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We report quantum-mechanical close-coupling calculations for rotational state resolved cross sections for p-H2+HD collisions. The low temperature limit of p-H2+HD is investigated, which is of significant astrophysical interest in regard to…

化学物理 · 物理学 2015-06-26 Renat A. Sultanov , Dennis Guster

Calculations are performed for electron collision with the methylene molecular ion CH$_2^+$ in its bent equilibrium geometry, with the goal to obtain cross sections for electron impact excitation and dissociation. The polyatomic version of…

等离子体物理 · 物理学 2024-05-22 K. Chakrabarti , J. Zs Mezei , I. F. Schneider , J. Tennyson

Motivated by recent observations with Herschel/PACS, and the availability of new rate coefficients for the collisional excitation of CO (Yang et al. 2010), the excitation of warm astrophysical CO is revisited with the use of numerical and…

星系天体物理 · 物理学 2015-06-04 David A. Neufeld

{\bf R}-matrix calculations combined with the adiabatic nuclei approximation are used to compute electron-impact rotiational excitation rates for three closed-shell diatomic cations, HeH$^+$, CH$^+$, ArH$^+$. Comparisons with previous…

星系天体物理 · 物理学 2015-12-02 James R. Hamilton , Alexandre Faure , Jonathan Tennyson

We analyze the quantum-mechanical rotational excitation/de-excitation spectrum and cross sections of CN molecules during low and high-energy collisions with protons, H+. The problem is of significant importance in astrophysics of the early…

太阳与恒星天体物理 · 物理学 2012-11-27 Madina R. Sultanova , Dennis Guster

Thermal rate coefficients for the astrochemical reaction C + CH$^+$ $\to$ C$_2^+$ + H were computed in the temperature range 20-300 K by using novel rate theory based on ring polymer molecular dynamics (RPMD) on a recently published…

化学物理 · 物理学 2017-02-08 Sergio Rampino , Yury V. Suleimanov

The modelling of emission spectra of molecules seen in interstellar clouds requires the knowledge of collisional rate coefficients. Among the commonly observed species, N$_2$H$^+$ is of particular interest since it was shown to be a good…

星系天体物理 · 物理学 2015-06-23 François Lique , Fabien Daniel , Laurent Pagani , Nicole Feautrier

Theoretical rotational quenching cross sections and rate coefficients of ortho- and para-H$_2$O due to collisions with He atoms are presented. The complete angular momentum close-coupling approach as well as the coupled-states approximation…

太阳与恒星天体物理 · 物理学 2015-06-15 Benhui Yang , M. Nagao , W. Satomi , M. Kimura , P. C. Stancil

Our knowledge about the "cold" Universe often relies on molecular spectra. A general property of such spectra is that the energy level populations are rarely at local thermodynamic equilibrium. Solving the radiative transfer thus requires…

天体物理仪器与方法 · 物理学 2018-01-23 Jérôme Loreau , François Lique , Alexandre Faure

The experimental determination of the reaction rate coefficients for production and destruction of $\text{HCN}^+$ and $\text{HNC}^+$ in collisions with $\text{H}_2$ is presented. A variable temperature 22 pole radio frequency ion trap was…

星系天体物理 · 物理学 2023-06-08 Petr Dohnal , Pavol Jusko , Miguel Jiménez-Redondo , Paola Caselli

A close coupling quantum-mechanical calculation is performed for rotational energy transfer in a HD+HD collision at very low energy, down to the ultracold temperatures: $T \sim 10^{-8}$ K. A global six-dimensional H$_2$-H$_2$ potential…

化学物理 · 物理学 2015-06-03 Renat A. Sultanov , Dennis Guster , S. K. Adhikari

Collisional (de-)excitation of H$_{2}$ by helium plays an important role in the thermal balance and chemistry of various astrophysical environments, making accurate rate coefficients essential for the interpretation of observations of the…

星系天体物理 · 物理学 2024-05-15 Hubert Jóźwiak , Franck Thibault , Alexandra Viel , Piotr Wcisło , François Lique

Rate coefficients for the dissociative recombination, vibrational excitation and vibrational de-excitation of the BeT$^{+}$ ion for all vibrational levels of its ground electronic state ($ X\ensuremath{^{1}\Sigma^{+}},v_{i}^{+}=0,\dots,27$)…

原子物理 · 物理学 2022-03-09 N. Pop , F. Iacob , S. Niyonzima , A. Abdoulanziz , V. Laporta , D. Reiter , I. F. Schneider , J. Zs Mezei

Interstellar aromatic molecules such as polycyclic aromatic hydrocarbons and polycyclic nitrogen and oxygen bearing molecules are thought to be abundant in the interstellar medium. In this class of molecules, benzonitrile ($c$-C$_6$H$_5$CN)…

星系天体物理 · 物理学 2024-01-19 M. Ben Khalifa , J. Loreau

Absolute cross sections for charge exchange, ionization, stripping and excitation in K^(+) - He collisions were measured in the ion energy range 0.7 - 10 keV. The experimental data and the schematic correlation diagrams are used to analyze…

Using a quantum-mechanical close-coupling method, we calculate cross sections for fine structure excitation and relaxation of Si and S atoms in collisions with atomic hydrogen. Rate coefficients are calculated over a range of temperatures…

原子物理 · 物理学 2024-12-10 Pei-Gen Yan , James F. Babb

We measure the energy-differential cross sections for collisional excitation of the soft X-ray electric-dipole K$\alpha$ ($x+y+w$) emission from He-like oxygen (O VII), using an electron beam ion trap. Values near their excitation…

Ammonia is one of the most widely observed molecules in space, and many observations are able to resolve the hyperfine structure due to the electric quadrupole moment of the nitrogen nucleus. The observed spectra often display anomalies in…

星系天体物理 · 物理学 2023-09-06 J. Loreau , A. Faure , F. Lique , S. Demes , P. J. Dagdigian

Cross sections are presented for dissociative recombination and electron-impact vibrational excitation of the ArH+ molecular ion at electron energies appropriate for the interstellar environment. The R-matrix method is employed to determine…

星系天体物理 · 物理学 2018-08-21 A. Abdoulanziz , F. Colboc , D. A. Little , Y. Moulane , J. Zs. Mezei , E. Roueff , J. Tennyson , I. F. Schneider , V. Laporta

Rate coefficients for inelastic Na+H collisions are calculated for all transitions between the ten levels up to and including the ionic state (ion-pair production), namely Na(3s,3p,4s,3d,4p,5s,4d,4f,5p)+H(1s) and Na+ + H-. The calculations…

太阳与恒星天体物理 · 物理学 2015-05-19 P. S. Barklem , A. K. Belyaev , A. S. Dickinson , F. X. Gadea