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An update on the two singlet Dark Matter model
High Energy Physics - Phenomenology · Submitted 19 May 2021
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim Further, we study the viability of explaining the observed gamma-ray excess in the galactic center in this model with a dark matter of mass in the $\sim 36-51$ GeV window and present our conclusions.
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The abstract, sentence by sentence
We revisit the two real singlet extension of the Standard Model with a $Z_2\times Z_2^\prime$ symmetry. One of the singlet scalars $S_2$, by virtue of an unbroken $Z_2^\prime$ symmetry, plays the role of a stable dark matter candidate. The other scalar $S_1$, with spontaneously broken $Z_2$-symmetry, mixes with the SM Higgs boson and acts as the scalar mediator. We analyze the model by putting in the entire set of theoretical and recent experimental constraints. The latest bounds from direct detection Xenon1T experiment severely restricts the allowed region of parameter space of couplings. To ensure the dark matter satisfies the relic abundance criterion, we rely on the Breit-Wigner enhanced annihilation cross-section. Further, we study the viability of explaining the observed gamma-ray excess in the galactic center in this model with a dark matter of mass in the $\sim 36-51$ GeV window and present our conclusions.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We revisit the two real singlet extension of the Standard Model with a $Z_2\times Z_2^\prime$ symmetry. | contribution 0.71 | 0.77 | 0.03 | asserted 0.69 |
| s1 | One of the singlet scalars $S_2$, by virtue of an unbroken $Z_2^\prime$ symmetry, plays the role of a stable dark matter candidate. | background 0.46 | 0.17 | 0.05 | asserted 1.00 |
| s2 | The other scalar $S_1$, with spontaneously broken $Z_2$-symmetry, mixes with the SM Higgs boson and acts as the scalar mediator. | background 0.53 | 0.22 | 0.03 | asserted 1.00 |
| s3 | We analyze the model by putting in the entire set of theoretical and recent experimental constraints. | method 0.68 | 0.91 | 0.03 | asserted 0.94 |
| s4 | The latest bounds from direct detection Xenon1T experiment severely restricts the allowed region of parameter space of couplings. | result 0.87 | 0.16 | 0.21 | asserted 1.00 |
| s5 | To ensure the dark matter satisfies the relic abundance criterion, we rely on the Breit-Wigner enhanced annihilation cross-section. | method 0.89 | 0.54 | 0.08 | asserted 0.95 |
| s6 | Further, we study the viability of explaining the observed gamma-ray excess in the galactic center in this model with a dark matter of mass in the $\sim 36-51$ GeV window and present our conclusions. | contribution 0.97 | 0.88 | 0.38 | asserted 0.38 |
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The paper
Original abstract
We revisit the two real singlet extension of the Standard Model with a $Z_2\times Z_2^\prime$ symmetry. One of the singlet scalars $S_2$, by virtue of an unbroken $Z_2^\prime$ symmetry, plays the role of a stable dark matter candidate. The other scalar $S_1$, with spontaneously broken $Z_2$-symmetry, mixes with the SM Higgs boson and acts as the scalar mediator. We analyze the model by putting in the entire set of theoretical and recent experimental constraints. The latest bounds from direct detection Xenon1T experiment severely restricts the allowed region of parameter space of couplings. To ensure the dark matter satisfies the relic abundance criterion, we rely on the Breit-Wigner enhanced annihilation cross-section. Further, we study the viability of explaining the observed gamma-ray excess in the galactic center in this model with a dark matter of mass in the $\sim 36-51$ GeV window and present our conclusions.
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4 arXiv papers cite this in 4 sentences
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Cites it as background 1 paper
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Different scenarios for two-scalar model with emphasis on dark matter phenomenology are investigated recently in [ref] .
Loop quantum effects on direct detection prediction in two-scalar dark matter scenario · Introduction · 0.98
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