#2549: inlcude FLRWSolver in ET
Reporter: Roland Haas
Status: new
Milestone: ET_2022_05
Version: development version
Type: enhancement
Priority: major
Component:
Comment (by Hayley Macpherson):
Thanks Roland! I usually put FLRWSolver in EinsteinInitialData/FLRWSolver, but whatever you think works best is fine by me.
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Ticket URL: https://bitbucket.org/einsteintoolkit/tickets/issues/2549/inlcude-flrwsolve…
#2549: inlcude FLRWSolver in ET
Reporter: Roland Haas
Status: new
Milestone: ET_2022_05
Version: development version
Type: enhancement
Priority: major
Component:
Comment (by Roland Haas):
I have added FLRWSolver to the main ET thornlist as:
```
# FLRW cosmological initial data
!TARGET = $ARR
!TYPE = git
!URL = https://github.com/hayleyjm/FLRWSolver_public
!REPO_PATH = ../$2_public
!CHECKOUT =
FLRWSolver/FLRWSolver
```
which checks out `FLRWSolver_public` and creates a thorn `FLRWSolver/FLRWSolver` for it.
If you would rather use a different arrangement or thorn name, please let me know.
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Ticket URL: https://bitbucket.org/einsteintoolkit/tickets/issues/2549/inlcude-flrwsolve…
#2602: include Regge-Wheeler-Zerilli gauge self-force code in ET
Reporter: Samuel Cupp
Status: new
Milestone: ET_2022_05
Version: development version
Type: enhancement
Priority: major
Component: Other
Comment (by Roland Haas):
@{557058:088051f9-5b94-4b5e-bfbe-71137030b9c1} now that Peter has given the “no harm” go ahead, please integrate the code into the “master” branch or otherwise provide updated checkout information so that the RWZM version can be tested and downloaded by interested parties.
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Ticket URL: https://bitbucket.org/einsteintoolkit/tickets/issues/2602/include-regge-whe…
#2616: Add NRPyEllipticET to the Einstein Toolkit
Reporter:
Status: new
Milestone:
Version:
Type: enhancement
Priority: major
Component:
Comment (by Roland Haas):
Please be reminded of the deadline to provide the “does no harm” initial review verdict before the deadline of Sept 1st 2022.
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Ticket URL: https://bitbucket.org/einsteintoolkit/tickets/issues/2616/add-nrpyelliptice…
#2485: include complex and real scalar evolution code from Canuda in ET
Reporter: Roland Haas
Status: open
Milestone:
Version:
Type: task
Priority: major
Component:
Comment (by Roland Haas):
Please provide the “does no harm” initial review verdict before the deadline of Sept. 1st 2022.
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Ticket URL: https://bitbucket.org/einsteintoolkit/tickets/issues/2485/include-complex-a…
#2549: inlcude FLRWSolver in ET
Reporter: Roland Haas
Status: new
Milestone: ET_2022_05
Version: development version
Type: enhancement
Priority: major
Component:
Comment (by Chi Tian):
Hi all, I have reviewed the documents and majority of the the codes. At least at physics level, everything looks fine to me. Only some tiny issues regarding the way FLRWSolver dealing with the extrinsic curvature:
1. It seems there is a typo in Eq. \(10\) in the document, where minus sign is missing \(at least for the case where the author mentions “Setting f =1/3 and n=2 in the above yields ∂tα=∂ta for EdS“\).
2. The name of the variable `kvalue` in several `flrw_*.f90` files seems a little confusing. From its name, it seems this variable represents the extrinsic curvature K. However, its true value seems to be `3 * kvalue` if my understanding was correct.
3. By following the gauge condition `\dot{\alpha} = f * K`, effectively it is setting the coordinate time to something closed to the conformal time `\eta`, and the value of `\alpha` will grow roughly following the growth of the scale factor `a`. Could this possibly introduce numerical instabilities to `GRhydro` when starting from a very high redshift, and universe keeps expanding for quit long? Since I would guess most of astrophysical GR simulations may choose gauge conditions that make `\alpha` close to 1.
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Ticket URL: https://bitbucket.org/einsteintoolkit/tickets/issues/2549/inlcude-flrwsolve…
#2636: CoordinateSymmetry has a parameter `rotating_90` that is never used
Reporter: Gabriele Bozzola
Status: new
Milestone:
Version:
Type: bug
Priority: major
Component:
As in title. Grepping “rotating” in the llama repository doesn’t produce any result.
Overall, it is unclear \(to me at least\) what symmetries are supported with multipatch grids.
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Ticket URL: https://bitbucket.org/einsteintoolkit/tickets/issues/2636/coordinatesymmetr…
#2630: WaveMoL example computes energy from unsynchronized grid variables
Reporter: Roland Haas
Status: open
Milestone:
Version:
Type: bug
Priority: major
Component:
Comment (by Roland Haas):
Unless objected I apply this after 2022-09-08
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Ticket URL: https://bitbucket.org/einsteintoolkit/tickets/issues/2630/wavemol-example-c…