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Coronal heating problem solution by means of axion origin photons
Physics of the Dark Universe ( IF 5.5 ) Pub Date : 2020-11-13 , DOI: 10.1016/j.dark.2020.100746
Vitaliy D. Rusov , Igor V. Sharph , Vladimir P. Smolyar , Maxim V. Eingorn , Margarita E. Beglaryan

In this paper we advocate for the idea that two seemingly unrelated mysteries with almost 90 year history – the nature of dark matter and the million-degree solar corona – may be but two sides of the same coin – the axions of dark matter born in the core of the Sun and photons of axion origin in the million-degree solar corona, whose modulations are controlled by the anticorrelated modulation of the asymmetric dark matter (ADM) density in the solar interior.

It is shown that the photons of axion origin, that are born in the almost empty magnetic flux tubes (with B107G) near the tachocline and then pass through the photosphere to the corona, are the result of the solar corona heating variations, and thus, the Sun luminosity variations. Since the spectrum of the incident photons of axion origin is modulated by the frequency dependence of the cross-section, then, first, the energy distribution of the emitted axions is far from being a blackbody spectrum, and second, for a typical solar spectrum, the maximum of the differential axion flux occurs at the average axion energy is EaT4.4 (Raffelt, 1986). This means that the average energy of the photon of axion origin can generate a temperature of the order of Ta1.11107K under certain conditions of coronal substances, which is close to the temperature Tcore1.55107K of the Sun core. As a result, the free energy accumulated by the photons of axion origin in a magnetic field by means of degraded spectra due to multiple Compton scattering, is quickly released and converted into heat and plasma motion with a temperature of 4106K at maximum and 1.5106K at minimum of solar luminosity.

Since the photons of axion origin are the result of the Sun luminosity variations, then, unlike the self-excited dynamo, an unexpected but simple question arises: is there a dark matter chronometer hidden deep in the Sun core?

A unique result of our model is the fact that the periods, velocities and modulations of S-stars are the fundamental indicator of the modulation of the ADM halo density in the fundamental plane of the Galaxy center, which closely correlates with the density modulation of the baryon matter near the SMBH. If the modulations of the ADM halo at the GC lead to modulations of the ADM density on the surface of the Sun (through vertical density waves from the disk to the solar neighborhood), then there is an “experimental” anticorrelation identity between the indicators, e.g. the modulation of the ADM density in the solar interior and the number of sunspots. Therefore, this is also true for the modulation of the ADM density in the solar interior, which is directly related to the identical periods of S-star cycles and the sunspot cycles.



中文翻译:

利用轴突起源光子解决冠状动脉供热问题

在本文中,我们提倡这样一种想法,即具有近90年历史的两个看似无关的谜团-暗物质的性质和百万度太阳日冕-可能只是同一枚硬币的两个侧面-暗物质的轴心诞生于太阳的核心和起源于轴的光子在百万度的日冕中,其调制度由太阳内部不对称暗物质(ADM)密度的反相关调制控制。

结果表明,在几乎空的磁通管(带有 1个07G)靠近Tachocline,然后穿过光球到达电晕,这是太阳电晕加热变化以及太阳光度变化的结果。由于轴心起源的入射光子的光谱是通过横截面的频率依赖性进行调制的,因此,首先,所发射轴的能量分布远非黑体光谱,其次,对于典型的太阳光谱,差动轴通量的最大值出现在平均轴力为Ë一种Ť44(Raffelt,1986)。这意味着,轴突起源的光子的平均能量可以产生大约Ť一种1个111个07ķ 在一定的冠状物质条件下,接近温度 ŤCØ[RË1个551个07ķ太阳核心。结果,轴的光子在磁场中由于多次康普顿散射而通过退化的光谱积累的自由能迅速释放,并转化为热量和等离子运动,温度为。41个06ķ 最多和 1个51个06ķ 最低的太阳光度。

由于轴突起源的光子是太阳光度变化的结果,因此,与自激发电机不同的是,出现了一个出乎意料但简单的问题:太阳核深处是否存在暗物质天文钟?

我们模型的独特结果是,S星的周期,速度和调制是银河系中心基本平面中ADM光晕密度调制的基本指标,这与银河系中心的密度调制密切相关。 SMBH附近的重子物质。如果GC上ADM晕的调制导致太阳表面上ADM密度的调制(通过从磁盘到太阳附近的垂直密度波),则指示器之间存在“实验”反相关身份,例如,太阳能内部的ADM密度和黑子数的调制。因此,对于太阳内部的ADM密度的调制也是如此,这直接与S星周期和太阳黑子周期的相同周期有关。

更新日期:2020-11-17
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