Compact QED in the dyon phase maps to a massive two-form field whose IR fixed-point string theory reproduces a generalized Arvis potential and matches heaviest quarkonium mass ratios to 2.5 percent while raising the Regge intercept above the Nambu-Goto value.
Compact gauge fields and the infrared catastrophe
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Refines charge quantization via homotopy type A whose homotopy groups classify brane charges and homology groups classify higher-form symmetries, deriving swampland-like constraints that rule out noncompact gauge groups and non-nilpotent Lie algebras for field strengths.
Field theories with ℤ_N p-form symmetry generically admit a Coulomb phase where the infrared theory is Abelian p-form electrodynamics, illustrated via continuum and lattice examples.
TransitionListener v2.0 supplies an end-to-end pipeline from scalar potential to gravitational wave spectra with improved handling of transition dynamics and bubble separation.
citing papers explorer
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Universal Confining Strings: From Compact QED to the Hadron Spectrum
Compact QED in the dyon phase maps to a massive two-form field whose IR fixed-point string theory reproduces a generalized Arvis potential and matches heaviest quarkonium mass ratios to 2.5 percent while raising the Regge intercept above the Nambu-Goto value.
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Generalised Symmetries and Swampland-Type Constraints from Charge Quantisation via Rational Homotopy Theory
Refines charge quantization via homotopy type A whose homotopy groups classify brane charges and homology groups classify higher-form symmetries, deriving swampland-like constraints that rule out noncompact gauge groups and non-nilpotent Lie algebras for field strengths.
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Discrete $p$-Form Symmetry and Higher Coulomb Phases
Field theories with ℤ_N p-form symmetry generically admit a Coulomb phase where the infrared theory is Abelian p-form electrodynamics, illustrated via continuum and lattice examples.
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TransitionListener v2.0 -- Robust gravitational wave predictions for cosmological phase transitions
TransitionListener v2.0 supplies an end-to-end pipeline from scalar potential to gravitational wave spectra with improved handling of transition dynamics and bubble separation.