Holographic compact stars meet gravitational wave constraints
From MaRDI portal
Publication:1712339
DOI10.1007/JHEP12(2018)078zbMath1405.83012arXiv1711.06244OpenAlexW2769259440MaRDI QIDQ1712339
David Rodríguez Fernández, Carlos Hoyos, Eemeli Annala, Aleksi Vuorinen, Christian Ecker, Niko Jokela
Publication date: 21 January 2019
Published in: Journal of High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1711.06244
Strong interaction, including quantum chromodynamics (81V05) Galactic and stellar structure (85A15) Gravitational waves (83C35)
Related Items (11)
Neutron-star tidal deformability and equation-of-state constraints ⋮ Brane nucleation instabilities in non-AdS/non-CFT ⋮ Holographic QCD in the Veneziano limit and neutron stars ⋮ Gravity dual of a multilayer system ⋮ Towards a holographic quark-hadron continuity ⋮ Low-energy modes in anisotropic holographic fluids ⋮ Quantum information probes of charge fractionalization in large-\(N\) gauge theories ⋮ Holographic fundamental matter in multilayered media ⋮ Interpreting binary neutron star mergers: describing the binary neutron star dynamics, modelling gravitational waveforms, and analyzing detections ⋮ Holographic spontaneous anisotropy ⋮ Novel color superconducting phases of \(\mathcal{N} = 4\) super Yang-Mills at strong coupling
Cites Work
- Unnamed Item
- Holographic phase transitions at finite chemical potential
- Holographic thermodynamics at finite baryon density: some exact results
- Holographic superfluidity in imbalanced mixtures
- Holographic equations of state and astrophysical compact objects
- Gauge theory correlators from non-critical string theory
- Holographic duality with a view toward many-body physics
- Anti de Sitter space and holography
- Coupling constant dependence in the thermodynamics of \({\mathcal N}=4\) supersymmetric Yang-Mills theory.
- Stiff phases in strongly coupled gauge theories with holographic duals
- Towards a holographic quark matter crystal
- Universal formula for the holographic speed of sound
- The large-\(N\) limit of superconformal field theories and supergravity
- Approximate universal relations for neutron stars and quark stars
- Holographic QCD in the Veneziano limit and neutron stars
- Thermodynamic properties of holographic multiquark and the multiquark star
- Dynamical evolution and leading order gravitational wave emission of Riemann-S binaries
- Collective excitations of massive flavor branes
- Holographic Phase Transitions with Fundamental Matter
- Lectures on holographic methods for condensed matter physics
- Adding flavor to AdS/CFT
- I-Love-Q relations for neutron stars in dynamical Chern Simons gravity
- Strongly correlated quantum fluids: ultracold quantum gases, quantum chromodynamic plasmas and holographic duality
- Gauge/String Duality, Hot QCD and Heavy Ion Collisions
- The Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity.
- Low Energy Hadron Physics in Holographic QCD
- Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity
- On Massive Neutron Cores
This page was built for publication: Holographic compact stars meet gravitational wave constraints
