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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.

how it is stated · asserted 0.38 read the record →

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arXiv ID2105.09044 (version 2)
Pith IDNUFU2IZT, Pith's permanent record of this paper and its review
CitationBaradhwaj Coleppa, Kousik Loho, Tanushree Basak. "An update on the two singlet Dark Matter model." arXiv:2105.09044 (2021). https://pith.science/paper/NUFU2IZT
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Compiled by classifier-1.13.0 via TypeSafe API, question bank abstract-p1-20260923, 2026-09-23: 1 request, 5,593 input tokens.

What the abstract itself states, as probabilities: claims first 0.02 · states limitation 0.57 · human participants 0.01 · controlled comparison 0.03 · randomized assignment 0.01 · states quantitative result 0.87 · compares with prior results 0.15 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v2. Results and the main claim are underlined; .

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

What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
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

What kind of paper the classifier reports this is: theoretical result 0.92 · evidence from analysis of existing data 0.83.

What was examined, and what was not

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  • figures and tables
  • references and citing sentences
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Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

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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References
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4 arXiv papers cite this in 4 sentences

Each citing sentence is taken from the citing paper's LaTeX source and typed by Pith's classifier. A label appears at probability 0.8 or more (0.95 for support), a contest at 0.7 or more; the quoted words are the citing authors'. How each label was checked · JSON

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