论文标题
恒星，太阳和银河光谱中的超快调制：暗物质和数字鬼，恒星耀斑和seti
Ultrafast modulations in stellar, solar and galactic spectra: Dark Matter and numerical ghosts, stellar flares and SETI
论文作者
论文摘要
From new results presented in the literature we discuss the hypothesis that the ultrafast periodic spectral modulations at $f_S \simeq 0.607$ THz found in the spectra of $236$ stars of the Sloan Digital Sky Survey (SDSS) [1] were due to oscillations induced by dark matter (DM) cores in their centers [2] behaving as oscillating boson stars [3,4].在红移校正的SDSS银河光谱中发现了另外两个频率[5]，$ f_ {1，g} \ simeq 9.5 $ thz，在$ f_s $和一个弹性频率之间的殴打，$ f_ {2，g} \ simeq 8.9 $ thz，在数据分析过程中引入了[6]。 $ f_s $可能是真实的迹象是它在真实的太阳谱中的检测，而不是在库鲁兹的人造太阳光谱中[6,7,8]。然后，对这些恒星中的四个星星的独立观察无法充满信心，但并非完全排除，在其功率谱中存在$ f_s $ [9]，而无线电seti深入学习分析则通过人工智能证实了$ f_s $检测到窄带多普勒多普勒在这些范围内的窄带多普勒在两个$ 7 $ 7 $ s/n n的样品中的窄带信号的信号。数值模拟表明，漂移可能是由于观察到的频率以$ 1.3-1.7 $ GHz和$ f_s $的频率和相位调制造成的。这意味着DM上质量限制$ M_A \ Lessim 2.4 \ times 10^{3}〜\ Mathrm {μev} $ [2]，这也与Gamma Ray burst Grb221009a [11,12,13]的结果一致，Laser干扰率[14]，建议新的物理学[15]。
From new results presented in the literature we discuss the hypothesis that the ultrafast periodic spectral modulations at $f_S \simeq 0.607$ THz found in the spectra of $236$ stars of the Sloan Digital Sky Survey (SDSS) [1] were due to oscillations induced by dark matter (DM) cores in their centers [2] behaving as oscillating boson stars [3,4]. Two additional frequencies in the redshift-corrected SDSS galactic spectra were found [5], $ f_{1,G} \simeq 9.5$ THz, the beating between $f_S$ and a spurious frequency, $f_{2,G} \simeq 8.9$ THz, introduced during the data analysis [6]. The indication that $f_S$ can be real is its detection in a real solar spectrum but not in the Kurucz's artificial solar spectrum [6,7,8]. Then, independent SETI observations of four of these stars could not confirm with high confidence, but not completely exclude, the presence of $f_S$ in their power spectra [9] while the radio SETI deep-learning analysis with artificial intelligence confirmed indirectly $f_S$ detecting a narrowband Doppler drifting of radio signals in two of these stars over a sample of $7$ with a high S/N [10]. Numerical simulations suggest that the drifting can be due to frequency and phase modulation in time of the observed frequencies at $1.3-1.7$ GHz with $f_S$. This would imply a DM upper mass limit $m_a \lesssim 2.4 \times 10^{3}~ \mathrm{μeV}$ [2] which also agrees with the results from the gamma ray burst GRB221009A [11,12,13], laser interferometry [14], suggesting new physics for the muon g-2 anomaly [15].
