<div dir="ltr">I have a master's student of mine that is working on NS-BH. We have a (private) thorn that can read NS-BH initial data generated with LORENE, but at the moment we are having problems generating good NS-BH initial data with LORENE (the main problem is getting a sufficiently small initial separation) and therefore we are currently working with KADATH (<a href="https://kadath.obspm.fr/fuka/">https://kadath.obspm.fr/fuka/</a>). Once we have the data ready, we plan to use their publicly available thorn to read those data within the Einstein Toolkit (<a href="https://bitbucket.org/fukaws/">https://bitbucket.org/fukaws/</a>).<div><br></div><div>Cheers,</div><div>Bruno</div></div><br><div class="gmail_quote"><div dir="ltr" class="gmail_attr">Il giorno ven 8 ott 2021 alle ore 15:51 Santiago Jaraba Gómez <<a href="mailto:santiago.jaraba@uam.es">santiago.jaraba@uam.es</a>> ha scritto:<br></div><blockquote class="gmail_quote" style="margin:0px 0px 0px 0.8ex;border-left:1px solid rgb(204,204,204);padding-left:1ex"><div dir="ltr">Yes, of course! If I end up getting something, I will be glad to share it.<div><br></div><div>I can't promise anything, though. It seems like a difficult task for me, so I may focus on other projects if I try it and don't make much progress.</div><div><br>Best,<br>Santiago</div></div><br><div class="gmail_quote"><div dir="ltr" class="gmail_attr">El vie, 8 oct 2021 a las 15:30, Erik Schnetter (<<a href="mailto:schnetter@cct.lsu.edu" target="_blank">schnetter@cct.lsu.edu</a>>) escribió:<br></div><blockquote class="gmail_quote" style="margin:0px 0px 0px 0.8ex;border-left:1px solid rgb(204,204,204);padding-left:1ex">Santiago<br>
<br>
The "usual" open source response that I can't help but mention here<br>
is: "We're looking forward to your updates to this parameter file, to<br>
a brief writeup in the form of a web page, and possibly a few figures<br>
/ pictures / maybe a movie..."<br>
<br>
Take this with a grain of salt, of course: There is no expectation<br>
from our side that you should be doing this. However, if you do end up<br>
investing time into cleaning up the parameter file and / or writing up<br>
some notes that help you run the parameter file, and if you end up<br>
making some figures or a movie, then we'd be happy to help you turn<br>
this into a new gallery page.<br>
<br>
-erik<br>
<br>
On Fri, Oct 8, 2021 at 8:59 AM Santiago Jaraba Gómez<br>
<<a href="mailto:santiago.jaraba@uam.es" target="_blank">santiago.jaraba@uam.es</a>> wrote:<br>
><br>
> Hi Miguel,<br>
><br>
> Okay, thanks! I had actually seen that thread and others, that's why I was asking for some kind of "official" .par file. I guess one has to go through unofficial thorns for this kind of simulation.<br>
><br>
> Anyway, I may try to get something from there. Thanks for the answer!<br>
><br>
> Best,<br>
> Santiago<br>
><br>
> El jue, 7 oct 2021 a las 22:42, Miguel Gracia (<<a href="mailto:mgracia@austin.utexas.edu" target="_blank">mgracia@austin.utexas.edu</a>>) escribió:<br>
>><br>
>> Hello Santiago,<br>
>><br>
>> The toolkit currently don’t have a BH-NS binary gallery example but this <a href="http://lists.einsteintoolkit.org/pipermail/users/2021-August/008168.html" rel="noreferrer" target="_blank">http://lists.einsteintoolkit.org/pipermail/users/2021-August/008168.html</a> email thread in the ET mailing list about BHNS simulations might be useful.<br>
>><br>
>> Best,<br>
>> Miguel<br>
>><br>
>> ——<br>
>><br>
>><br>
>> On Oct 1, 2021, at 11:02 AM, Santiago Jaraba Gómez <<a href="mailto:santiago.jaraba@uam.es" target="_blank">santiago.jaraba@uam.es</a>> wrote:<br>
