Context. The high degree of deuteration observed in some prestellar cores depends on the ortho-to-para H 2 ratio through the H + 3 fractionation. Aims. We want to constrain the ortho/para H 2 ratio across the L183 prestellar core. This is required to correctly describe the deuteration amplification phenomenon in depleted cores such as L183 and to relate the total (ortho+para) H 2 D + abundance to the sole ortho-H 2 D + column density measurement. Methods. To constrain this ortho/para H 2 ratio and derive its profile, we make use of the N 2 D + /N 2 H + ratio and of the ortho-H 2 D + observations performed across the prestellar core. We use two simple chemical models limited to an almost totally depleted core description. New dissociative recombination and trihydrogen cation-dihydrogen reaction rates (including all isotopologues) are presented in this paper and included in our models. Results. We estimate the H 2 D + ortho/para ratio in the L183 cloud, and constrain the H 2 ortho/para ratio: we show that it varies across the prestellar core by at least an order of magnitude, being still very high (≈0.1) in most of the cloud. Our time-dependent model indicates that the prestellar core is presumably older than 1.5−2 × 10 5 years but that it may not be much older. We also show that it has reached its present density only recently and that its contraction from a uniform density cloud can be constrained. Conclusions. A proper understanding of deuteration chemistry cannot be attained without taking into account the whole ortho/para family of molecular hydrogen and trihydrogen cation isotopologues as their relations are of utmost importance in the global scheme. Tracing the ortho/para H 2 ratio should also place useful constraints on the dynamical evolution of prestellar cores.
Numerical calculations of vibrational levels of alkali dimers close to the dissociation limit are developed in the framework of a Fourier Grid Hamiltonian method. The aim is to interpret photoassociation experiments in cold atom samples. In order to avoid the implementation of very large grids we propose a mapping procedure adapted to the asymptotic R Ϫn behavior of the long-range potentials. On a single electronic potential, this allows us to determine vibrational wave functions extending up to 500a 0 using a minimal number of grid points. Calculations with two electronic states, A 1 ⌺ u ϩ and b 3 ⌸ u states, both correlated to the Rb(5s)ϩRb(5 p) dissociation limit, coupled by fine structure are presented. We predict strong perturbation effects in the Rb 2 (0 u ϩ ͒ spectrum, manifested under the 5s, 5p 2 P 1/2 dissociation limit by an oscillatory behavior of the rotational constants.
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