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, 2023 Neutron stars are highly compact astrophysical objects and therefore of utmost relevance to learn about theories of gravity. Whereas the proper equation of state of the nuclear matter inside neutron stars is not yet known, and a wide range of equations of state is still compatible with observations, this uncertainty can be overcome to a large extent ...
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What can neutron stars reveal about the equation of state of dense matter? [PDF]
EPJ Web of Conferences, 2020 Neutron stars are astrophysical objects of extremes, reaching the highest densities we can observe in the cosmos, and probing matter under conditions that cannot be recreated in terrestrial experiments.
Tews Ingo
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Structure of Quark Stars [PDF]
, 2012 This paper gives an brief overview of the structure of hypothetical strange quarks stars (quark stars, for short), which are made of absolutely stable 3-flavor strange quark matter.
Orsaria, Milva +3 more
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Thermal properties of hot and dense matter: Influence of rapid rotation on protoneutron stars, hot neutron stars, and neutron star merger remnants [PDF]
EPJ Web of Conferences, 2021 The knowledge of the equation of state is a key ingredient for many dynamical phenomena that depend sensitively on the hot and dense nuclear matter, such as the formation of protoneutron stars and hot neutron stars.
Koliogiannis Polychronis +1 more
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Retention Fractions for Globular Cluster Neutron Stars [PDF]
, 1995 Fokker-Planck models are used to give estimates for the retention fractions for newly-born neutron stars in globular clusters as a function of kick velocity. These can be used to calculate the present day numbers of neutron stars in globular clusters and
Drukier, G. A.
core +2 more sources
Sonoluminescence in neutron stars [PDF]
Physics Letters B, 1998 After a brief discussion of a possible relationship between the electroweak phase transition in highly compressed matter and gravitational collapse, we examine the speculative possibility that the electroweak phase transition might be contemporarily occurring in processes in neutron stars. We conjecture that adiabatic compression of neutron star matter
John G. Learned +3 more
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On the formation history of Galactic double neutron stars [PDF]
Monthly notices of the Royal Astronomical Society, 2018 Double neutron stars (DNSs) have been observed as Galactic radio pulsars, and the recent discovery of gravitational waves from the DNS merger GW170817 adds to the known DNS population.
Alejandro Vigna-G'omez +11 more
semanticscholar +1 more source
Strangeness in neutron stars [PDF]
Nuclear Physics A, 2005 Invited review talk at the VIII International Conference on Hypernuclear and Strange Particle Physics, Jefferson Lab, Newport News, Virginia, October 14-18, 2003.
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Unified equations of state for cold non-accreting neutron stars with Brussels-Montreal functionals. I. Role of symmetry energy [PDF]
Monthly notices of the Royal Astronomical Society, 2018 The theory of the nuclear energy-density functional is used to provide a unified and thermodynamically consistent treatment of all regions of cold non-accreting neutron stars. In order to assess the impact of our lack of complete knowledge of the density
J. Pearson +6 more
semanticscholar +1 more source
Bounds on Neutron- Mirror Neutron Mixing from Pulsar Timings and Gravitational Wave Detections [PDF]
Phys. Rev. D 100, 123021 (2019), 2019 The mass loss in putative neutron star to mixed neutron - mirror neutron star transition implies a significant change of orbital period. The precise constancy of the latter can restrict scenarios recently suggested where neutron to mirror neutron mixing occurring in neutron stars, transforms them into mixed stars helping explain the narrow mass ...
arxiv +1 more source