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SU(2)$_R$ and its Axion in Cosmology: A common Origin for Inflation, Cold Sterile Neutrinos, and Baryogenesis

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Azadeh Maleknejad

High Energy Physics - Phenomenology · Submitted 21 Dec 2020

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim This model merges three milestones of modern cosmology, i.e., inflation, cold dark matter, and baryon asymmetry.

how it is stated · asserted 1.00 read the record →

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arXiv ID2012.11516 (version 2)
Pith IDSR3IH7TP, Pith's permanent record of this paper and its review
CitationAzadeh Maleknejad. "SU(2)$_R$ and its Axion in Cosmology: A common Origin for Inflation, Cold Sterile Neutrinos, and Baryogenesis." arXiv:2012.11516 (2020). https://pith.science/paper/SR3IH7TP
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The compiled record

The paper's own sentences, arranged. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.

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Compiled by classifier-1.13.0 via TypeSafe API, question bank abstract-p1-20260923, 2026-09-23: 1 request, 6,460 input tokens.

What the abstract itself states, as probabilities: claims first 0.05 · states limitation 0.42 · human participants 0.01 · controlled comparison 0.01 · randomized assignment 0.01 · states quantitative result 0.92 · compares with prior results 0.08 · mentions code or data availability 0.01.

The abstract, sentence by sentence

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

We introduce an axion-inflation model embedded in the Left-Right symmetric extension of the SM in which $W_R$ is coupled to the axion. This model merges three milestones of modern cosmology, i.e., inflation, cold dark matter, and baryon asymmetry. Thus, it can naturally explain the observed coincidences among cosmological parameters, i.e., $\eta_{B}\approx P_{\zeta}$ and $\Omega_{DM} \simeq 5~\Omega_{B}$. The source of asymmetry is spontaneous CP violation in the physics of inflation, and the lightest right-handed neutrino is the cold dark matter candidate with mass $m_{N_1}\sim 1~GeV$. The introduced mechanism does not rely on the largeness of the unconstrained CP-violating phases in the neutrino sector nor fine-tuned masses for the heaviest right-handed neutrinos. It has two unknown fundamental scales, i.e. scale of inflation $\Lambda_{\rm inf}=\sqrt{HM_{Pl}}$ and left-right symmetry breaking $\Lambda_{F}$. Sufficient matter asymmetry demands $\Lambda_{\rm inf}\approx\Lambda_{F}$. The baryon asymmetry and dark matter today are remnants of a pure quantum effect (chiral anomaly) in inflation, which, thanks to flavor effects, are memorized by cosmic evolution.

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 introduce an axion-inflation model embedded in the Left-Right symmetric extension of the SM in which $W_R$ is coupled to the axion. contribution 0.98 0.92 0.07 asserted 0.99
s1 This model merges three milestones of modern cosmology, i.e., inflation, cold dark matter, and baryon asymmetry. contribution 0.90 0.81 0.43 asserted 1.00
s2 Thus, it can naturally explain the observed coincidences among cosmological parameters, i.e., $\eta_{B}\approx P_{\zeta}$ and $\Omega_{DM} \simeq 5~\Omega_{B}$. interpretation 0.56 0.61 0.26 hedged possibility 0.51
s3 The source of asymmetry is spontaneous CP violation in the physics of inflation, and the lightest right-handed neutrino is the cold dark matter candidate with mass $m_{N_1}\sim 1~GeV$. result 0.56 0.71 0.23 asserted 1.00
s4 The introduced mechanism does not rely on the largeness of the unconstrained CP-violating phases in the neutrino sector nor fine-tuned masses for the heaviest right-handed neutrinos. result 0.36 0.73 0.06 asserted 1.00
s5 It has two unknown fundamental scales, i.e. scale of inflation $\Lambda_{\rm inf}=\sqrt{HM_{Pl}}$ and left-right symmetry breaking $\Lambda_{F}$. method 0.51 0.68 0.04 asserted 1.00
s6 Sufficient matter asymmetry demands $\Lambda_{\rm inf}\approx\Lambda_{F}$. result 0.83 0.73 0.13 asserted 1.00
s7 The baryon asymmetry and dark matter today are remnants of a pure quantum effect (chiral anomaly) in inflation, which, thanks to flavor effects, are memorized by cosmic evolution. interpretation 0.91 0.66 0.39 asserted 1.00

What kind of paper the classifier reports this is: theoretical result 1.00 · evidence from argument 0.57.

What was examined, and what was not

sources read
  • arXiv listing abstract v2
not examined
  • full text
  • figures and tables
  • references and citing sentences
  • relations to other papers
levels run
  • P abstract
not run
  • S sections
  • T body sentences
  • C citations
  • R cross-paper relations

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 introduce an axion-inflation model embedded in the Left-Right symmetric extension of the SM in which $W_R$ is coupled to the axion. This model merges three milestones of modern cosmology, i.e., inflation, cold dark matter, and baryon asymmetry. Thus, it can naturally explain the observed coincidences among cosmological parameters, i.e., $\eta_{B}\approx P_{\zeta}$ and $\Omega_{DM} \simeq 5~\Omega_{B}$. The source of asymmetry is spontaneous CP violation in the physics of inflation, and the lightest right-handed neutrino is the cold dark matter candidate with mass $m_{N_1}\sim 1~GeV$. The introduced mechanism does not rely on the largeness of the unconstrained CP-violating phases in the neutrino sector nor fine-tuned masses for the heaviest right-handed neutrinos. It has two unknown fundamental scales, i.e. scale of inflation $\Lambda_{\rm inf}=\sqrt{HM_{Pl}}$ and left-right symmetry breaking $\Lambda_{F}$. Sufficient matter asymmetry demands $\Lambda_{\rm inf}\approx\Lambda_{F}$. The baryon asymmetry and dark matter today are remnants of a pure quantum effect (chiral anomaly) in inflation, which, thanks to flavor effects, are memorized by cosmic evolution.

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References
How the literature uses it

20 arXiv papers cite this in 42 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

Papers citing it · 32 sentences without a confident label

Uses its method or tool 1 paper
  • To estimate the Chern-Simons number, one may first reform the term $F^'F^'$ into a total derivative, $2∂_μK^μ$, and take $K^0$ as the Chern-Simons number [ref] , n_CS ≡1/(2π)^2 𝒦 (ξ) a^3 H^3 =1/(2π)^2 ∑_λ=± λe^iκ_λπ ∫τ̃^3 dlnτ̃ W^*_κ_λ,μ(-2iτ̃)W_λ_σ,μ(-2iτ̃) a^3 H^3 in which one has defined the function $𝒦 (ξ)$.

    Axion-Inflation Baryogenesis via New U(1) gauge symmetries · Baryogenesis · 0.91

Cites it as background 8 papers

What it cites · 9 sentences without a confident label

Cites as background 1 paper

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