2017
DOI: 10.1088/1475-7516/2017/10/050
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Solar Extreme UV radiation and quark nugget dark matter model

Abstract: Abstract. We advocate the idea that the surprising emission of extreme ultra violet (EUV) radiation and soft x-rays from the Sun are powered externally by incident dark matter (DM) particles. The energy and the spectral shape of this otherwise unexpected solar irradiation is estimated within the quark nugget dark matter model. This model was originally invented as a natural explanation of the observed ratio Ω dark ∼ Ω visible when the DM and visible matter densities assume the same order of magnitude values. T… Show more

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Cited by 36 publications
(142 citation statements)
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“…It turns out that if one estimates the extra energy being produced within the AQN dark matter scenario one obtains the total extra energy ∼10 27 erg=s which surprisingly reproduces (1) for the observed EUVand soft x-ray intensities [27]. One should add that the estimate ∼10 27 erg=s for extra energy is derived exclusively in terms of known dark matter density ρ DM ∼ 0.3 GeV cm −3 and dark matter velocity v DM ∼ 10 −3 c surrounding the sun without adjusting any parameters of the model; see Sec.…”
Section: −7=6 Asupporting
confidence: 62%
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“…It turns out that if one estimates the extra energy being produced within the AQN dark matter scenario one obtains the total extra energy ∼10 27 erg=s which surprisingly reproduces (1) for the observed EUVand soft x-ray intensities [27]. One should add that the estimate ∼10 27 erg=s for extra energy is derived exclusively in terms of known dark matter density ρ DM ∼ 0.3 GeV cm −3 and dark matter velocity v DM ∼ 10 −3 c surrounding the sun without adjusting any parameters of the model; see Sec.…”
Section: −7=6 Asupporting
confidence: 62%
“…III, we highlight the basic arguments of Ref. [27] advocating the idea that the annihilation events of the antinuggets with the solar material can be interpreted as the nanoflares conjectured by Parker long ago. Precisely these annihilation events emit the axions and we compute the intensity and spectral properties of these axions in Sec.…”
Section: −7=6 Amentioning
confidence: 89%
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