5 research outputs found
Magnetic Black Holes: from Thomson Dipoles to the Penrose Process and Cosmic Censorship
We consider accretion of charged test matter by rotating, magnetic black
holes and discuss a number of aspects in which the interaction of the angular
momentum contained in the electromagnetic field and the spin of the hole plays
a fundamental role. First, we argue that such a black hole tends to lose its
angular momentum by accreting charges while remaining globally neutral. Then,
we show that accretion can happen in a superradiant manner via an enhanced
Penrose process. In particular, we find that the regions from which energy and
angular momentum can be extracted contain the axis of rotation and, in some
cases, consist of floating bubbles disconnected from the black hole itself.
Finally, we address the question of whether extremal dyonic rotating black
holes can be overcharged or overspun via accretion of arbitrary matter, and
prove that this can not happen if the null-energy condition holds. We conclude
by discussing some future research directions.Comment: 12+5 pages, 4 figures, one mathematica packag
Kerr-fully Diving into the Abyss: Analytic Solutions to Plunging Geodesics in Kerr
We present closed-form solutions for plunging geodesics in the extended Kerr
spacetime using Boyer-Lindquist coordinates. Our solutions directly solve for
the dynamics of generic timelike plunges, we also specialise to the case of
test particles plunging from a precessing innermost stable circular orbit
(ISSO). We find these solutions in the form of elementary and Jacobi elliptic
functions parameterized by Mino time. In particular, we demonstrate that
solutions for the ISSO case can be determined almost entirely in terms of
elementary functions, depending only on the spin parameter of the black hole
and the radius of the ISSO. This extends recent work on the case of equatorial
plunges from the innermost stable circular orbit. Furthermore, we introduce a
new equation that characterizes the radial inflow from the ISSO to the horizon,
taking into account the inclination. For ease of application, our results have
been implemented in the KerrGeodesics package in the Black Hole Perturbation
Toolkit.Comment: 22 pages, 7 Figure
Waveform Modelling for the Laser Interferometer Space Antenna
International audienceLISA, the Laser Interferometer Space Antenna, will usher in a new era in gravitational-wave astronomy. As the first anticipated space-based gravitational-wave detector, it will expand our view to the millihertz gravitational-wave sky, where a spectacular variety of interesting new sources abound: from millions of ultra-compact binaries in our Galaxy, to mergers of massive black holes at cosmological distances; from the beginnings of inspirals that will venture into the ground-based detectors' view to the death spiral of compact objects into massive black holes, and many sources in between. Central to realising LISA's discovery potential are waveform models, the theoretical and phenomenological predictions of the pattern of gravitational waves that these sources emit. This white paper is presented on behalf of the Waveform Working Group for the LISA Consortium. It provides a review of the current state of waveform models for LISA sources, and describes the significant challenges that must yet be overcome
Waveform Modelling for the Laser Interferometer Space Antenna
International audienceLISA, the Laser Interferometer Space Antenna, will usher in a new era in gravitational-wave astronomy. As the first anticipated space-based gravitational-wave detector, it will expand our view to the millihertz gravitational-wave sky, where a spectacular variety of interesting new sources abound: from millions of ultra-compact binaries in our Galaxy, to mergers of massive black holes at cosmological distances; from the beginnings of inspirals that will venture into the ground-based detectors' view to the death spiral of compact objects into massive black holes, and many sources in between. Central to realising LISA's discovery potential are waveform models, the theoretical and phenomenological predictions of the pattern of gravitational waves that these sources emit. This white paper is presented on behalf of the Waveform Working Group for the LISA Consortium. It provides a review of the current state of waveform models for LISA sources, and describes the significant challenges that must yet be overcome