Answers are grounded in this paper and cite their sources.
The neutrino entropy is comparable to, and slightly below, the photon entropy today, and adiabatic transport preserves the ratio through the bounce. If re-coupling occurred at the bounce temperature the background would be reprocessed rather than preserved, which would erase the decoupling signature; the preservation result therefore doubles as a statement about which bounce temperatures are compatible with an intact relic background. The computation is performed from stated assumptions in a density-limited bounce, in which the neutron-branch limit density sets a maximum density, a finite bounce temperature, and a minimum horizon size. Headline values from the deposited calculation are: T_nu_K = 1.95; n_nu_per_m3 = 3.36e+08; S_nu_kB = 3.78e+89; T_bounce_K = 3.28e+22; Tnu_over_Tbounce = 5.93e-23. The study is simulated and computed, not measured, and its conclusions are stated at the precision the stated assumptions support.
No takes yet. Share an insight, caveat, or question.
William Alexander Aldred (2026) studied this question.
Synapse has enriched 8 closely related papers on similar clinical questions. Consider them for comparative context: