Emission and cooling of a newborn quark star
astro-ph.HE, hep-ph
Submitted: 2026-09-28
Updated: 2026-09-28
Terminology
Sources
- Nonstrange and strange quark matter at finite temperature within modified NJL model and protoquark stars
- Interacting $ud$ and $uds$ quark matter at finite densities and quark stars
- Non-strange quark stars within resummed QCD
- Core-collapse Supernova Explosions Driven by the Hadron-quark Phase Transition as a Rare $r$-process Site
- On the formation of strange quark stars from supernova in compact binaries
- Thermal emission from bare quark matter surfaces of hot strange stars
- Thermalization of a nonequilibrium electron-positron-photon plasma
- Structure of pair winds from compact objects with application to emission from hot bare strange stars
- Numerical Simulation of the Hydrodynamical Combustion to Strange Quark Matter
- Combustion of a neutron star into a strange quark star: The neutrino signal
- Combustion of a hadronic star into a quark star: the turbulent and the diffusive regimes
- A Hydrodynamical Study on the Conversion of Hadronic Matter to Quark Matter: I. Shock-Induced Conversion
- Dynamical phase transition in neutron stars
- Neutrino diagnostics of hadron-quark phase transition in Neutron Stars
- Pair creation in hot electrosphere of compact astrophysical objects
- Bremsstrahlung emission from quark stars
- Effect of electric field of the electrosphere on photon emission from quark stars
- Photon emission from bare quark stars
- Cooling of quark stars from perturbative QCD
- Electron-positron plasma in GRBs and in cosmology
Related papers
- Numerical Studies of Accretion Flows onto a Neutron Star Engulfed in a Massive Star
- Collisionless Accretion of Finite-Angular-Momentum Plasma onto a Spinning Black Hole
- Impact of Magnetic Field Topology on Electromagnetic and Gravitational Waves from Binary Neutron Star Merger Remnants
- XRISM Resolve Spectroscopy of GX 5-1: Constraints on Iron Spectral Features in a Luminous Neutron-Star Binary
- SN 1006: A Cosmic Laboratory for Investigating Shock Acceleration Physics
- Neutrino Spectral Pinching in 3D Core-Collapse Supernovae: Late-Time Convergence, Failed-Explosion Signatures, and Viewing-Angle Dispersion