M7 Topic 3 Part 1: Black Body radiation Flashcards
what is a blackbody
a object that both emits and absorbs all incident radiation
what did Maxwell predict about EM radiation
accelerating charges emit EM radiation
what does maxwell’s prediction mean for objects at non zero (kelvin) temperatures
these objects contain charges that are in constant motion, which therefore are constantly emitting EM radiation
What determines the amount of electromagnetic radiation emitted from the object
the temperature of the object
what law relates to black body radiators
Wien’s Law
what is Wien’s law
入ₘₐₓ= b/T
what does each symbol in Wien’s law mean and give their unit of measurement
入ₘₐₓ = The maximum Wavelength (metres (m)) b = Wien's constant (2.898x10⁻³mK) T = temperature of the blackbody (kelvin (k))
what is the classical understanding of blackbodies (3)
Classical physics states:
- that each frequency of vibration should have the same energy. (equipartition theory)
- there is no limit to how great the frequency can be
- so there is no limit to the energy of the vibrating electrons at high frequencies.
what was the issue with classical theory of light when applied to a black body curve (2)
- classical theory shows that the trend should continue infinitely as the temperature increases
- experimental results show there is a sudden drop in emitted intensity in the UV region (Ultraviolet catastrophe)
Who fixed the Ultraviolet catastrophe
Max Planck
how did Max Planck attempt to solve the ultraviolet catastrophe (2)
Posed a Mathematical model:
- suggested the vibrational states of the charges in the black body were not continuous only specific states were available
- the transition between these states released discrete amounts of energy later known as photons.
how is the energy of each photon calculated
the plank relation
what is the the plank relation
E = hf
what do the symbols in the plank relation mean and what units are they measured in
E = energy of the photon (joules (J)) h = planck's constant (6.626x10⁻³⁴ m² kgs⁻¹) f = frequency (hz)
how did einstein change planck’s model to solve the ultraviolet catastrophe (2)
- he changed light from being a continuous wave to discrete packets of energy called photons
- explained that a blackbody can absorb and emit discrete photons rather than continuous waves (quantum theory)