Pre-midterm Flashcards
Molecular scale
Length of a cube with the volume of a molecule
Density field
ρ(x)= lim(l->Lmicro) Ml(x)/Vl
l is small but large enough for V to contain many molecules
Relative size of density fluctuations
Δρ/ρ = 1/sqrt(N)
More molecules = smaller changes in density due to molecular motion
Micro scale
Length at which density fluctuations are less than ε
Macro scale
Length over which density changes due to fluid
Continuum approximation
Valid for L»_space; Lmacro
Conservation laws (def)
Related cinematic and dynamic quantities
Conservation laws (examples)
dP/dt = F P = momentum (vector), F=force
dL/dt = M L= angular momentum, M=moment of force
dK/dt = P
K=kinetic energy, P=power (scalar)
Centre of mass
xm = 1/m * sum(N, i=1)mixi
Moment of force
M = sum(N, i=1) xi x(cross) fi
Angular momentum
L = sum(N, i=1) xi x(cross) mi*dxi/dt
Power
P=sum(N, i=1) fi*dxi/dt
Body force
External force that acts over the entire volume of the object
Contact force
Force that acts at contact of surfaces of objects
Tension
Normal component of force in same direction as unit outward normal
Shear
Tangential component of force
Pressure
Normal component of force in opposite direction of unit outward normal
Stress vector t
dF = t(x, t, n)dS
F=force, x=position, t=time, n=normal, S=surface
Part of “stress principle of Euler and Cauchy”
Fluid at rest cannot have shear stresses (t parallel to n)
Pascal’s law
The pressure in a fluid is the same in all directions
Hydrostatic equilibrium
Global: triple integral over V (ρg-nabla(p)) = 0
Local: nabla(p) = ρg
Barotropic
Independent of temperature
Density and pressure are functions of each other
Isothermal
Constant temperature
Polytropic and ideal gas density
ρ=(RT/C)^(1/γ-1)
Pressure potential
Gravity is conservative: g=-nabla(Φ)