FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W4205941025> ?p ?o ?g. }

• W4205941025 abstract "The beam energy dependence of the directed flow is a sensitive probe for the properties of strongly interacting matter. Hybrid models that simulate dense (core) and dilute (corona) parts of the system by combining the fluid dynamics and hadronic cascade model describe well the bulk observables, strangeness productions, and radial and elliptic flows in high-energy heavy-ion collisions in the high baryon density region. However, the beam energy dependence of the directed flow cannot be described in existing hybrid models. We focus on improving the corona part, i.e., the nonequilibrium evolution part of the system, by introducing the mean-field potentials into a hadronic cascade model. For this purpose, we consider different implementations of momentum-dependent hadronic mean fields in the relativistic quantum molecular dynamics (RQMD) framework. First, Lorentz scalar implementation of a Skyrme type potential is examined. Then, full implementation of the Skyrme type potential as a Lorentz vector in the RQMD approach is proposed. We find that scalar implementation of the Skyrme force is too weak to generate repulsion explaining observed data of sideward flows at $sqrt{{s}_{NN}}<10$ GeV, while vector implementation gives collective flows compatible with the data for a wide range of beam energies $2.7<sqrt{{s}_{NN}}<20$ GeV. We show that our approach reproduces the negative proton directed flow at $sqrt{{s}_{NN}}>10$ GeV discovered by experiments. We discuss the dynamical generation mechanisms of the directed flow within a conventional hadronic mean field. A positive slope of proton directed flow is generated predominantly during compression stages of heavy-ion collisions by the strong repulsive interaction due to high baryon densities. In contrast, at the expansion stages of the collision, the negative directed flow is generated more strongly than the positive one by the tilted expansion and shadowing by the spectator matter. At lower collision energies $sqrt{{s}_{NN}}<10$ GeV, the positive flow wins against the negative flow because of a long compression time. On the other hand, at higher energies $sqrt{{s}_{NN}}>10$ GeV, negative flow wins because of shorter compression time and longer expansion time. A transition beam energy from positive to negative flow is highly sensitive to the strength of the interaction." @default.
• W4205941025 created "2022-01-26" @default.
• W4205941025 creator A5004139253 @default.
• W4205941025 creator A5080894355 @default.
• W4205941025 date "2022-01-18" @default.
• W4205941025 modified "2023-10-15" @default.
• W4205941025 title "Mean-field update in the JAM microscopic transport model: Mean-field effects on collective flow in high-energy heavy-ion collisions at<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML><mml:mrow><mml:msqrt><mml:msub><mml:mi>s</mml:mi><mml:mrow><mml:mi>N</mml:mi><mml:mi>N</mml:mi></mml:mrow></mml:msub></mml:msqrt><mml:mo>=</mml:mo><mml:mn>2</mml:mn></mml:mrow></mml:math>–20 GeV energies" @default.
• W4205941025 cites W1676312485 @default.
• W4205941025 cites W1764327410 @default.
• W4205941025 cites W178757487 @default.
• W4205941025 cites W1819848952 @default.
• W4205941025 cites W1848634479 @default.
• W4205941025 cites W1898703770 @default.
• W4205941025 cites W1968059978 @default.
• W4205941025 cites W1972036178 @default.
• W4205941025 cites W1974222205 @default.
• W4205941025 cites W1975246608 @default.
• W4205941025 cites W1978856096 @default.
• W4205941025 cites W1982382996 @default.
• W4205941025 cites W1987865922 @default.
• W4205941025 cites W1989688932 @default.
• W4205941025 cites W1991087023 @default.
• W4205941025 cites W1991863639 @default.
• W4205941025 cites W1998260141 @default.
• W4205941025 cites W2001858316 @default.
• W4205941025 cites W2002095533 @default.
• W4205941025 cites W2004176311 @default.
• W4205941025 cites W2005933796 @default.
• W4205941025 cites W2006747606 @default.
• W4205941025 cites W2007796578 @default.
• W4205941025 cites W2009749270 @default.
• W4205941025 cites W2010792399 @default.
• W4205941025 cites W2016079325 @default.
• W4205941025 cites W2016975306 @default.
• W4205941025 cites W2018265820 @default.
• W4205941025 cites W2020889186 @default.
• W4205941025 cites W2021587707 @default.
• W4205941025 cites W2033339097 @default.
• W4205941025 cites W2036011427 @default.
• W4205941025 cites W2037335503 @default.
• W4205941025 cites W2037890362 @default.
• W4205941025 cites W2040316568 @default.
• W4205941025 cites W2044367805 @default.
• W4205941025 cites W2046784475 @default.
• W4205941025 cites W2049492844 @default.
• W4205941025 cites W2050777706 @default.
• W4205941025 cites W2053036324 @default.
• W4205941025 cites W2057017907 @default.
• W4205941025 cites W2060908529 @default.
• W4205941025 cites W2061964942 @default.
• W4205941025 cites W2062982119 @default.
• W4205941025 cites W2066246350 @default.
• W4205941025 cites W2067065753 @default.
• W4205941025 cites W2067310632 @default.
• W4205941025 cites W2072406256 @default.
• W4205941025 cites W2073317346 @default.
• W4205941025 cites W2077899510 @default.
• W4205941025 cites W2080473907 @default.
• W4205941025 cites W2084384119 @default.
• W4205941025 cites W2085824785 @default.
• W4205941025 cites W2091141229 @default.
• W4205941025 cites W2093134505 @default.
• W4205941025 cites W2094738525 @default.
• W4205941025 cites W2106558292 @default.
• W4205941025 cites W2108393730 @default.
• W4205941025 cites W2109033792 @default.
• W4205941025 cites W2110430419 @default.
• W4205941025 cites W2114090211 @default.
• W4205941025 cites W2121420139 @default.
• W4205941025 cites W2122721442 @default.
• W4205941025 cites W2122754752 @default.
• W4205941025 cites W2124745232 @default.
• W4205941025 cites W2125102738 @default.
• W4205941025 cites W2132764903 @default.
• W4205941025 cites W2135174380 @default.
• W4205941025 cites W2135649770 @default.
• W4205941025 cites W2136853825 @default.
• W4205941025 cites W2137265970 @default.
• W4205941025 cites W2138032498 @default.
• W4205941025 cites W2140711491 @default.
• W4205941025 cites W2147968749 @default.
• W4205941025 cites W2157284909 @default.
• W4205941025 cites W2214119209 @default.
• W4205941025 cites W2228360033 @default.
• W4205941025 cites W2246663975 @default.
• W4205941025 cites W2258584306 @default.
• W4205941025 cites W2387870873 @default.
• W4205941025 cites W2461964469 @default.
• W4205941025 cites W2468373643 @default.
• W4205941025 cites W2493986552 @default.
• W4205941025 cites W2523357503 @default.
• W4205941025 cites W2529511279 @default.
• W4205941025 cites W2530366902 @default.
• W4205941025 cites W2558175491 @default.
• W4205941025 cites W2581376877 @default.
• W4205941025 cites W2591722275 @default.
• W4205941025 cites W2619383416 @default.
• W4205941025 cites W2764217388 @default.
• W4205941025 cites W2792953013 @default.
• W4205941025 cites W2798926193 @default.

• next