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	<title>The Persian Thunderbolts &#187; High energy</title>
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		<title>تحلیل رفتار کهکشان IC310 با مدل کهکشان شناسی پلاسما</title>
		<link>http://persiantbolts.com/%d8%aa%d8%ad%d9%84%db%8c%d9%84-%d8%b1%d9%81%d8%aa%d8%a7%d8%b1-%da%a9%d9%87%da%a9%d8%b4%d8%a7%d9%86-ic310-%d8%a8%d8%a7-%d9%85%d8%af%d9%84-%da%a9%d9%87%da%a9%d8%b4%d8%a7%d9%86-%d8%b4%d9%86%d8%a7%d8%b3/</link>
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		<pubDate>Thu, 09 Feb 2017 21:48:14 +0000</pubDate>
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		<category><![CDATA[کیهان شناسی.]]></category>
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		<category><![CDATA[Farzin Hosseini]]></category>
		<category><![CDATA[High energy]]></category>
		<category><![CDATA[IC 310]]></category>
		<category><![CDATA[Jets]]></category>
		<category><![CDATA[Magnetosphere]]></category>
		<category><![CDATA[Plasmoid]]></category>
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		<category><![CDATA[کیهان شناسی پلاسما]]></category>

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		<description><![CDATA[Explanation on Ambiguous Behaviors of IC 310 Black Hole in Plasma Cosmology Farzin Hosseini Department of Physics, University of Kurdistan, Kurdistan province, Iran The Thunderbolts Project &#8211; Persian Division E-mail: Farzin@persiantbolts.com Abstract IC 310 is one of the high energetic -ray sources located in a distance  from the Perseus cluster’s centered galaxy, NGC 1275. This galaxy...]]></description>
				<content:encoded><![CDATA[<p dir="ltr" style="text-align: center;"><strong>Explanation on Ambiguous Behaviors of IC 310 Black Hole </strong><strong>in Plasma Cosmology</strong></p>
<p dir="ltr" style="text-align: center;"><strong><a href="http://persiantbolts.com/%D9%85%D8%B9%D8%B1%D9%81%DB%8C-3/">Farzin Hosseini</a></strong></p>
<p dir="ltr" style="text-align: center;"><strong><em>Department of Physics, University of Kurdistan, Kurdistan province, Iran </em></strong></p>
<p dir="ltr" style="text-align: center;"><strong><em>The Thunderbolts Project &#8211; Persian Division</em></strong></p>
<p dir="ltr" style="text-align: center;"><strong><em>E-mail: </em></strong><a href="mailto:Farzin@persiantbolts.com"><strong><em>Farzin@persiantbolts.com</em></strong></a></p>
<p dir="ltr" style="text-align: left;"><strong>Abstract</strong></p>
<p dir="ltr" style="text-align: left;">IC 310 is one of the high energetic -ray sources located in a distance  from the Perseus cluster’s centered galaxy, NGC 1275. This galaxy has been identified at GeV with Fermi-LAT and MAGIC at very high energies, IC 310 exhibit high rapid variability of -ray production that the observed variability time scale is 4.8 minutes. There are several conventional models suggested for -ray production of sub-horizon scale variability:  (I) mini-jet structures within the jets, (II) cloud/star-jet interactions, (III) magnetospheric model. This paper investigated the use of -ray bursts of Plasmoid and Photon bubbles as a new model to explain vague observed phenomenon of IC 310 black hole. In this model the photon are weightless in a local system of reference, but repelled in a reference system of distant observer, such as an observer on Earth looking at photon close to a black hole. The weightlessness of photons in the local system of reference eliminates the needs for black holes.</p>
<p dir="ltr" style="text-align: left;"><strong>Keyword:</strong> IC 310, High energy, Magnetosphere, Plasmoid, Black holes, Jets</p>
<p style="text-align: right;">ارائه برای کنفرانس:</p>
<p dir="ltr" style="text-align: left;">The 6th International Conference and Workshops on Basic and Applied Science (6th ICOWOBAS 2017)</p>
<p dir="ltr" style="text-align: left;">Erbil &#8211; Kurdistan region &#8211; Iraq</p>
<p style="text-align: right;">در صورت نیاز به اصل مقاله از طریق ایمیل اقدام نمایید.</p>
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