Revisiting the effect of H2, HD and LiH molecules in the cooling of primordial gas
| dc.creator | Prieto, Joaquin P. | |
| dc.creator | Infante, Leopoldo | |
| dc.creator | Jimenez, Raul | |
| dc.date | 2008-09-16 | |
| dc.date | 2009-02-13 | |
| dc.date.accessioned | 2026-07-07T12:40:49Z | |
| dc.date.available | 2026-07-07T12:40:49Z | |
| dc.description | We use a non-equilibrium chemical network to revisit and study the effect of H_{2}, HD and LiH molecular cooling on a primordial element of gas. We solve both the thermal and chemical equations for a gas element with an initial temperature T\approx 1000K and a gas number density in the range n_{tot}=1-10^{4} cm^{-3}. At low densities, n_{tot}<10^{2} cm^{-3}, the gas reaches temperatures \sim 100K and the main coolant is H_{2}, but at higher densities, n_{tot}>10^{2} cm^{-3}, the HD molecule dominates the gas temperature evolution. The effect of LiH is negligible in all cases. We studied the effect of D abundance on the gas cooling. The D abundance was set initially to be in the range n_{D}/n_{H}=10^{-7}-10^{-4.5}, with n_{HD}/n_{H}={D^{+}}/n_{H}=10^{-10}. The simulations show that at n_{tot}>10^{2} cm^{-3} the HD cooling dominates the temperature evolution for D abundances greater than 10^{-5}n_{H}. This number decrease at higher densities. Furthermore, we studied the effect of electrons and ionized particules on the gas temperature. We followed the gas temperature evolution with n_{H_{+}}/n_{H}=10^{-4}-10^{-1} and n_{D^{+}}/n_{H^{+}}=10^{-5}. The gas temperature reached lower values at high ionization degree because electrons, H^{+} and D^{+} are catalizers in the formation paths of the H_{2} and HD molecules, which are the main coolers at low temperatures. Finaly, we studied the effect of an OB star, with T_{eff}=4\times 10^{4}K, would have on gas cooling. It is very difficult for a gas with n_{tot} in the range between 1-100 cm^{-3} to drop its temperature if the star is at a distance less than 100 pc. | |
| dc.identifier | https://arxiv.org/abs/0809.2786 | |
| dc.identifier | http://arxiv.org/abs/0809.2786 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/219563 | |
| dc.subject | Astrophysics | |
| dc.title | Revisiting the effect of H2, HD and LiH molecules in the cooling of primordial gas | |
| dc.type | text |