Results 21 to 30 of about 6,843,697 (359)

Structure Factors of Neutron Matter at Finite Temperature [PDF]

open access: yesPhysical Review Letters, 2021
5 pages, 3 figures, data included in submission; further experimental data ...
Andrei Alexandru   +3 more
openaire   +4 more sources

PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter [PDF]

open access: yesAstrophysical Journal, 2019
Neutron stars are not only of astrophysical interest, but are also of great interest to nuclear physicists because their attributes can be used to determine the properties of the dense matter in their cores.
M. Miller   +22 more
semanticscholar   +1 more source

A new thermography using inelastic scattering analysis of wavelength-resolved neutron transmission imaging

open access: yesScientific Reports, 2023
Thermography using energy-dependent neutron transmission imaging can non-invasively and non-destructively visualize a real-space distribution of interior temperatures of a material in a container.
Hirotaka Sato   +4 more
doaj   +1 more source

A sample holder for simultaneous neutron and dielectric spectroscopy – dielectric tests with glycerol, glycerol-water, water and phosphoric acid [PDF]

open access: yesEPJ Web of Conferences, 2022
We report on dielectric test measurements of a rectangular flat sample holder which serves as capacitor and which is aimed for simultaneous neutron and dielectric (n-DE) spectroscopy of acidic liquid samples.
Frick Bernhard   +5 more
doaj   +1 more source

Transition density and pressure in hot neutron stars [PDF]

open access: yes, 2010
Using the momentum-dependent MDI effective interaction for nucleons, we have studied the transition density and pressure at the boundary between the inner crust and liquid core of hot neutron stars.
Chen, Lie-Wen   +3 more
core   +2 more sources

New temperature dependent hyperonic equation of state: Application to rotating neutron star models and I -Q relations [PDF]

open access: yes, 2017
In this work we present a newly constructed equation of state (EoS), applicable to stellar core collapse and neutron star mergers including the entire baryon octet.
M. Marques   +3 more
semanticscholar   +1 more source

Development of a powerful UCN source at PNPI's WWR-M reactor [PDF]

open access: yesEPJ Web of Conferences, 2019
The WWR-M reactor at PNPI is planned to be equipped with a high-flux source for ultracold neutrons (UCNs). The method of UCN production is based on neutron conversion in superfluid helium, exploiting the particular qualities of that quantum liquid.
Serebrov Anatolii   +10 more
doaj   +1 more source

WIMP Annihilation and Cooling of Neutron Stars [PDF]

open access: yes, 2007
We study the effect of WIMP annihilation on the temperature of a neutron star. We shall argue that the released energy due to WIMP annihilation inside the neutron stars, might affect the temperature of stars older than 10 million years, flattening out ...
A. Alpar   +3 more
core   +2 more sources

Investigation on the heat resistance of neutron shielding materials for reactor cavity

open access: yesHe jishu, 2021
BackgroundHigh temperature neutron shielding of the reactor cavity in the third generation nuclear power plant requires a high temperature resistant shielding material, but there is no suitable material that meets the design requirements in the market ...
LIU Xiaoqiang   +3 more
doaj   +1 more source

Signatures of Quark-Hadron Phase Transitions in General-Relativistic Neutron-Star Mergers. [PDF]

open access: yesPhysical Review Letters, 2018
Merging binaries of neutron-stars are not only strong sources of gravitational waves, but also have the potential of revealing states of matter at densities and temperatures not accessible in laboratories.
E. Most   +6 more
semanticscholar   +1 more source

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