Directed Flow in Heavy-Ion Collisions and Its Implications for Astrophysics
Analysis of directed flow ( v 1 ) of protons, antiprotons and pions in heavy-ion collisions is performed in the range of collision energies s N N = 2.7–39 GeV. Simulations have been done within a three-fluid model employing a purely hadronic equation of state (EoS) and two versions...
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| Format: | Article |
| Language: | English |
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MDPI AG
2017-11-01
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| Series: | Universe |
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| Online Access: | https://www.mdpi.com/2218-1997/3/4/79 |