the relation bw the wavelength of radiation w the frequency
as the wavelength of the radiation inc, the frequency dec
continuous spectrum
shows all available colour of the spectrum
higher amplitude =
greater intensity, determined by the number of e- ejected
smallest particle of em energy
photons
absorption spectrum
the wavelengths of light that hv been absorbed by the atom show up as dark bands
emission spectrum
colours present are the same as those that are missing from the absorption spectrum
process of exciting an e-
process of emission of energy
pros of bohr model
cons of bohr model
aufbau’s principle
tells us to fill in electron from lowest to highest energy
order: 1s (n=1, l=0), 2s2p(n=2, l=1), 3s3p3d, 4s4p4d4f, 5s5p5d5f, 6…etc.
paulis exclusion prcinciple
paired e- must be opposite spin, no 2 identical wavefunctions can exist
hunds rule
when filling out e- shells, leave unpaired for as long as possible
exceptions for filling e- orbitals
chromium/molybdenum - full unpaired d shell is lower energy than fully paired s shell
cu, ag, au - fully paired d shell is lower energy than full s shell
n codes for
avg distance from nucleus, is kinda like the base of the rest
l codes for
the shape of the e- orbital, is js n-1
l=0: s (spherical)
l=1: p (peanut)
l=2: d (flower and ringpop looking ahh)
ml (magneti quantum number) codes for
how many of each shaped orbital are allowed at that lvl
- [-l, l] e.g. l=1 ml = -1, 0, 1
magnetic spin number (ms) codes for
how e- acts in magnetic field
-1/2 or 1/2