star-fcv-l AT lists.bnl.gov
Subject: STAR Flow, Chirality and Vorticity PWG
List archive
- From: Helen Caines <helen.caines AT yale.edu>
- To: "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
- Subject: [Star-fcv-l] Fwd: Testing SMASH and RIVET
- Date: Mon, 18 Jul 2022 10:35:03 -0400
HI All,
Please see below a request from the SMASH team for input comparing the results of their latest release to our data. If you are interested please feel free to reach out to them, but also let me know so I am aware that someone is working on it. I think it would be great if STAR could become involved in this effort. At the recent PAC meeting there was a recommendation that we maintain our close relationship with the theory community, this is one way to do that.
Thanks
Helen
***********************
Yale University
Physics Dept. - Wright Lab.
PO Box 208120
New Haven, CT 06520
203-432-5831
***********************
she/her/hers
"Life is not about waiting for the storms to pass.
It's about learning how to dance in the rain." - Vivian Greene
Physics Dept. - Wright Lab.
PO Box 208120
New Haven, CT 06520
203-432-5831
***********************
she/her/hers
"Life is not about waiting for the storms to pass.
It's about learning how to dance in the rain." - Vivian Greene
Begin forwarded message:From: Hannah Elfner <elfner AT itp.uni-frankfurt.de>Subject: Testing SMASH and RIVETDate: July 15, 2022 at 8:44:44 AM EDTTo: Helen Caines <helen.caines AT yale.edu>Cc: Jan Staudenmaier <staudenmaier AT fias.uni-frankfurt.de>, Gabriele Inghirami <g.inghirami AT gsi.de>Dear Helen,
I am contacting you as STAR spokesperson with our question below. Please forward this to any of your collaborators who might be interested in running such a test and getting back to us.
We have recently finished a new SMASH release (SMASH-2.2), which finalizes our implementation of HepMC output and direct Rivet integration. Both can either just include the final hadrons of the calculation or the full event scattering history. For HepMC, we offer ASCII and now also ROOT format. We also added the functionality to include weak decay channels in order to match experimental particle detection.
We would be very happy to collect some feedback from our experimental colleagues, if our implementation is sufficent to be used by Rivet analysis in order to streamline comparions between theory and experiment. The ideal scenario would be to run some short test runs with real analysis, also ensuring our documentation is complete. We are happy to include further changes for the new version, if issues occur.
SMASH is online at Github https://github.com/smash-transport/smash and our documentation on Rivet and HepMC output are found in the SMASH User Guide (http://theory.gsi.de/~smash/userguide/2.2/index.html), specifically http://theory.gsi.de/~smash/userguide/2.2/output_hepmc_.html and http://theory.gsi.de/~smash/userguide/2.2/rivet_output_user_guide_.html.
With the feedback either reply to this mail or contact Jan and Gabriele (in CC) directly as the ones working on the implementation.Any feedback by September would be greatly appreciated, but of course also at any later point in time.
Cheers,
Hannah with Jan and Gabriele
--
Prof. Dr. Hannah Elfner (Petersen)
Professor for Theoretical Physics
Frankfurt Institute for Advanced Studies (FIAS)
Institut für Theoretische Physik
Goethe Universität
Ruth-Moufang-Straße 1
D-60438 Frankfurt am Main
Germany
Head of Department Hot and Dense QCD Matter
Coordinator of Theory Pillar
GSI Helmholtzzentrum für Schwerionenforschung GmbH
Phone: +49 (0)69 798 47652
E-mail: elfner AT fias.uni-frankfurt.de
Webpage: https://www.elfner-group.science
ORCID: https://orcid.org/0000-0002-6213-3613
- [Star-fcv-l] Fwd: Testing SMASH and RIVET, Helen Caines, 07/18/2022
Archive powered by MHonArc 2.6.24.