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version 4.2
authored
Oct 28, 2025
by
Udo Ziegler
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3-NIRVANA-user-guide/3.1-Code-basics.md
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@@ -437,11 +437,12 @@ the following criteria:
side) to decide whether a child block is to be created.
-
Jeans-length-based (important in simulations involving selfgravity):
$
$
\l
eft(
\f
rac{
\p
i}{G}
\f
rac{c_s^2}{
\v
arrho}
\r
ight)^{1/2}
$
\l
eft(
\f
rac{
\p
i}{G}
\f
rac{c_s^2}{
\v
arrho}
\r
ight)^{1/2}
\c
dot
\m
athcal{E}_
\m
athrm{Jeans}
\l
eft
\{\b
egin{array}{ll}
<
\d
elta s &
\m
box{refinement}
\\
>1.25\delta s & \mbox{derefinement}\\
\e
nd{array}
\r
ight.$$ where the first factor is the local Jeans
\e
nd{array}
\r
ight.$
where the first factor is the local Jeans
length with $c_s$ the sound speed and $G$ the gravitational
constant, and where $
\d
elta s=
\m
in
\{\d
elta x,h_y
\d
elta y, h_z
\d
elta z
\}
$.
$
\m
athcal{E}_
\m
athrm{Jeans}$ is a user-specific threshold giving the
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@@ -455,7 +456,8 @@ the following criteria:
\r
ight)^{1/2}
\c
dot
\m
athcal{E}_
\m
athrm{Field}
\l
eft
\{\b
egin{array}{ll}
<
\d
elta s &
\m
box{refinement}
\\
>1.25\delta s & \mbox{derefinement}\\
\e
nd{array}
\r
ight.$$ where the first factor is the Field length with
\e
nd{array}
\r
ight.$$
where the first factor is the Field length with
$L(
\v
arrho, T)$ the density- and temperature-dependent heatloss
function and $
\k
appa$ the thermal conduction coefficient.
$
\m
athcal{E}_
\m
athrm{Field}$ is a user-specific threshold giving the
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