Coronal heating problem solution by means of axion origin photons

作者: Vitaliy D Rusov , Igor V Sharph , Vladimir P Smolyar , Maxim V Eingorn , Margarita E Beglaryan

DOI: 10.1016/J.DARK.2020.100746

关键词: Dark matterAxionAstrophysicsPhotospherePhysicsGalaxySunspotSolar luminosityHaloTachocline

摘要: Abstract In this paper we advocate for the idea that two seemingly unrelated mysteries with almost 90 year history – nature of dark matter and million-degree solar corona may be but sides same coin axions born in core Sun photons axion origin corona, whose modulations are controlled by anticorrelated modulation asymmetric (ADM) density interior. It is shown origin, empty magnetic flux tubes (with B ∼ 1 0 7 G ) near tachocline then pass through photosphere to result heating variations, thus, luminosity variations. Since spectrum incident modulated frequency dependence cross-section, then, first, energy distribution emitted far from being a blackbody spectrum, second, typical maximum differential occurs at average 〈 E ∕ T 〉 ≈ 4 . (Raffelt, 1986). This means photon can generate temperature order 11 ⋅ K under certain conditions coronal substances, which close c o r e 55 core. As result, free accumulated field degraded spectra due multiple Compton scattering, quickly released converted into heat plasma motion 6 5 minimum luminosity. unlike self-excited dynamo, an unexpected simple question arises: there chronometer hidden deep core? A unique our model fact periods, velocities S-stars fundamental indicator ADM halo plane Galaxy center, closely correlates baryon SMBH. If GC lead on surface (through vertical waves disk neighborhood), “experimental” anticorrelation identity between indicators, e.g. interior number sunspots. Therefore, also true interior, directly related identical periods S-star cycles sunspot cycles.

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