Before recombination, tight coupling makes photons and baryons share an adiabatic perturbation. Since and only radiation supplies appreciable pressure,Thus the photon-baryon sound speed isBecause and ,After cosmological recombination, baryons decouple from radiation; for adiabatically cooling nonrelativistic gas, and .
The Comoving Jeans length isDuring radiation domination , so . During matter domination before recombination, and , so is approximately constant. Recombination causes a sharp downward jump in sound speed, after which . The requested log-log sketch therefore rises with slope one, reaches a plateau after equality, drops at recombination, and then declines with slope .
For collisionless particles, replace by their one-dimensional velocity dispersion :For a thermally produced cold relic, identify four epochs:
- while coupled and relativistic, and in radiation domination;
- after decoupling but while still relativistic, momentum redshifts but speed remains near , so the same scaling continues with collisionless free streaming;
- after becoming nonrelativistic but before equality, and , giving ;
- after equality, and , giving .
Its plot rises through the two relativistic epochs, turns onto a plateau at the nonrelativistic transition, and falls after equality. Recombination does not dynamically affect collisionless dark matter.
Treat the Milky Way and M31 as a radial Kepler orbit of total mass . At maximum separation the radial speed vanishes, so conservation of energy givesPut . Substitution into the energy equation and integration from the Big Bang gives the cycloidal orbitSince ,Differentiating the parametric solution givesEliminating numerically gives the stated accurate fit
A remote dwarf sees the Local Group primarily through its total monopole mass, so the same radial timing relation applies with its own . Dimensional consistency requiresrather than the cube-root exponent printed in the converted statement. Let . At the zero-velocity radius , and . For the dwarf, . Since ,Therefore
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