A single adjoint scalar plus singlet in a 5D domain-wall setup realizes dynamical branes, chiral fermion localization, SU(5) breaking, gauge trapping, and Higgs localization while reproducing weak-scale Yukawa couplings via renormalization-group flow.
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Scientific rewards in physics arise from contributions that transform the Polydoxon—the structured set of viable theories—via expansion, contraction, reconfiguration, or enabling moves, with reward scaling by the transformation's scope, centrality, depth, and leverage.
No evidence found; excludes semiclassical black holes below 8.4-11.4 TeV and string balls below 9.0-10.7 TeV at 95% CL, and caps the quark-quark sphaleron fraction above 9 TeV at 0.0034.
Conformal and scale-invariant gravity theories in d dimensions have distinct properties from 4D analogues, enabled by a new formulation method.
DESI data indicating evolving dark energy may allow string theory to describe observed universes without violating swampland constraints on constant dark energy.
citing papers explorer
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Five benefits of grand unified $SU(5)$ brane world scenario
A single adjoint scalar plus singlet in a 5D domain-wall setup realizes dynamical branes, chiral fermion localization, SU(5) breaking, gauge trapping, and Higgs localization while reproducing weak-scale Yukawa couplings via renormalization-group flow.
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Polydoxon Transformations and Scientific Reward in Physics
Scientific rewards in physics arise from contributions that transform the Polydoxon—the structured set of viable theories—via expansion, contraction, reconfiguration, or enabling moves, with reward scaling by the transformation's scope, centrality, depth, and leverage.
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A search for microscopic black holes, string balls, and sphalerons in proton-proton collisions at $\sqrt{s}$ = 13 TeV
No evidence found; excludes semiclassical black holes below 8.4-11.4 TeV and string balls below 9.0-10.7 TeV at 95% CL, and caps the quark-quark sphaleron fraction above 9 TeV at 0.0034.
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How to deal with conformal and pure scale-invariant theories of gravity in d dimensions?
Conformal and scale-invariant gravity theories in d dimensions have distinct properties from 4D analogues, enabled by a new formulation method.
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Breaking Free from the Swampland of Impossible Universes through the DESI Portal
DESI data indicating evolving dark energy may allow string theory to describe observed universes without violating swampland constraints on constant dark energy.