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March 8, 20260 citationsOpen Access

Two-Component Dark Matter and Cosmology in the TQF Framework (v2)

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SRSUdhakar Rajnikant

Key Points

  • The aim is to explore dark matter candidates and cosmological implications within the Timeless Quantum Field framework, tied to gauge theories.
  • Formulated a scale-invariant gauge theory based on SU(5) symmetry.
  • Identified a viable Higgs-portal dark matter candidate through portal interactions.
  • Applied analytic estimates and a numerical scan of parameter space for dark matter relic density.
  • Considered multi-component dark matter scenarios involving both scalar and axion-like particles.
  • Investigated the gravitational sector's influence on inflationary dynamics.
  • Identified regions consistent with observed dark matter relic density and detection constraints.
  • Predicted dark matter masses near the electroweak scale.
  • Established a scaling relation linking dark matter mass with nonminimal couplings in gravity.
  • Demonstrated that inflation is driven by a scalaron influenced by curvature terms.

Abstract

We investigate the dark matter and cosmological implications of the Timeless Quantum Field (TQF), formulated as a scale-invariant extension of a grand unified gauge theory based on SU (5) symmetry. The model contains an extended scalar sector including an adjoint field responsible for grand unified symmetry breaking together with additional singlet scalars. Within this setup, a real scalar field X, stabilized by a discrete Z₂ symmetry, emerges as a viable Higgs-portal dark matter candidate. The dark matter particle interacts with the visible sector through portal interactions of the form (H†H) X2, which govern the annihilation processes responsible for setting the thermal relic abundance. Using analytic freeze-out estimates and a numerical scan of the parameter space, we identify regions consistent with the observed dark matter relic density and current direct-detection constraints. The framework also naturally admits a multi-component dark matter scenario in which the scalar particle X provides a WIMP component while an axion-like particle associated with the scale-invariant sector may contribute a dominant fraction of the cosmological dark matter density. The gravitational sector of the model includes quadratic curvature terms together with nonminimal couplings between scalar fields and gravity. Inflation is driven primarily by the scalaron generated by the R² term, while scalar nonminimal couplings influence the inflationary dynamics. In this setup, inflationary normalization leads to an approximate scaling relation linking the dark matter mass with the nonminimal coupling appearing in the gravitational sector. The TQF framework therefore provides a unified scenario connecting grand unified symmetry breaking, dark matter phenomenology, and inflationary cosmology within a single scale-invariant theory. The resulting parameter space predicts dark matter masses near the electroweak scale and can be probed by current and upcoming direct detection experiments as well as collider searches.

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Cite This Study

SUdhakar Rajnikant (2026) studied this question.

synapsesocial.com/papers/69ada962bc08abd80d5bcaa7https://doi.org/10.5281/zenodo.18898564
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