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Generalized Three-Family Supersymmetric Pati-Salam Models from Type IIA Intersecting D6-Branes

Tianjun Li, Qi Sun, Rui Sun, Lina Wu

TL;DR

This work broadens the landscape of ${ m N}=1$ supersymmetric Pati-Salam models from Type IIA intersecting D6-branes by generalizing the three-family condition to $I_{ac}=-(3+h)$, $I_{ac'}=h$ and identifying four new model classes that realize three generations without requiring parallel brane configurations. It introduces a systematic, Diophantine-based construction strategy, analyzes the massless spectra and hidden USp sectors of the four models, and demonstrates that distinct gauge-coupling relations emerge at the string scale. To achieve string-scale unification, the authors deploy two mechanisms: (i) symmetry breaking of ${ m SU}(2)_{L_1} imes{ m SU}(2)_{L_2}$ to a diagonal ${ m SU}(2)_{L'}$ which suppresses $g_{L'}$, and (ii) the inclusion of vector-like exotics from ${ m N}=2$ subsectors that modify two-loop RG running. Through detailed RG analyses, they show that these ingredients can yield precise gauge-coupling unification near $M_{ m string}\,(\sim 5 imes10^{17} ext{ GeV})$ for the extended Pati-Salam models. Overall, the paper expands the model-building landscape and provides viable pathways to reconcile low-energy phenomenology with a string-scale unification framework.

Abstract

Generalizing three-family chiral fermion conditions to $I_{ac}=-(3+h)$ and $I_{ac'}=h$, with positive integer $h$, we extend the landscape of three-family ${\cal N}=1$ supersymmetric Pati-Salam models in a broader region. Differing from the former investigation with $I_{ac}=-3$ and $I_{ac'}=0$, we do not restrict that the $a$ stack of D6-branes must be parallel to the orientifold image of the $c$-stack along one of the three two-tori. In this investigation, without the simple parallel construction, we find four new classes of supersymmetric Pati-Salam models that are allowed by the extended three generation condition with $I_{ac}=3, I_{ac'}=-6$ and $I_{ac}=-1, I_{ac'}=-2$ through the intersections of $a$- and $c/c'$-branes. Moreover, with the $SU(2)_{L'}$ gauge coupling realized from $SU(2)_{L_1}\times SU(2)_{L_2}$ symmetry breaking, the canonical normalization requirement of the gauge kinetic term provides an alternative approach that can be imposed before the renormalization group equation evolution for $SU(2)_{L'}$ gauge coupling. This turns out to be an effective mechanism to realize the string-scale gauge coupling relation, especially for the new supersymmetric Pati-Salam models with large $g_b/g_a$ ratio. We show that this symmetry-breaking modified renormalization group evolution can highly suppress $g_b/g_a$, and finally realizes string-scale gauge coupling relations for the extended supersymmetric Pati-Salam models as well.

Generalized Three-Family Supersymmetric Pati-Salam Models from Type IIA Intersecting D6-Branes

TL;DR

This work broadens the landscape of supersymmetric Pati-Salam models from Type IIA intersecting D6-branes by generalizing the three-family condition to , and identifying four new model classes that realize three generations without requiring parallel brane configurations. It introduces a systematic, Diophantine-based construction strategy, analyzes the massless spectra and hidden USp sectors of the four models, and demonstrates that distinct gauge-coupling relations emerge at the string scale. To achieve string-scale unification, the authors deploy two mechanisms: (i) symmetry breaking of to a diagonal which suppresses , and (ii) the inclusion of vector-like exotics from subsectors that modify two-loop RG running. Through detailed RG analyses, they show that these ingredients can yield precise gauge-coupling unification near for the extended Pati-Salam models. Overall, the paper expands the model-building landscape and provides viable pathways to reconcile low-energy phenomenology with a string-scale unification framework.

Abstract

Generalizing three-family chiral fermion conditions to and , with positive integer , we extend the landscape of three-family supersymmetric Pati-Salam models in a broader region. Differing from the former investigation with and , we do not restrict that the stack of D6-branes must be parallel to the orientifold image of the -stack along one of the three two-tori. In this investigation, without the simple parallel construction, we find four new classes of supersymmetric Pati-Salam models that are allowed by the extended three generation condition with and through the intersections of - and -branes. Moreover, with the gauge coupling realized from symmetry breaking, the canonical normalization requirement of the gauge kinetic term provides an alternative approach that can be imposed before the renormalization group equation evolution for gauge coupling. This turns out to be an effective mechanism to realize the string-scale gauge coupling relation, especially for the new supersymmetric Pati-Salam models with large ratio. We show that this symmetry-breaking modified renormalization group evolution can highly suppress , and finally realizes string-scale gauge coupling relations for the extended supersymmetric Pati-Salam models as well.

Paper Structure

This paper contains 11 sections, 44 equations, 3 figures, 54 tables.

Figures (3)

  • Figure 1: The evolution of two-loop gauge couplings in the Model 1 with vector-like particles $(XU, \overline{XU})$ and $(XD, \overline{XD})$. The masses of these particles are set as $M_{XU}=1.0\times 10^{13}$ GeV (left panel) and $M_{XD}=5\times 10^{16}$ GeV, $M_{XU}=3.2\times 10^{13}$ GeV (right panel).
  • Figure 2: The evolution of two-loop gauge couplings in the Model 2 with vector-like particles $(XU, \overline{XU})$ and $(XD, \overline{XD})$. The masses of these particles are set as $M_{XU}=2.0\times 10^{6}$ GeV (left panel) and $M_{XD}=2.24\times 10^{13}$ GeV, $M_{XU}=1.78\times 10^{10}$ GeV (right panel).
  • Figure 3: The evolution of two-loop gauge couplings in the Model 3-m with vector-like particles $5(XQ, \overline{XQ})+3XG$. The masses of these particles are set as $M_{XQ}=M_{XG}=6.0\times 10^{15}$ GeV.