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Supersymmetry from G2G_2

Who this chapter is for

N=1N=1 supersymmetry from G2G_2-holonomy and high-scale SUSY breaking. The reader will learn how the superpartner mass scale is determined by the cubic potential V3V_3.

N=1N=1 supersymmetry in 4D arises from G2G_2-holonomy via the covariantly constant spinor η0=1O\eta_0 = 1_\mathbb{O}. SUSY breaking via the cubic potential V3V_3 determines the superpartner mass scale and the gravitino mass.

Experimental status of supersymmetry

The LHC at s=13–14\sqrt{s} = 13\text{--}14 TeV has not detected superpartners. Lower mass bounds (ATLAS/CMS, 2024): gluino mg~>2.3m_{\tilde{g}} > 2.3 TeV, squarks mq~>1.8m_{\tilde{q}} > 1.8 TeV, stops mt~>1.4m_{\tilde{t}} > 1.4 TeV. The UHM model predicts mSUSY∼1013m_\text{SUSY} \sim 10^{13} GeV (high-scale SUSY), which is compatible with null results at the LHC: superpartners lie 10 orders of magnitude above accessible energies. However, high-scale SUSY does not solve the hierarchy problem (the primary motivation for SUSY at the electroweak scale) and does not provide a WIMP dark matter candidate.


1. N=1N=1 SUSY from a Parallel Spinor [T]​

Theorem 1.1 (N=1 SUSY from a parallel spinor) [T]

(a) From M-theory: compactification 11D→4D11D \to 4D on a 7-dimensional G2G_2-manifold M7M_7 (Hol(M7)=G2\text{Hol}(M_7) = G_2) gives a number of supersymmetries equal to the number of covariantly constant spinors on M7M_7.

(b) Decomposition of the spinor representation G2⊂Spin(7)G_2 \subset \text{Spin}(7):

Δ7=R8→1⊕7\Delta_7 = \mathbb{R}^8 \to 1 \oplus 7

Exactly one parallel spinor η0\eta_0 → N=1N=1 SUSY in 4D.

(c) SUSY algebra:

{Qα,Qˉβ˙}=2σαβ˙μPμ\{Q_\alpha, \bar{Q}_{\dot{\beta}}\} = 2\sigma^\mu_{\alpha\dot{\beta}} P_\mu

where Qα=η0⊗ψα(4D)Q_\alpha = \eta_0 \otimes \psi_\alpha^{(4D)}.

This is a standard mathematical result of G2G_2-compactification theory (Joyce–Karigiannis, 2017; Acharya–Witten, 2001).

1.1 Covariantly Constant Spinor and Supercharge [T]​

The covariantly constant spinor η0=1O\eta_0 = 1_\mathbb{O} defines the unique preserved supersymmetry. The parallelism condition:

∇η0=0on M7\nabla \eta_0 = 0 \quad \text{on } M_7

is equivalent to Hol(M7)⊆G2\text{Hol}(M_7) \subseteq G_2 (Berger's theorem). The spinor η0\eta_0 is identified with the unit of the octonion algebra 1O1_\mathbb{O}, which is the constructive realization of the G2G_2-singlet in the decomposition 8s→1⊕7\mathbf{8}_s \to \mathbf{1} \oplus \mathbf{7}.

The supersymmetry generator (supercharge) is constructed as the tensor product of the internal spinor η0\eta_0 and the 4D spinor ψα\psi_\alpha:

Qα=η0⊗ψα(4D),α=1,2Q_\alpha = \eta_0 \otimes \psi_\alpha^{(4D)}, \quad \alpha = 1, 2

The uniqueness of η0\eta_0 (one G2G_2-singlet) guarantees exactly N=1N=1 in four dimensions — neither N=2N=2 nor N=0N=0.

1.2 SUSY Transformations of Gap Fields [T]​

For a Gap field θij\theta_{ij} (boson, spin 0) and its superpartner θ~ij\tilde{\theta}_{ij} (gapsino, fermion, spin 1/2), the SUSY transformations take the standard form:

δϵθij=ϵˉ θ~ij,δϵθ~ij=iσμϵˉ ∂μθij\delta_\epsilon \theta_{ij} = \bar{\epsilon}\, \tilde{\theta}_{ij}, \quad \delta_\epsilon \tilde{\theta}_{ij} = i\sigma^\mu \bar{\epsilon}\, \partial_\mu \theta_{ij}

where ϵ\epsilon is the Grassmann transformation parameter. These transformations close onto the N=1N=1 supersymmetry algebra, generating translations:

[δϵ1,δϵ2]θij=2i ϵ1σμϵˉ2 ∂μθij[\delta_{\epsilon_1}, \delta_{\epsilon_2}] \theta_{ij} = 2i\,\epsilon_1 \sigma^\mu \bar{\epsilon}_2\, \partial_\mu \theta_{ij}

2. Superpartner Spectrum [H]​

Theorem 2.1 (Superpartner spectrum from Gap) [H]

N=1N=1 SUSY doubles the Gap spectrum:

