% IMPORTANT: The following is UTF-8 encoded. This means that in the presence
% of non-ASCII characters, it will not work with BibTeX 0.99 or older.
% Instead, you should use an up-to-date BibTeX implementation like “bibtex8” or
% “biber”.
@ARTICLE{Staudenmaier:238891,
author = {Staudenmaier, Jan and Kübler, Natey and Elfner, Hannah},
title = {{P}article production in {A}g{A}g collisions at
{E}$_{{K}in}$ = 1.58 {A} {G}e{V} within a hadronic transport
approach},
journal = {Physical review / C},
volume = {103},
number = {4},
issn = {2469-9993},
address = {Woodbury, NY},
publisher = {Inst.},
reportid = {GSI-2021-00898},
pages = {044904},
year = {2021},
note = {ISSN 2469-9993 not unique: **2 hits**. "Published by the
American Physical Society under the terms of the Creative
Commons Attribution 4.0 International license. Further
distribution of this work must maintain attribution to the
author(s) and the published article's title, journal
citation, and DOI. Funded by SCOAP3."},
abstract = {Heavy-ion collisions at low beam energies explore the high
density regime of strongly interacting matter. The dynamical
evolution of these collisions can be successfully described
by hadronic transport approaches. In March 2019, the HADES
Collaboration took data for AgAg collisions at
EKin=1.58AGeV, and in this work we provide predictions for
particle production and spectra within the Simulating Many
Accelerated Strongly interacting Hadrons (smash) approach.
The multiplicities and spectra of strange and nonstrange
particles follow the expected trends as a function of system
size. In particular, in ArKCl (and pNb) collisions, much
higher yields of double-strange baryons were observed
experimentally than expected from a thermal model.
Therefore, we incorporate a previously suggested mechanism
to produce Ξ baryons via rare decays of high mass N*
resonances and predict the multiplicities. In addition, we
predict the invariant mass spectrum for dilepton emission
and explore the most important sources of dileptons above 1
GeV, that are expected to indicate the temperature of the
medium. Interestingly, the overall dilepton emission is very
similar to the one in AuAu collisions at 1.23AGeV, a hint
that the smaller system at a higher energy behaves very
similarly to the larger system at lower beam energy.},
cin = {TES},
ddc = {530},
cid = {I:(DE-Ds200)TES-20160901OR397},
pnm = {612 - Cosmic Matter in the Laboratory (POF4-612) / FAIR
Phase-0 - FAIR Phase-0 Research Program (GSI-FAIR-Phase-0) /
CRC-TR211 - TRR 211 Strong-Interaction Matter Under Extreme
Conditions (315477589)},
pid = {G:(DE-HGF)POF4-612 / G:(Ds200)GSI-FAIR-Phase-0 /
G:(GEPRIS)315477589},
experiment = {$EXP:(DE-Ds200)no_experiment-20200803$},
typ = {PUB:(DE-HGF)16},
UT = {WOS:000647602200003},
doi = {10.1103/PhysRevC.103.044904},
url = {https://repository.gsi.de/record/238891},
}