| dc.contributor.author | Zacharias, Michael | |
| dc.date.accessioned | 2017-03-10T07:27:42Z | |
| dc.date.available | 2017-03-10T07:27:42Z | |
| dc.date.issued | 2017 | |
| dc.identifier.citation | Zacharias, M. 2017. Implications of time-dependent injection in relativistic jets. AIP Conference Proceedings, 1792(1): Article no 050022. [http://dx.doi.org/10.1063/1.4968968] | en_US |
| dc.identifier.issn | 0094-243X | |
| dc.identifier.issn | 1551-7616 (Online) | |
| dc.identifier.uri | http://hdl.handle.net/10394/20761 | |
| dc.identifier.uri | http://dx.doi.org/10.1063/1.4968968 | |
| dc.identifier.uri | http://aip.scitation.org/doi/abs/10.1063/1.4968968 | |
| dc.description.abstract | Rapid blazar flaring events and their rich behavior require time-dependent modeling. One important approach is time-dependent injection causing non-linear cooling effects, since the inevitable SSC cooling depends on the time-dependent electron distribution function γ˙∝∫γ2n(γ,t)dγ. This results in a collective and faster energy loss of the electrons in the jet, which could explain the extremely short variability times. The most obvious result of the non-linear cooling is the appearance of unique breaks in the time-integrated SED, which would normally be attributed to a complicated electron distribution. The knowledge of the observation time is important to interpret the observed spectra, because of the non-trivial evolution of the time-dependent SED. Intrinsic gamma-gamma absorption processes in the emission region are only of minor importance | en_US |
| dc.language.iso | en | en_US |
| dc.publisher | AIP | en_US |
| dc.title | Implications of time-dependent injection in relativistic jets | en_US |
| dc.type | Presentation | en_US |
| dc.contributor.researchID | 29092086 - Zacharias, Michael | |