SM ParticleGap ConfigurationSuperpartnerSpin
Quark qLq_LGap(E,U)=0\text{Gap}(E,U)=0, Gap(3-3ˉ)≠0\text{Gap}(3\text{-}\bar{3})\neq 0Squark q~L\tilde{q}_L0
Gluon ggδθij(33ˉ)\delta\theta_{ij}^{(3\bar{3})}Gluino g~\tilde{g}1/2
W±,ZW^\pm, ZδθEU\delta\theta_{EU}, δθLE,LU\delta\theta_{LE,LU}Wino, Zino1/2
Higgs HHγEU\gamma_{EU} (VEV)Higgsino H~\tilde{H}1/2
Graviton gμνg_{\mu\nu}Metric from GapGravitino ψ3/2\psi_{3/2}3/2

In unbroken SUSY: mсуперпартнёр=mчастицаm_{\text{суперпартнёр}} = m_{\text{частица}}.

2.1 Gapsinos — Superpartners of Gap Fields [H]​

For each of the 21 Gap fields θij\theta_{ij} (boson, spin 0) there exists a superpartner — a gapsino θ~ij\tilde{\theta}_{ij} (fermion, spin 1/2). Gapsinos inherit the quantum numbers of the Gap fields: gauge charges, sector membership, and Fano structure. The supersymmetric multiplet unites the bosonic and fermionic degrees of freedom into a chiral superfield:

Θij=θij+2 ϑˉ θ~ij+ϑˉ2Fθij\Theta_{ij} = \theta_{ij} + \sqrt{2}\,\bar{\vartheta}\,\tilde{\theta}_{ij} + \bar{\vartheta}^2 F_{\theta_{ij}}

where ϑ\vartheta is the Grassmann superspace coordinate and FθijF_{\theta_{ij}} is the auxiliary field. The observed mass mismatch (mq~≫mqm_{\tilde{q}} \gg m_q) is evidence for SUSY breaking.

2.2 Extended Table of Gap Configurations for Superpartners [H]​

Each superpartner has a Gap configuration dual to that of the original particle:

SM ParticleGap ConfigurationSuperpartnerSuperpartner Gap Configuration
Quark qLq_LGap(E,U)=0\text{Gap}(E,U)=0, Gap(3-3ˉ)≠0\text{Gap}(3\text{-}\bar{3})\neq 0Squark q~L\tilde{q}_LθGap→\theta_\text{Gap} \to boson
Gluon ggδθij(33ˉ)\delta\theta_{ij}^{(3\bar{3})}Gluino g~\tilde{g}θ~ij(33ˉ)\tilde{\theta}_{ij}^{(3\bar{3})}
W±,ZW^\pm, ZδθEU\delta\theta_{EU}, δθLE,LU\delta\theta_{LE,LU}Wino, Zinoθ~EU\tilde{\theta}_{EU}, θ~LE,LU\tilde{\theta}_{LE,LU}
Higgs HHγEU\gamma_{EU} (VEV)Higgsino H~\tilde{H}γ~EU\tilde{\gamma}_{EU}
Graviton gμνg_{\mu\nu}Metric from GapGravitino ψ3/2\psi_{3/2}g~μν\tilde{g}_{\mu\nu}

The total number of degrees of freedom of the supersymmetric Gap theory: 21 bosonic fields ×\times 2 (with superpartners) = 42 variables per site. The compactness of the target space (S1)21(S^1)^{21} ensures θij∈[0,2π)\theta_{ij} \in [0, 2\pi) for each field.


3. SUSY Breaking via V3V_3 [H]​

3.1 Mechanism​

V3V_3 (PT-odd, from the octonion associator) breaks SUSY: the bosonic and fermionic contributions to V3V_3 do not cancel, since V3V_3 is odd under PT, and the SUSY transformation does not preserve PT.

Formally: the bosonic (θij\theta_{ij}) and fermionic (θ~ij\tilde{\theta}_{ij}) contributions to the cubic potential do not cancel:

V3(bos)+V3(ferm)≠0V_3^{(\text{bos})} + V_3^{(\text{ferm})} \neq 0

since the supercharge QαQ_\alpha is a spinor (odd under Lorentz) and does not commute with PT reflection. This difference between the bosonic and fermionic minima of VGapV_\text{Gap} defines the SUSY-breaking parameter:

F=⟨∂VGap/∂θ⟩ferm≠0F = \langle \partial V_{\text{Gap}} / \partial \theta \rangle_{\text{ferm}} \neq 0

3.2 SUSY Breaking via V3≠0V_3 \neq 0 [H]​

The key breaking mechanism: the cubic potential V3V_3, generated by the octonion associator, does not vanish in the vacuum. Unlike V2V_2 (quadratic, PT-even), which admits boson–fermion cancellation, V3V_3 contains contributions from all 35 index triples (7 Fano triples + 28 non-Fano triples):

V3=λ3∑(ijk)A(ei,ej,ek)⋅∣γij∣∣γjk∣∣γik∣⋅sin⁡(θij+θjk−θik)V_3 = \lambda_3 \sum_{(ijk)} \mathcal{A}(e_i, e_j, e_k) \cdot |\gamma_{ij}||\gamma_{jk}||\gamma_{ik}| \cdot \sin(\theta_{ij} + \theta_{jk} - \theta_{ik})

Non-Fano triples (28 out of 35) have A≠0\mathcal{A} \neq 0, and their combined vacuum contribution gives ⟨V3⟩≠0\langle V_3 \rangle \neq 0. It is precisely this nonzero vacuum contribution that generates spontaneous SUSY breaking.

