Stability of generalized Einstein-Maxwell-scalar black holes

نویسندگان

چکیده

A bstract We study the stability of static black holes in generalized Einstein-Maxwell-scalar theories. derive master equations for odd and even parity perturbations. The sufficient necessary conditions under odd-parity perturbations are derived. show that these usually not similar to energy simplest case a minimally coupled scalar field. obtain even-parity also derived speed propagation five degrees freedom obtained class theories which all propagate at light. Finally, we have applied our results various nonlinear electrodynamics, scalar-tensor Einstein-Maxwell-dilaton theory. For latter, calculated quasinormal modes.

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

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Einstein-Maxwell-Chern-Simons Black Holes

5-dimensional Einstein-Maxwell-Chern-Simons theory with Chern-Simons coefficient λ = 1 has supersymmetric black holes with vanishing horizon angular velocity, but finite angular momentum. Here supersymmetry is associated with a borderline between stability and instability, since for λ > 1 a rotational instability arises, where counterrotating black holes appear, whose horizon rotates in the opp...

متن کامل

On uniqueness of static Einstein-Maxwell-dilaton black holes

We prove uniqueness of static, asymptotically flat spacetimes with nondegenerate black holes for three special cases of Einstein-Maxwell-dilaton theory: For the coupling “α = 1” (which is the low energy limit of string theory) on the one hand, and for vanishing magnetic or vanishing electric field (but arbitrary coupling) on the other hand. Our work generalizes in a natural, but non-trivial way...

متن کامل

Black holes with regular horizons in Maxwell - scalar gravity .

A class of exact static spherically symmetric solutions of the Einstein-Maxwell gravity coupled to a massless scalar field has been obtained in harmonic coordinates of the Minkowski space-time. For each value of the coupling constant a, these solutions are characterized by a set of three parameters, the physical mass μ0, the electric charge Q0 and the scalar field parameter k. We have found tha...

متن کامل

Cold Black Holes in the Einstein-Scalar Field System

We study Einstein gravity coupled to a massless scalar field in a static spherically symmetric space-time in four dimensions. Black hole solutions exist when the kinetic energy of the scalar field is negative, that is, for a phantom field. These “scalar black holes” have an infinite horizon area and zero temperature. They are related through a conformal transformation with similar objects in th...

متن کامل

Structure and Stability of Cold Scalar-tensor Black Holes

We study the structure and stability of the recently discussed spherically symmetric Brans-Dicke black-hole type solutions with an infinite horizon area and zero Hawking temperature, existing for negative values of the coupling constant ω . These solutions split into two classes: B1, whose horizon is reached by an infalling particle in a finite proper time, and B2, for which this proper time is...

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

ژورنال

عنوان ژورنال: Journal of High Energy Physics

سال: 2022

ISSN: ['1127-2236', '1126-6708', '1029-8479']

DOI: https://doi.org/10.1007/jhep02(2022)020