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相关论文: Models for jet power in elliptical galaxies: A cas…

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Recently, Allen et al. measured a tight correlation between the Bondi accretion rates and jet powers of the nuclei of nearby X-ray luminous elliptical galaxies. We employ two models of jet powering to understand the above correlation and…

天体物理学 · 物理学 2007-05-23 Rodrigo S. Nemmen , Richard G. Bower , Arif Babul , Thaisa Storchi-Bergmann

We calculate the jet power of the classical Blandford-Znajek(BZ) model and hybrid model developed by Meier based on the global solutions of advection dominated accretion flows (ADAFs) surrounding Kerr black holes. We find that the jet power…

天体物理学 · 物理学 2009-11-13 Qingwen Wu , Xinwu Cao

One of the major open questions related to the production of jets by accreting black holes is: why do sources with similar accretion powers produce so vastly different jet powers? What conditions are required to make a powerful jet? If jets…

高能天体物理现象 · 物理学 2025-02-19 Tuomas Savolainen , Wara Chamani

The interaction of large scale magnetic fields with the event horizon of rotating black holes (the Blandford-Znajek [1977] mechanism) forms the basis for some models of the most relativistic jets. We explore a scenario in which the central…

高能天体物理现象 · 物理学 2011-02-11 David Garofalo

A rotating black hole probably powers ultrarelativistic jets in gamma-ray bursts, relativistic jets from some active galactic nuclei, and jets from some black hole x-ray binaries. Prior estimates of the power output of a black hole have…

天体物理学 · 物理学 2009-11-11 Jonathan C. McKinney

We consider the Blandford-Znajek (BZ) mechanism for extracting black hole spin energy to drive astrophysical jets. Analyses of the BZ mechanism generally take no account of any electric charge on the black hole. But, as noted by Wald and…

高能天体物理现象 · 物理学 2021-09-29 A. R. King , J. E. Pringle

Relativistic jets from black holes can extract energy not only from accretion but also directly from the black hole's spin, as described by the Blandford-Znajek mechanism. A longstanding question is whether magnetic flux can accumulate near…

高能天体物理现象 · 物理学 2026-02-27 Antonios Nathanail

Recently it has been observed that the scaling of jet power with black hole spin in galactic X-ray binaries is consistent with the predictions of the Blandford-Znajek (BZ) jet model. These observations motivate us to revisit the BZ model…

高能天体物理现象 · 物理学 2015-06-16 Robert F. Penna , Ramesh Narayan , Aleksander Sadowski

Three energy mechanisms invoking large-scale magnetic fields are incorporated in a model to interpret jet production in black hole (BH) systems, i.e., the Blandford-Znajek (BZ), the magnetic coupling (MC) and Blandford-Payne (BP) processes.…

天体物理学 · 物理学 2009-11-13 Ding-Xiong Wang , Yong-Chun Ye , Yang Li , Zhao-Jiang Ge

Aims. A simplified model of jet power from active galactic nuclei is proposed in which the relationship between jet power and disk luminosity is discussed by combining disk accretion with two mechanisms of extracting energy magnetically…

天体物理学 · 物理学 2009-11-13 Yang Li , Ding-Xiong Wang , Zhao-Ming Gan

The rotational energy of a black hole can be extracted via the Blandford-Znajek mechanism and numerical simulations suggest a strong dependence of the power of the produced jet on the black hole spin. A recent study has found no evidence…

广义相对论与量子宇宙学 · 物理学 2012-12-21 Cosimo Bambi

The mechanism by which outflows and plausible jets are driven from black hole systems, still remains observationally elusive. Notwithstanding, several observational evidences and deeper theoretical insights reveal that accretion and…

高能天体物理现象 · 物理学 2014-11-20 Debbijoy Bhattacharya , Shubhrangshu Ghosh , Banibrata Mukhopadhyay

In this paper we study the wind accretion onto a rotating black hole in the close binary system harboring a young massive star. It is shown that the angular momentum of the accreted stellar wind material is not sufficient for the formation…

高能天体物理现象 · 物理学 2015-05-30 Maxim V. Barkov , Dmitry V. Khangulyan

Under the coronal magnetic field, we estimate the maximal jet power of the Blandford-\Znajek (BZ) mechanism, Blandford-\Payne (BP) mechanism, and hybrid model. The jet power of the BZ and Hybrid model mechanisms depends on the spin of a…

高能天体物理现象 · 物理学 2022-09-26 Chen Yongyun , Gu Qiusheng , Fan Junhui , Yu xiaoling , Ding Nan , Guo Xiaotong , Xiong Dingrong

We investigate the correlation between 151 MHz radio luminosity, L_151MHz, and jet power, P_jet, for a sample of low-power radio galaxies, of which the jet power is estimated from X-ray cavities. The jet power for a sample of FR I radio…

高能天体物理现象 · 物理学 2015-05-27 Qingwen Wu , Xinwu Cao , Ding-Xiong Wang

We use a sample of radio-loud active galactic nuclei (AGNs) with measured black hole masses to explore the jet formation mechanisms in these sources. Based on the K\"{o}nigl's inhomogeneous jet model, the jet parameters, such as the bulk…

宇宙学与河外天体物理 · 物理学 2015-06-11 Bo Chai , Xinwu Cao , Minfeng Gu

It was suggested that the relativistic jets in gamma-ray bursts (GRBs) are powered via the Blandford-Znajek (BZ) mechanism or the annihilation of neutrinos and anti-neutrinos from a neutrino cooling-dominated accretion flow (NDAF). The…

高能天体物理现象 · 物理学 2015-06-19 Xinwu Cao , En-Wei Liang , Ye-Fei Yuan

The extraction of rotational energy from a spinning black hole via the Blandford-Znajek mechanism has long been understood as an important component in models to explain energetic jets from compact astrophysical sources. Here we show more…

高能天体物理现象 · 物理学 2015-05-20 David Neilsen , Luis Lehner , Carlos Palenzuela , Eric W. Hirschmann , Steven L. Liebling , Patrick M. Motl , T. Garrett

Theoretical models show that the power of relativistic jets of active galactic nuclei depends on the spin and mass of the central supermassive black holes, as well as the accretion. Here we report an analysis of archival observations of a…

高能天体物理现象 · 物理学 2021-06-09 Yongyun Chen , Qiusheng Gu , Junhui Fan , Hongyan Zhou , Yefei Yuan , Weimin Gu , Qinwen Wu , Dingrong Xiong , Xiaotong Guo , Nan Ding , Xiaoling Yu

Using long-duration general relativistic magnetohydrodynamic simulations of radiatively inefficient accretion discs, the energy, momentum and mass outflow rates from such systems are estimated. Outflows occur via two fairly distinct modes:…

高能天体物理现象 · 物理学 2015-06-16 A. Sadowski , R. Narayan , R. Penna , Y. Zhu
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