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Change in internal energy
ΔU = Q - W by system
ΔU = Q in - Q out + W on - W by
Half life
A = A0(1/2)^n
t(1/2) = 0.693/k
Energy of electron
E = -Ry/n^2
E = hc/lambda = -Ry(1/ni^2 - 1/nf^2)
Number of electrons in shell n
2n^2
Zero order reaction
Rate = k
First order reaction
Rate = k[A]
Second order reaction
Rate = k[A]^2
Rate = k[A][B]
Rate = k[B]^2
Gibbs free energy
ΔG = ΔH - TΔS
Standard free energy
ΔG0= -RT lnKeq
Keq > 1 = forward
Keq
Density of gas
d = P(molar mass)/RT = m/V
Dalton's Law of Partial Pressures
Ptotal = P1 + P2 + P3...
P1 = X1Ptotal
Boyle's Law
P1V1=P2V2
Like boil, squeezing pimple (P and V)
Charle's Law
V1/T1=V2/T2
Charlie Brown on TV (T and V)
Avogardo's Law
V1/n1 = V2/n2
V and n are directly proportional
Volume of one mole of gas at STP
22.4 L
Comparative ideal gas equation (gets rid of R)
PV/PstpVstp = nT/nstpTstp
stp = standard temperature + pressure
Molality
moles of solute/kg of solvent
Density can be helpful here
Dilution
M1V1=M2V2
Solubility Rules
See review notes
Vapor pressure depression
ΔPsoln = Xsolute*Psolvent (STP)
More solute = less surface area available for evaporation
Boiling point elevation
ΔTb = iKbm
Since boiling occurs when Pvapor = Psolvent, lowering Pvapor by adding solute increases boiling point
Freezing point depression
ΔTf = iKfm
Solute interrupts ability of solvent to form solid crystals, lowering freezing point
Osmotic pressure
π = iMRT
Pressure needed to prevent osmosis
Factors affecting solubility in water
Increase temperature: solubility of solid solute increases and solubility of gas solute decreases
Acid dissociation constant
Ka = [H+][A-]/[HA]
Base dissociation constant
Kb = [HB+][OH-]/[B]
Autoionization of water
Kw = [H+][OH-] = 1*10^-14
Log shortcut (p function)
If [anything] = m*10^-n
Then p[anything] = (n-1).(10-m)
Titration equivalence point
VaNa = VbNb
Normality equation
N = M(equivalents/mol)
Henderson-Hasselbalch equation
pH = pKa + log [A-]/[HA]
pOH = pKb + log [HB]/[B]
Electromotive force (emf)
Ecell° = Ecathode° - Eanode°
Faraday's Law of Electrolysis
It = nF
Gibbs free energy (related to emf)
ΔG = -nFEcell°
ΔG = -RTlnKeq
nFEcell° = RTlnKeq
R = 8.314
Alpha decay
Lose He: - 2 protons and neutrons
Only decay that changes atomic mass
Beta minus decay
Electron emission
One of atom's neutrons turns into a proton by emitting an electron
atomic number increases by 1
Electron capture
Beta minus decay in reverse: proton to neutron
Beta plus decay
Positron emission
atomic number decreases by 1
Gamma decay
Emission of high energy photon
no changes to atom's atomic structure
Fraction remaining after n half-lives
(1/2)^n
Fraction of nuclei decayed after n half-lives
1 - (1/2)^n