Publication: Relativistic magnetic reconnection in laser laboratory for testing an emission mechanism of hard-state black hole system
Дата
2020
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Аннотация
Magnetic reconnection in a relativistic electron magnetization regime was observed in a laboratory plasma produced by a high-intensity, large energy, picoseconds laser pulse. Magnetic reconnection conditions realized with a laser-driven several kilotesla magnetic field is comparable to that in the accretion disk corona of black hole systems, i.e., Cygnus X-1. We observed particle energy distributions of reconnection outflow jets, which possess a power-law component in a high-energy range. The hardness of the observed spectra could explain the hard-state x-ray emission from accreting black hole systems.
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Relativistic magnetic reconnection in laser laboratory for testing an emission mechanism of hard-state black hole system / Law, KFF [et al.] // Physical Review E. - 2020. - 102. - № 3. - 10.1103/PhysRevE.102.033202
URI
https://www.doi.org/10.1103/PhysRevE.102.033202
https://www.scopus.com/record/display.uri?eid=2-s2.0-85093910784&origin=resultslist
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https://openrepository.mephi.ru/handle/123456789/22354
https://www.scopus.com/record/display.uri?eid=2-s2.0-85093910784&origin=resultslist
http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=Alerting&SrcApp=Alerting&DestApp=WOS_CPL&DestLinkType=FullRecord&UT=WOS:000567769400003
https://openrepository.mephi.ru/handle/123456789/22354