Results 11 to 20 of about 6,843,697 (359)

Study on Moderation Properties of Cold Mesitylene using KUANS [PDF]

open access: yesEPJ 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
doaj   +1 more source

Finite-temperature equation of state with hyperons [PDF]

open access: yesEPJ 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
doaj   +1 more source

Smoke and mirrors: Neutron star internal heating constraints on mirror matter [PDF]

open access: yesPhys. Rev. Lett. 127, 061805 (2021), 2021
Mirror sectors have been proposed to address the problems of dark matter, baryogenesis, and the neutron lifetime anomaly. In this work we study a new, powerful probe of mirror neutrons: neutron star temperatures. When neutrons in the neutron star core convert to mirror neutrons during collisions, the vacancies left behind in the nucleon Fermi seas are ...
arxiv   +1 more source

Neutron matter at finite temperature [PDF]

open access: yesNuclear Physics A, 2008
We calculate the neutron matter equation of state at finite temperature based on low-momentum two- and three-nucleon interactions. The free energy is obtained from a loop expansion around the Hartree-Fock energy, including contributions from normal and anomalous diagrams.
Achim Schwenk, Laura Tolos, Bengt Friman
openaire   +3 more sources

Finite-temperature Extension for Cold Neutron Star Equations of State [PDF]

open access: yesAstrophysical 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

Neutron scattering in the proximate quantum spin liquid α-RuCl3 [PDF]

open access: yesScience, 2017
Sighting of magnetic Majorana fermions? Quantum spin liquids—materials whose magnetic spins do not settle into order even at absolute zero temperature—have long captured the interest of physicists. A particularly lofty goal is finding a material that can
A. Banerjee   +9 more
semanticscholar   +2 more sources

Finite-temperature equations of state for neutron star mergers [PDF]

open access: yesPhysical 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.
P. Chesler   +3 more
semanticscholar   +1 more source

Neutron yield scaling law in laser-cluster fusion experiments

open access: yesNuclear Fusion, 2023
We present a scaling law ( $Y\sim {E^\beta }$ ) of fusion neutron yields ( Y ) for laser pulse energy ( E ) in laser-cluster fusion experiments. We compare the available neutron yield data from previous deuterium cluster fusion experiments with those ...
Junho Won   +4 more
doaj   +1 more source

Diffusive nuclear burning in cooling simulations and application to new temperature data of the Cassiopeia A neutron star [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2019
A critical relation in the study of neutron star cooling is the one between surface temperature and interior temperature. This relation is determined by the composition of the neutron star envelope and can be affected by the process of diffusive nuclear ...
M. Wijngaarden   +7 more
semanticscholar   +1 more source

Spontaneous scalarization in proto-neutron stars

open access: yesEuropean Physical Journal C: Particles and Fields, 2023
Proto-neutron stars are born when a highly evolved and massive star collapses under gravity. In this paper, we investigate the spontaneous scalarization in proto-neutron stars.
Fahimeh Rahimi, Zeinab Rezaei
doaj   +1 more source

Home - About - Disclaimer - Privacy