Appendix A · Kitcey 2026 · v5.0.7
Symbol Reference
Comprehensive symbol glossary for the Intrinsic Response framework — spacetime geometry through the Baryonic Tully–Fisher Relation.
11
Sections
93
Symbols
Gμν = 8πG (T̅ + Tᴿᵉˢᵖ)μν
Framework
SPARC-175
Dataset
I
Spacetime Geometry
8 symbols| Symbol | Definition | Units | Notes / Context |
|---|---|---|---|
| gμν | Metric tensor — encodes the geometry (distances and angles) of spacetime at every point | dimensionless | Symmetric 4×4 tensor; μ,ν ∈ {0,1,2,3}. All curvature quantities are derived from it. |
| Gμν | Einstein tensor — measures spacetime curvature; shorthand for Rμν − ½gμνR | m⁻² | Left-hand side of the field equations. Contains second-order partial derivatives of gμν. |
| Rμν | Ricci tensor — contraction of the Riemann tensor; encodes how volumes distort | m⁻² | Rμν = Rλμλν; symmetric. |
| R | Ricci scalar — full contraction of the Ricci tensor; single number summarizing curvature | m⁻² | R = gμνRμν. Used in the Lagrangian and in the definition of Gμν. |
| Rλμνσ | Riemann curvature tensor — the fundamental curvature object; measures how parallel transport fails to close | m⁻² | 4-index tensor; 20 independent components in 4D. |
| Γλμν | Christoffel symbols (connection coefficients) — encode how basis vectors change across spacetime | m⁻¹ | Not a tensor; computed from first derivatives of gμν. |
| ds² | Spacetime interval — invariant proper distance/time between events | m² (or s²) | ds² = gμν dxμ dxν. Negative = timelike; positive = spacelike. |
| √−g | Square root of the absolute value of the metric determinant — volume element factor in integrals | dimensionless | Ensures coordinate-invariant integration over spacetime. |
II
Weak-Field Metric Potentials
6 symbols| Symbol | Definition | Units | Notes / Context |
|---|---|---|---|
| Φ | Newtonian-gauge scalar potential — governs non-relativistic gravitational acceleration | km² s⁻² | Defined by ds² = −(1+2Φ)c²dt² + (1−2Ψ)dx². Non-relativistic dynamics probes ∇Φ. |
| Ψ | Spatial curvature potential — second scalar potential in Newtonian gauge | km² s⁻² | Lensing probes (Φ+Ψ). In standard GR with no anisotropic stress, Φ = Ψ. |
| η | Gravitational slip parameter — ratio of the two scalar potentials η ≡ Ψ/Φ | dimensionless | GR prediction: η = 1 everywhere. Edge-response predicts η ≠ 1 in the boundary-layer zone — a key falsification target. |
| Φ̅Φ_bar | Baryonic contribution to the Newtonian potential | km² s⁻² | Sourced by T̅μν via the Poisson equation. |
| Φ_resp | Response-sector contribution to the Newtonian potential | km² s⁻² | Asymptotically Φ_resp ≈ v∞² ln(R); gradient gives the 1/R tail in extra acceleration. |
| Φ_obs | Effective potential inferred from observed rotation curve by integrating g_obs(R) | km² s⁻² | Defined up to an additive constant. Computed as ∫ g_obs dR from R_min. |
III
Stress–Energy Tensors
7 symbols| Symbol | Definition | Units | Notes / Context |
|---|---|---|---|
| Tμν | Total stress–energy tensor — the full matter/energy source on the right-hand side of the field equation | kg m⁻¹ s⁻² | Tμν = T̅μν + Tᴿᵉˢᵖμν in the response-sector decomposition. |
| T̅μνT_bar | Baryonic stress–energy tensor — contribution from ordinary (observable) matter: protons, electrons, gas, stars | kg m⁻¹ s⁻² | Directly observed via photometry and HI surveys. |
| TᴿᵉˢᵖμνT^resp | Response-sector stress–energy — the effective source required so that the observed metric satisfies the Einstein equation | kg m⁻¹ s⁻² | Ontologically agnostic: not a new particle. Can be realized as an extra field, EFT correction, or constitutive closure. |
