J/A+A/671/A51       Rate coefficients for H2O + H2O collisions   (Mandal+, 2023)

Rate coefficients for rotational state-to-state transitions in H2O + H2O collisions for cometary and planetary applications, as predicted by mixed quantum-classical theory. Mandal B., Babikov D. <Astron. Astrophys. 671, A51 (2023)> =2023A&A...671A..51M 2023A&A...671A..51M (SIMBAD/NED BibCode)
ADC_Keywords: Models ; Comets ; Planets ; Spectra, millimetric/submm Keywords: molecular data - submillimiter: general - comets: general - ISM: molecules - planets and satellites: fundamental parameters - astronomical databases: miscellaneous - comets: general Abstract: We present new calculations of collision cross sections for state-to-state transitions between the rotational states in H2O + H2O system, that are used to generate new database of collisional rate coefficients for cometary and planetary applications. Calculations are carried out using mixed quantum/ classical theory approach implemented in MQCT code. Large basis set of rotational states used in these calculations permits to predict thermally averaged cross sections for 441 transitions in para- and ortho-H2O in a broad range of temperatures. It is found that all state-to-state transitions in H2O + H2O system split onto two well defined groups, one with larger values of cross sections and smaller energy transfer, that corresponds to the dipole-dipole driven processes, are the other with smaller cross sections and larger energy transfer, driven by higher-order interaction terms. Detailed analysis of theoretical error bars is presented, and symmetrization of state-to-state transition matrixes is carried out to ensure that excitation and quenching processes for each transition satisfy the principle of microscopic reversibility. Comparison with other data available from literature for H2O + H2O collisions is also presented. Description: This program calculates Thermally Averaged Cross Sections (TACS) for transitions in H2O + H2O at any given temperature in the range between T=150K and 800K, by numerical qubic spline interpolation between six pre-computed data points. The unit of input temperature is K and the unit of output TACS is Angstrom^2. The driver program is in the file named "Generate_TACS.f90". User needs to indicate the value of temperature by assigning the value of variable "req_temp". The interpolated TACS for all transitions will be printed in the file named "Output_TACS.out". The output file first lists j, ka and kc for the initial state followed by the same for the final state. The TACS are printed at the end of the line. In the "Makefile", user can indicate any standard Fortran compiler. To compile and execute: $ make $ ./compute_tacs File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file Generate_TACS.f90 105 25 Driver program MQCT_TACS.dat 69 5304 Precomputed TACS for 441 transitions at six values of temperature Makefile 33 4 Makefile engines.f90 512 18 Cubic spline interpolation code -------------------------------------------------------------------------------- Acknowledgements: Dmitri Babikov, dmitri.babikov(at)mu.edu
(End) Dmitri Babikov [Marquette University], Patricia Vannier [CDS] 24-Jan-2023
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line