>><br>
>> Hi everyone,<br>
>><br>
>> I would like to simulate a BH-NS binary with the Einstein Toolkit. I have some experience with black hole simulations, but I am new to introducing neutron stars.<br>
>><br>
>> I have seen there are some publications in this line but, as far as I know, there are no examples like in the BBH or BNS case, which are displayed in the gallery.<br>
>><br>
>> My question is: is there any .par file that one can take as a starting point to these simulations? And maybe a more subjective question: is it currently possible to simulate BH-NS binaries in the Einstein Toolkit with similar confidence as BBH or BNS?<br>
>><br>
>> Thank you in advance!<br>
>><br>
>> Best regards,<br>
>> Santiago<br>
>> _______________________________________________<br>
>> Users mailing list<br>
>> <a href="mailto:Users@einsteintoolkit.org" target="_blank">Users@einsteintoolkit.org</a><br>
>> <a href="http://lists.einsteintoolkit.org/mailman/listinfo/users" rel="noreferrer" target="_blank">http://lists.einsteintoolkit.org/mailman/listinfo/users</a><br>
>><br>
>><br>
> _______________________________________________<br>
> Users mailing list<br>
> <a href="mailto:Users@einsteintoolkit.org" target="_blank">Users@einsteintoolkit.org</a><br>
> <a href="http://lists.einsteintoolkit.org/mailman/listinfo/users" rel="noreferrer" target="_blank">http://lists.einsteintoolkit.org/mailman/listinfo/users</a><br>
<br>
<br>
<br>
-- <br>
Erik Schnetter <<a href="mailto:schnetter@cct.lsu.edu" target="_blank">schnetter@cct.lsu.edu</a>><br>
<a href="http://www.perimeterinstitute.ca/personal/eschnetter/" rel="noreferrer" target="_blank">http://www.perimeterinstitute.ca/personal/eschnetter/</a><br>
</blockquote></div>
_______________________________________________<br>
Users mailing list<br>
<a href="mailto:Users@einsteintoolkit.org" target="_blank">Users@einsteintoolkit.org</a><br>
<a href="http://lists.einsteintoolkit.org/mailman/listinfo/users" rel="noreferrer" target="_blank">http://lists.einsteintoolkit.org/mailman/listinfo/users</a><br>
</blockquote></div><br clear="all"><div><br></div>-- <br><div dir="ltr" class="gmail_signature"><div dir="ltr"><div><div dir="ltr"><div><div dir="ltr"><div dir="ltr"><p><font color="#000000">Pr<font face="arial, sans-serif">of. Bruno Giacomazzo<br>Department of Physics<br>University of Milano-Bicocca<br></font></font><span style="color:rgb(0,0,0)"><font face="arial, sans-serif">Piazza della Scienza 3<br></font></span><span style="color:rgb(0,0,0)"><font face="arial, sans-serif">20126 Milano<br></font></span><span style="font-size:12.8px;color:rgb(0,0,0)">Italy</span></p><p><font color="#000000"><span style="font-size:12.8px">email: </span><span style="font-size:12.8px"><a href="mailto:bruno.giacomazzo@unimib.it" target="_blank">bruno.giacomazzo@unimib.it</a><br></span><span style="font-size:12.8px">phone: (+39) 02 6448 2321</span></font><br><font color="#000000"><span style="font-size:12.8px">web: </span></font><span style="color:rgb(0,0,0);font-size:12.8px"><a href="http://www.brunogiacomazzo.org/" style="font-size:12.8px" target="_blank">http://www.brunogiacomazzo.org</a></span></p><p><font color="#000000">----------------------------------------------------------------------<br><span style="font-size:12.8px">There are only 10 types of people in the world:<br></span><span style="font-size:12.8px">Those who understand binary, and those who don't<br></span><span style="font-size:12.8px">----------------------------------------------------------------------<br></span></font></p></div></div></div></div></div></div></div>