[PDF] Top 20 Equation of State of Dense Matter and Consequences for Neutron Stars

... of matter in neutron ...at matter in beta–equilibrium above roughly 3 times nuclear matter density, we discuss the constraints on the possible maximum mass when hyperons are included in the ... See full document

... current state-of-the-art for nuclear forces, and make it especially suited when studying systems that are not accessible in experiments, like neutron-rich ... See full document

... interacting matter at densities of a few times saturation den- sity, which are likely to be reached in the core of neutron stars, is one of the most interesting and challenging problem in nuclear and ... See full document

... However, independent of the interaction model, including hyperons (or other states) as additional degrees of freedom softens the equation of state and in turn reduces the maximum star mass. There- fore, ... See full document

... hadronic matter description is based on relativis- tic density functional of nuclear matter with density-dependent couplings, see ...quark matter equation of state is based on the ... See full document

... a neutron star binary ...of matter at the extreme conditions found in the interior of these ...on neutron star ...were neutron stars that are described by the same equation of ... See full document

... a neutron star binary ...of matter at the extreme conditions found in the interior of these ...on neutron star ...were neutron stars that are described by the same equation of ... See full document

... relativistic stars and the research on gravitational collapse is of fundamental importance in astrophysics since the formulation of general theory of ...relativistic stars we can refer to the pioneering ... See full document

... in dense hadronic matter. Many NS equation of states (EOS) with medium dependent hadronic properties have been calculated but is’s still quite uncertain which EOS is ... See full document

... of neutron stars and microscopic quantities of nuclear matter, such as consistency of hadronic nuclear models and observed masses of neutron ...and neutron matter is inadequate ... See full document

... The equation of state of pure neutron matter is shown in ...the equation of state given by ...of neutron drops with N near closed shells can be used to adjust the ... See full document

... nuclear matter are calculated from the exact in-medium single-particle ...Dyson equation, where medium effects are taken into account by the irreducible self-energy that is ob- tained from an expansion in ... See full document

... quark matter first within a purely theo- retical approach, by using three different chiral models for quark matter and after within phenomeno- logical approach through the measurements of masses and radii ... See full document

... a neutron star?, is a question whose answer is not unique and depends on who is ...little stars observed as radio pulsars or sources of X- and γ-rays, whereas particle physicists would say that they are ... See full document

... The neutron star is considered as a nonrotating spherical object com- posed of a degenerate neutron gas at zero ...(TOV) equation [5], generalized by inclusion of neutrostriction ... See full document

... the neutron-star matter con- sists of only protons and neutrons without Λ (the dashed lines), the proton fraction and therefore the electron fraction increase gradually as the density increases, while the ... See full document

... bright stars or active late-type ...2003). Stars with spectral types A–M can have some detectable X-ray emission (largely dependent on rotation and magnetic fields) that appears as a hot (5–7 × 10 6 K) ... See full document

... accreting neutron stars systems as probes of neutron star ...accreting neutron stars during ...these neutron stars do not show evidence of spin variations during the ... See full document

... Gravitational-wave chirp created from the collision of two neutron stars..[r] ... See full document

... find an answer through experiment, we could use a photographic camera whose shutter time can be reduced at will. What would we find? When the shutter time approaches the oscillation period of light, the sharpness of the ... See full document