Five-dimensional electrostatic black holes in a background field

نویسندگان

چکیده

We consider $5$ dimensional electrostatic solutions to Einstein-Maxwell gravity with $2$ commuting spacelike Killing fields. Taking two distinct reductions from dimensions a $3$ base space, we write the equations using some axially symmetric functions on $\mathbb{R}^3$. These can be viewed as arising harmonic map coupled 3-dimensional isometries of target space this revealing hidden $SL(2,\mathbb{R})$ symmetry sector theory. Depending choice reduction then gives rise different 1-parameter families transformations corresponding either charging black hole or immersing it in background electric field. use these charge static Saturn and $L(n,1)$ lens spacetime by tuning strength external field, cure conical singularities give new regular solutions. Notably electrified generated is first example topologically trivial asymptotics.

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

Notes on Five-dimensional Kerr Black Holes

The geometry of five-dimensional Kerr black holes is discussed based on geodesics and Weyl curvatures. Kerr-Star space, Star-Kerr space and Kruskal space are naturally introduced by using special null geodesics. We show that the geodesics of AdS Kerr black hole are integrable, which generalizes the result of Frolov and Stojkovic. We also show that five-dimensional AdS Kerr black holes are isosp...

متن کامل

Fermion Emission from Five-Dimensional Black Holes

We calculate semiclassically the emission rate of spin 1 2 particles from charged, nonrotating black holes in D = 5, N = 8 supergravity. The relevant Dirac equation is solved by the same approximation as in the bosonic case. The resulting expression for the emission rate has a form which is predicted from D-brane effective field theory. 1 E-mail: [email protected]

متن کامل

Five-Dimensional Charged Rotating Black Holes

We consider charged rotating black holes in 5-dimensional EinsteinMaxwell theory. These black holes are asymptotically flat, they possess a regular horizon of spherical topology and two independent angular momenta associated with two distinct planes of rotation. We discuss their global and horizon properties, and derive a generalized Smarr formula. We construct these black holes numerically, fo...

متن کامل

Phases of Five-Dimensional Black Holes

We argue that the configurations of maximal entropy in five-dimensional asymptotically flat vacuum gravity, for fixed mass and angular momentum, are ‘black Saturns’ with a central, close to static, black hole and a very thin black ring around it. For any value of the angular momentum, the upper bound on the entropy is equal to the entropy of a static black hole of the same total mass. For fixed...

متن کامل

Supersymmetric Quantum Black Holes in Five Dimensional Heterotic String Vacua

Exact black hole solutions of the five dimensional heterotic S-T -U model including all perturbative quantum corrections and preserving 1/2 of N = 2 supersymmetry are studied. It is shown that the quantum corrections yield a bound on electric charges and harmonic functions of the solutions.

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: Classical and Quantum Gravity

سال: 2022

ISSN: ['1361-6382', '0264-9381']

DOI: https://doi.org/10.1088/1361-6382/ac5814