Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011phrvl.107b3201h&link_type=abstract
Physical Review Letters, vol. 107, Issue 2, id. 023201
Astronomy and Astrophysics
Astrophysics
3
Chemical Reactions, Energy Disposal, And Angular Distribution, As Studied By Atomic And Molecular Beams, Quantum Theory Of Reaction Cross Section, Rate Constants, Reaction Cross Sections, And Activation Energies, Molecular And Chemical Processes And Interactions
Scientific paper
We report extensive, accurate fully quantum, time-independent calculations of cross sections at low collision energies, and rate coefficients at low temperatures for the H++H2(v=0,j)→H++H2(v=0,j') reaction. Different transitions are considered, especially the ortho-para conversion (j=1→j'=0) which is of key importance in astrophysics. This conversion process appears to be very efficient and dominant at low temperature, with a rate coefficient of 4.15×10-10cm3molecule-1s-1 at 10 K. The quantum mechanical results are also compared with statistical quantum predictions and the reaction is found to be statistical in the low temperature regime (T<100K).
Faure Alex
Gonzalez-Lezana T.
Honvault Pascal
Jorfi M.
Pagani Laurent
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