Abstract (English) We isolate four exact identities that arise within the infrared benchmark defined by rhoDE = kappaQCD GN mu_*⁶, muLambda = (2 rhoDE) ^ (1/4), m₁ = yS muLambda, and MPl = (8 pi GN) ^ (-1/2). The first relates the lightest neutrino mass to the hadronic scale and the reduced Planck mass, m₁² MPl = yS² sqrtkappaQCD/ (4 pi) mu_*³. The second eliminates GN between dark energy and MOND, rhoDE = sqrt (3 pi kappaQCD) / (2 c) mu_*³ a₀. The third shows that an absolute measurement of m₁, together with an independent determination of yS, would allow a non-gravitational extraction of GN within the benchmark. The fourth rewrites the de Sitter entropy as SdS = 3 kappaQCD² yS¹2 (mu_*/m₁) ¹2. In addition, if one promotes GN -> Gₑff in a scalar-tensor deformation, the vacuum sector acquires a response coefficient chiG = (partial rhoᵥac / partial Gₑff) _ (kappa, mu_*) = kappaQCD mu_*⁶. We stress that these expressions are exact algebraic corollaries of the benchmark rather than independent derivations of GN, or identifications between neutrinos and dark energy. Resumen (Español) Aislamos cuatro identidades exactas que aparecen dentro del benchmark infrarrojo definido por rhoDE = kappaQCD GN mu_*⁶, muLambda = (2 rhoDE) ^ (1/4), m₁ = yS muLambda y MPl = (8 pi GN) ^ (-1/2). La primera relaciona la masa del neutrino más ligero con la escala hadrónica y la masa de Planck reducida, m₁² MPl = yS² sqrtkappaQCD/ (4 pi) mu_*³. La segunda elimina GN entre energía oscura y MOND, rhoDE = sqrt (3 pi kappaQCD) / (2 c) mu_*³ a₀. La tercera muestra que una medida absoluta de m₁, junto con una determinación independiente de yS, permitiría una extracción no gravitacional de GN dentro del benchmark. La cuarta reescribe la entropía de de Sitter como SdS = 3 kappaQCD² yS¹2 (mu_*/m₁) ¹2. Además, si se promueve GN -> Gₑff en una deformación escalar-tensorial, el sector de vacío adquiere un coeficiente de respuesta chiG = (partial rhoᵥac / partial Gₑff) _ (kappa, mu_*) = kappaQCD mu_*⁶. Subrayamos que estas expresiones son corolarios algebraicos exactos del benchmark y no derivaciones independientes de GN, ni identificaciones entre neutrinos y energía oscura.
Miguel Ángel Moreno Barajas (Mon,) studied this question.
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