APPENDIX Z: THE STANDARD MODEL OF NCNG UNIVERSAL CONSTANTS
Standard model 10/1/2023
This list is a work in progress, and it will depend upon internal constraints and observations that are not suspect. The model of 10/1/2023 is the first version based on plausible constraints and some reliable observations. There are more than a thousand equations in this document and some of them create a framework of internal constraints. Thus, the 43 values below are not independent. Examples of an internal constraint are Eq. (2.25) or Eq. (5.7).
Our ability to make observations about winter will always be extremely limited. One must rely on plausible requirements during the transitions.
Five symbols below have no model value. Three control the magnitude of energy density for the apex and epoch fields relative to the energy density of matter—unknown but must be very large. Two are related to summer values via Eq. (7.8) for use in RN.
| Symbol | Association | Appears at | Model Value | Dimensions |
|---|---|---|---|---|
| \(L_{ax}\) | apex field | Eq. (2.3) | 9.0 | \(10^9\) LY |
| \(d_1^{ax}\) | apex field | Eq. (2.24) | 1.400253 | |
| \(d_2^{ax}\) | apex field | Eq. (2.24) | -0.9284 | |
| \(d_3^{ax}\) | apex field | Eq. (2.24) | 0.473062 | |
| \(\mathcal{N}_{ax}\) | apex field | Eq. (2.2) | ||
| \(\alpha_W^{ax}\) | apex field | Eq. (2.24) | 0.03 | |
| \(L_{ep}\) | epoch field | Eq. (2.10) | meters | |
| \(\mathcal{N}_{ep}\) | epoch field | Eq. (2.10) | ||
| \(\lambda_{ep}\) | epoch field | Eq. (2.12) | -0.013232 | |
| \(\beta_{ep}\) | epoch field | Eq. (2.12) | 0.25 | |
| \(\Gamma_{ep}\) | epoch field | Eq. (2.12) | 55700 | |
| \(a_{ep}\) | epoch field | Eq. (2.11) | 0.35 | |
| \(A_{ep}\) | epoch field | Eq. (2.12) | 0.99936 | |
| \(\beta_{cl}\) | clock | Eq. (3.29) | 118 | |
| \(\kappa_{cl}\) | clock | Eq. (3.29) | 0.1 | |
| \(\Gamma_{cl}\) | clock | Eq. (3.29) | 10 | |
| \(N_q\) | NG | Eq. (4.1) | 5 | |
| \(L_{g1}\) | NG | Eq. (4.1) | 1.118 | \(10^6\) LY |
| \(Z_{g1}\) | NG | Eq. (4.1) | -657 | |
| \(Z_{g2}\) | NG | Eq. (4.1) | 960 | |
| \(Z_{g3}\) | NG | Eq. (4.1) | -405.1 | |
| \(Z_{g4}\) | NG | Eq. (4.1) | 110 | |
| \(Z_{g5}\) | NG | Eq. (4.1) | -6.9 | |
| \(Q(1,1)\) | NG | Eq. (5.9) | 1 | |
| \(Q(2,1)\) | NG | Eq. (5.9) | 1.30832 | |
| \(Q(3,1)\) | NG | Eq. (5.9) | 0.99091 | |
| \(Q(4,1)\) | NG | Eq. (5.9) | -1.59420 | |
| \(Q(5,1)\) | NG | Eq. (5.9) | 0 | |
| \(\Gamma_{SL}\) | Strong limit | Eq. (6.10) | >>1 | |
| \(\varepsilon_{SL}\) | Strong limit | Eq. (6.12) | 0.487 | |
| \(\gamma_{SL}\) | Strong limit | Eq. (6.12) | \(2.8\times10^{-7}\) | |
| \(\delta_{SL}\) | Strong limit | Eq. (6.12) | 0.95 | |
| \(\alpha_{SL}\) | Strong limit | Eq. (6.12) | -1.9 | |
| \(N_{RN}\) | RN | Eq. (7.2) | 0.25 | meters\(^{-3}\) |
| \(\vartheta_{RN}\) | RN | Eq. (7.2) | 0.125 | |
| \(m_{\nu e}^W\) | RN | Eq. (7.4) | 30 | MeV |
| \(m_W^W\) | RN | Eq. (7.4) | MeV | |
| \(g_W^W\) | RN | Eq. (7.4) | \(g_W^S\) | |
| \(x_{Bera}\) | Bubble era | II(C) | \(10^{-5}\) | |
| \(\Gamma_W\) | Weak changes | Eq. (7.4) | 10000 | |
| \(E_W\) | Weak changes | Eq. (7.4) | 0.013 | |
| \(\Gamma_G\) | Gravity changes | Eq. (7.5) | 10000 | |
| \(E_G\) | Gravity changes | Eq. (7.5) | 0.015 |