resonances in Ca+Ca, Ni+Ni and Au+Au reactions from 1 AGeV to 2 AGeV: Consistency between yields, mass shifts and decoupling temperatures
arXiv:2004.10539 · doi:10.1016/j.nuclphysa.2020.122058
Abstract
The Ultra-relativistic Quantum Molecular Dynamics (UrQMD) transport approach is used to calculate (1232) yields in Ca+Ca, Ni+Ni and Au+Au collisions between 1 AGeV and 2 AGeV. We compare and validate two different methods to extract the yields of (1232) resonances in such low energy nuclear collisions: Firstly, the spectra at low are used to infer the (1232) yield in A+A collisions, a method employed by the GSI/FOPI experiment. Secondly, we employ the invariant mass method used by the HADES collaboration, which has recently reported data in the channel. We show that both methods are compatible with each other and with the theoretical calculations, indicating that the new HADES results are compatible with the previous FOPI measurements. Then we use the ratio to extract the kinetic decoupling temperatures of the (1232) resonances. We find that the extracted temperatures are consistent with the predicted mass shift of the resonance and the freeze-out parameters estimated from complementary studies (blast wave fits, coarse graining).
6 pages, 4 figures
References in corpus (2)
Cited by in corpus (8)
- Comparison of heavy ion transport simulations: Ag+Ag collisions at Elab = 1.58 AGeV
- Ambiguities in the hadro-chemical freeze-out of Au+Au collisions at SIS18 energies and how to resolve them
- Magnetic moments of the octet, decuplet, low-lying charm, and low-lying bottom baryons in a nuclear medium
- Decoding the flow evolution in Au+Au reactions at GeV using hadron flow correlations and dileptons
- Correlated pion-proton pair emission off hot and dense QCD matter
- Harmonic flow correlations in Au+Au reactions at 1.23 AGeV: A new testing ground for the Equation-of-State and expansion geometry
- Investigating the cluster production mechanism with isospin triggering: Thermal models versus coalescence models
- Hubble Expansion and Freeze-Out at RHIC-BES Energies from UrQMD