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Electron config.
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S1.3.1 EM spectrum
Range of f’s carrying all EM-radiation & their E and λ.
Devided into regions; radio, micro, infra,visual, uv, x, gamma: →^E,f, ←=^λ
Gamma, x, uv dangerous (high f/E)
(c=speed light)c=λf. E = hf (h=planks)
f = waves/second, λ = distance between 2 consecutive peaks.
S1.3.2 Continuous vs line emmission spectra
Continuous: all colours; red→purple
Line: only certain λ: e- have quantines E, non continuous so see certain
Emmission: e- move around nucleus rapidly in energy cells: further = more E. When excited; bc of stimulus like light shining on it, move up an energy level; then immidiately move down; releasing energy in the form of a photon; photon carries specific amount of energy, the energy it emits has a specific λ, which is seen on the line emmission spectrum. The emitted photon is of the same energy as the one it initially absorbed.
Absorption spectrum: shows rainbow - black lines
Emmission spectrium: Shows black screen + rainbow lines
Use spectrometer to measure stuff…
As higher E-level; energies closer and closer, so blue end more convergent lines
Max E = ionization energy: from n=1,2,3 → n=infinity: leave atom
ninfin→n=3: IR, ninfin→n=2: visible, ninfin→n=1: UV
S1.3.3 Electron configuration
= The arrangement of electrons. Around nucleus in principal energy levels/quantum shells of discrete energies. Nr of available spots for e- per nucleus = 2,8,18,32: 2n2… Subshells: s,p,d, E increases
s carries 1 pair(2e), p carries 3 pairs(6e), d carries 5 pairs(10e).
Subshell = orbitals: specific E levels; e is found here, nowhere else
S=round, P=dumbell (x,y,z), D=weird whatever.
Ground state = most stable config. & lowest E: Aufbau: fill 1s, then 2s, then 2p etc…. 4s has lower E than 3d so fill first, then 4p etc.
EXCEPT: Cr: 3d54s1 and Cu 3d104s1 (energetically more favorible)
1s22s22p6……., shorten using noble gases: [Ne]3s2 blabla
Hund’s rule: 1st fill up 1 per orbital:[1][1][1] instead of [1I][1][ ] → bc of spin pair repulsion: one north one south: so prefer to seperate
Pauli Exclusion: hold 2 only, opposing spins
Diagrams like up for more E and to the right n shit….
S1.3.4 Ionization Energies
Energy required to ionize an atom/remove an electron: X → X+ + e-
for hydrogen, E = 13.6/n2 where n is the initial energy level lalala
In kJ mol-1. Succesive IE of element : increase in general: nuclear charge pull in. Big change = change of shell (1,2,3), small change = change of orbital (s,p,d)
1st IE: increase as you move up periodic table: increase to right too: atom rad, inner e repuls, nuclear charge, spin pair repulsion
Radius: increase: down group, to left, inner shield: same perio, increase down