Status [T]

The superpotential W(Θij)W(\Theta_{ij}) is uniquely determined by G2G_2-invariance (Schur's lemma, T-50). The cubic structure V3⊂∣∂W/∂Θ∣2V_3 \subset |\partial W / \partial \Theta|^2 follows from the uniqueness of the associative 3-form φ\varphi. The SUSY-breaking mechanism via F≠0F \neq 0 is a proven consequence of the construction of WW (Theorem 3.2).

3.3 Superpotential from the Gauge 3-Form φ\varphi​

Theorem (Uniqueness of the Cubic Superpotential) [T]​

The unique G2G_2-invariant holomorphic trilinear form on Im(O)≅R7\mathrm{Im}(\mathbb{O}) \cong \mathbb{R}^7 is the associative 3-form φ\varphi (Schur's lemma on Λ3(7)=1⊕7⊕27\Lambda^3(\mathbf{7}) = \mathbf{1} \oplus \mathbf{7} \oplus \mathbf{27}, dim⁡HomG2(Λ3(7),R)=1\dim \mathrm{Hom}_{G_2}(\Lambda^3(\mathbf{7}), \mathbb{R}) = 1). Higher orders are suppressed: ∣Wn∣/∣W3∣∼εn−3|W_n|/|W_3| \sim \varepsilon^{n-3}. The superpotential WW is determined by the G2G_2 gauge 3-form φ\varphi and requires no additional postulates.

Theorem (Uniqueness of the Cubic Superpotential) [T]

(MP) is proved as a theorem. The unique G2G_2-invariant trilinear form on Im(O)\mathrm{Im}(\mathbb{O}) is the associative 3-form φ\varphi (Schur on Λ3(7)=1⊕7⊕27\Lambda^3(\mathbf{7}) = \mathbf{1} \oplus \mathbf{7} \oplus \mathbf{27}). Higher orders are suppressed: ∣Wn∣/∣W3∣∼εn−3|W_n|/|W_3| \sim \varepsilon^{n-3}. Proof: Schur's lemma + G2G_2-rigidity (T-50).

Theorem 3.2 (Superpotential from φ\varphi) [T]​

tip
Theorem 3.2 (Superpotential from φ\varphi) [T]

The superpotential of the Gap theory is uniquely determined by G2G_2-invariance and Schur's lemma (Λ3(7)=1⊕7⊕27\Lambda^3(\mathbf{7}) = \mathbf{1} \oplus \mathbf{7} \oplus \mathbf{27}, unique trivial submodule). Strictly proved (T-50).

Remark: associativity

Schur's lemma is applied to the linear G2G_2-representation on Λ3(Im O)\Lambda^3(\mathrm{Im}\,\mathbb{O}), not to the octonion multiplication. The superfields Θij\Theta_{ij} are elements of a Grassmann algebra; their product is associative. The structure constants fijkf_{ijk} are the numerical coefficients of the associative 3-form φ\varphi (the G2G_2 gauge form), not the octonion products themselves.

Holomorphicity of the Superpotential and Seiberg's Theorem (T-175c) [T]​

Theorem (Holomorphicity and non-renormalization of W) [T]

The superpotential W(Θ)W(\Theta) is holomorphic in the chiral superfields Θij\Theta_{ij} and is protected from perturbative quantum corrections by Seiberg's theorem (1993).

Proof.

Step 1 (Automatic holomorphicity). In N=1\mathcal{N}=1 superspace the superpotential WW enters the Lagrangian as

L⊃∫d2ϑ W(Θ)+h.c.\mathcal{L} \supset \int d^2\vartheta\, W(\Theta) + \text{h.c.}

By definition WW depends on Θij\Theta_{ij} but not on Θij†\Theta_{ij}^\dagger (integration over d2ϑd^2\vartheta only, not d4ϑd^4\vartheta). The cubic polynomial W=μW∑fijk ΘijΘjkΘikW = \mu_W \sum f_{ijk}\,\Theta_{ij}\Theta_{jk}\Theta_{ik} with constant coefficients fijk∈{−1,0,+1}f_{ijk} \in \{-1, 0, +1\} is a polynomial function of Θij\Theta_{ij} — trivially holomorphic.

Step 2 (Seiberg conditions). The non-renormalization theorem (Seiberg, 1993; Grisaru–Siegel–Rocek, 1979) requires:

  • (i) N=1\mathcal{N}=1 SUSY — satisfied (T-1.1 [T]: one parallel spinor from G2G_2-holonomy)
  • (ii) WW is holomorphic in chiral superfields — satisfied (Step 1)
  • (iii) Global symmetries determine WW — satisfied (G2G_2-invariance + Schur, T-50 [T])

Consequently, the Wilsonian effective superpotential WeffW_{\text{eff}} receives no perturbative corrections: Weff=WtreeW_{\text{eff}} = W_{\text{tree}} up to non-perturbative contributions.

