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Thermally Generated Gauge Singlet Scalars as Self-Interacting Dark Matter

John McDonald

TL;DR

The paper explores whether a gauge-singlet scalar $S$ coupled to the Standard Model through the Higgs portal $\lambda_S S^\dagger S H^\dagger H$ can serve as self-interacting dark matter (SIDM) while achieving the observed relic density via thermal generation. Using Boltzmann equation analysis, it shows that $S$ can obtain $\Omega_S \approx 0.3$ with $m_S$ in the MeV range, particularly when $m_S$ is generated entirely by the Higgs vev, leading to a predictive relation $m_S = 2.9\left(\frac{\Omega_S}{0.3}\right)^{1/5}\left(\frac{h}{0.7}\right)^{2/5}\left(\frac{m_h}{115\mathrm{GeV}}\right)^{3/5}\mathrm{MeV}$. The SIDM cross-section requirements then favor a self-coupling of order $\eta \sim 0.1$, while the corresponding Higgs-portal coupling is $\lambda_S \approx 2.7\times10^{-10}\left(\frac{\Omega_S}{0.3}\right)^{2/5}\left(\frac{h}{0.7}\right)^{4/5}\left(\frac{m_h}{115\mathrm{GeV}}\right)^{6/5}$, ensuring very weak SM interactions. This framework yields a self-consistent picture where light DM with small SM couplings can naturally exhibit sizable self-interactions in agreement with SIDM phenomenology, linking relic density to SIDM cross-sections in a testable way.

Abstract

We show that a gauge singlet scalar S, with a coupling to the Higgs doublet of the form lambda_{S} S^{\dagger}S H^{\dagger}H and with the S mass entirely generated by the Higgs expectation value, has a thermally generated relic density Omega_{S} \approx 0.3 if m_{S} \approx (2.9-10.5)(Omega_{S}/0.3)^{1/5}(h/0.7)^{2/5} MeV for Higgs boson masses in the range 115 GeV to 1 TeV. Remarkably, this is very similar to the range (m_{S} = (6.6-15.4)η^{2/3} MeV) required in order for the self-interaction (η/4)(S^{\dagger}S)^{2} to account for self-interacting dark matter when ηis not much smaller than 1. The corresponding coupling is lambda_{S} \approx (2.7 \times 10^{-10} - 3.6 \times 10^{-9})(Omega_{S}/0.3)^{2/5}(h/0.7)^{4/5}, implying that such scalars are very weakly coupled to the Standard Model sector.

Thermally Generated Gauge Singlet Scalars as Self-Interacting Dark Matter

TL;DR

The paper explores whether a gauge-singlet scalar coupled to the Standard Model through the Higgs portal can serve as self-interacting dark matter (SIDM) while achieving the observed relic density via thermal generation. Using Boltzmann equation analysis, it shows that can obtain with in the MeV range, particularly when is generated entirely by the Higgs vev, leading to a predictive relation . The SIDM cross-section requirements then favor a self-coupling of order , while the corresponding Higgs-portal coupling is , ensuring very weak SM interactions. This framework yields a self-consistent picture where light DM with small SM couplings can naturally exhibit sizable self-interactions in agreement with SIDM phenomenology, linking relic density to SIDM cross-sections in a testable way.

Abstract

We show that a gauge singlet scalar S, with a coupling to the Higgs doublet of the form lambda_{S} S^{\dagger}S H^{\dagger}H and with the S mass entirely generated by the Higgs expectation value, has a thermally generated relic density Omega_{S} \approx 0.3 if m_{S} \approx (2.9-10.5)(Omega_{S}/0.3)^{1/5}(h/0.7)^{2/5} MeV for Higgs boson masses in the range 115 GeV to 1 TeV. Remarkably, this is very similar to the range (m_{S} = (6.6-15.4)η^{2/3} MeV) required in order for the self-interaction (η/4)(S^{\dagger}S)^{2} to account for self-interacting dark matter when ηis not much smaller than 1. The corresponding coupling is lambda_{S} \approx (2.7 \times 10^{-10} - 3.6 \times 10^{-9})(Omega_{S}/0.3)^{2/5}(h/0.7)^{4/5}, implying that such scalars are very weakly coupled to the Standard Model sector.

Paper Structure

This paper contains 5 sections, 23 equations.