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The non-linear stability of the Schwarzschild family of black holes
M Dafermos, G Holzegel, I Rodnianski… - arxiv preprint arxiv …, 2021 - arxiv.org
We prove the non-linear asymptotic stability of the Schwarzschild family as solutions to the
Einstein vacuum equations in the exterior of the black hole region: general vacuum initial …
Einstein vacuum equations in the exterior of the black hole region: general vacuum initial …
Hyperboloidal approach for static spherically symmetric spacetimes: a didactical introduction and applications in black-hole physics
R Panosso Macedo - Philosophical Transactions of the …, 2024 - royalsocietypublishing.org
This work offers a didactical introduction to the calculations and geometrical properties of a
static, spherically symmetric spacetime foliated by hyperboloidal time surfaces. We discuss …
static, spherically symmetric spacetime foliated by hyperboloidal time surfaces. We discuss …
Research status and evolution trends of emergency information resource management: based on bibliometric analysis from 2003 to 2022
Q Cheng, S Zhang - International journal of disaster risk reduction, 2023 - Elsevier
As big data and artificial intelligence technologies are being increasingly applied in
emergency management activities, effective information resource management has become …
emergency management activities, effective information resource management has become …
A sharp version of Price's law for wave decay on asymptotically flat spacetimes
P Hintz - Communications in Mathematical Physics, 2022 - Springer
We prove Price's law with an explicit leading order term for solutions ϕ (t, x) of the scalar
wave equation on a class of stationary asymptotically flat (3+ 1)-dimensional spacetimes …
wave equation on a class of stationary asymptotically flat (3+ 1)-dimensional spacetimes …
Linear waves on asymptotically flat spacetimes. I
P Hintz - arxiv preprint arxiv:2302.14647, 2023 - arxiv.org
We introduce a novel framework for the analysis of linear wave equations on nonstationary
asymptotically flat spacetimes, under the assumptions of mode stability and absence of zero …
asymptotically flat spacetimes, under the assumptions of mode stability and absence of zero …
Late time tail of waves on dynamic asymptotically flat spacetimes of odd space dimensions
J Luk, SJ Oh - arxiv preprint arxiv:2404.02220, 2024 - arxiv.org
We introduce a general method for understanding the late time tail for solutions to wave
equations on asymptotically flat spacetimes with odd space dimensions. In particular, for a …
equations on asymptotically flat spacetimes with odd space dimensions. In particular, for a …
The case against smooth null infinity I: heuristics and counter-examples
LMA Kehrberger - Annales Henri Poincare, 2022 - Springer
This paper initiates a series of works dedicated to the rigorous study of the precise structure
of gravitational radiation near infinity. We begin with a brief review of an argument due to …
of gravitational radiation near infinity. We begin with a brief review of an argument due to …
Sharp decay for Teukolsky equation in Kerr spacetimes
In this work, we derive the global sharp decay, as both a lower and an upper bounds, for the
spin±s components, which are solutions to the Teukolsky equation, in the black hole exterior …
spin±s components, which are solutions to the Teukolsky equation, in the black hole exterior …
Generalized Price's law on fractional-order asymptotically flat stationary spacetimes
We obtain estimates on the rate of decay of a solution to the wave equation on a stationary
spacetime that tends to Minkowski space at a rate $ O (\lvert x\rvert^{-\kappa}), $$\kappa\in …
spacetime that tends to Minkowski space at a rate $ O (\lvert x\rvert^{-\kappa}), $$\kappa\in …
Instability of gravitational and electromagnetic perturbations of extremal Reissner–Nordström spacetime
MA Apetroaie - Annals of PDE, 2023 - Springer
We study the linear stability problem to gravitational and electromagnetic perturbations of
the extremal,| Q|= M, Reissner–Nordström spacetime, as a solution to the Einstein–Maxwell …
the extremal,| Q|= M, Reissner–Nordström spacetime, as a solution to the Einstein–Maxwell …