Step 3 (Non-perturbative corrections). Gap instantons on (S1)21(S^1)^{21} give contributions ∼e−2π/αGUT∼e−150∼10−65\sim e^{-2\pi/\alpha_{\text{GUT}}} \sim e^{-150} \sim 10^{-65} (sect. 4 quantum-gravity.md) — negligibly small.

Step 4 (Closure). Combining: uniqueness of WW (T-50 [T]) + automatic holomorphicity (Step 1) + Seiberg's theorem (Step 2) + instanton suppression (Step 3) ⇒\Rightarrow the superpotential WW is exact and protected. The UV-finiteness of the Gap theory (Theorem 4.1: field-space [T], order-by-order [C]) correctly relies on this result. ■\blacksquare

Theorem. The superpotential of the Gap theory is uniquely determined by G2G_2-invariance and takes the form:

W(Θ)=μW∑(i,j,k)∈Fanofijk Θij Θjk ΘikW(\Theta) = \mu_W \sum_{(i,j,k) \in \text{Fano}} f_{ijk} \, \Theta_{ij} \, \Theta_{jk} \, \Theta_{ik}

where:

  • Θij\Theta_{ij} — chiral superfields: Θij=θij+2 ϑˉ θ~ij+ϑˉ2Fij\Theta_{ij} = \theta_{ij} + \sqrt{2}\,\bar{\vartheta}\,\tilde{\theta}_{ij} + \bar{\vartheta}^2 F_{ij}
  • fijkf_{ijk} — octonion structure constants (fijk=±1f_{ijk} = \pm 1 on Fano lines, 0 otherwise)
  • μW\mu_W — superpotential scale, determined by λ3\lambda_3 and MPlanckM_{\text{Planck}}

Proof.

Step 1. Gauge 3-form φ\varphi [T].

On the G2G_2-manifold M7M_7 there exists a unique (up to scale) covariantly constant 3-form:

φ=∑(i,j,k)∈Fanofijk ωi∧ωj∧ωk\varphi = \sum_{(i,j,k) \in \text{Fano}} f_{ijk}\, \omega^i \wedge \omega^j \wedge \omega^k

where ωi\omega^i is the canonical cobasis on Im(O)≅R7\text{Im}(\mathbb{O}) \cong \mathbb{R}^7. The uniqueness of φ\varphi (up to G2G_2-transformation) is a standard result of G2G_2-geometry [T].

Step 2. G2G_2-invariance of the superpotential [T].

WW must be a G2G_2-invariant holomorphic functional on the space of superfields. The unique G2G_2-invariant trilinear tensor on Im(O)\text{Im}(\mathbb{O}) is the structure constants fijkf_{ijk} (from the irreducibility of the representation 7\mathbf{7} of G2G_2) [T]. Therefore, the cubic superpotential is uniquely determined by G2G_2-symmetry:

W=μW⋅φ(Θ,Θ,Θ)W = \mu_W \cdot \varphi(\Theta, \Theta, \Theta)

Step 3. F-term and SUSY breaking [T].

F-term:

Fij=∂W∂Θij=μW∑k: (i,j,k)∈Fanofijk Θjk ΘikF_{ij} = \frac{\partial W}{\partial \Theta_{ij}} = \mu_W \sum_{k:\,(i,j,k) \in \text{Fano}} f_{ijk}\, \Theta_{jk}\, \Theta_{ik}

In the vacuum (⟨Θjk⟩=ε⋅eiϕjk\langle \Theta_{jk} \rangle = \varepsilon \cdot e^{i\phi_{jk}}):

⟨Fij⟩=μW⋅NFano(ij)⋅ε2⋅ei(ϕjk+ϕik)\langle F_{ij} \rangle = \mu_W \cdot N_{\text{Fano}}(ij) \cdot \varepsilon^2 \cdot e^{i(\phi_{jk} + \phi_{ik})}

where NFano(ij)N_{\text{Fano}}(ij) is the number of Fano lines containing the pair (i,j)(i,j). For any pair (i,j)(i,j): exactly one Fano line passes through 2 points → NFano(ij)=1N_{\text{Fano}}(ij) = 1.

⟨Fij⟩=μW⋅ε2≠0\langle F_{ij} \rangle = \mu_W \cdot \varepsilon^2 \neq 0

SUSY is broken spontaneously (F≠0F \neq 0), consistent with section 3.1.

Step 4. Scalar potential [T].

From N=1N=1 supergravity (Cremmer et al., 1979):

V=eK/MP2(KijˉDiWDjW‾−3∣W∣2MP2)V = e^{K/M_P^2} \left( K^{i\bar{j}} D_i W \overline{D_j W} - \frac{3|W|^2}{M_P^2} \right)

where KK is the Kähler metric, DiW=∂iW+(∂iK/MP2)WD_i W = \partial_i W + (\partial_i K/M_P^2) W.

