Difference between revisions of "ET Workshop Fall 2011 EOS"
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Discussion about which EOS interfaces Cactus has/had: | Discussion about which EOS interfaces Cactus has/had: | ||
| − | - EOS_Base | + | * EOS_Base |
| − | - | + | * EOSG_Base |
| − | - EOS_Omni | + | * EOS_Omni |
| + | Who uses what: | ||
| + | * EOS_Omni: ET | ||
| + | * EOSG_Base: "nobody" -> to be archived | ||
| + | * EOS_Base: GaTech code, Whisky_Exp -> to remain, but will be dropped from the ET thornlist | ||
| + | * some version of Whisky has "own" interface to tabulated EOS | ||
| + | MHD | ||
| + | * MHD-Con2Prim assumes polytrope EOS | ||
| + | * Code in Wiki: is general, works for polytrope, ideal gas, and hybrid EOSs | ||
| + | * Josh: implementation of C2P for general EOS is now written for the "General" EOS, case, with th "Polytype" coming soon | ||
| + | * Josh: Some functions are not be fully implemented for the non-polytropic EOS_Omni code, but not critical, mostly atmosphere-related functions | ||
| − | + | Christian: | |
| − | + | * To fix: single NS case for hot EOS | |
| − | - some | + | * handle multiple composition evolutions, requires EOS tweaks |
| + | * more important working EOS + MHD | ||
| + | |||
| + | == MHD Con2Prim == | ||
| + | To perform Conservative to Primitive variable conversion in MHD for a generic EOS, we need to use code that is not dependent on the adiabatic index, since it will not be constant. Some notes describing a possible way to implement a more generic Newton-Raphson routine have been uploaded, along with some code to perform this task. | ||
| + | |||
| + | Notes: [[Image:Con2prim_eosomni.pdf]] | ||
| + | |||
| + | Code: [[Image:GRHydro_Con2PrimM_pt.c]] | ||
Latest revision as of 11:33, 1 November 2011
EOS
Discussion about which EOS interfaces Cactus has/had:
- EOS_Base
- EOSG_Base
- EOS_Omni
Who uses what:
- EOS_Omni: ET
- EOSG_Base: "nobody" -> to be archived
- EOS_Base: GaTech code, Whisky_Exp -> to remain, but will be dropped from the ET thornlist
- some version of Whisky has "own" interface to tabulated EOS
MHD
- MHD-Con2Prim assumes polytrope EOS
- Code in Wiki: is general, works for polytrope, ideal gas, and hybrid EOSs
- Josh: implementation of C2P for general EOS is now written for the "General" EOS, case, with th "Polytype" coming soon
- Josh: Some functions are not be fully implemented for the non-polytropic EOS_Omni code, but not critical, mostly atmosphere-related functions
Christian:
- To fix: single NS case for hot EOS
- handle multiple composition evolutions, requires EOS tweaks
- more important working EOS + MHD
MHD Con2Prim
To perform Conservative to Primitive variable conversion in MHD for a generic EOS, we need to use code that is not dependent on the adiabatic index, since it will not be constant. Some notes describing a possible way to implement a more generic Newton-Raphson routine have been uploaded, along with some code to perform this task.
Notes: File:Con2prim eosomni.pdf
