2019
DOI: 10.1007/jhep11(2019)147
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Scalar dark matter coannihilating with a coloured fermion

Abstract: We analyze the phenomenology of a simplified model for a real scalar dark matter candidate interacting with quarks via a coloured fermionic mediator. In the coannihilation regime, the dark matter abundance is controlled by the dynamics of the coloured fermions which can be significantly affected by non-perturbative effects. We employ a non-relativistic effective field theory which allows us to systematically treat the Sommerfeld effect and bound state formation in the early Universe. The parameter space compat… Show more

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Cited by 37 publications
(41 citation statements)
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“…By using another formalism valid at high temperature but limited to the assumption of ionization equilibrium, environmental corrections to the upper formula of (5.9) have been studied in the literature [90][91][92][93][94][95]. The method is based on an effective in-medium potential, which shows next to the expected Debye screening mass, a temperature dependent energy shift (Salpeter correction), as well as an imaginary thermal width [96,97].…”
Section: Jhep09(2020)086mentioning
confidence: 99%
“…By using another formalism valid at high temperature but limited to the assumption of ionization equilibrium, environmental corrections to the upper formula of (5.9) have been studied in the literature [90][91][92][93][94][95]. The method is based on an effective in-medium potential, which shows next to the expected Debye screening mass, a temperature dependent energy shift (Salpeter correction), as well as an imaginary thermal width [96,97].…”
Section: Jhep09(2020)086mentioning
confidence: 99%
“…As discussed above, the coannihilation of the dark matter S with the VLQs would play a crucial role in explaining the relic density. It has been also shown in [33][34][35][36][37] that the annihilation among the VLQs themselves can give a significant contribution towards the relic density of the DM. The relic density of the DM with mass m S is given by [5]…”
Section: A Methodologymentioning
confidence: 96%
“…1, one can see that the dark matter S can also annihilate into gluon pair (gg) at one loop (through box diagram). It has been shown in [33][34][35][36][37] that with a larger choice of Yukawa coupling (here α) this annihilation of S to the gluon pair can provide a significant contribution to the relic of S. In [34], the authors notice that for the mass regime m S < m t with the Yukawa coupling of ∼Oð10Þ the correct relic density can be satisfied. This large Yukawa coupling (involving upquark) however can create a problem in the DD of the dark matter as it will generate a large spin independent cross section and hence can be on the verge of being excluded by the DD searches.…”
Section: Combined Analysis Of Dm and Ew Vacuum Stabilitymentioning
confidence: 99%
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