An Introduction to Modern Astrophysics · Problem 12.5

Main-Sequence and Post-Main-Sequence Stellar Evolution — Carroll & Ostlie

Physics — Astrophysics · molecular-cloud-collision-rate

Problem

Using an approach analogous to the development of Eq. (10.29) for nuclear reaction rates, make a crude estimate of the number of random collisions per cubic meter per second between CO and H2_2 molecules in a giant molecular cloud that has a temperature of 15 K and a number density of nH2=108n_{\mathrm{H}_2} = 10^8 m−3^{-3}. Assume (incorrectly) that the molecules are spherical in shape with radii of approximately 0.1 nm, the characteristic size of an atom.

Related theory

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