Chem Equations Flashcards
Energy of a quantum?
E=hf, where h=planck’s constant=6.626e-34 J/s; and f=freq of radiation
angular momentum?
L=mvr
kinetic energy?
K=mv^2/2
angular momentum using classical physics and planck’s constant
L=nh/2pi; where n=principal quantum number, h=planck’s constant=6.626e-34
energy of an electron
E=-Ry/n^2; where Ry=Rydberg constant=2.18e-18 J/electron
electromagnetic radiation of a photon emitted by an excited electron
Ep=hc/lambda
where h=planck’s constant=6.626e-34, c=velocity of light in a vacuum=3.00e8 m/s, lambda is the wavelength of the radiation
Lyman series
Final E level=1=>emits UV light
Balmer series
Final E level= 2 => emits UV and visible light
Paschen series
Final E level= 3 => emits IR light
energy of an electron
Ee=Ry(1/ni^2-1/nf^2)
Energy of electron and photon?? lol idk
E=hc/lambda= -Ry(1/ni^2-1/nf^2)
max number of electrons in an electron shell
2n^2
number of e-s within a subshell
4l+2
formal charge
V-1/2Nbonding-Nnonbonding
where V=number of VEs, or V-#sticks-#dots
dipole moment of a polar molecule
mu=qr, where q= charge mag; r=distance bw two partial charges
moles exchanged in a rxn
M^n+ne- –> M
charge of an electron
1.6e-19 C
charge of one moles of e
1.6e-19 x 6.02e23 = 96 487 C/mol e-
1 Farad
96 487 C or J/V; ~ 10e5
Boiling point elevation
extent to which a bp of a sol’n is raised relative to that on the pure solvent;
dTb=i Kb m; i = van’t Hoff factor;
osmotic pressure
pi= i M R T; i= van’t Hoff factor; M= molarity; R=ideal gas constant; T= temp in K
Raoult’s law
Pa=XaPa and Pb= XbPb; applies only when the attraction between a & b is equal to the attraction between a & a and b and b
atm to Pa to torr to mmHg
1 atm = 10e5 Pa= 760 torr = 760 mmHg
Boyle’s law
P1V1=P2V2
Charles law
V1/T1=V2/T2
Avagadro’s principle
n1/V1=n2/V2
ideal gas law
PV=nRT
1 mole gas occupies 22.4L under STP (273 K, 1 atm)
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moles transferred by electrochem cel
i t = n F
where t= time is secs
n= # of moles of e-s
F = faraday constant (10e5 C)
electromotive force
Ecell = Ered + E* ox
Gibbs free e of a cell
dG= -n F E*cell
nFE*cell = RTlnKeq
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Nernst eq
for non-standard conditions; Ecell= E*cell- (RT/nF)(ln Q), where Q = ([C]^c[D]^d)/([A]^a[B]^b)
rate of reaction
-[dR]/t or [dP]/t
rate for forward, irreversible rxn aA+bB–> cC+dD
rate= k [A]^x[B]^y
overall rxn rate
sum of orders (x+y)
0-order rxn rate, conc A at time t, half life
rate = k, conc A = [A]=[A0]-(k0)(t), t1/2 = 1/2*A0/k0
1st-order rxn rate, conc A at time t, half life
rate = k[A] or k[B]; conc a time t = [At] = [A0] e^(-kt); t1/2= ln2/l = 0.693/k
2nd order RR
k[A]^2, k[B]^2 or k[A][B]
collision theory reaction rate:
rate = fZ, where Z is total # of collisions, f is the fraction of effective collisions
heat absorbed or released in a rxn
q=mcT
change in heat (enthalpy) at constant pressure
heat rxn= Hprod-Hreact
standard heat of formation is for ONE MOLE of product–product must have ONE in front of it in a rxn–even if there are fractions
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standard heat of rxn
sum of Hfprods - sum of Hfreactants
standard entropy change of a rxn
sum of Sprod-sum of Sreactants
entropy in the universe
must remain constant– Suni= Ssystem+Ssurroundings > 0
Free E of a system
dG= H-TS, where T - abs temp in Kelvin
standard free e
stGrxn= sum of Gfprods-sum of Gf react at 25 C, 1 atm
G with Keq
G=-RTlnKeq
G rxn not at eq
G= stG + RTlnQ, where stG= -RTlnKeq
Keq
Keq= [C]^c[D]^d/[A]^a[B]^b
le chatelier’s principle
increase in pressure–>favours side of rxn with fewest moles of gas cules; increase in volume–> eq shifts so more prod of substances with highest amount of moles
Ion product
for rxn AmBn–> mA(aq) + nB (aq),
Qsp= [A]^m[B]^n
solubility prod constant
Ksp = [A]^m[B]^n, in a saturated sol’n; varies with temp,
describe the relationships bw Ksp and Qsp
if a salt’s:
Ksp=Qsp, system is at equil, saturated
Ksp>Qsp, system is undersat
Ksp
conv of cal to joule
1 cal = 4.184 J
specific heat gained or lost by a substance
Q=mcT=mc(Tf-Ti)
specific heat capacity for water
c= 1 cal/g K = 1cal/g C = 4.184 j/g K
heat of transformation
Q=m Hl where Hl is the latent heat–i.e. amount of heat needed for 1 kg of substance to change phase–>temp remains constant during phase changes
heat of fusion
Hf–> for solid liquid
heat of vaporization
Hv: for liquid gas
freezing point depression
dTf= i Kp M where Kp=proportionality constant for a given solvent; m=molality (mol solute/ kg solvent); i -van’t Hoff factor–>accounts for number of particles that dissociate from original ‘cule
dalton’s law
partial pressure’s – Pt= Pa + Pb + Pc… + Pz
Partial p of a gas
Pa= Ptot Xa
average KE of gas?
3/2 kT where k = boltzmann constant, T in kelvin
rate pf gas diffusion
r1/r2= sqrt (MM2/MM1)– under isothermal and isobaric conditions
Kw
[H][OH] = 1e-14
percent ionization
ionized acid conc @eq/ initial conc of acid x 100
review nuclear decay
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