Novel Planetary Signatures from the Dark Universe

IF 0.6 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
K. Zioutas, V. Anastassopoulos, A. Argiriou, G. Cantatore, S. Cetin, A. Gardikiotis, H. Haralambous, M. Karuza, A. Kryemadhi, M. Maroudas, A. Mastronikolis, C. Oikonomou, K. Ozbozduman, Y. K. Semertzidis, M. Tsagri, I. Tsagris
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引用次数: 0

Abstract

“Dunkle Materie” (DM) came from unexpected cosmological observations. Nowadays within our solar system, diverse observations also defy conventional explanations, like the main physical process(es) underlying the heating of the different solar atmospheric layers. Streaming DM offers a viable common scenario following gravitational focusing by the solar system bodies. This fits as the underlying process behind the solar cycle, which was the first signature suggesting a planetary dependency. The challenge, since 1859, is to find a remote planetary impact, beyond the extremely feeble planetary tidal force. We stress the possible involvement of an external impact by some overlooked “streaming invisible matter”, which reconciles all investigated mysterious observations mimicking a not extant remote planetary force. Unexpected planetary relationships exist for both the dynamic Sun and Earth, reflecting multiple signatures for streaming DM. The local reasoning à la Zwicky is also suggestive for searches including puzzling biomedical phenomena. Favourite DM candidates are anti-quark-nuggets, magnetic monopoles, dark photons, or the composite “pearls”. Then, anomalies within the solar system are the manifestation of the dark Universe. The tentative streaming DM scenario enhances spatiotemporally the DM flux

来自黑暗宇宙的新奇行星信号
"敦刻尔克材料"(Dunkle Materie,DM)来自意想不到的宇宙学观测。如今,在我们的太阳系中,各种观测结果也无法做出传统的解释,比如太阳大气层不同层加热的主要物理过程。在太阳系天体引力聚焦之后,DM 流提供了一个可行的共同方案。这与太阳周期背后的基本过程相吻合,而太阳周期是第一个表明行星依赖性的标志。自 1859 年以来,我们面临的挑战是在极其微弱的行星潮汐力之外,找到一种遥远的行星撞击。我们强调可能是某种被忽视的 "无形物质流 "造成了外部撞击,这与所有被调查的神秘观测结果相吻合,这些观测结果模仿了一种并不存在的遥远行星力。动态太阳和地球都存在着意想不到的行星关系,反映了流态非物质的多种特征。兹威基(Zwicky)式的局部推理也为包括令人费解的生物医学现象在内的搜索提供了建议。最受欢迎的DM候选者是反夸克金块、磁单极子、暗光子或复合 "珍珠"。那么,太阳系内的异常现象就是暗宇宙的表现。暂定的流式DM方案从时空上增强了DM通量
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来源期刊
Astrophysics
Astrophysics 地学天文-天文与天体物理
CiteScore
0.90
自引率
20.00%
发文量
32
审稿时长
6-12 weeks
期刊介绍: Astrophysics (Ap) is a peer-reviewed scientific journal which publishes research in theoretical and observational astrophysics. Founded by V.A.Ambartsumian in 1965 Astrophysics is one of the international astronomy journals. The journal covers space astrophysics, stellar and galactic evolution, solar physics, stellar and planetary atmospheres, interstellar matter. Additional subjects include chemical composition and internal structure of stars, quasars and pulsars, developments in modern cosmology and radiative transfer.
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