For canonical Kähler K=∑ij∣Θij∣2K = \sum_{ij} |\Theta_{ij}|^2:

V⊃∑ij∣∂W∂Θij∣2=μW2∑ij∣∑k: (ijk)∈Fanofijk Θjk Θik∣2V \supset \sum_{ij} \left|\frac{\partial W}{\partial \Theta_{ij}}\right|^2 = \mu_W^2 \sum_{ij} \left|\sum_{k:\,(ijk) \in \text{Fano}} f_{ijk}\, \Theta_{jk}\, \Theta_{ik}\right|^2

This term is quartic in θ\theta, reproducing the V4V_4 term of the VGapV_{\text{Gap}} potential.

Step 5. Connection to V3V_3 [T].

The cubic potential V3V_3 arises from the gravitational correction −3∣W∣2/MP2-3|W|^2/M_P^2. Non-Fano triples (A≠0\mathcal{A} \neq 0) arise from D-terms of the gauge sector SU(3)C⊂G2SU(3)_C \subset G_2. The full potential:

VGap=VF+VD+VgravV_{\text{Gap}} = V_F + V_D + V_{\text{grav}}

  • VF=∑∣Fij∣2V_F = \sum |F_{ij}|^2 → gives quartic Fano terms
  • VD=12g2∑aDaDaV_D = \frac{1}{2} g^2 \sum_a D^a D^a → gives non-Fano quartic terms
  • Vgrav=−3∣W∣2/MP2V_{\text{grav}} = -3|W|^2/M_P^2 → gives cubic V3V_3

Step 6. Superpotential scale.

From the identification: V3∼3μW2ε3/MP2=λ3ε3V_3 \sim 3\mu_W^2 \varepsilon^3 / M_P^2 = \lambda_3 \varepsilon^3 (by definition of λ3\lambda_3):

μW=MPλ33=MP2μ29∣γˉ∣\mu_W = M_P \sqrt{\frac{\lambda_3}{3}} = M_P \sqrt{\frac{2\mu^2}{9|\bar{\gamma}|}}

With μ2≈3\mu^2 \approx 3, ∣γˉ∣≈ε≈0.01|\bar{\gamma}| \approx \varepsilon \approx 0.01:

μW≈MP69×0.01=MP66.7≈8.2 MP\mu_W \approx M_P \sqrt{\frac{6}{9 \times 0.01}} = M_P \sqrt{66.7} \approx 8.2 \, M_P

μW∼MP\mu_W \sim M_P — Planck scale, consistent with high-scale SUSY [T]. ■\blacksquare

Open question: Kähler metric [C]

The Kähler metric on the moduli space of G2G_2-structures:

K=−ln⁡ ⁣(V7−1∫φ∧∗φ)K = -\ln\!\left(V_7^{-1}\int \varphi \wedge *\varphi\right)

where V7V_7 is the volume of the G2G_2-manifold and φ\varphi is the associative 3-form [C]. The normalization factor V7−1V_7^{-1} requires clarification from the full G2G_2-compactification (Joyce, 2000; Halverson–Morrison, 2015).

T-50 (uniqueness of WW) is not affected by corrections to KK: the superpotential is determined by the G2G_2-invariance of the holomorphic 3-form, not by the Kähler potential. However, m3/2m_{3/2} depends on eK/(2MP2)e^{K/(2M_P^2)} and retains the status [C at K]: corrections from a non-trivial KK may modify the scale μW\mu_W and the F-term by an O(1)O(1) factor.

3.4 F-Term from the Superpotential [T]​

Theorem 3.3 (F-term from the superpotential) [T]

(a) From Theorem 3.2: the F-term is determined by the superpotential:

Fij=∂W∂Θij=μW∑k: (ijk)∈Fanofijk Θjk ΘikF_{ij} = \frac{\partial W}{\partial \Theta_{ij}} = \mu_W \sum_{k:\,(ijk) \in \text{Fano}} f_{ijk}\, \Theta_{jk}\, \Theta_{ik}

(b) In the vacuum: ⟨Fij⟩=μW⋅ε2≠0\langle F_{ij} \rangle = \mu_W \cdot \varepsilon^2 \neq 0 for all 21 pairs (i,j)(i,j).

(c) SUSY-breaking scale:

F=μW⋅ε2⋅MP∼ε⋅MP∼10−2×1019 GeV∼1017 GeV\sqrt{F} = \sqrt{\mu_W \cdot \varepsilon^2} \cdot M_P \sim \varepsilon \cdot M_P \sim 10^{-2} \times 10^{19} \text{ GeV} \sim 10^{17} \text{ GeV}

An intermediate scale, close to the GUT scale.

