An Albert algebra description of the horizon yields a Volterra memory law on the Reissner-Nordstrom evaporation trajectory whose spectral overlap reconstructs the Page curve envelope without restoring standard AMPS tensor factorization.
(V.21), the source-fixed action has the near- extremal expansion S∗(E) =µE+ν √ E+c 3/2E3/2 +O(E 2), c3/2 = 5 √ 2π 4 √ Q0
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Albertian Channel Memory in Black-Hole Evaporation
An Albert algebra description of the horizon yields a Volterra memory law on the Reissner-Nordstrom evaporation trajectory whose spectral overlap reconstructs the Page curve envelope without restoring standard AMPS tensor factorization.