Strichartz Estimates on Schwarzschild Black Hole Backgrounds

نویسندگان

  • JEREMY MARZUOLA
  • JASON METCALFE
  • DANIEL TATARU
  • MIHAI TOHANEANU
چکیده

We study dispersive properties for the wave equation in the Schwarzschild space-time. The rst result we obtain is a local energy estimate. This is then used, following the spirit of [29], to establish global-in-time Strichartz estimates. A considerable part of the paper is devoted to a precise analysis of solutions near the trapping region, namely the photon sphere.

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

The Strauss Conjecture on Kerr Black Hole Backgrounds

We examine solutions to semilinear wave equations on black hole backgrounds and give a proof of an analog of the Strauss conjecture on the Schwarzschild and Kerr, with small angular momentum, black hole backgrounds. The key estimates are a class of weighted Strichartz estimates, which are used near infinity where the metrics can be viewed as small perturbations of the Minkowski metric, and a lo...

متن کامل

Strichartz Estimates on Kerr Black Hole Backgrounds

We study the dispersive properties for the wave equation in the Kerr space-time with small angular momentum. The main result of this paper is to establish Strichartz estimates for solutions of the aforementioned equation. This follows a local energy decay result for the Kerr space-time obtained in the earlier work [23] and uses the techniques and results from [13] by the author and collaborator...

متن کامل

Localized Energy Estimates for Wave Equations on (1+4)-dimensional Myers-Perry Space-times

Localized energy estimates for the wave equation have been increasingly used to prove various other dispersive estimates. This article focuses on proving such localized energy estimates on (1+4)-dimensional Myers-Perry black hole backgrounds with small angular momenta. The Myers-Perry space-times are generalizations of higher dimensional Kerr backgrounds where additional planes of rotation are ...

متن کامل

Energy Distribution in 2d Stringy Black Hole Backgrounds

We utilize Møller’s and Einstein’s energy-momentum complexes in order to explicitly evaluate the energy distributions associated with the two-dimensional “Schwarzschild” and “Reissner-Nordström” black hole backgrounds. While Møller’s prescription provides meaningful physical results, Einstein’s prescription fails to do so in the aforementioned gravitational backgrounds. These results hold for a...

متن کامل

Scalar Wave Falloff in Asymptotically Anti - de Sitter Backgrounds

Conformally invariant scalar waves in black hole spacetimes which are asymptotically anti-de Sitter are investigated. We consider both the (2 + 1)-dimensional black hole and (3 + 1)-dimensional Schwarzschild-anti-de Sitter spacetime as backgrounds. Analytical and numerical methods show that the waves decay exponentially in the (2 + 1) dimensional black hole background. However the falloff patte...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2008