Finite-temperature equations of state for neutron star mergers [PDF]
Physical Review D, 2019 The detection of gravitational waves from a neutron star merger has opened up the possibility of detecting the presence or creation of deconfined quark matter using the gravitational wave signal.
Paul M. Chesler +3 more
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Determining the relaxation time from a temperature-dependent scan of the neutron spin-echo signal amplitude [PDF]
EPJ Web of Conferences, 2022 Temperature-dependent scans of the neutron scattering intensity are commonly employed in high energy-resolution quasielastic measurements. Besides serving as a useful diagnostic tool for identifying the temperature range that could give rise to a ...
Mamontov Eugene, Zolnierczuk Piotr
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Simulation of neutron transmission performance of metallic spherical shell under temperature dependent neutron cross section [PDF]
EPJ Web of Conferences, 2020 To study the effect of temperature dependent neutron cross section on the neutron transmission performance of typical metallic spherical shells, this paper generated the temperature dependent neutron cross section data by using NJOY program, and ...
Zuo Yinghong, Zhu Jinhui, Xie Honggang
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Cooling of neutron stars with quark-hadron continuity [PDF]
EPJ Web of Conferences, 2022 Neutron stars are high-density objects formed by the gravitational collapse of massive stars, and the whole star can be likened to a giant nucleus. The interior of a neutron star is considered to contain exotic particles and states which do not appear in
Noda Tsuneo +4 more
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Measurement of temperature-dependent thermal neutron spectrum in CaH2 moderator material for space reactor [PDF]
EPJ Web of Conferences, 2020 In order to accurately design a CaH2 moderated small high-temperature reactor, it is necessary to experimentally confirm the temperature-dependent thermal neutron spectrum in the CaH2 moderator material.
lee Jaehong +6 more
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Materials & Design, 2021 The effects of vacuum induction melting (VIM) vacuum (
Liang Zheng +6 more
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Gravitational wave signatures of phase transition from hadronic to quark matter in isolated neutron stars and binaries [PDF]
EPJ Web of Conferences, 2022 The fundamental constituent of matter at high temperature and density has intrigued physicists for quite some time. Recent results from heavy-ion colliders have enriched the Quantum Chromodynamics phase diagram at high temperatures and low baryon density.
Mallick Ritam
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Finite-temperature equation of state with hyperons [PDF]
EPJ Web of Conferences, 2022 We present the novel finite-temperature FSU2H* equation-of-state model that covers a wide range of temperatures and lepton fractions for the conditions in proto-neutron stars, neutron star mergers and supernovae.
Kochankovski Hristijan +2 more
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Study on Moderation Properties of Cold Mesitylene using KUANS [PDF]
EPJ Web of Conferences, 2020 Neutron moderation properties from the cold mesitylene moderator have been studied. Kyoto University Accelerator driven Neutron Source has been used for these experiments. The container of the mesitylene moderator is situated in front of the polyethylene
Tasaki Seiji +4 more
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Finite-temperature Extension for Cold Neutron Star Equations of State [PDF]
Astrophysical Journal, 2019 Observations of isolated neutron stars place constraints on the equation of state (EOS) of cold, neutron-rich matter, while nuclear physics experiments probe the EOS of hot, symmetric matter.
C. Raithel, F. Özel, D. Psaltis
semanticscholar +1 more source