| ρ_resp | Effective energy density of the response sector | kg m⁻³ | For a flat rotation curve, ρ_resp ∝ 1/R² — same radial profile as an isothermal dark-matter halo, but derived rather than assumed. |
| p_resp | Effective pressure of the response sector | Pa | Cosmological completion requires specifying the equation of state w = p_resp / ρ_resp. |
| πμν | Anisotropic stress tensor of the response sector | Pa | Determines the slip η. If πμν ≠ 0 then η ≠ 1. |
| ∇μTμν = 0 | Bianchi identity / conservation law — the total stress–energy must be covariantly conserved | — | Imposes consistency on Tᴿᵉˢᵖμν. If baryons are minimally coupled, then ∇μTᴿᵉˢᵖμν = 0 independently. |
IV
Galactic Kinematics & Observables
12 symbols| Symbol | Definition | Units | Notes / Context |
|---|---|---|---|
| R | Galactocentric radius — projected distance from galaxy center in the disc plane | kpc | Primary independent variable in rotation-curve analysis. 1 kpc ≈ 3.086 × 10¹⁹ m. |
| R_max | Maximum observed radius — outermost data point for a given galaxy | kpc | Determines the extent of the ‘outer subset’ used by Q_est. |
| v_obs | Observed circular speed — measured Doppler-shift rotation velocity | km s⁻¹ | Primary observable from HI 21-cm or Hα spectroscopy. |
| e_{v_obs} | 1σ observational uncertainty on v_obs | km s⁻¹ | Used to construct χ² and propagate uncertainty bands in all panels. |
| v̅v_bar | Baryonic circular speed — prediction from observed baryonic mass alone | km s⁻¹ | v̅² = V²_gas + Υ_disk V²_disk + Υ_bul V²_bul. |
| v_model | Total model circular speed — baryons plus response sector | km s⁻¹ | v²_model = v̅² + Qχ′(R)·R. |
| v∞ | Asymptotic flat rotation velocity — the constant value v_obs approaches at large R | km s⁻¹ | Defines the logarithmic potential: Φ_resp ≈ v∞² ln(R). |
| V_flat | SPARC-catalogue flat velocity — tabulated asymptotic speed from the Lelli+2016 database | km s⁻¹ | Used as a proxy for galaxy mass scale; correlated with Q. |
| g_obs | Observed centripetal acceleration — kinematic inference from circular orbit condition | km² s⁻² kpc⁻¹ | g_obs = v²_obs / R. The fundamental empirical quantity; no dynamical model assumed. |
| g̅g_bar | Baryonic acceleration — Newtonian prediction from baryonic mass model | km² s⁻² kpc⁻¹ | g̅ = v̅² / R. |
| g_extra | Residual (extra) acceleration — empirical excess over baryonic prediction | km² s⁻² kpc⁻¹ | g_extra = g_obs − g̅. Framework interprets this as g_resp from the response sector. |
| g_resp | Response-sector acceleration — theoretical prediction from Tᴿᵉˢᵖμν | km² s⁻² kpc⁻¹ | Asymptotically g_resp ≈ Q/R. Matches g_extra in the successful-fit regime. |
V
Response-Sector Model Parameters
12 symbols| Symbol | Definition | Units | Notes / Context |
|---|---|---|---|
| a₀ | Critical acceleration scale — the MOND / boundary-layer activation threshold | m s⁻² or km² s⁻² kpc⁻¹ | a₀ ≈ 1.2 × 10⁻¹⁰ m s⁻². Empirical scale at which baryonic gravity equals the response activation level. Possibly linked to cH₀. |
| R_t | Transition radius — galactocentric radius where g̅(R_t) ≈ a₀ | kpc | Marks the inner edge of the boundary layer; the source bump S(R) is localized near R_t. Determined deterministically from g̅. |
| χ | Auxiliary response field — scalar field whose gradient outside the activation zone produces the acceleration tail | dimensionless (normalized) | ∂_Rχ ≈ 1/R outside activation region. |
