BA Elias Saarmann: Difference between revisions
Jump to navigation
Jump to search
m (Reverted edits by Lothar.brendel (talk) to last revision by Elias.S) Tag: Rollback |
m (LaTeX, engl.) |
||
| Line 1: | Line 1: | ||
* [https://www.overleaf.com/project/6a2548a24fcac02449144d80 Diss auf Overleaf] | * [https://www.overleaf.com/project/6a2548a24fcac02449144d80 Diss auf Overleaf] | ||
= | = Literature = | ||
* [https://arxiv.org/pdf/2603.20373 Radiating Bondi Flows I] | * [https://arxiv.org/pdf/2603.20373 Radiating Bondi Flows I] | ||
= | = Bondary Conditions = | ||
== in [https://arxiv.org/pdf/2603.20373 Radiating Bondi Flows I] == | == in [https://arxiv.org/pdf/2603.20373 Radiating Bondi Flows I] == | ||
For the outer boundry conditions | For the outer boundry conditions \(r \rightarrow \infty\) | ||
\[ | \[ | ||
(\tilde{\rho},\mathcal{M}, s, \tilde{L}, \tilde{E}_\text{r}) \rightarrow (1, 0, s_\infty, \tilde{L}_\infty, 1) | (\tilde{\rho},\mathcal{M}, s, \tilde{L}, \tilde{E}_\text{r}) \rightarrow (1, 0, s_\infty, \tilde{L}_\infty, 1) | ||
| Line 16: | Line 16: | ||
<nowiki>With dimensionless density \( \tilde{\rho} = \frac{\rho(r)}{\rho_\infty}\), Mach number \(\mathcal{M} = \frac{v(r)}{c_s(r)}\), dimensionless entropy \( s = \frac{S}{c_\text{V}}\) and dimensionless radiation Energy density \(\tilde{E}_\text{r} = \frac{E_\text{r}}{a_\text{r}T_\infty^4}\).</nowiki> | <nowiki>With dimensionless density \( \tilde{\rho} = \frac{\rho(r)}{\rho_\infty}\), Mach number \(\mathcal{M} = \frac{v(r)}{c_s(r)}\), dimensionless entropy \( s = \frac{S}{c_\text{V}}\) and dimensionless radiation Energy density \(\tilde{E}_\text{r} = \frac{E_\text{r}}{a_\text{r}T_\infty^4}\).</nowiki> | ||
== in PLUTO/belt == | |||
... | |||
= Code-Anpassungen für konstante Zentralmasse = | = Code-Anpassungen für konstante Zentralmasse = | ||
Revision as of 13:33, 24 June 2026
Literature
Bondary Conditions
in Radiating Bondi Flows I
For the outer boundry conditions \(r \rightarrow \infty\) \[ (\tilde{\rho},\mathcal{M}, s, \tilde{L}, \tilde{E}_\text{r}) \rightarrow (1, 0, s_\infty, \tilde{L}_\infty, 1) \]
With dimensionless density \( \tilde{\rho} = \frac{\rho(r)}{\rho_\infty}\), Mach number \(\mathcal{M} = \frac{v(r)}{c_s(r)}\), dimensionless entropy \( s = \frac{S}{c_\text{V}}\) and dimensionless radiation Energy density \(\tilde{E}_\text{r} = \frac{E_\text{r}}{a_\text{r}T_\infty^4}\).
in PLUTO/belt
...
Code-Anpassungen für konstante Zentralmasse
(Lothar)
M_centr(o.Ä.) als weiteren Parameter in user_defined_parameters.h definieren und die AnzahlUSER_DEF_PARAMETERSentsprechend erhöhen- den Wert von
M_centrin pluto.ini unter[Parameters]setzen (in Gramm) - body-force.c aus belt/src/Misc in den Run-Folder kopieren und in Zeile 64 die
M_X1_BEGdurch(g_inputParam[M_centr]/ReferenceMass)ersetzen