2008
DOI: 10.1007/978-3-540-74203-6_7
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7 Relativistic Nucleus-Nucleus Collisions and the QCD Matter Phase Diagram

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Cited by 5 publications
(9 citation statements)
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“…It was the experience with astrophysical objects like supernovae and neutron stars, and with thermonuclear ignition which led the authors to the idea that the nuclear matter shock compression [31] of about five-fold normal nuclear density should be accomplished in violent head-on collisions of heavy nuclei [11]. The goal was to find out the response of the nuclear medium under compression by pressure resisting that compression; i.e., to study the nuclear matter EoS.…”
Section: Heavy Ion Acceleratorsmentioning
confidence: 99%
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“…It was the experience with astrophysical objects like supernovae and neutron stars, and with thermonuclear ignition which led the authors to the idea that the nuclear matter shock compression [31] of about five-fold normal nuclear density should be accomplished in violent head-on collisions of heavy nuclei [11]. The goal was to find out the response of the nuclear medium under compression by pressure resisting that compression; i.e., to study the nuclear matter EoS.…”
Section: Heavy Ion Acceleratorsmentioning
confidence: 99%
“…The particle physics community began to adapt existing high-energy proton accelerators to provide heavy-ion nuclear beams in the mid-1970s. The Berkeley Bevalac and JINR Synchrophasotron started to accelerate nuclei to kinetic energies from few hundreds of MeV to several GeV per nucleon [11,125]. By the mid-1980s, the first ultra-relativistic nuclear beams became available.…”
Section: Heavy Ion Acceleratorsmentioning
confidence: 99%
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