Worldsheet computation of heavy-light correlators
High Energy Physics - Theory
family
n-point function
QC770-798
AdS-CFT Correspondence
01 natural sciences
General Relativity and Quantum Cosmology
membrane model
decoupling
conformal
charge
https://purl.org/becyt/ford/1.3
black hole
String (physics)
Worldsheet
String theory
correlation function
string model
High-Energy Collider
Quantum electrodynamics
[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]
BLACK HOLES IN STRING THEORY
Physics
Particle physics
Conformal Field Models in String Theory
Mathematical physics
twist
Physical Sciences
[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]
duality
Theoretical physics
CONFORMAL FIELD MODELS IN STRING THEORY
Non-critical string theory
Nuclear and High Energy Physics
5
FOS: Physical sciences
General Relativity and Quantum Cosmology (gr-qc)
field theory
530
Quantum mechanics
Nuclear and particle physics. Atomic energy. Radioactivity
Black Holes in String Theory
0103 physical sciences
anti-de Sitter
vertex
Cosmological Parameters and Dark Energy
Particle Physics and High-Energy Collider Experiments
https://purl.org/becyt/ford/1
background
fluctuation
Astronomy and Astrophysics
ADS-CFT CORRESPONDENCE
Holographic Derivation of Field Theories and Gravity
radiation
chiral
Orbifold
Physics and Astronomy
High Energy Physics - Theory (hep-th)
Hawking
Wess-Zumino-Witten model
string
operator
microstate
orbifold
holography
coset space
DOI:
10.1007/jhep03(2023)066
Publication Date:
2023-03-11T04:35:08Z
AUTHORS (4)
ABSTRACT
Abstract
We compute a large collection of string worldsheet correlators describing light probes interacting with heavy black hole microstates. The heavy states consist of NS5 branes carrying momentum and/or fundamental string charge. In the fivebrane decoupling limit, worldsheet string theory on a family of such backgrounds is given by exactly solvable null-gauged WZW models. We construct physical vertex operators in these cosets, including all massless fluctuations. We compute a large class of novel heavy-light-light-heavy correlators in the AdS3 limit, where the light operators include those dual to chiral primaries of the holographically dual CFT. We compare a subset of these correlators to the holographic CFT at the symmetric product orbifold point, and find precise agreement in all cases, including for light operators in twisted sectors of the orbifold CFT. The agreement is highly non-trivial, and includes amplitudes that describe the analogue of Hawking radiation for these microstates. We further derive a formula for worldsheet correlators consisting of n light insertions on these backgrounds, and discuss which subset of these correlators are likely to be protected. As a test, we compute a heavy-light five-point function, obtaining precisely the same result both from the worldsheet and the symmetric orbifold CFT. This paper is a companion to and extension of [1].
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