Gauge theory meets cosmology
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Publication:6670455
DOI10.1088/1475-7516/2024/12/040MaRDI QIDQ6670455
J. F. Morales, Massimo Bianchi, Giuseppe Dibitetto
Publication date: 23 January 2025
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Cites Work
- Gauge theories on {\(\Omega\)}-backgrounds from non commutative Seiberg-Witten curves
- Type IIB superstrings, BPS monopoles, and three-dimensional gauge dynamics
- Seiberg-Witten prepotential from instanton counting
- Deforming SW curve
- Domain-wall/cosmology correspondence in AdS/dS supergravity
- Infinite conformal symmetry in two-dimensional quantum field theory
- Analytic black hole perturbation approach to gravitational radiation
- QNMs of branes, BHs and fuzzballs from quantum SW geometries
- More on the SW-QNM correspondence
- Black hole quasinormal modes and Seiberg-Witten theory
- Bootstrapping inflationary correlators in Mellin space
- Liouville correlation functions from four-dimensional gauge theories
- CFT description of BH's and ECO's: QNMs, superradiance, echoes and tidal responses
- Irregular Liouville correlators and connection formulae for Heun functions
- Black hole perturbation
- Quantization of Integrable Systems and Four Dimensional Gauge Theories
- Stability of a Schwarzschild Singularity
- AN ALGORITHM FOR THE MICROSCOPIC EVALUATION OF THE COEFFICIENTS OF THE SEIBERG–WITTEN PREPOTENTIAL
- Primordial black holes—perspectives in gravitational wave astronomy
- Cosmological parameters from SDSS and WMAP
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Hybrid α-attractors, primordial black holes and gravitational wave backgrounds
- Charge instability of JMaRT geometries
- 2-charge circular fuzz-balls and their perturbations
- On the stability and deformability of top stars
- Post Newtonian emission of gravitational waves from binary systems: a gauge theory perspective
- Tidal resonances for fuzzballs
- Renormalisation of IR divergences and holography in de Sitter
- Charge (in)stability and superradiance of topological stars
- Non-spinning tops are stable
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