#2518: retire BlueGene/Q support in thorn vectors
Reporter: Roland Haas
Status: open
Milestone:
Version: development version
Type: task
Priority: minor
Component:
Comment (by Roland Haas):
Unless objected I will apply this after 2022-04-13
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Ticket URL: https://bitbucket.org/einsteintoolkit/tickets/issues/2518/retire-bluegene-q…
#2172: Test "Binary black hole GW150914" example
Reporter: Roland Haas
Status: open
Milestone: ET_2021_11
Version: development version
Type: task
Priority: major
Component: EinsteinToolkit website
Changes (by Roland Haas):
status: open (was resolved)
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Ticket URL: https://bitbucket.org/einsteintoolkit/tickets/issues/2172/test-binary-black…
#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
The RWZ self-force code extends Peter Diener’s 1D self-force code to be able to evolve the gravitational self-force in the Regge-Wheeler-Zerilli gauge using master functions. The code is currently capable of handling circular orbits and will be extended to eccentric orbits and inspirals in the future.
It also includes observers for metric reconstruction, energy and angular momentum flux, and strain output.
The pull request for the new code can be found at [https://bitbucket.org/peterdiener/selfforce-1d/pull-requests/2](https://bit….
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Ticket URL: https://bitbucket.org/einsteintoolkit/tickets/issues/2602/include-regge-whe…
#2601: Add four more parameters for carpet
Reporter: Liwei Ji
Status: new
Milestone:
Version: development version
Type: enhancement
Priority: major
Component: Carpet
Hi all,
we have added four more parameters to `carpet`:
1. `uniformly_split_interior_points_x`
2. `uniformly_split_interior_points_y`
3. `uniformly_split_interior_points_z`
4. `symmetrically_distribute_points_y`
The first three parameters are used to distribute the grid points across processors uniformly according to interior points only.
The fourth parameter is used to distribute the \(even number of\) grid points across \(even number of\) processors with the first and second half being translational symmetric to each other in y-dir, when the grid points are not divisible by the number of processors in y-dir.
Attached please find the diff with the `master` branch. Thanks!
attachment: diff.out (https://api.bitbucket.org/2.0/repositories/einsteintoolkit/tickets/issues/2…)
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Ticket URL: https://bitbucket.org/einsteintoolkit/tickets/issues/2601/add-four-more-par…
#2600: `CCTK_CENTERING_GF` is applied to grid scalars
Reporter: Erik Schnetter
Status: new
Milestone:
Version: development version
Type: bug
Priority: major
Component:
It seems that Cactus applies the `CCTK_CENTERING_GF` macro not just to grid functions, but also to grid scalars. This fails at run time since CarpetX notices that the `GF3D2` class doesn’t work for grid scalars.
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Ticket URL: https://bitbucket.org/einsteintoolkit/tickets/issues/2600/cctk_centering_gf…
#2599: nsnstohmns cannot be reproduced using LORENE2
Reporter: Ken Hui
Status: open
Milestone: ET_2021_05
Version: ET_2021_05
Type: bug
Priority: minor
Component: Cactus
Comment (by Roland Haas):
So based on your tests their seems to be good evidence that indeed the change in constants in `unites.h` is responsible or the failure \(since you can make LORENE1 runs fail but only changing `unites.h`\).
Unfortunately, I doubt there is much the ET can do about this since the changes in the constants are all on the <1% level. Other than a warning to use “compatible” versions of LORENE when reading in data files, which in itself is not terribly helpful. If LORENE encodes a version number in its output files, then the ET can try and check the number and warn if the version number in the file disagrees with the runtime version. It will generate a lot of false positive “version does not match, be careful” warnings so most likely will be ignored by most researchers.
For the gallery example, it may be possible to make things work by using a slightly higher resolution \(the one the gallery is very low, and really not science-worthy\).
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Ticket URL: https://bitbucket.org/einsteintoolkit/tickets/issues/2599/nsnstohmns-cannot…
#963: Improve McLachlan accuracy
Reporter: Erik Schnetter
Status: open
Milestone:
Version:
Type: enhancement
Priority: minor
Component: EinsteinToolkit thorn
Comment (by Roland Haas):
@{557058:f7fd5133-6eee-4385-a5e5-3e03342a0b24} did you have time to look into this?
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Ticket URL: https://bitbucket.org/einsteintoolkit/tickets/issues/963/improve-mclachlan-…