Comparison Between Classification Using Impact Parameter and Using Number of Participants in Relativistic Nuclear Collisions
Using the hydrodynamical code NeXSPheRIO, we compare predictions as usually done in hydrodynamics, usingcentrality windows defined through the impact parameter, and as obtainable experimentally, using windowsin participant number.
I tiakina i:
| I whakaputaina i: | Brazilian Journal of Physics |
|---|---|
| Ngā kaituhi matua: | , , , , , , |
| Hōputu: | Artigo |
| Reo: | Inglês |
| I whakaputaina: |
Sociedade Brasileira de Física
2004
|
| Ngā marau: | |
| Urunga tuihono: | https://www.redalyc.org/articulo.oa?id=46400138 |
| Ngā Tūtohu: |
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
|