3 Radiation & Atomic Theory+
3.4 Matter Interactions with EM Radiation
3.5 Atomic Theory for those in a Hurry
3.6 Quantum Numbers
3.8 Nomenclature
3.9 Ionic Bonding
3.11 Covalent Bonding
3.42 Learning Outcomes
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Let's face it - a LOT of science and hard work went in to get us to modern day atomic theory. You are going to study the tail end of it all. I'm not even going to hound you about the details leading up to it. It was really hard. Lots of math/differential equations, experiments, analyzing line-spectra developing models, and on, and on... The valuable bits for US is the outcome from all of that. Before I go on though, here is a graphic with lots of stuff in it - all part of modern day atomic theory.
We thank them for their service and contributions to science. So what do YOU need to know from all of that? Energy Levels! Let's dig in and get those sorted out.
* the relative masses of electron : proton : neutron are 1 : 1836 : 1839
average radius of an atomic nucleus is 3 fm while the atom itself is more like 105 pm which is a factor of 35000. If you calculate volumes off of those radii, you'll find that the nucleus occupies only 0.0000000000023% of the space of an atom. The other 99.9999999999987% is occupied by the electron cloud surrounding it.