实现宏观高重子密度物质的最佳碰撞能量

Hidetoshi Taya, Asanosuke Jinno, Masakiyo Kitazawa, Yasushi Nara
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引用次数: 0

摘要

我们研究了重离子碰撞中产生的高重子密度物质的体积和寿命,并估计了在大时空体积上实现高重子密度区域的最佳碰撞能量。我们用微观输运模型JAM模拟了每核子对质量中心能量$\sqrt{s_{NN}}=2.4 - 19.6\;{\rm GeV}$的金离子中心碰撞。我们发现,最佳碰撞能量大约为$\sqrt{s_{NN}}=3 - 4\;{\rm GeV}$,在这里,重子密度超过了正常核密度的三倍,而空间时间体积却非常大。更高和更低的能量分别由于寿命短和密度低而不受欢迎。我们还指出,时空密度曲线的逐个事件波动很大,这表明事件选择在实验分析中的重要性。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Optimal collision energy for realizing macroscopic high baryon-density matter
We investigate the volume and lifetime of the high baryon-density matter created in heavy-ion collisions and estimate the optimal collision energy to realize the high baryon-density region over a large spacetime volume. We simulate central collisions of gold ions for the center-of-mass energy per nucleon pair $\sqrt{s_{NN}}=2.4 - 19.6\;{\rm GeV}$ with a microscopic transport model JAM. We discover that the optimal collision energy is around $\sqrt{s_{NN}}=3 - 4\;{\rm GeV}$, where a baryon density exceeding three times the normal nuclear density is realized with a substantially large spacetime volume. Higher and lower energies are disfavored due to short lifetime and low density, respectively. We also point out that event-by-event fluctuations of the spacetime density profile are large, indicating the importance of the event selection in the experimental analysis.
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