| χ′_unit | Unit-normalized auxiliary response — the shape function, normalized so that χ′_unit → 1/R at large R | kpc⁻¹ | Computed from S(R) via the runner’s numerical integration. Multiplied by Q to give the model. |
| S(R) | Source bump — localized activation function centered near R_t | kpc⁻¹ | Gaussian with width σ_kpc (default 2.0 kpc). Drives χ in the boundary-layer equation. |
| σ_kpc | Source bump width — Gaussian half-width of the activation region | kpc | Runner default: 2.0 kpc. Controls how sharply the response is localized near R_t. |
| Q | Edge-response amplitude — the single free parameter per galaxy; asymptotic extra v² contribution | km² s⁻² | v²_extra → Q as R → ∞. Estimated two ways: Q_best (fitted) and Q_est (robust outer). |
| Q_best | Fitted edge amplitude — best-fit Q from χ² minimization over all data points | km² s⁻² | Non-negative by construction. Sensitive to inner kinematics; produced by the SPARC runner. |
| Q_est | Robust outer deficit estimator — Huber M-estimator of Δ(R) = V²_obs − V̅² over the outer data subset (R ≥ 0.6 R_max) | km² s⁻² | Model-free; can be negative (rarefaction-phase). Spearman ρ(v_best, v_est) = 0.972 across 175 galaxies. |
| v_best | Fitted asymptotic extra speed — √Q_best | km s⁻¹ | Comparable to v_est for ranking purposes. |
| v_est | Robust asymptotic extra speed — √max(Q_est, 0) | km s⁻¹ | Set to ‘neg’ if Q_est < 0 (rarefaction-phase galaxy). |
| Δ(R) | Velocity-squared deficit profile — V²_obs − V̅² at each radius R | km² s⁻² | The raw signal the framework must explain. Sign changes in Δ(R) indicate oscillatory response; 46/175 SPARC galaxies show at least one sign change. |
VI
Baryonic Mass Components
11 symbols| Symbol | Definition | Units | Notes / Context |
|---|---|---|---|
| V_gas | Gas circular-speed template from SPARC rotmod file | km s⁻¹ | HI + He contribution; enters v̅² with coefficient 1 (no Υ multiplier). |
| V_disk | Stellar-disc circular-speed template from SPARC rotmod file | km s⁻¹ | Scaled by Υ_disk before adding to v̅². |
| V_bul | Bulge circular-speed template from SPARC rotmod file | km s⁻¹ | Scaled by Υ_bul. Zero for bulgeless galaxies. |
| Υ_disk | Stellar mass-to-light ratio of the disc — converts surface brightness to surface mass density | M☉/L☉ | Runner default: 0.5. Sensitivity sweep over {0.3, 0.4, 0.5, 0.6, 0.7} shows ≤17% change in Q_est for ±40% variation. |
| Υ_bul | Stellar mass-to-light ratio of the bulge | M☉/L☉ | Runner default: 0.7. |
| M_b | Total baryonic mass — integral of baryonic surface density over the disc | M☉ | Appears in the baryonic Tully–Fisher relation: M_b ∝ v⁴_flat. |
| M_HI | HI (neutral hydrogen) mass | M☉ | Correlated with Q_est; HI-rich discs have extended, diffuse edges → shallower boundary-layer gradient → weaker response. |
| R_disk | Disc scale length — exponential scale radius of the stellar disc | kpc | SPARC metadata. Used as a galaxy size proxy; controls Q base-line. |
| Q_flag | SPARC photometric quality flag: 1 = best, 2 = moderate, 3 = poorest | — | Spearman ρ(Q_est, outer_rms_z) = −0.035; photometric quality has zero detectable correlation with outer residual scatter. |
| T | Hubble morphological type index (e.g., 5 = Sc, 9 = Irr, 10 = Im) | — | From RC3 / SPARC Table 1. |
| D | Distance to galaxy | Mpc | From SPARC catalogue; used to convert angular to physical scales. |
VII
Statistical Diagnostics
11 symbols| Symbol | Definition | Units | Notes / Context |
|---|---|---|---|
| χ² | Chi-squared statistic — weighted sum of squared residuals between model and data | dimensionless | χ² = Σ_i [(v_model(R_i) − v_obs(R_i)) / e_{v_obs}(R_i)]². |
