How do weak interactions maintain thermal equilibrium in the early universe?

Question

When reading about why SM neutrinos are not a candidate for DM, it was stated:
"Neutrinos are involved in weak interactions that keep them in thermal equilibrium in the early Universe down to the temperatures of few MeV."
A similar statement can be found here.
I don't understand how these interactions could maintain a thermal equilibrium. Could someone give me an example of such an interaction?
My "guess" is that in a weak interaction, such as $mu^- + W^+ to nu_mu$ this would be exothermal and release heat to compensate the clear mass difference between the neutrino (lighter) and the other SM particles.
But to keep an equilibrium wouldn't there need to be isothermic interactions? How could this be done if neutrinos don't decay?

anna v · Answer

You have  to give the time in the early universe. Before the electroweak symmetry breaking mechanism is activated as the universe cools, all particles in the standard model are massless, so there are no decays, just interactions.  As the neutrinos are neutral and do not interact with gluons, only the weak interaction could give rise to the energy loss or increase of neutrino energies due to scatterings.

I don't understand how these interactions could maintain a thermal equilibrium.

The term "thermal" implies that thermodynamics is used in modeling the neutrinos during this epoch, like an ideal gas the scatterings happening with the weak interaction.

How do weak interactions maintain thermal equilibrium in the early universe?

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