Black hole gravitohydromagnetics

By B. Punsly. 2001

207 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Electrical and Electronic Engineering, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/e41fbdc67fde350b6d350c62636fcf7e49b897af

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. J. McKinney
2. A. Tchekhovskoy
3. Ramesh Narayan
4. Charles F. Gammie
5. Serguei Komissarov
6. I. Okamoto
7. A. Sa̧dowski
8. A. Spitkovsky

In Electrical and Electronic Engineering

1. Serguei Komissarov
2. G. E. Romero
3. Komissarov S S
4. D. Torres
5. I. Okamoto
6. J. McKinney
7. Ernesto F. Eiroa
8. Francisco S. N. Lobo

In Nuclear and High Energy Physics

1. J. McKinney
2. Ramesh Narayan
3. A. Tchekhovskoy
4. I. Okamoto
5. Komissarov S S
6. Charles F. Gammie
7. Serguei Komissarov
8. G. E. Romero

Citations in the corpus

• Reissner-Nordstrom black hole lensing (2002, methodology): “mple: black hole in the galactic halo In this section we consider as a lens a black hole with mass M = 7M⊙ , negligible angular momentum (S ≈ 0) and charge Q placed at the galactic halo (D ol = 4kpc) [10]. The source is a star with radius R s = R⊙ located in the galactic bulge (D os = 8kpc). This pr”
• General relativistic magnetohydrodynamic simulations of the jet formation and large-scale propagation from black hole accretion systems (2006, background): “…jet that is launched by the BZ effect has an arbitrary Lorentz factor that is determined by the detailed high-energy physics of the mass-loading of the jet, so low mass-loading can explain highly relativistic jets (see, e.g. Phinney 1983; Beskin 1997; Punsly 2001; Levinson 2005; McKinney 2005a,b).”
• Total and Jet Blandford-Znajek Power in the Presence of an Accretion Disk (2005, methodology): “…lines tie the black hole to large distances, the energy flux is determined by the Blandford-Znajek (BZ) process (Blandford & Znajek 1977; for reviews, see Ruffini & Wilson 1975; Rees et al. 1982; Begelman et al. 1984; Beskin & Kuznetsova 2000; Punsly 2001; McKinney & Gammie 2004; Levinson 2005).”
• Observations of the Blandford–Znajek process and the magnetohydrodynamic Penrose process in computer simulations of black hole magnetospheres (2005, background): “…and the fact that no proper physicalinterpretation had been pushed forward also m adetheresultvulnerableto criticism on theoreticalgroundsand stim ulated attem ptsto nd alternativewaysofm agneticextraction ofrotationalen- ergy ofblack holes(Punsly & Coroniti1990a;Punsly 2001; Takahashietal.1990).”
• Electrodynamics of black hole magnetospheres (2004, background): “Apart from the absence of the proper unipolar inductor, Punsly & Coroniti (1990a) and Punsly (2001) criticized the electromagnetic mechanism on the grounds of the causality principle.”
• Electromagnetic Extraction of Energy from Kerr Black Holes (2005, background): “…of a dynamo process or the driving force of the BZ process has recently been suggested again to exist somewhere between the inner and outer Alfvénic surfaces, well outside of the horizon (e.g., Takahashi et al. 1990; Beskin, Kuznetsova 2000; Punsly 2001; Komissarov 2002b; Blandford 2002).”
• HARM: A Numerical Scheme for General Relativistic Magnetohydrodynamics (2003, background): “While it was recognized throughout the 1970s that relativistic MHD would be relevant to problems related to black hole accretion (particularly following the seminal work of Blandford & Znajek 1977 and Phinney 1983; see also Punsly 2001), no further work appeared until Yokosawa (1993).”