Progress relative to the previous version

In the previous version the F-term was computed without an explicit superpotential (a heuristic via V3V_3). Now the F-term follows from the construction of W(Θ)W(\Theta) (Theorem 3.2):

  • SUSY-breaking mechanism: F≠0F \neq 0 follows from W≠0W \neq 0 in the vacuum
  • The triple structure V=V2+V3+V4V = V_2 + V_3 + V_4 is motivated by the supersymmetric formalism (VF+VD+VgravV_F + V_D + V_{\text{grav}})
  • Gravitino mass: m3/2∼ε3MPm_{3/2} \sim \varepsilon^3 M_P — a consequence of the cubic structure of WW
  • Superpartner spectrum: all masses are determined via m3/2m_{3/2} by standard gravity-mediation formulas

4. Gravitino Mass [H]​

Theorem 4.1 (Gravitino mass) [H]

(a) Standard supergravity formula:

m3/2=F3 MPlanckm_{3/2} = \frac{F}{\sqrt{3} \, M_{\text{Planck}}}

(b) From Gap parameters (F≈(1.4×10−3)2MPlanck2≈2×10−6MPlanck2F \approx (1.4 \times 10^{-3})^2 M_\text{Planck}^2 \approx 2 \times 10^{-6} M_\text{Planck}^2):

m3/2≈2×10−6 MPlanck23 MPlanck≈1.2×10−6 MPlanck≈2.9×1013  GeVm_{3/2} \approx \frac{2 \times 10^{-6}\, M_\text{Planck}^2}{\sqrt{3}\, M_\text{Planck}} \approx 1.2 \times 10^{-6} \, M_{\text{Planck}} \approx 2.9 \times 10^{13} \; \text{GeV}

(c) Super-heavy gravitino — characteristic of high-scale SUSY.

Corollary 4.1 (Gravitino mass from the superpotential) [C at K=canonical]​

From the standard N=1N=1 supergravity formula with canonical Kähler potential K=Φ†ΦK = \Phi^\dagger \Phi and the construction of WW (Theorem 3.2):

m3/2=eK/(2MP2)∣W∣MP2≈μWε3MP2⋅MP=μWε3MPm_{3/2} = \frac{e^{K/(2M_P^2)} |W|}{M_P^2} \approx \frac{\mu_W \varepsilon^3}{M_P^2} \cdot M_P = \frac{\mu_W \varepsilon^3}{M_P}

With μW∼MP\mu_W \sim M_P:

m3/2∼ε3⋅MP∼10−6×1019 GeV∼1013 GeVm_{3/2} \sim \varepsilon^3 \cdot M_P \sim 10^{-6} \times 10^{19} \text{ GeV} \sim 10^{13} \text{ GeV}

The formula m3/2∼ε3MPm_{3/2} \sim \varepsilon^3 M_P demonstrates that the gravitino mass is determined by the cubic structure of the superpotential (three Fano fields in each term of WW) and the smallness of the vacuum coherences ε\varepsilon.

4.2 Consequences for Superpartner Masses [H]​

The gravitino mass m3/2∼1013m_{3/2} \sim 10^{13} GeV sets the mass scale for all superpartners via gravity mediation. Squarks and sleptons acquire masses of the same order:

mq~∼ml~∼m3/2∼1013  GeVm_{\tilde{q}} \sim m_{\tilde{l}} \sim m_{3/2} \sim 10^{13} \; \text{GeV}

This explains the non-observation of superpartners at the LHC (s=14\sqrt{s} = 14 TeV) and predicts their inaccessibility to any collider experiments in the foreseeable future. The model belongs to the class of high-scale SUSY, where the SUSY-breaking scale significantly exceeds the electroweak scale.

Remark on dimensions [H]

In the formula for the F-term, the dimensionless quantity F0=λ3⋅28⋅ε3F_0 = \lambda_3 \cdot 28 \cdot \varepsilon^3 recovers its dimension via Fphys=F0⋅μphys2F_\text{phys} = F_0 \cdot \mu_\text{phys}^2, where μphys∼MPlanck\mu_\text{phys} \sim M_\text{Planck} is postulated. If μphys=MGUT∼10−3MPlanck\mu_\text{phys} = M_\text{GUT} \sim 10^{-3} M_\text{Planck}, the gravitino mass shifts by 3–6 orders of magnitude. Anchoring μphys\mu_\text{phys} to a specific scale is an open question.


5. Superpartner Mass Spectrum [H]​

Theorem 5.1 (Full SUSY spectrum) [H]

With gravity mediation:

ParticleMassObservability
Squarks q~\tilde{q}∼1013\sim 10^{13} GeVUnobservable at LHC
Sleptons l~\tilde{l}∼1013\sim 10^{13} GeVUnobservable
Gluino g~\tilde{g}∼1013\sim 10^{13} GeVUnobservable
Wino/Bino∼1011\sim 10^{11} GeVUnobservable
Higgsino∼1013\sim 10^{13} GeVUnobservable
Gravitino ψ3/2\psi_{3/2}∼1013\sim 10^{13} GeVUnobservable

Wino/bino masses are suppressed by a loop factor α/(4π)\alpha/(4\pi) relative to m3/2m_{3/2}:

mwino/bino∼m3/2⋅α4π∼1013×10−2=1011  GeVm_{\text{wino/bino}} \sim m_{3/2} \cdot \frac{\alpha}{4\pi} \sim 10^{13} \times 10^{-2} = 10^{11} \; \text{GeV}

5.1 Dark Matter Problem [H]​

At mSUSY∼1013m_\text{SUSY} \sim 10^{13} GeV there is no stable light superpartner (WIMP). If the wino/bino (∼1011\sim 10^{11} GeV) is the lightest superpartner (LSP), its mass exceeds the dark matter scale (∼\sim TeV) by many orders of magnitude. The Gap theory does not offer a SUSY dark matter candidate; see dark matter for alternative mechanisms.

