Fig. 6
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Demanding a lower value of 100 for γej (Zhang & Kobayashi 2005), Eq. (46) provides an upper limit for 
. The requirement that the total pressure generated by the FS be stronger than the total pressure of the ejecta significantly lowers the value of this upper limit. Depending on the ratio between the unshocked CBM and ejecta baryon number densities, this upper limit can realistically range from 𝒪(l02) to 𝒪(101).
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