Physics of Matter Equations

Descripción

Physics of Matter equations
Lauren Clark
Fichas por Lauren Clark, actualizado hace más de 1 año
Lauren Clark
Creado por Lauren Clark hace alrededor de 9 años
58
2

Resumen del Recurso

Pregunta Respuesta
Critical temperature Temperature at which critical point occurs T=deltaE/kb
Intermolecular potential per unit volume U=1/2 p^2INTEGRAL(gV) g is radial distribution function
Flux J = 1/4 n <c> n number density
Pressure of a gas (think flux) P=1/3 nm <c^2>
Pressure difference in gas P=Po e^(-mgh/kbT)
Maxwell-Boltzmann distribution function 1/N dN/dc = 4pic^2 (m/2pikbT)^3/2 e^(-mc^2/2kbT)
Most probable speed of a molecule c* = SQRT(2kbT/pim)
Mean speed <c> = SQRT(8kbT/pim)
Root mean square speed SQRT(<c^2>) = SQRT(3kT/m)
Mean free path mfp=1/pio^2n o diameter of molecule, radius of cylinder swept out by particle
Effusion relation pressure and temperature P1/P2=SQRT(T2/T1)
Fick's Law For diffusion J=-D dn/dz
Diffusion coefficient D= -mfp/3 <c> dn/dz
Viscosity VISC=1/3 m mfp n <c> n number of molecules
Thermal conductivity k = 1/3 n mfp (cv) cv = heat capacity constant v
First law of thermodynamics deltaU = Q + W
Work done on gas at constant pressure W = -P(Vf-Vi)
Work done in a reversible isothermal expansion W=-NRTln(Vf/Vi)
Heat capacity at constant V dQ/dT=dU/dT
Heat capacity constant P dQ/dT
Enthalpy H=U+PV
Spacing between rotational energy levels e=hbar^2/4pi^2I I moment of inertia
Relationship between cV and cP cP=Cv +(dU/dV +P)dV/dT
Change in volume due to isobaric thermal expansivity deltaV=B V delta T
Change in volume due to isothermal compressibility k+ - 1/V (dV/dP)
Ratio of cP and cV -V/P dP/dV = gamma
Relationship between P and V for adiabatic expansion P1V1^gamma = P2V2^gamma... etc Gamma is the ratio of cP to cV
Cooling due to adiabatic expansion T2/T1 = (V1/V2)^gamma-1= (P2/P1)^((gamma - 1)/gamma)
Entropy dS=dQ/T = dH/T
2nd law of thermodynamics delta S(univ) >/ 0
Gibb's Free Energy G=H-TS
Master Equations dH=TdS+vdP dG =VdP - SdT
Clapeyron Equation dP/dT = Svap-Ssol/Vvap-Vsol
Clasius Clapeyron Equation ln(P2/P1) = - deltaH/R (1/T2-1/T1)
Latent heat of vaporisation L= deltaHvap
Van der Waals equation P=RT/V-b - a/V^2 v = volume of one mole
b in Van der Waals Equation b=4Nav=2pi/3 Na o^3 v = volume of one molecule o = diameter of one molecule
Missing neighbours of a molecule approaching a wall n-no = - ano^2/kT a = alpha = some constant
Critical temperature of liquid Tc=8a/27Rb = 26 deltae/27k a and b are constants from the Van der Waals equation n
Keesom interaction U = -2u1^2u2^2/3kT(4piEo)^2r^6 ui = dipole moment r = distance between two charges in dipole
Induced dipole moment u = aE a = alpha = polarizability
Lennard Jone's Potential U = 4e((o/r)^12 - (o/r)^6) o = distance at which U is zero r = distance between particles
Surface free energy eNbrok/2ro^2 = NbrokL/qNa(pNa/M)^2/3 ro = average seperation Nbrok = number of neighbours lost e = depth of Lennard Jones potential L = latent heat q = number of nearest neighbours
Latent heat of vapourisation L = 1/2 qNae q = number of near neighbours
Young's Equation gamma(sv) = gamma(sl) +gamma(l)costheta found by decomposing the surface free energies at a contact angle between liquid and a solid
Pressure difference across curved interface P1=P2 = gamma(1/R1+1/R2)
Bernoullis Equation P1/p1 +1/2 v1^2 +phi1 = P2/p2 +1/2 v2^2+phi2 p = density phi = gz
Stoke's Equations Viscous force F = 6pinRv n = viscosity R = radius
Reynolds Number Re = pvR/n n viscosity p density R radius
Ionic pair potential U = 1.481e[+/- (o/r)+(o/r)^9]
Packing Fraction PF = NpVp/Vuc
Plane spacing d = a/SQRT[h^2+k^2+l^2)] h,k,l miller indices
Lattice energy of Van der Waal solid Ut<2eNa[12(o/r1)^12 - 14.05(o/r1)^6]
Ionic lattice energy Ut=0.741eNa[6(o/r1)^9-1.75(o/r1)]
Braggs Law Cubic System (sin0)^2 = lambda^2(h^2+k^2+l^2)/4a^2
Einstein model for specific heat Cv = 3R(0e/T)^2 e^(0e/T) / [(e^(0/T)-1)^2] 0e = hbarw/k
Debye frequency w = k0/hbar 0 = debye temp
Young's Modulus 72e/ro^3 e = strain ro = distance
Mostrar resumen completo Ocultar resumen completo

Similar

Forces and motion
Catarina Borges
AQA Physics P1 Quiz
Bella Statham
GCSE AQA Physics - Unit 3
James Jolliffe
Using GoConqr to study science
Sarah Egan
GCSE AQA Physics 1 Energy & Efficiency
Lilac Potato
Waves
kate.siena
Forces and their effects
kate.siena
Junior Cert Physics formulas
Sarah Egan
CHEMISTRY TEST
kingi kigongo
OCR Physics P4 Revision
Dan Allibone
P2 Radioactivity and Stars
dfreeman