2025MNRAS.542.2377M


Query : 2025MNRAS.542.2377M

2025MNRAS.542.2377M - Mon. Not. R. Astron. Soc., 542, 2377-2388 (2025/September-3)

Photoionization study of simple organic compounds using the R-matrix method.

MAHLA S. and ANTONY B.

Abstract (from CDS):

R-matrix calculations using the Quantemol-N expert system on the photoionization of acetylene, ethylene, methanol, and dimethyl ether for photon energies ranging from near-threshold to 40 eV were performed and reported here. Partial low-energy photoionization cross-sections have been calculated for ionization out of the two outermost valence orbitals ($1\pi _u$ and $3\sigma _g$) leading to the $\mathrm{X}^2 \mathit{\Pi _u}$ and $\mathrm{A}^2 \mathit{\Sigma _g^{+}}$ states of the $\mathrm{C}_2 \mathrm{H}_2^{+}$ ion, four valence orbitals ($1b_{3u}$, $1b_{3g}$, $3a_{g}$, and $1b_{2u}$) corresponding to the $\mathrm{X}^{2} \mathrm{B}_{3u}$, $\mathrm{A}^{2} \mathrm{B}_{3g}$, $\mathrm{B}^{2} \mathrm{A}_{g}$, and $\mathrm{C}^{2} \mathrm{B}_{2u}$ states of the $\mathrm{C}_2 \mathrm{H}_4^{+}$ ion, four ionic states $\left(2 a^{\prime \prime -1}\right) { }^2 \mathrm{A}^{\prime \prime }$, $\left(7 a^{\prime -1}\right) { }^2 \mathrm{A}^{\prime }$, $\left(6 a^{\prime -1}\right) { }^2 \mathrm{A}^{\prime }$, and $\left(1 a^{\prime \prime -1}\right) { }^2 \mathrm{A}^{\prime \prime }$ of $\mathrm{CH}_3 \mathrm{OH}$, and at last exclusively for the ionization from the first valence orbital ($2b_1$) of dimethyl ether. We have presented high-resolution cross-section data near the photoionization threshold for the first time. These cross-sections are computed by incorporating electron correlation effects and large resonance structures, which have not been included in previous studies. We also did the calculations using different active spaces and target states to see if the current results were consistent and how they changed when the model was changed. Our best results, compared with available experimental and theoretical data, find reasonable agreement that confirms the reliability of our calculations. It is worth noting that previous studies have not fully accounted for autoionization, multichannel coupling, and correlation-polarization, which may be the reason for the slight variations in the results.

Abstract Copyright: © The Author(s) 2025. Published by Oxford University Press on behalf of Royal Astronomical Society.

Journal keyword(s): molecular data - molecular processes - radiation mechanisms: general - scattering - methods: numerical

Simbad objects: 9

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Number of rows : 9
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NAME W3 IRS 5 Y*O 02 25 40.54 +62 05 51.4           B1 367 0
2 TMC-1 MoC 04 41 45.9 +25 41 27           ~ 1872 0
3 NAME OMC-1 MoC 05 35 14 -05 22.4           ~ 1249 2
4 [RLK73] IRc 2 IR 05 35 14.51548 -05 22 30.5943           ~ 673 1
5 NAME Orion Molecular Cloud MoC 05 56 -01.8           ~ 1227 1
6 IRC +10216 C* 09 47 57.40632 +13 16 43.5648           C9,5e 2455 0
7 IRAS 16293-2422 cor 16 32 22.56 -24 28 31.8           ~ 1357 1
8 NAME Sgr B2 MoC 17 47 20.4 -28 23 07           ~ 2443 1
9 RAFGL 2591 Y*O 20 29 24.8230 +40 11 19.590           ~ 640 0

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