Hi Bruno,

I have gone through the notebook in the past and from what I could see, the 
version of paper I (10.1103/PhysRevD.85.064040)
is implemented in the code, kappa_3 is encoded in the parameter 
'ML_CCZ4::GammaShift', and the changes for the
scaling of kappa_1 and kappa_2 with the lapse (eq.  27 and 28 in paper II, 
2013) are not implemented.

I hope this helps.
Best,
Michael Müller
________________________________
From: [email protected] <[email protected]> on 
behalf of Bruno Giacomazzo <[email protected]>
Sent: Thursday, June 2, 2022 10:04 AM
To: Erik Schnetter <[email protected]>
Cc: Einstein Toolkit Users <[email protected]>; Paolo Garimberti 
<[email protected]>
Subject: Re: [Users] question about ML_CCZ4 parameters


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Hi Erik,
   thanks a lot for the offer to help. I will try to have a look by myself 
first at the mathematica notebook.

Unless anybody else knows on what paper CCZ4 in McLachlan is based on. :-)

Cheers,
Bruno


Il giorno mer 1 giu 2022 alle ore 22:48 Erik Schnetter 
<[email protected]<mailto:[email protected]>> ha scritto:
Bruno

Although I was probably around when the CCZ4 formulation was
implemented, I don't recall.

I usually resolve to archaeology, comparing the equations in the
respective Mathematica scripts to equations found in publications. If
no one else speaks up, I can assist with this – we'd set up a Zoom
meeting, and I can show how to read (or modify!) the Mathematica
script that implements these equations.

-erik

On Tue, May 31, 2022 at 6:21 AM Bruno Giacomazzo
<[email protected]<mailto:[email protected]>> wrote:
>
> Together with a student of mine we are trying to use the CCZ4 formulation 
> implemented in McLachlan.  We saw that most parameters are the same as in 
> BSSN, but there are damping factors that need to be selected.
>
> In Alic et al 2013 (https://link.aps.org/doi/10.1103/PhysRevD.88.064049) they 
> mention 3 damping factors (k1, k2, and k3), but in the param.ccl of 
> McLachlan/ML_CCZ4 only k1 and k2 are mentioned (assuming they are the same).
>
> Is it because k3 is hardcoded to the value suggested in Alic et al 2013? Or 
> does McLachlan/ML_CCZ4 use a different set of evolution equations (in which 
> case, is there a reference)?
>
> We were able to find some example parameter files (for example the ones from 
> the Parma group https://einstein.pr.infn.it/gravity/Research/BNS2015.html) 
> and we found that they used indeed k1 and k2 from Alic et al 2013:
> ML_CCZ4::dampk1 = 0.05
> ML_CCZ4::dampk2 = 0
>
> We also saw that they added  ML_CCZ4::ML_Theta to the Dissipation vars and set
> ML_CCZ4::apply_dissipation   = "never".
> The other parameters look the same as when using BSSN.
>
> Since I never used ML_CCZ4 I want to be sure that I'm setting the parameters 
> correctly and the damping factors seem to be the most delicate point.
>
> Thanks,
> Bruno
>
> --
>
> Prof. Bruno Giacomazzo
> Department of Physics
> University of Milano-Bicocca
> Piazza della Scienza 3
> 20126 Milano
> Italy
>
> email: [email protected]<mailto:[email protected]>
> phone: (+39) 02 6448 2321
> web: http://www.brunogiacomazzo.org
>
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--
Erik Schnetter <[email protected]<mailto:[email protected]>>
http://www.perimeterinstitute.ca/personal/eschnetter/


--

Prof. Bruno Giacomazzo
Department of Physics
University of Milano-Bicocca
Piazza della Scienza 3
20126 Milano
Italy

email: [email protected]<mailto:[email protected]>
phone: (+39) 02 6448 2321
web: http://www.brunogiacomazzo.org<http://www.brunogiacomazzo.org/>

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