Hawking emission of gravitons in higher dimensions: non-rotating black holes

نویسنده

  • Vitor Cardoso
چکیده

We compute the absorption cross section and the total power carried by gravitons in the evaporation process of a higher-dimensional non-rotating black hole. These results are applied to a model of extra dimensions with standard model fields propagating on a brane. The emission of gravitons in the bulk is highly enhanced as the spacetime dimensionality increases. The implications for the detection of black holes in particle colliders and ultrahigh-energy cosmic ray air showers are briefly discussed.

برای دانلود 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

Graviton Emission from a Schwarzschild Black Hole in the Presence of Extra Dimensions

In this talk I presented a previously published work concerning the evaporation of (4 + n)-dimensional non-rotating black holes into gravitons [1] . In this work we calculated the energy emission rate for gravitons in the bulk obtaining analytical solutions of the master equation satisfied by all three types (S,V,T) of gravitational perturbations and presented graphs for the absorption probabil...

متن کامل

Emissivities for the various Graviton Modes in the Background of the Higher-Dimensional Black Hole

The Hawking emissivities for the scalar-, vector-, and tensor-mode bulk gravitons are computed in the full range of the graviton’s energy by adopting the analytic continuation numerically when the spacetime background is (4 +n)dimensional non-rotating black hole. The total emissivity for the gravitons is only 5.16% of that for the spin-0 field when there is no extra dimension. However, this rat...

متن کامل

No Hawking-Page phase transition in three dimensions

We investigate whether or not the Hawking-Page phase transition is possible to occur in three dimensions. Starting with the simplest class of LanczosLovelock action, thermodynamic behavior of all AdS-type black holes without charge falls into two classes: Schwarzschild-AdS black holes in even dimensions and Chern-Simons black holes in odd dimensions. The former class can provide the Hawking-Pag...

متن کامل

Greybody factors for rotating black holes in four dimensions

We present the wave equation for a minimally coupled scalar field in the background of a rotating four-dimensional black hole that is parametrized by its mass, angular momentum, and four independent U(1) charges. The near horizon structure is identical to the five-dimensional case, and suggestive of an underlying description in string theory that is valid in the general non-extremal case. We ca...

متن کامل

Hawking radiation from rotating brane black holes ∗

We review recent work [1, 2, 3] on the Hawking radiation of rotating brane black holes, as may be produced at the LHC. We outline the methodology for calculating the fluxes of particles, energy and angular momentum by spin-0, spin-1/2 and spin1 quantum fields on the brane. We briefly review some of the key features of the emission, in particular the changes in the spectra as the number of extra...

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

برای دانلود 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

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2006