Equations Flashcards
Keplers 3rd Law
a^3 / P^2 = G(m1 +m2) / (4*pi^2)
Virial Thm
1/2 d^2 I / dt^2 = 2K + U
= 3 integral PdV + U
Magnetic Pressure
P_b = B^2 / (8 Pi)
Radiative Transfer Equation - General
dI_nu/dTau_nu = -I_nu + S_nu
Planck Blackbody
B_nu = (2 h v^3 / c^2) * 1/(exp(h nu / k T)-1)
Stellar Mass Conservation
d M / d r = 4 Pi r^2 rho
Stellar Energy Conservation
d L / d r = 4 Pi r^2 rho epsilon
Stellar HSE
d P / d r = - G M rho / r^2
Stellar Radiative Energy Transp.
dT / dr = - 3 Kappa rho L / (4 a c T^3 4 Pi r^2)
Lamor
dE / dt = 2 q^2 a^2 / (3 c^3)
Fluid - continuity
drho / dt + del dot (rho u) = 0
Fluid - momentum
d(pu) / dt + del dot (rho u u + P - pi) = rho g +f
fluids - energy
dE / dt + del dot [u(E+P)] = -rho u dot del Phi
d(p v^2 / 2 + E) +del dot [v(p v^2 / 2 + (P + E) -
pi + F_c] = rho v Fi / m
eqn of state
P = rho k T / m_bar
Convective energy transport
dT/dR_ad = (1-1/Gamma)T/Pg dP/dr
PE of sphere
- 3 / 5 G M^2 / R
M of elliptical gal or glob cluster
M = 5 (sigma_los)^2 * R / G