ExoMol line lists -- LX. Molecular line list for the ammonia isotopologue $^{15}$NH$_3$

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Hauptverfasser: Yurchenko, Sergei N., Bowesman, Charles A., Brady, Ryan P., Guest, Elizabeth R., Kefala, Kyriaki, Mitev, Georgi B., Owens, Alec, Perri, Armando N., Pezzella, Marco, Smola, Oleksiy, Sokolov, Andrei, Zhang, Jingxin, Tennyson, Jonathan
Format: Preprint
Veröffentlicht: 2024
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author Yurchenko, Sergei N.
Bowesman, Charles A.
Brady, Ryan P.
Guest, Elizabeth R.
Kefala, Kyriaki
Mitev, Georgi B.
Owens, Alec
Perri, Armando N.
Pezzella, Marco
Smola, Oleksiy
Sokolov, Andrei
Zhang, Jingxin
Tennyson, Jonathan
author_facet Yurchenko, Sergei N.
Bowesman, Charles A.
Brady, Ryan P.
Guest, Elizabeth R.
Kefala, Kyriaki
Mitev, Georgi B.
Owens, Alec
Perri, Armando N.
Pezzella, Marco
Smola, Oleksiy
Sokolov, Andrei
Zhang, Jingxin
Tennyson, Jonathan
contents A theoretical line list for $^{15}$NH$_3$ CoYuTe-15 is presented based on the empirical potential energy and ab initio dipole moments surfaces developed and used for the production of the ExoMol line list CoYuTe for $^{14}$NH$_3$. The ro-vibrational energy levels and wavefunctions are computed using the variational program TROVE. The line list ranges up to 10000 cm$^{-1}$ ($λ\geq 1$ $μ$m) and contains 929 795 249 transitions between 1 269 961 states with $J\le 30$. The line list should be applicable for temperatures up to $\sim$1000 K. To improve the accuracy of the line positions, a set of experimentally-derived energy levels of $^{15}$NH$_3$ is produced using the MARVEL procedure. To this end, 37 experimental sources of the line positions of $^{15}$NH$_3$ available in the literature are collected, combined and systematised to produce a self-consistent spectroscopic network of 21095 $^{15}$NH$_3$ transitions covering 40 vibrational bands ranging up to 6818 cm$^{-1}$ and resulting in 2777 energy term values. These MARVEL energies are then used to replace the theoretical values in the CoYuTe-15 line list and also complemented by pseudo-MARVEL energies obtained by an isotopologue extrapolation using the previously reported MARVEL energies of the $^{14}$NH$_3$ parent isotopologue of ammonia. A list of 53856 high resolution transitions between MARVEL states and theoretical intensities is provided in the HITRAN format. Comparison with the recent experimental spectra of $^{15}$NH$_3$ illustrate the potential of the line list for detections and as an efficient assistant in spectroscopic assignments. The line list is available from www.exomol.com.
format Preprint
id arxiv_https___arxiv_org_abs_2410_04295
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle ExoMol line lists -- LX. Molecular line list for the ammonia isotopologue $^{15}$NH$_3$
Yurchenko, Sergei N.
Bowesman, Charles A.
Brady, Ryan P.
Guest, Elizabeth R.
Kefala, Kyriaki
Mitev, Georgi B.
Owens, Alec
Perri, Armando N.
Pezzella, Marco
Smola, Oleksiy
Sokolov, Andrei
Zhang, Jingxin
Tennyson, Jonathan
Earth and Planetary Astrophysics
Astrophysics of Galaxies
Instrumentation and Methods for Astrophysics
A theoretical line list for $^{15}$NH$_3$ CoYuTe-15 is presented based on the empirical potential energy and ab initio dipole moments surfaces developed and used for the production of the ExoMol line list CoYuTe for $^{14}$NH$_3$. The ro-vibrational energy levels and wavefunctions are computed using the variational program TROVE. The line list ranges up to 10000 cm$^{-1}$ ($λ\geq 1$ $μ$m) and contains 929 795 249 transitions between 1 269 961 states with $J\le 30$. The line list should be applicable for temperatures up to $\sim$1000 K. To improve the accuracy of the line positions, a set of experimentally-derived energy levels of $^{15}$NH$_3$ is produced using the MARVEL procedure. To this end, 37 experimental sources of the line positions of $^{15}$NH$_3$ available in the literature are collected, combined and systematised to produce a self-consistent spectroscopic network of 21095 $^{15}$NH$_3$ transitions covering 40 vibrational bands ranging up to 6818 cm$^{-1}$ and resulting in 2777 energy term values. These MARVEL energies are then used to replace the theoretical values in the CoYuTe-15 line list and also complemented by pseudo-MARVEL energies obtained by an isotopologue extrapolation using the previously reported MARVEL energies of the $^{14}$NH$_3$ parent isotopologue of ammonia. A list of 53856 high resolution transitions between MARVEL states and theoretical intensities is provided in the HITRAN format. Comparison with the recent experimental spectra of $^{15}$NH$_3$ illustrate the potential of the line list for detections and as an efficient assistant in spectroscopic assignments. The line list is available from www.exomol.com.
title ExoMol line lists -- LX. Molecular line list for the ammonia isotopologue $^{15}$NH$_3$
topic Earth and Planetary Astrophysics
Astrophysics of Galaxies
Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2410.04295