An Electromagnetic Model for Jet Power from an Advection Dominated Accretion Flow around a Rotating Black Hole

Details An Electromagnetic Model for Jet Power from an Advection Dominated Accretion Flow around a Rotating Black Hole An Electromagnetic Model for Jet Power from an Advection Dominated Accretion Flow around a Rotating Black Hole

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005chphl..22.1293g&link_type=abstract

Chinese Physics Letters, Volume 22, Issue 5, pp. 1293-1295 (2005).

Physics

Scientific paper

We discuss jet production from an advection dominated accretion flow (ADAF) around a rotating black hole (BH) in an electromagnetic regime. An analytical expression for the jet power is derived by using an equivalent circuit in the BH magnetosphere. It turns out that a large fraction of jet powers is contributed from the inner region of the ADAF, and the jet power depends sensitively on the degree to which the flow is advection-dominated. In addition, we use our model to fit the strong jet powers of several BL Lac objects, which cannot be explained by virtue of the BZ process.

Affiliated with

Also associated with

No associations

Rating

An Electromagnetic Model for Jet Power from an Advection Dominated Accretion Flow around a Rotating Black Hole does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with An Electromagnetic Model for Jet Power from an Advection Dominated Accretion Flow around a Rotating Black Hole, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and An Electromagnetic Model for Jet Power from an Advection Dominated Accretion Flow around a Rotating Black Hole will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-770045