| χ̅²χ²_bar | Baryons-only chi-squared — χ² when v_model = v̅ (no response sector) | dimensionless | Baseline for Δχ² comparison. |
| χ²_model | Fitted-model chi-squared — χ² with best-fit Q | dimensionless | Always ≤ χ̅² by construction. |
| Δχ² | Chi-squared improvement — χ̅² − χ²_model; measures how much the response sector helps | dimensionless | Z ≈ √Δχ² gives approximate Gaussian significance for 1 added parameter. |
| Z | Approximate Gaussian significance of Δχ² | σ | Z = √Δχ². Classes: weak Z < 2, moderate 2–3, strong 3–5, very-strong Z > 5. |
| rχ² | Reduced chi-squared — χ² / (n − k) where n = data points, k = free parameters | dimensionless | Reported separately for inner (R < 0.6 R_max) and outer (R ≥ 0.6 R_max) regions. Inner/outer ratio = 3.54× confirms shape inadequacy, not Υ bias. |
| BIC | Bayesian Information Criterion — k ln(n) − 2 ln(L̂); penalizes model complexity | dimensionless | ΔBIC = BIC_model − BIC̅ < 0 required to pass. 97% of 175 SPARC galaxies pass. Guards against overfitting. |
| ρ_s | Spearman rank correlation coefficient — non-parametric measure of monotonic association | dimensionless | Used throughout to quantify correlations between Q, galaxy properties, and environment. Range [−1, +1]. |
| r | Pearson linear correlation coefficient | dimensionless | Used alongside Spearman ρ for robustness. r(v_best, v_est) = 0.950 across 175 galaxies. |
| σ_Δv | Propagated uncertainty on velocity deficit Δv | km s⁻¹ | σ_Δv ≈ e_{v_obs} when model is treated as exact. |
| outer_rms_z | Outer-region residual RMS in units of observational uncertainty — (v_obs − v_model) / e_{v_obs} over R ≥ 0.6 R_max | dimensionless | Key diagnostic for fit quality in the outer disc, where the 1/R tail is most active. |
VIII
Oscillatory Boundary-Layer Response
8 symbols| Symbol | Definition | Units | Notes / Context |
|---|---|---|---|
| Φ_resp(r) | Oscillatory response potential — the full spatial form of the response-sector potential | km² s⁻² | Φ_resp = A cos(κr + δ) e⁻ʳ/L; encoding amplitude, wavenumber, phase, and decay scale. |
| A | Oscillation amplitude — peak response-potential strength | km² s⁻² | Related to Q in the asymptotic regime. |
| κ | Radial wavenumber of the oscillatory response | kpc⁻¹ | κ = 2π/λ. Galaxy-size dependent, not a fixed cosmological scale. |
| λ | Oscillation wavelength — spatial period of the boundary-layer standing wave | kpc | Median λ ≈ 45.6 kpc across the 46 sign-change galaxies; scales with R_max, not a cosmological constant. |
| δ | Phase offset of the oscillatory response at R_t | rad | Depends on initial conditions. |
| L | Damping / decay scale of the oscillatory response | kpc | Characterizes how quickly the oscillation envelope falls off with radius. |
| λ/2 | Half-wavelength of oscillation | kpc | Median ≈ 22.8 kpc. Scaling λ/2 ≈ R_max / 2 is the key empirical result distinguishing galaxy-geometry resonance from cosmological scale. |
| Δ(R) = 0Nodal radius | Galactocentric radius where V²_obs = V̅² exactly | kpc | Stars at this radius orbit on pure baryonic gravity. Framework predicts morphological ring features here — a testable prediction. |
IX
Action Principle & Field Theory
8 symbols| Symbol | Definition | Units | Notes / Context |
|---|---|---|---|
| S | Action — integral of the Lagrangian density over spacetime; extremizing S yields the field equations | J·s | S = ∫ d⁴x √−g [R/(16πG) + L̅ + L_χ + L_int]. |
| L̅L_bar | Baryonic Lagrangian density — standard matter fields (ψ) | J m⁻³ | Minimally coupled to gravity. |
