Talk detail

Participant	Karlica, Mile
Institution	ICRANet - Piazza della Repubblica 10 - Pescara - Abruzzo - Italy

Session	BN3	Accepted		Order	Time
Talk	Oral abstract	Title	X-ray and radio emission within WD-WD merger model
Coauthors
Abstract	We are presenting the X-ray and radio band emission as the emerging optically thin regime within the Wd-WD ejecta. We compare our results with the GRB170817 as an example.
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Session	GB8	Accepted		Order	Time
Talk	Oral abstract	Title	Synchrotron Radiation in the Afterglows of GRB 130427A and GRB160625B
Coauthors
Abstract	Gamma-ray burst (GRB) within the paradigm of the binary driven hypernova (BdHN) clearly points to its mildly relativistic regime during afterglow phase which is confirmed by early X-ray thermal component measurements around 100 seconds and optical emission lines measurement around $10^6$ seconds. Radiation in optical and X-ray band of the GRB afterglow within this paradigm come from the synchrotron radiation of relativistic electrons inside hypernova (HN) ejecta mainly magnetised by a newly created neutron star ($\nu$NS). To model the temporal behaviour of the GRB afterglow spectra we have developed a kinetic equation code which tracks the evoultion of injected electrons inside HN ejecta taking into account all the important energy losses and their temporal dependence. In this talk we present the basic physical elements of our code and the relevant results for GRB130427A and GRB160625B as a clear example.
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Session	GB9	Accepted		Order	Time
Talk	Oral abstract	Title	Radio and X-ray
Coauthors
Abstract
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