01612nas a2200229   4500008004100000022001400041245009200055210006900147260000900216300001100225490000600236520083200242653003301074653002601107653003001133653004001163653002801203100002501231700001501256700001701271856009401288       2021                        eng d  a2296-264600aInsights into chemical reactions at the beginning of the universe: from HeH+ to H-3 (+)0 aInsights into chemical reactions at the beginning of the univers  cJUN   a6797500 v93 aAt the dawn of the Universe, the ions of the light elements produced in the Big Bang nucleosynthesis recombined with each other. In our present study, we have tried to mimic the conditions in the early Universe to show how the recombination process would have led to the formation of the first ever formed diatomic species of the Universe: HeH+, as well as the subsequent processes that would have led to the formation of the simplest triatomic species: H-3 (+). We have also studied some special cases: higher positive charge with fewer number of hydrogen atoms in a dense atmosphere, and the formation of unusual and interesting linear, dicationic He chains beginning from light elements He and H in a positively charged atmosphere. For all the simulations, the ab initio nanoreactor (AINR) dynamics method has been employed.10aab initio molecular dynamics10aab initio nanoreactor10aDensity functional theory10aorigin of molecules in the universe10athe earliest lewis acid1 aDash, Soumya, Ranjan1 aDas, Tamal1 aVanka, Kumar  uhttps://library.ncl.res.in/content/insights-chemical-reactions-beginning-universe-heh-h-3