| L_χ | Response-field Lagrangian density — kinetic and potential terms for χ | J m⁻³ | Choice of L_χ (e.g., f(X) − V(χ)) controls the field equations for χ and the form of Tᴿᵉˢᵖμν. |
| L_int | Interaction Lagrangian — couples χ to baryonic fields ψ | J m⁻³ | Must tie activation to a baryonic invariant so the response is not a free function per galaxy. |
| X | Kinetic invariant of the response field — X = gμν ∂μχ ∂νχ | kpc⁻² | Used in k-essence / AQUAL-type response fields: f(X) controls the equation of motion. |
| f(X) | Non-linear kinetic function for the response field | J m⁻³ | Choosing f so that the static equation has conserved radial flux outside activation yields ∂_Rχ ∼ 1/R. |
| G | Newton’s gravitational constant | m³ kg⁻¹ s⁻² | G ≈ 6.674 × 10⁻¹¹ m³ kg⁻¹ s⁻². Appears in the coupling 8πG between geometry and stress-energy. |
| 8πG | Gravitational coupling constant in the field equation Gμν = 8πG Tμν | m kg⁻¹ s⁻² | Right-hand side coefficient. |
X
Cosmological Sector
7 symbols| Symbol | Definition | Units | Notes / Context |
|---|---|---|---|
| ΛCDM | Standard cosmological model — Lambda (dark energy) + Cold Dark Matter | — | The empirically successful baseline the response sector must be consistent with at large scales. |
| H₀ | Hubble constant — present-day rate of cosmic expansion | km s⁻¹ Mpc⁻¹ | H₀ ≈ 70 km s⁻¹ Mpc⁻¹. The product cH₀ motivates a possible cosmological origin for the acceleration scale a₀. |
| w | Equation-of-state parameter of the response sector — w = p_resp / ρ_resp | dimensionless | Cosmological viability requires w ≈ 0 (dust-like) over structure-formation epochs. |
| a(t) | Cosmological scale factor — dimensionless ratio of physical to comoving distances | dimensionless | Cosmological completion requires specifying how Tᴿᵉˢᵖμν evolves with a. |
| ρ_resp(a) | Redshift evolution of response-sector energy density | kg m⁻³ | Must behave approximately as ∝ a⁻³ (pressureless) over target epochs to preserve structure formation. |
| κ_lens | Lensing convergence — integral of (Φ+Ψ) along the line of sight | dimensionless | κ_lens ∝ Φ+Ψ. With η ≠ 1, the lensing signal differs from the kinematic signal — the primary cluster/lensing prediction. |
| δ_env | Environment overdensity — local large-scale density contrast around a galaxy | dimensionless | Used in SPARC analysis as an environment proxy. Partial correlations with Q_est should become weak once internal (scale) covariates are controlled. |
XI
Baryonic Tully–Fisher Relation
3 symbols| Symbol | Definition | Units | Notes / Context |
|---|---|---|---|
| BTFR | Baryonic Tully–Fisher Relation — M_b ∝ v⁴_flat | — | Tight empirical scaling relation across 4 orders of magnitude in baryonic mass. Emerges as a consequence of the response-sector mechanism rather than an imposed prior. |
| M_b ∝ v⁴_flat | BTFR functional form | M☉ vs km s⁻¹ | Derivable when g_extra is the geometric mean of g̅ and a₀, i.e., when the response sector couples to g̅ at the transition scale. |
| Q ∝ V²_flat | BTF-anchor prediction — the response amplitude Q scales as the square of the asymptotic velocity | km² s⁻² | Mechanism, not a mass-accounting identity. Confirmed empirically across SPARC-175. |
Source: Kitcey, R. D. (2026). Intrinsic Response Sector as Dark Gravity: A GR-Compatible Candidate Identity for the Cold Dark Matter Role (SPARC-175) (v5.0.7). Zenodo. https://doi.org/10.5281/zenodo.18778896. Appendix A: Comprehensive Symbol Glossary (Table 5). Lernaean Research™.
