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Wave
transfer of energy through a disturbance through space and time
Wavelength
Distance between identical points of successive waves
Amplitude(A)
Measure of waves displacement
Intensity(I)
Energy passing through per unit per time(A²)
Frequency(f)
number of waves passing a point per second
Wavelength formula
v=λf
Wave equation for EM radiation:
c=λf
Order of EM spectrum from high frequency to low frequency
Gamma, X, UV, visible, IR, microwave, radio(FM to AM)
Plancks relation
E=hf; graph is a slope
Photoelectric effect
Electrons are ejected from the surface of certain materials when they absorb light of specific frequencies(called threshold frequency)
Problem with Photoelectric effect
Could not be explained by wave theory
Wave-particle duality:
Light acts as both a wave and a particle
de Broglie wave equation
E=hv/λ; λ=h/mv (m is in kg!)
Problems with Rutherford’s model
Orbiting electrons are not stable. They are constantly accelarating (rotation), releasing energy as EM radiation in the process. The loss of energy means that the electrons will eventually crash into the nucleus.
Could not explain the line spectra: Why was light only emitted/absorbed at specific wavelengths?
Could not explain periodic trend of elements
Bohr model
Electrons orbit the nucleus at specific distances(quantized distances) called n
Rydberg constant
2.18×10⁻¹⁸J
Quantum jumps
Atom absorbing/releasing energy causes the electron to jump/fall; more energy→towards violet light
Spectral series
Lyman, UV
Balmer, UV/vis
Paschen, IR
Brackett, IR
Problem with Bohr model
Only matched spectra lines of hydrogen and one electron species
Schrodingers Equation
Describes waves. Electrons were waves with specific energies and spacial distributions(quantized). Wavefunction/orbital represented by greek letter psi. Solutions can gbe approximated for atoms with more than one electron
Heisenberg uncertainty principle
It is impossible to know both the position and the momentum of a particle with certainty
Quantum numbers:
n, l, ml, mn
n
shell, orbital size and distance of electron to nucleus
l
subshell, shape of orbital
ml
Orientation of the orbital
ms
spin up/spin down
Stern Gerlach experiment
Predict existence of spin by passing beam of silver atoms through magnetic field. Half deflect up, half deflect down.
Hydrogen orbital energy
All orbitals with the same n have the same energy(degenerate)
Aufbau principle
Lowest energy levels filled before higher energy levels(reflected on periodic table)
Pauli exclusion principle
Electrons in same orbital have opposite spins
Hund’s rule
MMost stable arrangement of electrons are ones with greatest number of parallel spins. Arrows face upwards
Electron configuration exceptions for full d shells:
Copper, gold, silver
Electron configuration exceptions for half filled d shells
Molybdenum, Chromium
Valence electrons composition
number of s and p electrons of outermost occupied shell. Based on periodic table group number
duet rule:
H and He have full outer shell with 2 valence electrons
Coulombs law
Opposite charges attract, like charges repel
Force increases with increasing charge
Force decreases with increasing distance between charges
Zeff
Effective nuclear charge: essentially what charge valence electrons feel since they are shielded from nucleus. Total charge(# protons)-number of core electrons
Atomic radius
Size of an atom determined by size of electron cloud. Half distance between two nuclei in adjacent atoms.
Atomic radius trends
Increases going down and left
Increases going down because of n (shell) increasing
Increases going left because there is a decreasing Zeff, electrons are sucked in less
Ionic radius
Size of ions compared to atoms
Ionic radius Trends:
As atoms become more negatively charged, they become bigger. More electrons means more shielding
Ionization energy (IE)
Minimum energy it takes to remove an electron
Ionization energy trends
Increase ionization going up and right; again bc of Zeff and n levels
Ionization energy trends exceptions:
group 2vs13 and 15vs16. Group 2 has full s shell. Group 15 has half filled shell
Electron affinity (EA)
Energy released when electron is added to atom. How badly an atom wants an electron. More positive →more easily atom excepts. Negative of energy change
EA Trends:
Increases going up and right. Group 17 and 1 have higher EA’s since they are close to having full shells. Group 2 and 18 have lower EAs since their shells are already full.
Metallic character
increases going down and left. Francium is the most metallic since it has the lowest IE.
Nonmetallic character
Increase going up and right. Fluorine is the most nonmetallic since it has high EA.
Diamagnetic
electrons are all paired
Paramagnetic
at least one unpaired electron
Filled d subshells prefered
Au, Ag, Cu
Half filled d subshells prefered
Mo, Cr
Electronegativity
tendency for atom to attract electrons