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<title>
<string language="el">Rarefaction acceleration in magnetized gamma-ray burst jets</string>
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<language>eng</language>
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<entry>http://hdl.handle.net/10795/2946</entry>
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<subject>
<string language="el">ιοντίζουσα ακτινοβολία</string>
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<description>
<string language="el">Relativistic jets associated with long/soft gamma-ray bursts are formed and initially propagate in the interior of the progenitor star. Because of the subsequent loss of their external pressure support after they cross the stellar surface, these flows can be modelled as moving around a corner. A strong steady-state rarefaction wave is formed, and the sideways expansion is accompanied by a rarefaction acceleration. We investigate the efficiency and the general characteristics of this mechanism by integrating the steady-state, special relativistic, magnetohydrodynamic equations, using a special set of partial exact solutions in planar geometry (r self-similar with respect to the ‘corner’). We also derive analytical approximate scalings in the ultrarelativistic cold/magnetized, and hydrodynamic limits. The mechanism is more effective in magnetized than in purely hydrodynamic flows. It substantially increases the Lorentz factor without much affecting the opening of the jet; the resulting values of their product can be much greater than unity, allowing for possible breaks in the afterglow light curves. These findings are similar to the ones from numerical simulations of axisymmetric jets by Komissarov et al. and Tchekhovskoy et al., although in our approach we describe the rarefaction as a steady-state simple wave and self-consistently calculate the opening of the jet that corresponds to zero external pressure.</string>
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<string language="el">10 pp.</string>
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<entity><![CDATA[BEGIN:VCARD
FN: Sapountzis, Konstantinos
N: Sapountzis, Konstantinos
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<value>Scientific Coordinator</value>
<entity><![CDATA[BEGIN:VCARD
FN: Βλαχάκης, Νεκτάριος
N: Βλαχάκης, Νεκτάριος
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FN: Εθνικό και Καποδιστριακό Πανεπιστήμιο Αθηνών (ΕΚΠΑ)
N: Εθνικό και Καποδιστριακό Πανεπιστήμιο Αθηνών (ΕΚΠΑ)
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<date>
<dateStamp>2013-07-15</dateStamp>
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<string language="el">MHD</string>
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<keyword>
<string language="el">Relativistic processes</string>
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<keyword>
<string language="el">Methods</string>
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<keyword>
<string language="el">Analytical</string>
</keyword>
<keyword>
<string language="el">Gamma-ray burst</string>
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<location>http://repository.edulll.gr/edulll/bitstream/10795/2946/2/2946_1.5_%ce%91%ce%9d_15_7_13.pdf</location>
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<entry>http://hdl.handle.net/10795/2946</entry>
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FN:National Documentation Centre - National Hellenic Research Foundation
N:National Documentation Centre - National Hellenic Research Foundation
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<date><dateTime>2016-04-27T07:28:50Z</dateTime></date>
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FN:National Documentation Centre - National Hellenic Research Foundation
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<date><dateTime>2016-04-27T07:28:50Z</dateTime></date>
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<language>gre</language>
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<cost>no</cost>
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<description>Copyright EYD-EPEDBM (Operational Programme "Education and Lifelong Learning")</description>
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