Rate coefficients for dielectronic recombination of N-like Ne

Dielectronic recombination (DR) for the process Ne$^{3+}$ + e$^{-}$ $\rightarrow$ Ne$^{2+}$ was investigated in a merged-beams arrangement at the heavy-ion storage ring CRYRING@ESR.

The energy-dependent DR rate coefficient, $\alpha(E)$ was measured over the electron-ion collision energy range from 0 to 25 eV.

The measurements cover the complete set of DR resonance series associated with $2s\to2p$ core excitations.

The primary ion beam is estimated to have consisted of $44\%$ of the ions in the ground state, with the remainder distributed among long-lived metastable levels.

In addition to the measurements we carried out quantum mechanical calculations of DR cross sections.

The theoretical treatment includes contributions from the ground and excited metastable initial levels, weighted according to the estimated beam composition.

From the experimental energy-resolved spectra, we derive a temperature dependent DR plasma recombination rate coefficient $\alpha_\mathrm{exp}(T)$ (PRRC).

In the temperature domain where Ne$^{3+}$ is abundant in collisionally ionized plasmas, the present results show a good agreement with the present and with previous theoretical predictions.

In the low-temperature regime characteristic for photoionized plasmas, the experimentally derived DR plasma rate coefficient is slightly larger than the published theoretical ones and does not agree within the experimental uncertainties.

Parametrized fits of the experimentally derived DR PRRC are presented in order to facilitate an easy inclusion into astrophysical modelling codes.