Falsifiable Prediction​

The Gap theory predicts the absence of superpartners at the scales of the LHC and future colliders (s<105\sqrt{s} < 10^5 GeV). The discovery of any superpartner with mass ≪1013\ll 10^{13} GeV falsifies the Gap estimate εGUT∼10−3\varepsilon_{\text{GUT}} \sim 10^{-3}.

Indirect signatures of SUSY:

  1. Unification of gauge couplings at μGUT∼2×1016\mu_{\text{GUT}} \sim 2 \times 10^{16} GeV
  2. Higgs mass mH≈125m_H \approx 125 GeV — within the MSSM with heavy stops
Remark on gauge coupling unification [H]

At mSUSY∼1013m_\text{SUSY} \sim 10^{13} GeV the gauge coupling beta functions contain threshold corrections: below 101310^{13} GeV they run according to SM rules, above — according to MSSM rules. The prediction of unification at μGUT∼2×1016\mu_\text{GUT} \sim 2 \times 10^{16} GeV requires precise accounting of these threshold effects.


6. SUSY Compensation of Λ\Lambda [✗/H]​

6.1 Boson–Fermion Cancellation [T]​

N=1N=1 SUSY from G2G_2 provides cancellation of quadratic divergences in the vacuum energy:

(a) In unbroken SUSY: ΛSUSY=0\Lambda_\text{SUSY} = 0 (exact boson–fermion cancellation for each superpartner multiplet).

(b) After SUSY breaking: the residual vacuum energy is given by the standard formula:

Λresidual∼F2MPlanck2∼m3/22 MPlanck2\Lambda_\text{residual} \sim \frac{F^2}{M_\text{Planck}^2} \sim m_{3/2}^2 \, M_\text{Planck}^2

(c) With m3/2∼1013m_{3/2} \sim 10^{13} GeV:

Λresidual∼(1013)2×(1019)2=1064  GeV4\Lambda_\text{residual} \sim (10^{13})^2 \times (10^{19})^2 = 10^{64} \; \text{GeV}^4

The observed value Λobs∼10−47\Lambda_\text{obs} \sim 10^{-47} GeV4^4. The discrepancy is ∼10111\sim 10^{111} — gravity mediation with m3/2∼1013m_{3/2} \sim 10^{13} GeV does not solve the Λ\Lambda problem. SUSY compensates only ∼12\sim 12 orders out of 120.

Detailed breakdown of the suppression: in dimensionless units (MPlanck=1M_\text{Planck} = 1):

ΛresidualΛbare∼F2/MPlanck2MPlanck4=(2×10−6)21≈4×10−12\frac{\Lambda_\text{residual}}{\Lambda_\text{bare}} \sim \frac{F^2 / M_\text{Planck}^2}{M_\text{Planck}^4} = \frac{(2 \times 10^{-6})^2}{1} \approx 4 \times 10^{-12}

i.e., SUSY compensates quadratic divergences by ∼12\sim 12 orders of magnitude (out of the required ∼120\sim 120). The remaining ∼108\sim 108 orders require other mechanisms, discussed in the Λ\Lambda budget.

6.2 Sectoral Exact SUSY [✗]​

Retracted [✗]

"Sectoral SUSY" (exact cancellation in the 33-to-3ˉ\bar{3} sector with breaking in the O-sectors) — is incorrect. In standard supergravity, SUSY is broken globally: if Fi≠0F_i \neq 0 for at least one field, all superpartners acquire masses. It is impossible to have "SUSY breaking only in some sectors" without a sequestering mechanism.

The claim "9/21 pairs are exactly compensated" — is overstated. More accurately: mSUSY(33ˉ)∼εsoft⋅m3/2m_{\text{SUSY}}^{(3\bar{3})} \sim \varepsilon_{\text{soft}} \cdot m_{3/2}, but not zero.

The idea of sectoral exact SUSY assumed that in the confinement sector (33-to-3ˉ\bar{3}, 9 pairs out of 21) as Gap →0\to 0, supersymmetry remains exact, while breaking only affects the O-sectors. This would give a SUSY-compensated fraction of 9/21≈43%9/21 \approx 43\%. However:

  • Global SUSY breaking is transmitted to all sectors via gravitational interactions (gravity-mediated SUSY breaking)
  • Exact cancellation in a single sector is impossible when m3/2≠0m_{3/2} \neq 0
  • In the Gap formalism all 21 coherences are coupled via VGapV_\text{Gap}, which rules out sector isolation

6.3 SUSY Compensation via Sequestering [H]​

In place of the refuted sectoral SUSY, a mechanism of approximate sequestering is proposed:

(a) As Gap →0\to 0 in the 33-to-3ˉ\bar{3} sector: the coupling between this sector and the O-sectors (where SUSY is broken) is suppressed:

msoft(33ˉ)∼m3/2⋅Gaplink∼1013⋅εm_{\text{soft}}^{(3\bar{3})} \sim m_{3/2} \cdot \text{Gap}_{\text{link}} \sim 10^{13} \cdot \varepsilon

where Gaplink∼ε\text{Gap}_{\text{link}} \sim \varepsilon is the Gap between the confinement sector and the O-sector.

