Exploring how Higgs vacuum dynamics and spacetime geometry may jointly explain galaxies, inflation, and cosmic acceleration.
If you’re curious about where the HGVM framework stands today, HGVM is now being developed as a step-by-step research program rather than a finished theory. The papers below present its current pillars across galaxies, inflation, and late-time cosmic acceleration, while making clear what is established, what remains phenomenological, and what is still open.
HGVM Paper I — Galaxy Rotation Curves without Dark Matter
Paper I provides the first quantitative galactic test of HGVM. Applied to the full 171-galaxy SPARC sample, it shows that the framework can reproduce galaxy rotation curves with three universal parameters, while also identifying the transition scale r0 as an effective quantity whose microscopic origin remains open.
HGVM Paper II — Cosmic Inflation
Paper II focuses on the inflationary sector and shows that, in the specific case h(phi) = phi², HGVM reduces to a viable Higgs-inflation / Starobinsky-type limit consistent with observations. It also shows that the inflationary sector is coherent but not the main distinctive observational signature of the framework.
HGVM Paper III — Late-Time Cosmic Acceleration
Paper III extends HGVM to late-time cosmic acceleration and explores how a geometric threshold may connect galactic and cosmological acceleration scales. It should be read as a further pillar of the program rather than a final first-principles completion, since one key galactic ingredient still remains to be derived in Paper IV.
