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Cosmic rays: Skirtumas tarp puslapio versijų
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(Naujas puslapis: So-called "<b>cosmic rays</b>" are high-speed high-energy particles <br> which shoot throughout the universe in all directions. <br> Most of them are protons, and most of the rest are electrons, <br> but there are also anti-protons, alpha-particles (helium nuclei), <br> and heavier nuclei among them. Most of the cosmic rays, including the protons, electrons, and antiprotons, <br> are created by massive quark-stars (which are commonly called "black holes"), <br> whi...) |
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Most of the cosmic rays, including the protons, electrons, and antiprotons, | Most of the cosmic rays, including the protons, electrons, and antiprotons, | ||
<br> are created by massive [[quark- | <br> are created by massive [[quark-spheres]] (which are commonly called "[[black holes]]"), | ||
<br> which emit high-energy gamma-rays, which then split-into high-speed | <br> which emit high-energy gamma-rays, which then split-into high-speed | ||
<br> proton-antiproton pairs. Those antiprotons in-turn decay into electrons. | <br> proton-antiproton pairs. Those antiprotons in-turn decay into electrons. | ||
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<br> intergalactic distances before they are stopped. | <br> intergalactic distances before they are stopped. | ||
[[Kategorija:Astronomy and astrophysics]] | [[Kategorija:Astronomy and astrophysics]] | ||