Pressure collimation of relativistic jets

Details Pressure collimation of relativistic jets Pressure collimation of relativistic jets

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989acaps...9..123l&link_type=abstract

(Acta Astrophysica Sinica, vol. 9, no. 2, 1989, p. 123-126) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 13, Sept.

Astronomy and Astrophysics

Astronomy

Active Galactic Nuclei, Black Holes (Astronomy), Collimation, Jet Flow, Radio Jets (Astronomy), Relativistic Plasmas, Curvature, Gravitational Effects, Pressure Effects, Space-Time Functions

Scientific paper

Spacetime curvature around a black hole decollimates jets produced near the hole. For fluid jets, pressure effects in most cases can dominate over gravitational effects, thus leading to an overall collimation of the flow. In order to keep a jet flowing in regions far from the black hole, the external pressure Pe of the medium shoud not drop with increasing radial distance faster than an inverse third power.

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