Calculating the initial energy density in heavy ion collisions by including the finite nuclear thickness
arXiv:2012.13825 · doi:10.1103/PhysRevC.103.024907
Abstract
The initial energy density produced in heavy ion collisions can be estimated with the Bjorken energy density formula after choosing a proper formation time . However, the Bjorken formula breaks down at low energies because it neglects the finite nuclear thickness. Here we include both the finite time duration and finite longitudinal extension of the initial energy production. When is not too much smaller than the crossing time of the two nuclei, our results are similar to those from a previous study that only considers the finite time duration. In particular, we find that at low energies the initial energy density has a much lower maximum value but evolves much longer than the Bjorken formula, while at large-enough and/or high-enough energies our result approaches the Bjorken formula. We also find a qualitative difference in that our maximum energy density at is finite, while the Bjorken formula diverges as and the previous result diverges as at low energies but as at high energies. Furthermore, our solution of the energy density approximately satisfies a scaling relation. As a result, the -dependence of determines the -dependence, and the weaker -dependence of in our results at low energies means a slower increase of with .
arXiv comment10 pages, 8 figures, 1 table; typos in Eq.(19) and Fig.8 corrected; final published version
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