increasing the frequency (using UV instead of visible light) we find a threshold frequency (fo) where photoelectrons start to be emitted. Wave theory suggests the energy should not be different depending on the frequency. So this also contradicts the wave theory.
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10
Q

Define Threshold frequency and Work function

A

Threshold frequency - the frequency that is just large enough to liberate electrons, fo (ø=hfo)
Work function - the bare minimum energy needed to just remove an electron from the surface of a metal with no kinetic energy.

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11
Q

What is the Einstein’s photoelectric equation?

A
hf = ø + 1/2 mv^2 max
hf - energy of photons; ø - work function; 1/2 mv^2 max - maximum kinetic energy of photoelectrons 
hf = hfo + 1/2 mv^2
h(f-fo) = 1/2 mv^2
h(f-fo) = eVstop
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12
Q

Describe different types of photcells

A

A phototube is the name given to a particular type of photocell that generates photoelectrons when light falls on a specially coated metal cathode. The other types of photocells are photovoltaic photocells, in which an emf is generated by the presence of light across the boundary of two semiconducting materials, and photoconductive cells or light-dependent resistors (LDRs). An LDR is a semiconductor whose resistance decreases when it is exposed to electromagnetic radiation (it becomes a good conductor). This is because the photon energy release more electrons to act as charge carriers: n increases in I=nAvq.

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13
Q

Describe how a phototube can be used to find the work function

A

We apply a stopping voltage (reverse voltage) to an evacuated tube containing two electrodes. One electrode is irradiated with light of a known wavelength (so we can calculate its frequency)
The stopping potential is increased until the photoelectrons just fail to reach the negatively charged electrode (the photoelectric current goes to zero)
Therefore the work done on the photoelectrons by the electric field is equal to the KE of the photoelectrons. eVstop = 1/2 mv^2 max
so hf = ø + eVstop
and Vstop = (h/e)f - (ø/e)
y = mx + c
So graph of Vstop against Frequency

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14
Q

Define the Electron-volt

A

An electron-volt is the work done on (or the energy gained by) an electron when it moves through a potential difference of 1 volt.
It is used to avoid using powers of 10^-19 but as it is not an SI unit, it needs to be converted in the end result.

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15
Q

What is the expression for energy of a photon and this expression but in the emission spectrum

A

E = hf; E - energy of a photon; h- Planck constant; f - frequency of the radiation

hf = E2-E1

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16
Q

Describe the atomic line spectra in terms of transitions between discrete energy levels

A

Gases are poor conductors of electricity. To make them conduct we need to have low pressure and high voltage. The electrons passing through the gas collide with the atoms, or molecules, of the gas and cause them to become excited so that they give out light. We can examine the emitted light using a spectrometer and a diffraction grating. We find that only certain wavelengths of light are emitted so that we see a line spectrum.
This means that the hydrogen atom can only have particular levels, and not “any” energy level, otherwise we would see photons of all wavelengths and frequencies (ie all energies)
This means that the energy levels are quantised. Only certain energy levels are allowed.
If we consider the wave-like properties of electrons as we can consider the energies that the electron may have as corresponding to standing waves in the hydrogen.

17
Q

Why are the energy levels all negative?

A

When the electron is infinitely far away from the proton (so it feels no force of attraction) and is not moving (so it has no KE) it seems reasonable to say it has no energy. Therefore we define the zero of energy to be infinitely far away from the hydrogen atom. This means that all the energy levels in hydrogen are negative (as work has to be done on an electron in the hydrogen atom against the force of attraction between the proton and the electron)

18
Q

What is the difference between Emission and Absorption?

A

Emission - from high energy state to low energy state

Absorption - from low energy state to high energy state

19
Q

Define Intensity(Radiation flux density) and give a formula for it

A

Intensity is defined as the energy passing normally (at 90 degrees) through a surface per unit area per unit time/ is the power per unit area.

Radiation flux density = Intensity = Power/Area

I = E/At = P/A

20
Q

Define Efficiency

A

Efficiency of the system is the ability to transfer the input energy to desired (useful) energy

Efficiency = (useful energy/power output / total energy/power input) * 100

21
Q

Explain the wave-particle duality and the complimentary principle

A

Wave-particle duality: particles can sometimes behave like waves and waves can sometimes behave like particles. De Broglie equation links waves and particles:
λ=h/p

The complimentary principle says that sometimes electrons have the properties of particles Andy sometimes the properties of waves but never both together.

22
Q

Evaluate the use of solace cells

A

Solar cells provide electricity from a free, renewable source
Considerations include:
- efficiency of the cells
- cost
- availability of materials
- global energy prices
- impact of continuing use of fossil fuels

23
Q

Explain remote sensing and its uses

A

Remote sensing is the process of detecting and monitoring the physical characteristics of an area by measuring it reflected and emitted radiation at a distance from the targeted area. Special cameras collect remotely sensed images of the Earth, which help us “sense” things about the Earth. Examples:

  • Cameras on satellites and airplanes take images of large ares on the Earth’s surface. allowing us to see much more than we can see standing on the ground (clouds, volcanoes, fires, growth of trees)
  • Sonar systems on ships can be used to create images of the ocean floor without needing to travel to the bottom of the ocean
  • Cameras on satellites can be used to make images of temperature changes in the oceans