Semiclassical Effects in Color Flavor Locked Strange Stars
arXiv:2107.06052 · doi:10.1007/s13538-022-01161-0
Abstract
Strange stars in the color flavor locked phase, as described by a generalization of the phenomenological MIT bag model proposed in the context of color superconductivity, are studied through a model motivated by the semiclassical solutions for hydrostatic equilibrium. Results show that within this framework it is possible to find ultracompact configurations situated between regular compact stars and black holes.
References in corpus (32)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- GW170817: Measurements of Neutron Star Radii and Equation of State
- GW190814: Gravitational Waves from the Coalescence of a 23 M Black Hole with a 2.6 M Compact Object
- Color superconductivity in dense quark matter
- A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy
- Refined Mass and Geometric Measurements of the High-Mass PSR J0740+6620
- Strange Quark Matter and Compact Stars
- Is the gravitational-wave ringdown a probe of the event horizon?
- Decoupling gravitational sources in general relativity: from perfect to anisotropic fluids
- The observational evidence for horizons: from echoes to precision gravitational-wave physics
- Tests for the existence of horizons through gravitational wave echoes
- Fate of gravitational collapse in semiclassical gravity
- Color-flavor locked strange matter
- Was GW190814 a black hole -- strange quark star system?
- Causality and the speed of sound
- Visual Distortions Near a Neutron Star and Black Hole
- A CDM bounce scenario
- Stellar equilibrium in semiclassical gravity
- On gravitational echoes from ultracompact exotic stars
- Constraining color flavor locked strange stars in the gravitational wave era
- On gravitational-wave echoes from neutron-star binary coalescences
- Constraining the Neutron Star Mass--Radius Relation and Dense Matter Equation of State with NICER. III. Model Description and Verification of Parameter Estimation Codes
- Awaking the vacuum in relativistic stars
- Vacuum polarization in the Schwarzschild spacetime and dimensional reduction
- Mass bounds for compact spherically symmetric objects in generalized gravity theories
- Gravity-induced vacuum dominance
- THERMODYNAMIC PROPERTIES OF --FLUIDS AND THE QUANTUM VACCUM
- Gravitational vacuum polarization
- Gravitational Waves from Perturbed Black Holes and Relativistic Stars
- Bag vs. NJL models for color-flavor-locked strange quark matter
- Vacuum fluctuation inside a star and their consequences for neutron stars, a simple model
- Wormhole geometries supported by quark matter at ultra-high densities