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Electroweak breaking and Dark Matter from the common scale

Branimir Radovcic, Sanjin Benic

TL;DR

This work proposes a classically scale-invariant extension of the Standard Model featuring a dark $U(1)_X$ sector with a doubly charged scalar $Φ$ and a Majorana fermion $N$. The Coleman–Weinberg mechanism induces a radiative breaking along a flat direction, linking the electroweak scale to the dark-sector scale via the Higgs portal, while a remnant $Z_2$ stabilizes $N$ as a dark matter candidate. DM annihilation proceeds mainly through $NN\to φφ$, fixing the relic abundance and driving the dark-sector couplings to values that yield a scalon mass $m_φ^2=8 B v_r^2$; the interplay yields a DM mass in the range $500$ GeV to a few TeV and typically order-one hidden-sector couplings. The scenario also imposes collider constraints on the Higgs–scalon mixing, with the overall result that a consistent, testable connection between electroweak breaking and dark matter mass can arise from a common scale in a scale-invariant framework.

Abstract

We propose a classically scale invariant extension of the Standard Model where the electroweak symmetry breaking and the mass of the Dark Matter particle come from the common scale. We introduce $U(1)_X$ gauge symmetry and $X$-charged scalar $Φ$ and Majorana fermion $N$. Scale invariance is broken via Coleman-Weinberg mechanism providing the vacuum expectation value of the scalar $Φ$. Stability of the dark matter candidate $N$ is guaranteed by a remnant $Z_2$ symmetry. The Higgs boson mass and the mass of the Dark Matter particle have a common origin, the vacuum expectation value of $Φ$. Dark matter relic abundance is determined by annihilation $NN \to ΦΦ$. We scan the parameter space of the model and find the mass of the dark matter particle in the range from 500 GeV to a few TeV.

Electroweak breaking and Dark Matter from the common scale

TL;DR

This work proposes a classically scale-invariant extension of the Standard Model featuring a dark sector with a doubly charged scalar and a Majorana fermion . The Coleman–Weinberg mechanism induces a radiative breaking along a flat direction, linking the electroweak scale to the dark-sector scale via the Higgs portal, while a remnant stabilizes as a dark matter candidate. DM annihilation proceeds mainly through , fixing the relic abundance and driving the dark-sector couplings to values that yield a scalon mass ; the interplay yields a DM mass in the range GeV to a few TeV and typically order-one hidden-sector couplings. The scenario also imposes collider constraints on the Higgs–scalon mixing, with the overall result that a consistent, testable connection between electroweak breaking and dark matter mass can arise from a common scale in a scale-invariant framework.

Abstract

We propose a classically scale invariant extension of the Standard Model where the electroweak symmetry breaking and the mass of the Dark Matter particle come from the common scale. We introduce gauge symmetry and -charged scalar and Majorana fermion . Scale invariance is broken via Coleman-Weinberg mechanism providing the vacuum expectation value of the scalar . Stability of the dark matter candidate is guaranteed by a remnant symmetry. The Higgs boson mass and the mass of the Dark Matter particle have a common origin, the vacuum expectation value of . Dark matter relic abundance is determined by annihilation . We scan the parameter space of the model and find the mass of the dark matter particle in the range from 500 GeV to a few TeV.

Paper Structure

This paper contains 4 sections, 17 equations, 2 figures.

Figures (2)

  • Figure 1: Mass of the DM candidate $m_N$ (left) and dark sector gauge coupling $g_X$ (right) as a function of dark gauge boson mass $m_X$ and the scalon mass $m_\phi$. The lower region on the plot is excluded by the LHC bound on $\sin\theta$.
  • Figure 2: Mixing angle $\sin\theta$ (left) and the vev of $\Phi$, $v_\Phi$ (right) as a function of dark gauge boson mass $m_X$ and the scalon mass $m_\phi$. The lower region on the plot is excluded by the LHC bound on $\sin\theta$.