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Light and matter vocabulary

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AB
refraction towards normal when:light slows down
diffractionproportional to wavelength/gap
reflectionangle of incidence = angle of reflection
interferenceconstructive and destructive; due to superposition
path difference = n x wavelengthconstructive interference
path difference = (2n - 1)/2 x wavelengthdestructive interference
PE gain from battery of voltage VE = qV
KE gain of electron from voltage VKE = qV
Einstein equation for the PE effecthf = work function + KE
work function'unbinding' energy of electrons
electronvolt (eV)1.6 x 10^-19 J
gradient of KE vs f graph for photoelectronsh
y-intercept of KE vs f graph for photoelectronswork function
reactive metals have:low value of work function
unreactive metals have:high value of work function
pressure formulap = F/A
single photonsdiffract and interefere
de Broglie wavelength of particle= h/p
momentum of photons= h/wavelength
mass of photons0
electron orbitalsstanding waves around the atom
atomic energy levelsonly special PE values allowed
formula for photon energy emitted after atomic transitionE = hf
absorption spectraabsorb photons whose energy is equal to atomic energy level gaps
emission spectraemit photons whose energy is equal to atomic energy level gaps
ionisation levelenough energy given to atom to totally free an electron
energy of a single photonhf
two units for heV s and J s
de Broglie for particleh/(2*m*KE)^0.5
momentum of photonp = E/c
incoherent lightphotons with random phases
wide spectrumcontinuous range of wavelengths
line spectrumonly specific (discrete) wavelengths
quantisedspecific (discrete) values only
wave-like natureexbitis wave effects (diffraction, interference...)
stopping voltagestops most energetic photoelectrons
threshold frequency= work function/h
higher intensity lightmore photons
Power of a light source=nhc/wavelength
in phasewill interfere constructively
out of phasewill interfere destructively
thermal motion of electronscollisions produce light
qualitativeno numbers required
quantitativeinvolves numbers, calculations.


University Lecturer in Physics and Science Education
University of Melbourne
Melbourne, Victoria

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