scholarly journals Is there a breakdown of effective field theory at the horizon of an extremal black hole?

2017 ◽  
Vol 2017 (12) ◽  
Author(s):  
Shahar Hadar ◽  
Harvey S. Reall
Keyword(s):  
Field Theory ◽  
Black Hole ◽  
Effective Field Theory ◽  
Effective Field ◽  
Extremal Black Hole

A UV complete picture of black hole conforming to low energy effective field theory

2018 ◽  
Vol 33 (36) ◽  
pp. 1850219
Author(s):  
Biplab Paik
Keyword(s):  
Field Theory ◽  
Black Hole ◽  
Effective Field Theory ◽  
Effective Field ◽  
Radiation Process ◽  
Quantum Black Hole ◽  
Classical Geometry ◽  
Characteristic Radius ◽  
Hole Geometry ◽  
Principle Of Causality

In this paper, we propose a UV complete, quantum improved picture of a black hole geometry that conforms to the IR gravity of effective field theory. Our work builds on identifying an effective space-distributed notion of black hole fluid in quantum improved regular Einstein gravity and its theoretical correspondence with a cosmology inspired power law fluctuation of matter. Hence, we make use of phenomenological asymptotic scales of matter fluctuation in static space to consequently derive a UV complete line-element of black hole space–time. In this appraisal, it gets explicit how principle of causality is preserved even while there is an effective spread of black hole fluid across horizon(s). Gravity changes from its conventional classical geometry-state to a quantum masked profile across a hypersurface of characteristic radius [Formula: see text]. We make analyses that probe the newly proposed quantum improved gravity in the contexts of regularity of Einstein fields, complete predictability of Hawking radiation process, and first law of black hole thermodynamics. It emerges that quantum black hole geometry self-regulates a regular timelike core that is abide by every quantum theoretical constraint while being flat around its center.

scholarly journals Black hole entropy sourced by string winding condensate

2021 ◽  
Vol 2021 (10) ◽  
Author(s):  
Ram Brustein ◽  
Yoav Zigdon
Keyword(s):  
Field Theory ◽  
Black Hole ◽  
Effective Field Theory ◽  
Thermal Cycle ◽  
Black Hole Entropy ◽  
Effective Field ◽  
Schwarzschild Black Hole ◽  
Asymptotically Linear ◽  
Linear Dilaton ◽  
Linear Dilaton Black Hole

Abstract We calculate the entropy of an asymptotically Schwarzschild black hole, using an effective field theory of winding modes in type II string theory. In Euclidean signature, the geometry of the black hole contains a thermal cycle which shrinks towards the horizon. The light excitations thus include, in addition to the metric and the dilaton, also the winding modes around this cycle. The winding modes condense in the near-horizon region and source the geometry of the thermal cycle. Using the effective field theory action and standard thermodynamic relations, we show that the entropy, which is also sourced by the winding modes condensate, is exactly equal to the Bekenstein-Hawking entropy of the black hole. We then discuss some properties of the winding mode condensate and end with an application of our method to an asymptotically linear-dilaton black hole.

scholarly journals Effective field theory of black hole echoes

2018 ◽  
Vol 2018 (9) ◽  
Author(s):  
C. P. Burgess ◽  
Ryan Plestid ◽  
Markus Rummel
Keyword(s):  
Field Theory ◽  
Black Hole ◽  
Effective Field Theory ◽  
Effective Field

scholarly journals Spinning black hole binary dynamics, scattering amplitudes, and effective field theory

2021 ◽  
Vol 104 (6) ◽  
Author(s):  
Zvi Bern ◽  
Andres Luna ◽  
Radu Roiban ◽  
Chia-Hsien Shen ◽  
Mao Zeng
Keyword(s):  
Field Theory ◽  
Black Hole ◽  
Scattering Amplitudes ◽  
Effective Field Theory ◽  
Effective Field ◽  
Black Hole Binary

Euclidean gravity and holography

2021 ◽  
pp. 2141005
Author(s):  
Daniel Harlow ◽  
Edgar Shaghoulian
Keyword(s):  
Field Theory ◽  
Black Holes ◽  
Black Hole ◽  
Effective Field Theory ◽  
Effective Field ◽  
Low Energy ◽  
Recent Proposal ◽  
Black Hole Evaporation ◽  
Natural Mechanism ◽  
Deep Ultraviolet

We discuss a recent proposal that the Euclidean gravity approach to quantum gravity is correct if and only if the theory is holographic, providing several examples and general arguments to support the conjecture. This provides a natural mechanism for the low-energy gravitational effective field theory to access a host of deep ultraviolet properties, like the Bekenstein–Hawking entropy of black holes, the unitarity of black hole evaporation, and the lack of exact global symmetries.

scholarly journals THE DELOCALIZED EFFECTIVE DEGREES OF FREEDOM OF A BLACK HOLE AT LOW FREQUENCIES

2008 ◽  
Vol 17 (13n14) ◽  
pp. 2617-2624 ◽  
Author(s):  
BARAK KOL
Keyword(s):  
Field Theory ◽  
Black Hole ◽  
Effective Field Theory ◽  
Degrees Of Freedom ◽  
World Line ◽  
Low Frequency ◽  
Effective Field ◽  
Theory Approach ◽  
Low Frequencies ◽  
Long Wavelength

Identifying the fundamental degrees of freedom of a black hole poses a long-standing puzzle. Recently Goldberger and Rothstein forwarded a theory of the low frequency degrees of freedom within the effective field theory approach, where they are relevancy-ordered but of unclear physical origin. Here these degrees of freedom are identified with near-horizon but non-compact gravitational perturbations which are decomposed into delocalized multipoles. Their world-line (kinetic) action is determined within the classical effective field theory (CLEFT) approach and their interactions are discussed. The case of the long-wavelength scattering of a scalar wave off a Schwarzschild black hole is treated in some detail, interpreting within the CLEFT approach the equality of the leading absorption cross section with the horizon area.

scholarly journals Effective field theory of black hole quasinormal modes in scalar-tensor theories

2019 ◽  
Vol 2019 (2) ◽  
Author(s):  
Gabriele Franciolini ◽  
Lam Hui ◽  
Riccardo Penco ◽  
Luca Santoni ◽  
Enrico Trincherini
Keyword(s):  
Field Theory ◽  
Black Hole ◽  
Effective Field Theory ◽  
Quasinormal Modes ◽  
Effective Field
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