Charge exchange of N/3 plus/ ions with atomic hydrogen in the interstellar gas

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

18

Atomic Collisions, Charge Exchange, Hydrogen Atoms, Interstellar Gas, Ion Atom Interactions, Nitrogen, Astronomical Models, Graphs (Charts), Interstellar Matter, Ion Charge, Tables (Data)

Scientific paper

The cross section for the N(3 plus)-H charge exchange reaction is calculated within the framework of the molecular model of atomic collisions. The potential energy curves of the NH(3 plus) molecular ion are determined by a model potential method. The scattering equations describing the collision are derived in a fully quantal approach and solved to obtain the S-matrix. For temperatures less than 400 K, the reaction rate remains fairly constant of the order of 2-3 x 10 to the -10 cu cm/s (a minimum of 2 x 10 to the -10 cu cm/s occurs at 300 K). For temperatures exceeding 400 K the reaction rate increases with T, attaining 8 x 10 to the -9 cu cm/s at 30,000 K.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Charge exchange of N/3 plus/ ions with atomic hydrogen in the interstellar gas does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Charge exchange of N/3 plus/ ions with atomic hydrogen in the interstellar gas, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Charge exchange of N/3 plus/ ions with atomic hydrogen in the interstellar gas will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1817273

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.