Changes between Version 21 and Version 22 of u/erica/scratch4

Timestamp:

02/16/16 19:53:15 (9 years ago)

Author:

Erica Kaminski

Comment:

—

u/erica/scratch4

@@ -21 +21 @@
 = Tracking accretion luminosity in the code = 
 
-At each time-step i, the luminosity is computed as:
+At each time step i, the luminosity is computed as:
 
 [[latex($L_i=\frac{G M_i dm_i}{R ~dt}$)]]
 
-where [[latex($M_i$)]] is the mass of the sink particle at i, [[latex($dm_i$)]] is the total accreted mass for that time-step, [[latex($G$)]] is the gravitational constant in computational units, [[latex($R$)]] is the radius of the star, taken to be 1 solar radius by default, but modifiable by the user at run-time, and [[latex($dt$)]] is the hydro time-step. 
+where [[latex($M_i$)]] is the mass of the sink particle at i, [[latex($dm_i$)]] is the total accreted mass for that time-step, [[latex($G$)]] is the gravitational constant in computational units, [[latex($R$)]] is the radius of the star, taken to be 1 solar radius by default, but modifiable by the user at run-time, and [[latex($dt$)]] is the hydro time step. 
 
 == Kernel ==
@@ -64 +64 @@
 [[latex($ source(i,j,k,iaccretion\_energy)= info\%workarray(i,j,k,iaccretion\_energy)*dt_{rad} $)]]
 
-where we now enter the total ''specific'' (recall k has units of 1/volume) accretion energy into the source function averaged over a radiative timestep. And now, we are ready to begin testing.
+where we now enter the total ''specific'' (recall k has units of 1/volume) accretion energy into the source function averaged over a radiative time step. And now, we are ready to begin testing.
 
 == Physical meaning of the accretion energy source term ==