The minimal cosmological standard model.

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Title: The minimal cosmological standard model.
Authors: Barenboim, Gabriela1,2 (AUTHOR) gabriela.barenboim@uv.es, Ko, Pyungwon3 (AUTHOR) pko@kias.re.kr, Park, Wan-Il1,2,4 (AUTHOR) wipark@jbnu.ac.kr
Source: Nuclear Physics B. Sep2025, Vol. 1018, pN.PAG-N.PAG. 1p.
Subjects: Physical cosmology, Dark matter, Inflationary universe, Antimatter, Mathematical symmetry, Neutrino mass, CP violation
Abstract: We propose a novel minimal scenario which simultaneously addresses the following theoretical/cosmological/phenomenological puzzles: (i) the origin of scales, (ii) primordial inflation, (iii) matter-antimatter asymmetry, (iv) tiny neutrino masses, (v) dark matter, and (vi) the strong CP-problem. Exact scale-symmetry was assumed. A global U (1) PQ -symmetry was also assumed but only in the matter sector. The novelty of the scenario is the introduction of explicit U (1) PQ -breaking terms with field-dependent coefficients in the gravity sector. Such a term does not disturb the axion solution whereas naturally realizes an axi-majoron hybrid inflation which allows a natural realization of Affleck-Dine mechanism for generating Peccei-Quinn number asymmetry. The asymmetry can be transferred to the visible sector via the right-handed neutrino portal through non-thermal decay and thermal processes, even without the presence of a CP-violating phase in the matter sector. Dark matter and dark radiation are obtained by cold and hot components of axi-majorons, respectively. [ABSTRACT FROM AUTHOR]
Copyright of Nuclear Physics B is the property of Elsevier B.V. and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
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  Data: The minimal cosmological standard model.
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  Data: <searchLink fieldCode="AR" term="%22Barenboim%2C+Gabriela%22">Barenboim, Gabriela</searchLink><relatesTo>1,2</relatesTo> (AUTHOR)<i> gabriela.barenboim@uv.es</i><br /><searchLink fieldCode="AR" term="%22Ko%2C+Pyungwon%22">Ko, Pyungwon</searchLink><relatesTo>3</relatesTo> (AUTHOR)<i> pko@kias.re.kr</i><br /><searchLink fieldCode="AR" term="%22Park%2C+Wan-Il%22">Park, Wan-Il</searchLink><relatesTo>1,2,4</relatesTo> (AUTHOR)<i> wipark@jbnu.ac.kr</i>
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  Data: <searchLink fieldCode="JN" term="%22Nuclear+Physics+B%22">Nuclear Physics B</searchLink>. Sep2025, Vol. 1018, pN.PAG-N.PAG. 1p.
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  Data: <searchLink fieldCode="DE" term="%22Physical+cosmology%22">Physical cosmology</searchLink><br /><searchLink fieldCode="DE" term="%22Dark+matter%22">Dark matter</searchLink><br /><searchLink fieldCode="DE" term="%22Inflationary+universe%22">Inflationary universe</searchLink><br /><searchLink fieldCode="DE" term="%22Antimatter%22">Antimatter</searchLink><br /><searchLink fieldCode="DE" term="%22Mathematical+symmetry%22">Mathematical symmetry</searchLink><br /><searchLink fieldCode="DE" term="%22Neutrino+mass%22">Neutrino mass</searchLink><br /><searchLink fieldCode="DE" term="%22CP+violation%22">CP violation</searchLink>
– Name: Abstract
  Label: Abstract
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  Data: We propose a novel minimal scenario which simultaneously addresses the following theoretical/cosmological/phenomenological puzzles: (i) the origin of scales, (ii) primordial inflation, (iii) matter-antimatter asymmetry, (iv) tiny neutrino masses, (v) dark matter, and (vi) the strong CP-problem. Exact scale-symmetry was assumed. A global U (1) PQ -symmetry was also assumed but only in the matter sector. The novelty of the scenario is the introduction of explicit U (1) PQ -breaking terms with field-dependent coefficients in the gravity sector. Such a term does not disturb the axion solution whereas naturally realizes an axi-majoron hybrid inflation which allows a natural realization of Affleck-Dine mechanism for generating Peccei-Quinn number asymmetry. The asymmetry can be transferred to the visible sector via the right-handed neutrino portal through non-thermal decay and thermal processes, even without the presence of a CP-violating phase in the matter sector. Dark matter and dark radiation are obtained by cold and hot components of axi-majorons, respectively. [ABSTRACT FROM AUTHOR]
– Name: AbstractSuppliedCopyright
  Label:
  Group: Ab
  Data: <i>Copyright of Nuclear Physics B is the property of Elsevier B.V. and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
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RecordInfo BibRecord:
  BibEntity:
    Identifiers:
      – Type: doi
        Value: 10.1016/j.nuclphysb.2025.116983
    Languages:
      – Code: eng
        Text: English
    PhysicalDescription:
      Pagination:
        PageCount: 1
        StartPage: N.PAG
    Subjects:
      – SubjectFull: Physical cosmology
        Type: general
      – SubjectFull: Dark matter
        Type: general
      – SubjectFull: Inflationary universe
        Type: general
      – SubjectFull: Antimatter
        Type: general
      – SubjectFull: Mathematical symmetry
        Type: general
      – SubjectFull: Neutrino mass
        Type: general
      – SubjectFull: CP violation
        Type: general
    Titles:
      – TitleFull: The minimal cosmological standard model.
        Type: main
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            NameFull: Barenboim, Gabriela
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          Name:
            NameFull: Ko, Pyungwon
      – PersonEntity:
          Name:
            NameFull: Park, Wan-Il
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          Dates:
            – D: 01
              M: 09
              Text: Sep2025
              Type: published
              Y: 2025
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            – Type: issn-print
              Value: 05503213
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            – Type: volume
              Value: 1018
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            – TitleFull: Nuclear Physics B
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