ET Workshop Fall 2011 EOS - Revision history

Jfaber: /* EOS */ update to current status

2011-11-01T11:33:40Z

‎EOS: update to current status

2011-11-01T11:31:43Z

‎MHD Con2Prim: The code now works

2011-10-31T16:06:38Z

2011-10-31T14:39:26Z

‎EOS

2011-10-31T14:04:33Z

‎EOS

2011-10-31T13:51:15Z

‎EOS

2011-10-31T13:50:37Z

‎EOS

2011-10-31T13:34:31Z

‎EOS

2011-10-31T13:34:12Z

‎EOS

2011-10-31T13:33:56Z

‎EOS

@@ Line 12: / Line 12: @@
 MHD
 * MHD-Con2Prim assumes polytrope EOS
-* Code in Wiki: is general, works for polytrope EOS, but is not tested otherwise
+* Code in Wiki: is general, works for polytrope, ideal gas, and hybrid EOSs
-* Josh: implementing should not be a big problem
+* 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
+* Josh: Some functions are not be fully implemented for the non-polytropic EOS_Omni code, but not critical, mostly atmosphere-related functions
 Christian:

@@ Line 22: / Line 22: @@
 == 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 untested code to perform this task.
+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_EOSOmni.c]]
+Code: [[Image:GRHydro_Con2PrimM_pt.c]]

@@ Line 15: / Line 15: @@
 * Josh: implementing should not be a big problem
 * Josh: Some functions are not be fully implemented for the non-polytropic EOS_Omni code
 == 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 untested code to perform this task.

←Older revision		Revision as of 14:39, 31 October 2011
Line 15:		Line 15:
	* Josh: implementing should not be a big problem		* Josh: implementing should not be a big problem
	* Josh: Some functions are not be fully implemented for the non-polytropic EOS_Omni code		* Josh: Some functions are not be fully implemented for the non-polytropic EOS_Omni code
		+	== 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 untested code to perform this task.
		+
		+	Notes: [[Image:Con2prim_eosomni.pdf]]
		+
		+	Code: [[Image:GRHydro_Con2PrimM_pt_EOSOmni.c]]

←Older revision		Revision as of 14:04, 31 October 2011
Line 14:		Line 14:
	* Code in Wiki: is general, works for polytrope EOS, but is not tested otherwise		* Code in Wiki: is general, works for polytrope EOS, but is not tested otherwise
	* Josh: implementing should not be a big problem		* Josh: implementing should not be a big problem
		+	* Josh: Some functions are not be fully implemented for the non-polytropic EOS_Omni code

←Older revision		Revision as of 13:50, 31 October 2011
Line 10:		Line 10:
	* EOS_Base: GaTech code, Whisky_Exp -> to remain, but will be dropped from the ET thornlist		* 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		* some version of Whisky has "own" interface to tabulated EOS
		+	MHD
		+	* MHD-Con2Prim assumes polytrope EOS
		+	* Code in Wiki: is general, works for polytrope EOS, but is not tested otherwise
		+	*

@@ Line 6: / Line 6: @@
 * EOS_Omni
 Who uses what:
-* ET: EOS_Omni
+* EOS_Omni: ET
-* Who uses EOSG_Base: "nobody" -> to be archived
+* EOSG_Base: "nobody" -> to be archived
-* Who uses EOS_Base: GaTech code, Whisky_Exp -> to remain, but will be dropped from the ET thornlist
+* 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