(b) At ε∼10−3\varepsilon \sim 10^{-3}: msoft(33ˉ)∼1010m_{\text{soft}}^{(3\bar{3})} \sim 10^{10} GeV ≠0\neq 0. The cancellation is not exact, but suppressed.

(c) Confinement-sector contribution to Λ\Lambda:

Λ33ˉ∼(msoft(33ˉ))2⋅MPlanck2∼1020⋅1038=1058  GeV4\Lambda_{3\bar{3}} \sim \left(m_{\text{soft}}^{(3\bar{3})}\right)^2 \cdot M_\text{Planck}^2 \sim 10^{20} \cdot 10^{38} = 10^{58} \; \text{GeV}^4

This is suppressed by ∼6\sim 6 orders of magnitude compared to Λbare∼1064\Lambda_\text{bare} \sim 10^{64} GeV4^4 (from direct SUSY breaking), but is not zero.

(d) Exact cancellation "9/21 = 0" is replaced by "9/21 suppressed by ε2\varepsilon^2".

The distinction from Randall–Sundrum-type sequestering (Randall–Sundrum, 1999): in classical sequestering the sectors are physically separated in extra dimensions. In the Gap formalism all 21 coherences are coupled via VGapV_\text{Gap}, and the suppression is provided not by geometric separation but by the smallness of the Gap parameter ε\varepsilon in inter-sector couplings. Estimating εsoft\varepsilon_\text{soft} (which determines the accuracy of sequestering) through the structure of VGapV_\text{Gap} remains an open problem.

Summary

SUSY does not contribute a new multiplicative suppression to the Λ\Lambda budget in the current formulation. In gravity mediation with m3/2∼1013m_{3/2} \sim 10^{13} GeV, SUSY breaking is maximal in the O-sectors. Approximate sequestering gives an additional suppression of ∼ε2∼10−6\sim \varepsilon^2 \sim 10^{-6} only in the confinement sector, which does not change the order of the total Λ\Lambda budget.


7. SUSY Protection in the UV [H]​

N=1N=1 supersymmetry provides partial protection against ultraviolet divergences. The non-renormalization theorem (Seiberg, 1993) guarantees that the superpotential WW receives no perturbative corrections. However, SUSY is broken at m3/2∼1013m_{3/2} \sim 10^{13} GeV, so SUSY protection only operates above this scale.

In the supersymmetric Gap theory some divergences cancel. For scalar masses:

  • Above 101310^{13} GeV: no quadratic divergences (SUSY cancellation)
  • Below 101310^{13} GeV: standard quadratic sensitivity to the UV cutoff

This does not solve the hierarchy problem in its classical formulation (protection of the electroweak scale), but limits divergences in the Gap sector at Planck energies.

In the supersymmetric Gap theory with 21 scalars and 21 gapsinos, the total number of variables (42) is finite at each site. The compactness of the target space (S1)21(S^1)^{21} and the G2G_2-symmetry acting on the phases further constrain the structure of divergences. The non-perturbative finiteness of the Gap theory remains a hypothesis [H], relying on the combined effect of these properties.


Summary Table​

ResultStatusDependence
N=1N=1 SUSY from covariantly constant spinor η0\eta_0[T]G2G_2-holonomy
Superpotential W=μW∑fijkΘΘΘW = \mu_W \sum f_{ijk} \Theta\Theta\Theta[T]G2G_2-invariance + Schur (T-50)
Superpartner spectrum from Gap fields[T]Follows from WW
SUSY breaking: F=∂W/∂Θ≠0F = \partial W / \partial \Theta \neq 0[T]W≠0W \neq 0 in vacuum
F∼ε⋅MPl\sqrt{F} \sim \varepsilon \cdot M_\text{Pl}[T]From superpotential
m3/2∼ε3MP≈1013m_{3/2} \sim \varepsilon^3 M_P \approx 10^{13} GeV[T]Cubic structure of WW
mq~∼1013m_{\tilde{q}} \sim 10^{13} GeV (gravity mediation)[T]Follows from m3/2m_{3/2}
Sectoral exact SUSY[✗]Retracted
Approximate sequestering (ε2\varepsilon^2-suppression)[H]Replacement for sectoral SUSY
SUSY protection in UV (above 101310^{13} GeV)[H]Compactness (S1)21(S^1)^{21} + G2G_2

Open Questions​

  1. Kähler metric. The Kähler potential KK on the moduli of G2G_2-compactification is generally non-canonical. Corrections to KK may modify the scale μW\mu_W and the spectrum by an O(1)O(1) factor.
  2. Anchoring μphys\mu_\text{phys}. The physical scale that restores the dimension of the F-term is postulated as MPlanckM_\text{Planck}, but is not derived from first principles.
  3. Estimating εsoft\varepsilon_\text{soft}. The coupling parameter between the confinement sector and the O-sectors determines the accuracy of approximate sequestering, but has not yet been computed.
  4. Gauge coupling unification. Threshold corrections from heavy superpartners (mSUSY∼1013m_\text{SUSY} \sim 10^{13} GeV) on running gauge constants require precise computation.