Black hole horizon edge partition functions

نویسندگان

چکیده

A bstract We extend a formula for 1-loop black hole determinants by Denef, Hartnoll, and Sachdev (DHS) to spinning fields on any ( d + 1)-dimensional static spherically symmetric hole. By carefully analyzing the regularity condition imposed Euclidean eigenfunctions, we reveal an unambiguous bulk-edge split in partition function tensor of arbitrary integer spin: bulk part captures “renormalized” thermal canonical recently discussed [1]; edge is related quasinormal modes (QNMs) that fail analytically continue subset with enhanced fall-offs near origin. Since takes form path integral S d− 1 , this suggests these are associated degrees freedom living bifurcation surface Lorentzian two-sided geometry. For massive higher spin BTZ vector Nariai holes, find QNMs lowest overtone numbers.

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

Duality and Black Hole Partition Functions

Supersymmetric black holes provide an excellent theoretical laboratory to test ideas about quantum gravity in general and black hole entropy in particular. When four-dimensional supergravity is interpreted as the low-energy approximation of ten-dimensional string theory or eleven-dimensional M-theory, one has a microscopic description of the black hole which allows one to count microstates and ...

متن کامل

From Special Geometry to Black Hole Partition Functions

These notes are based on lectures given at the Erwin-Schrödinger Institut in Vienna in 2006/2007 and at the 2007 School on Attractor Mechanism in Frascati. Lecture I reviews special geometry from the superconformal point of view. Lecture II discusses the black hole attractor mechanism, the underlying variational principle and black hole partition functions. Lecture III applies the formalism int...

متن کامل

On Black Hole Horizon Fluctuations

A study of the high angular momentum particles ’atmosphere’ near the Schwarzschild black hole horizon suggested that strong gravitational interactions occur at invariant distance of the order of 3 √ M . We present a generalization of this result to the Kerr-Newman black hole case. It is shown that the larger charge and angular momentum black hole bears, the larger invariant distance at which st...

متن کامل

Entanglement entropy of the black hole horizon

We examine a possibility that, when a black hole is formed, the information on the collapsed star is stored as the entanglement entropy between the outside and the thin region (of the order of the Planck length) of the inside the horizon. For this reason, we call this as the entanglement entropy of the black hole “horizon”. We construct two models, one is in the Minkowski spacetime and the othe...

متن کامل

Black hole thermodynamics from Euclidean horizon constraints.

To explain black hole thermodynamics in quantum gravity, one must introduce constraints to ensure that a black hole is actually present. I show that for a large class of black holes, such "horizon constraints" allow the use of conformal field theory techniques to compute the density of states, reproducing the Bekenstein-Hawking entropy in a nearly model-independent manner. One standard string t...

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: 2023

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

DOI: https://doi.org/10.1007/jhep06(2023)025