原始行星的生命起源
The Origin of Life from Primordial Planets
摘要：
生命的起源和宇宙的起源是科学中最重要的问题之一，它们可能是密不可分的。流体引力动力学（HGD）宇宙学预测，星系中的暗物质是氢氦气体行星，每颗恒星有数百万颗行星。这一意想不到的预测得到了星系类星体微透镜和太空望远镜大量新数据的支持。恒星对行星的过度吸积产生的超新星产生了化学物质（C，N，O，P等）。以及第一生命所需的丰富液态水域和广泛散布生命原型的手段。第一个生命可能在大爆炸后30万年，当行星仍然温暖时，等离子体向气体转变后立即发生，行星之间的物质交换基本上构成了宇宙学的原始汤。来自光学、无线电和红外线太空望远镜的图像表明，地球上的生命既不是最初的，也不是必然的。
英文摘要：
The origin of life and the origin of the universe are among the most important problems of science and they might be inextricably linked. Hydro-gravitational-dynamics (HGD) cosmology predicts hydrogen-helium gas planets in clumps as the dark matter of galaxies, with millions of planets per star. This unexpected prediction is supported by quasar microlensing of a galaxy and a flood of new data from space telescopes. Supernovae from stellar over-accretion of planets produce the chemicals (C, N, O, P etc.) and abundant liquid water domains required for first life and the means for wide scattering of life prototypes. The first life likely occurred promptly following the plasma to gas transition 300,000 years after the big bang while the planets were still warm, and interchanges of material between planets constituted essentially a cosmological primordial soup. Images from optical, radio, and infrared space telescopes suggest life on Earth was neither first nor inevitable.
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