We employ a coalescence model to form deuterons (), tritons () and helium-3 () nuclei from a uniformly distributed volume of protons ({\rm p}) and neutrons ({\rm n}). We study the ratio of light nuclei yields as a function of the neutron density fluctuations. We investigate the effect of finite transverse momentum () acceptance on the ratio, in particular, the “extrapolation factor” () for the ratio as functions of the spectral shape and the magnitude of neutron density fluctuations. It is found that is monotonic in spectra “temperature” parameter and neutron density fluctuation magnitude; variations in the latter are relatively small. We also examine in realistic simulations using kinematic distributions of protons measured in heavy ion collision data. It is found that is smooth and monotonic as a function of beam energy. We conclude that extrapolation from limited ranges would not create, enhance, or reduce a local peak of the ratio in beam energy. Our study provides a necessary benchmark for light nuclei ratios as a probe of nucleon density fluctuations, an important observable in the search for the critical point of nuclear matter.

生成讲解博客的中文版本

生成AI智能校验的中文版本