We develop a complete and systematic analytical approach to field perturbations of extremal Kerr spacetime based on the formalism of Mano, Suzuki and Takasugi (MST) for the Teukolsky equation. Analytical expressions for the radial solutions and frequency-domain Green function in terms of infinite series of special functions are presented. As an application, we compute the leading late-time behavior due to the branch point at zero frequency of scalar, gravitational, and electromagnetic field perturbationson and off the event horizon
We analytically study the linear response of a near-extremal Kerr black hole to external scalar, ele...
In this brief note, we revisit the study of the leading order late time decay tails of massless scal...
It is well-known that the dominant late time behavior of waves propagating on a Schwarzschild spacet...
We present a new analytic approach for the study of late time evolution of linear test-fields, propa...
We present an analytic method for calculating the late-time tails of a linear scalar field outside a...
We study analytically the asymptotic late-time evolution of realistic rotating collapse. This is don...
The numerical investigation of wave propagation in the asymptotic domain of Kerr spacetime has only ...
Outside a black hole, perturbation fields die off in time as 1/t n. For spherical holes n = 2ℓ + 3 w...
We present an analytic method for calculating the late-time tails of a linear scalar field outside a...
We study analytically, via the Newman-Penrose formalism, the late time decay of scalar, electromagne...
Dans cette thèse, nous étudions l'équation de Teukolsky sur les espaces-temps de Kerr sous-extrémaux...
In this thesis, we study the Teukolsky equation on subextremal Kerr spacetimes. The latter are expli...
We present a new approach to solve the 2+1 Teukolsky equation for gravitational perturbations of a K...
We present a new approach to solve the 2+1 Teukolsky equation for gravitational perturbations of a K...
We study analytically, via the Newman-Penrose formalism, the late-time decay of linear electromagnet...
We analytically study the linear response of a near-extremal Kerr black hole to external scalar, ele...
In this brief note, we revisit the study of the leading order late time decay tails of massless scal...
It is well-known that the dominant late time behavior of waves propagating on a Schwarzschild spacet...
We present a new analytic approach for the study of late time evolution of linear test-fields, propa...
We present an analytic method for calculating the late-time tails of a linear scalar field outside a...
We study analytically the asymptotic late-time evolution of realistic rotating collapse. This is don...
The numerical investigation of wave propagation in the asymptotic domain of Kerr spacetime has only ...
Outside a black hole, perturbation fields die off in time as 1/t n. For spherical holes n = 2ℓ + 3 w...
We present an analytic method for calculating the late-time tails of a linear scalar field outside a...
We study analytically, via the Newman-Penrose formalism, the late time decay of scalar, electromagne...
Dans cette thèse, nous étudions l'équation de Teukolsky sur les espaces-temps de Kerr sous-extrémaux...
In this thesis, we study the Teukolsky equation on subextremal Kerr spacetimes. The latter are expli...
We present a new approach to solve the 2+1 Teukolsky equation for gravitational perturbations of a K...
We present a new approach to solve the 2+1 Teukolsky equation for gravitational perturbations of a K...
We study analytically, via the Newman-Penrose formalism, the late-time decay of linear electromagnet...
We analytically study the linear response of a near-extremal Kerr black hole to external scalar, ele...
In this brief note, we revisit the study of the leading order late time decay tails of massless scal...
It is well-known that the dominant late time behavior of waves propagating on a Schwarzschild spacet...