Saturday 14 December 2019

string theory - What happens if the holonomy group lies in $SU(2)$ for a CY 3-fold?



I am a mathematician and reading a physics paper about the holonomy group of Calabi-Yau 3-folds.


In that paper, a Calabi-Yau 3-fold $X$ is defined as a compact 3-dimensional complex manifold with Kahler metric such that the holonomy group $G \subset SU(3)$ but not contained in any $SU(2)$ subgroup of $SU(3)$.


They remark "the condition that $G$ is not contained in $SU(2)$ is a really serious condition for physics since otherwise it would change the supersymmetry".


Could anyone kindly explain this sentence in more detail? I think that if $G\subset SU(2)$ the physics derived from the Calabi-Yau 3-fold has more supersymmetry (because less restriction), but what is wrong about it? One possibility is that too symmetric theory is trivial.


I would appreciate it if someone could kindly explain the physics behind it to a mathematician.



Answer



Let me elaborate on Ryan's correct comments.


The flat background makes all components of the spinors covariantly constant; so the geometry is compatible with all of SUSY.


A generic curved 6-real-dimensional manifold has an $O(6)$ holonomy or $SO(6)\sim SU(4)$ if it is orientable. The $SU(3)$ subgroup preserves 1/4 of the original supercharges – it is the single charge among $4$ in $SU(4)$ that is not included in $3$ of $SU(3)$ and therefore "not participating in the mixing" that destroys the covariant constancy. If the holonomy is $SU(2)$, then 2/4 of the original spinor components i.e. 1/2 of the supersymmetry is preserved.


In reality, the $SU(3)$ holonomy manifolds are the the usual generic Calabi-Yau three-folds. Starting from 16 supercharges i.e. $N=4$ of heterotic string theory, for example, they produce the realistic $N=1$. However, $SU(2)$ holonomy would produce $N=2$ in four dimensions which is too much. $N=2$ SUSY is too large for realistic models – at least for quarks and leptons – because it guarantees too large multiplets, left-right symmetry of spacetime (no chirality), and other strong constraints on the spectrum and the strength of various interactions that would disagree with observations.



The manifolds with the $SU(2)$ holonomy are pretty much just Calabi-Yaus of the form $K3\times T^2$ and perhaps some orbifolds of this manifold. So two of the six dimensions remain flat and decoupled from the other, curved four.


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