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	<id>https://www.pipedija.com/index.php?action=history&amp;feed=atom&amp;title=Cosmic_rays</id>
	<title>Cosmic rays - Versijų istorija</title>
	<link rel="self" type="application/atom+xml" href="https://www.pipedija.com/index.php?action=history&amp;feed=atom&amp;title=Cosmic_rays"/>
	<link rel="alternate" type="text/html" href="https://www.pipedija.com/index.php?title=Cosmic_rays&amp;action=history"/>
	<updated>2026-04-29T21:51:00Z</updated>
	<subtitle>Šio puslapio versijų istorija projekte</subtitle>
	<generator>MediaWiki 1.37.1</generator>
	<entry>
		<id>https://www.pipedija.com/index.php?title=Cosmic_rays&amp;diff=91602&amp;oldid=prev</id>
		<title>Eengglish 17:42, 10 lapkričio 2025</title>
		<link rel="alternate" type="text/html" href="https://www.pipedija.com/index.php?title=Cosmic_rays&amp;diff=91602&amp;oldid=prev"/>
		<updated>2025-11-10T17:42:56Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Ankstesnė versija&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;20:42, 10 lapkričio 2025 versija&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l6&quot;&gt;6 eilutė:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;6 eilutė:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br/&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br/&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Most of the cosmic rays, including the protons, electrons, and antiprotons,&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Most of the cosmic rays, including the protons, electrons, and antiprotons,&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;br&amp;gt; are created by massive [[quark-&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;stars&lt;/del&gt;]] (which are commonly called &amp;quot;[[black holes]]&amp;quot;),&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;br&amp;gt; are created by massive [[quark-&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;spheres&lt;/ins&gt;]] (which are commonly called &amp;quot;[[black holes]]&amp;quot;),&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;br&amp;gt; which emit high-energy gamma-rays, which then split-into high-speed&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;br&amp;gt; which emit high-energy gamma-rays, which then split-into high-speed&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;br&amp;gt; proton-antiproton pairs. Those antiprotons in-turn decay into electrons.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;br&amp;gt; proton-antiproton pairs. Those antiprotons in-turn decay into electrons.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Eengglish</name></author>
	</entry>
	<entry>
		<id>https://www.pipedija.com/index.php?title=Cosmic_rays&amp;diff=91601&amp;oldid=prev</id>
		<title>Eengglish 17:38, 10 lapkričio 2025</title>
		<link rel="alternate" type="text/html" href="https://www.pipedija.com/index.php?title=Cosmic_rays&amp;diff=91601&amp;oldid=prev"/>
		<updated>2025-11-10T17:38:51Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
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				&lt;tr class=&quot;diff-title&quot; lang=&quot;lt&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Ankstesnė versija&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;20:38, 10 lapkričio 2025 versija&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l17&quot;&gt;17 eilutė:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;17 eilutė:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;br&amp;gt; intergalactic distances before they are stopped.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;br&amp;gt; intergalactic distances before they are stopped.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br/&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br/&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;.&lt;/del&gt;&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt; &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[Kategorija:Astronomy and astrophysics]]&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[Kategorija:Astronomy and astrophysics]]&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Eengglish</name></author>
	</entry>
	<entry>
		<id>https://www.pipedija.com/index.php?title=Cosmic_rays&amp;diff=91600&amp;oldid=prev</id>
		<title>Eengglish: Naujas puslapis: So-called &quot;&lt;b&gt;cosmic rays&lt;/b&gt;&quot; are high-speed high-energy particles &lt;br&gt; which shoot throughout the universe in all directions. &lt;br&gt; Most of them are protons, and most of the rest are electrons, &lt;br&gt; but there are also anti-protons, alpha-particles (helium nuclei), &lt;br&gt; and heavier nuclei among them.  Most of the cosmic rays, including the protons, electrons, and antiprotons, &lt;br&gt; are created by massive quark-stars (which are commonly called &quot;black holes&quot;), &lt;br&gt; whi...</title>
		<link rel="alternate" type="text/html" href="https://www.pipedija.com/index.php?title=Cosmic_rays&amp;diff=91600&amp;oldid=prev"/>
		<updated>2025-11-10T17:38:02Z</updated>

		<summary type="html">&lt;p&gt;Naujas puslapis: So-called &amp;quot;&amp;lt;b&amp;gt;cosmic rays&amp;lt;/b&amp;gt;&amp;quot; are high-speed high-energy particles &amp;lt;br&amp;gt; which shoot throughout the universe in all directions. &amp;lt;br&amp;gt; Most of them are protons, and most of the rest are electrons, &amp;lt;br&amp;gt; but there are also anti-protons, alpha-particles (helium nuclei), &amp;lt;br&amp;gt; and heavier nuclei among them.  Most of the cosmic rays, including the protons, electrons, and antiprotons, &amp;lt;br&amp;gt; are created by massive &lt;a href=&quot;/index.php/Quark-stars&quot; class=&quot;mw-redirect&quot; title=&quot;Quark-stars&quot;&gt;quark-stars&lt;/a&gt; (which are commonly called &amp;quot;&lt;a href=&quot;/index.php/Black_holes&quot; class=&quot;mw-redirect&quot; title=&quot;Black holes&quot;&gt;black holes&lt;/a&gt;&amp;quot;), &amp;lt;br&amp;gt; whi...&lt;/p&gt;
&lt;p&gt;&lt;b&gt;Naujas puslapis&lt;/b&gt;&lt;/p&gt;&lt;div&gt;So-called &amp;quot;&amp;lt;b&amp;gt;cosmic rays&amp;lt;/b&amp;gt;&amp;quot; are high-speed high-energy particles&lt;br /&gt;
&amp;lt;br&amp;gt; which shoot throughout the universe in all directions.&lt;br /&gt;
&amp;lt;br&amp;gt; Most of them are protons, and most of the rest are electrons,&lt;br /&gt;
&amp;lt;br&amp;gt; but there are also anti-protons, alpha-particles (helium nuclei),&lt;br /&gt;
&amp;lt;br&amp;gt; and heavier nuclei among them.&lt;br /&gt;
&lt;br /&gt;
Most of the cosmic rays, including the protons, electrons, and antiprotons,&lt;br /&gt;
&amp;lt;br&amp;gt; are created by massive [[quark-stars]] (which are commonly called &amp;quot;[[black holes]]&amp;quot;),&lt;br /&gt;
&amp;lt;br&amp;gt; which emit high-energy gamma-rays, which then split-into high-speed&lt;br /&gt;
&amp;lt;br&amp;gt; proton-antiproton pairs. Those antiprotons in-turn decay into electrons.&lt;br /&gt;
&amp;lt;br&amp;gt; Thus, high-speed protons and high-speed electrons are produced.&lt;br /&gt;
&lt;br /&gt;
There are menny gas-atoms in intergalactic space,&lt;br /&gt;
&amp;lt;br&amp;gt; which those particles often collide with, and which change their direction,&lt;br /&gt;
&amp;lt;br&amp;gt; but do not stop them.&lt;br /&gt;
&amp;lt;br&amp;gt; Becuz of their high momentum, cosmic-ray particles can travel vast&lt;br /&gt;
&amp;lt;br&amp;gt; intergalactic distances before they are stopped.&lt;br /&gt;
&lt;br /&gt;
.&lt;br /&gt;
[[Kategorija:Astronomy and astrophysics]]&lt;/div&gt;</summary>
		<author><name>Eengglish</name></author>
	</entry>
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