IndisputableMonolith.Cosmology.EntropyPerPhoton
Defines the standard-model bookkeeping constants for cosmological entropy density: photon, electron, and neutrino internal degrees of freedom, the 7/8 fermion weight, pre/post e⁺e⁻ annihilation g-factors, the (4/11) neutrino dilution cube, g_*s = 43/11, and ζ(3). Cosmologists deriving η_γ, N_eff, or T_ν/T_γ cite these as the MODEL layer. The module is definitional; identities such as dilutionCubed_eq and gStarS_eq are algebraic equalities, not deep proofs.
claimFix the internal dof $g_\gamma=2$, $g_e=4$, $g_\nu=6$, the fermion entropy weight $7/8$, and the effective counts $g_{\mathrm{before}}=2+\frac78(4+6)$, $g_{\mathrm{after}}=2+\frac78\cdot 6$. Set the dilution cube $(T_\nu/T_\gamma)^3=4/11$ and $g_{*s}=43/11$, and record $\zeta(3)=\sum_{n\ge1}n^{-3}$ as a summable series used in number-density integrals.
background
In early-universe thermodynamics the entropy density of a relativistic species is $s=(2\pi^2/45)g_{*s}T^3$, with $g_{*s}$ an effective count of bosonic and fermionic degrees of freedom. Photons contribute $g_\gamma=2$ (two helicities). Electrons and positrons together contribute $g_e=4$; three neutrino species (left-handed, plus antineutrinos) contribute $g_\nu=6$. Fermions enter with a weight $7/8$ relative to bosons because the Fermi–Dirac energy integral is $7/8$ of the Bose–Einstein one.
Before $e^+e^-$ annihilation the full relativistic content is $g_{\mathrm{before}}=g_\gamma+(7/8)(g_e+g_\nu)$; afterward only photons and neutrinos remain, so $g_{\mathrm{after}}=g_\gamma+(7/8)g_\nu$. Entropy conservation then forces the neutrino temperature to dilute relative to the photon bath by $(T_\nu/T_\gamma)^3=g_{\mathrm{after}}/g_{\mathrm{before}}=4/11$, and the present-day $g_{*s}$ becomes $43/11$. The Riemann value $\zeta(3)$ appears in the number-density integrals that convert energy densities into particle counts per photon.
This module records those constants as MODEL inputs. Downstream modules discharge the $7/8$ weight and the dilution law from series and FRW identities.
proof idea
Definition module: no substantive proofs. Constants gPhoton, gElectron, gNeutrino, and fermionWeight are numeric MODEL inputs. gBefore and gAfter are arithmetic combinations of those inputs. dilutionCubed_eq and gStarS_eq are one-line algebraic rewrites equating the named symbols to the rationals $4/11$ and $43/11$. zeta3 is the series $\sum n^{-3}$ with a summability certificate zeta3_summable imported from Mathlib.
why it matters in Recognition Science
This is the MODEL layer that every entropy-per-photon identity in the Cosmology stack imports. FermionWeight upgrades the bare fermionWeight = 7/8 input to the series identity $\eta(4)=(7/8)\zeta(4)$; FermionWeightIntegral lifts that to the thermodynamic Fermi–Dirac versus Bose–Einstein energy integrals. NumberDensityIntegral closes the $s=3$ number-density layer (including the $3/4$ fermion weight) that feeds entropyPerPhoton_eq_ratio. NeutrinoDilution turns dilutionCubed and gStarS into theorems $(T_\nu/T_\gamma)^3=4/11$ and $g_{*s}=43/11$ once comoving entropy conservation and the $1/a$ redshift law are discharged from the FRW continuity equation.
Without these named constants the later modules would have nowhere to attach their discharges. In the broader Recognition framework they sit in the cosmology bookkeeping that connects the eight-tick and $\phi$-ladder structure to observable $N_{\mathrm{eff}}$ and baryon-to-photon ratios, but the present file itself is pure Standard-Model thermodynamics.
scope and limits
- Does not derive the 7/8 fermion weight; that is discharged in FermionWeight and FermionWeightIntegral.
- Does not prove neutrino dilution or g_*s from FRW; NeutrinoDilution and EntropyConservationFRW do.
- Does not evaluate number-density or energy-density integrals; those live in NumberDensityIntegral.
- Does not claim RS-native forcing of g_γ, g_e, or g_ν; they remain MODEL inputs.
- Does not address non-equilibrium or beyond-Standard-Model entropy sources.
used by (4)
declarations in this module (43)
-
def
gPhoton -
def
gElectron -
def
gNeutrino -
def
fermionWeight -
def
gBefore -
def
gAfter -
def
dilutionCubed -
theorem
dilutionCubed_eq -
def
gStarS -
theorem
gStarS_eq -
def
zeta3 -
lemma
zeta3_summable -
lemma
tail_summable -
lemma
zeta3_split -
def
gLo -
lemma
gLo_nonneg -
lemma
gLo_tendsto -
lemma
gLo_step -
lemma
gLo_antitone -
lemma
hasSum_gLo -
lemma
term_lo -
lemma
tail_ge -
def
gHi -
lemma
gHi_tendsto -
lemma
gHi_step -
lemma
gHi_antitone -
lemma
hasSum_gHi -
lemma
term_hi -
lemma
tail_le -
lemma
S40_gt -
lemma
S40_lt -
theorem
zeta3_gt -
theorem
zeta3_lt -
theorem
zeta3_pos -
theorem
pi4_gt -
theorem
pi4_lt -
def
entropyPerPhoton -
theorem
entropyPerPhoton_eq_formula -
theorem
entropyPerPhoton_eq_ratio -
theorem
entropyPerPhoton_gt -
theorem
entropyPerPhoton_lt -
theorem
entropyPerPhoton_pos -
theorem
entropyPerPhoton_near_704