This analysis reveals exact identities linking neutrino mass, dark energy, and vacuum response, suggesting new insights into quantum gravity.
Abstract (English) We isolate four exact identities that arise within the infrared benchmark defined by rho_DE = kappa_QCD G_N mu_*^6, mu_Lambda = (2 rho_DE)^(1/4), m_1 = y_S mu_Lambda, and M_Pl = (8 pi G_N)^(-1/2). The first relates the lightest neutrino mass to the hadronic scale and the reduced Planck mass, m_1^2 M_Pl = y_S^2 sqrt[kappa_QCD/(4 pi)] mu_*^3. The second eliminates G_N between dark energy and MOND, rho_DE = [sqrt(3 pi kappa_QCD)/(2 c)] mu_*^3 a_0. The third shows that an absolute measurement of m_1, together with an independent determination of y_S, would allow a non-gravitational extraction of G_N within the benchmark. The fourth rewrites the de Sitter entropy as S_dS = 3 kappa_QCD^2 y_S^12 (mu_*/m_1)^12. In addition, if one promotes G_N -> G_eff in a scalar-tensor deformation, the vacuum sector acquires a response coefficient chi_G = (partial rho_vac / partial G_eff)_(kappa, mu_*) = kappa_QCD mu_*^6. We stress that these expressions are exact algebraic corollaries of the benchmark rather than independent derivations of G_N, or identifications between neutrinos and dark energy. Resumen (Español) Aislamos cuatro identidades exactas que aparecen dentro del benchmark infrarrojo definido por rho_DE = kappa_QCD G_N mu_*^6, mu_Lambda = (2 rho_DE)^(1/4), m_1 = y_S mu_Lambda y M_Pl = (8 pi G_N)^(-1/2). La primera relaciona la masa del neutrino más ligero con la escala hadrónica y la masa de Planck reducida, m_1^2 M_Pl = y_S^2 sqrt[kappa_QCD/(4 pi)] mu_*^3. La segunda elimina G_N entre energía oscura y MOND, rho_DE = [sqrt(3 pi kappa_QCD)/(2 c)] mu_*^3 a_0. La tercera muestra que una medida absoluta de m_1, junto con una determinación independiente de y_S, permitiría una extracción no gravitacional de G_N dentro del benchmark. La cuarta reescribe la entropía de de Sitter como S_dS = 3 kappa_QCD^2 y_S^12 (mu_*/m_1)^12. Además, si se promueve G_N -> G_eff en una deformación escalar-tensorial, el sector de vacío adquiere un coeficiente de respuesta chi_G = (partial rho_vac / partial G_eff)_(kappa, mu_*) = kappa_QCD mu_*^6. Subrayamos que estas expresiones son corolarios algebraicos exactos del benchmark y no derivaciones independientes de G_N, ni identificaciones entre neutrinos y energía oscura.
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Miguel Ángel Moreno Barajas (2026) studied this question.
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