Extraction of Black Hole Rotational Energy by a Magnetic Field and the Formation of Relativistic Jets

By S. Koide, Kazunari Shibata, T. Kudoh, D. Meier. Science, 2002

159 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/b7c9ca92db9f3d7a14453db48b0a27007bd09347

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. Ramesh Narayan
2. J. McKinney
3. J. E. McClintock
4. A. Tchekhovskoy
5. J. Steiner
6. F. Yuan
7. A. Sa̧dowski
8. Charles F. Gammie

In Nuclear and High Energy Physics

1. Ramesh Narayan
2. J. McKinney
3. J. E. McClintock
4. J. Steiner
5. A. Tchekhovskoy
6. Y. Kovalev
7. A. Pushkarev
8. T. Savolainen

Citations in the corpus

• Black Hole Spin via Continuum Fitting and the Role of Spin in Powering Transient Jets (2013, background): “GRMHD simulations of accreting black holes have found MHD jets forming spontaneously from generic initial conditions (e.g., Koide et al. 2002; McKinney & Gammie 2004; McKinney 2005; Beckwith et al. 2008; McKinney & Blandford 2009).”
• MOJAVE: Monitoring of Jets in Active galactic nuclei with VLBA Experiments (2012, background): “The jets take away a substantial fraction of the energy and angular momentum stored in the accretion flow (Hujeirat et al. 2003) and spinning central black hole (Koide et al. 2002; Komissarov 2005).”
• A Fundamental plane of black hole activity (2003, background): “Also to be taken into account is the influence of the black hole spin on jet formation (Blandford & Znajek 1977; Koide et al. 2002).”
• HARM: A Numerical Scheme for General Relativistic Magnetohydrodynamics (2003, methodology): “A pioneering GRMHD code has been developed by Koide and collaborators (e.g., Koide et al. 2000, 2002; Koide, Shibata, & Kudoh 1999; Meier, Koide, & Uchida 2001).”
• Total and Jet Blandford-Znajek Power in the Presence of an Accretion Disk (2005, background): “…is created in the ergosphere, and the electromagnetic energy at infinity completely dominates the hydrodynamic energy at infinity associated with the MHD Penrose process, in basic agreement with the results of Komissarov (2005) and counter to the results of Koide et al. (2002) and Punsly (2005).”
• Circularization of Tidally Disrupted Stars around Spinning Supermassive Black Holes (2015, background): “A SMBH-disk system can also work as an engine to convert the black hole’s rotational energy into outflows and jets (Blandford & Znajek 1977; Koide et al. 2002).”
• Black holes in astrophysics (2005, background): “Koide et al. (2002) and Koide (2004) describe simulations of a magnetized plasma in the ergosphere of a spinning BH.”
• Electromagnetic Extraction of Energy from Kerr Black Holes (2005, background): “MHD simulations As a topic supporting his process for “gravitomagnetohydrodynamic dynamo”, Punsly (2003) pointed out the results of some numerical simulations on the extraction process of a hole’s rotational energy (e.g., Koide et al. 2002; also see Koide 2003).”