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Uniqueness of the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi mathvariant="normal">S</mml:mi><mml:mrow><mml:msub><mml:mrow><mml:mi mathvariant="normal">U</mml:mi></mml:mrow><mml:mrow><mml:mi>N</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math>gauge groups for implementing absolute proton stability with a global<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi mathvariant="normal">U</mml:mi></mml:mrow><mml:mrow><mml:mn>1</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math>of color

Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fieldsPublished 15 July 1978
Paul Langacker, Gino Segrè, H. Arthur Weldon
Citations18

Abstract

The problem of ensuring proton stability in grand unified models of the strong, weak, and electromagnetic interactions by means of a new conserved quantum number is investigated. It is assumed that spontaneous symmetry breaking will preserve an $\mathrm{S}{\mathrm{U}}_{3}^{c}$ of color. To guarantee that the new quantum number $\ensuremath{\chi}$ be conserved after the spontaneous symmetry breaking, we require that all color-singlet Higgs fields in the theory have $\ensuremath{\chi}=0$. This assumption has the following consequences: The gauge symmetry must be $\mathrm{S}{\mathrm{U}}_{N}$, the global symmetry must be ${\mathrm{U}}_{N}$, $\ensuremath{\chi}$ must generate the ${\mathrm{U}}_{1}^{c}$ of color, and only certain representations for the Higgs scalars are possible. Conservation of $\ensuremath{\chi}$ also restricts the possible $\mathrm{S}{\mathrm{U}}_{N}$ fermion assignments. In particular, if all fermions are either singlets, triplets, or antitriplets of color and if the only massless fermions are $\ensuremath{\chi}=0$ neutrinos, then conservation of $\ensuremath{\chi}$ requires that either the model is vectorlike or that there are many fermion representations, some of which include families of particles with unusual values of $\ensuremath{\chi}$. Both cases are anomaly free.

Keywords

Physics and Astronomy