Results 21 to 30 of about 202,682 (289)
Neutron-Mirror Neutron oscillations in Matter
, 2021 12 pages, 3 figures, submitted to MDPI "Symmetry ...
Kamyshkov, Yuri +3 more
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Triplet pairing in neutron matter [PDF]
Nuclear Physics A, 2001 The separation method developed earlier by us [Nucl. Phys. {\bf A598} 390 (1996)] to calculate and analyze solutions of the BCS gap equation for $^1$S$_0$ pairing is extended and applied to $^3$P$_2$--$^3$F$_2$ pairing in pure neutron matter. The pairing matrix elements are written as a separable part plus a remainder that vanishes when either momentum
Khodel, V. V. +2 more
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npj Quantum Materials, 2021 Materials with exceptional magnetism and superconductivity usually conceive emergent physical phenomena. Here, we investigate the physical properties of the (Eu,La)FeAs2 system with double magnetic sublattices.
Jia Yu +10 more
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Probing Mechanical and Chemical Instabilities in Neutron-Rich Matter [PDF]
, 2001 The isospin-dependence of mechanical and chemical instabilities is investigated within a thermal and nuclear transport model using a Skyrme-type phenomenological equation of state for neutron-rich matter.
Akmal +49 more
core +2 more sources
Square and rhombic lattices of magnetic skyrmions in a centrosymmetric binary compound
Nature Communications, 2022 Typically, skyrmions appear in magnet systems which are non-centrosymmetric. Here, using neutron and X-ray scattering, Takagi et al show the emergence of a skyrmion phase in the centrosymmetric material EuAl4.
Rina Takagi +15 more
doaj +1 more source
Universe, 2020 Neutron stars change their structure with accumulation of dark matter. We study how their mass is influenced from the environment. Close to the sun, the dark matter accretion from the neutron star does not have any effect on it.
Antonino Del Popolo +2 more
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The Astrophysical Journal, 1978 A relativistic theory of high-density matter is presented which takes into account the short-range interaction due to the exchange of spin-2 mesons. An equation of state is derived and used to compute neutron-star properties. The prediction of the theory for the values of maximum mass and moment of inertia for a stable neutron star are 1.75 solar ...
V. Canuto, B. Datta, G. Kalman
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Proton and neutron superfluidity in neutron star matter [PDF]
Nuclear Physics A, 1992 Abstract The 3 P 2 neutron superfluidity and the 1 S 0 proton superfluidity in neutron star matter are investigated by solving the gap equation exactly for a realistic nucleon-nucleon potential, namely the Argonne v 14 potential. For the 3 P 2 case, our results point to a nearly isotropic pairing function, in close analogy with the rigorous ...
Cugnon, Joseph +3 more
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Isospin Asymmetry in Nuclei and Neutron Stars [PDF]
, 2004 The roles of isospin asymmetry in nuclei and neutron stars are investigated using a range of potential and field-theoretical models of nucleonic matter.
A.W. Steiner +95 more
core +1 more source
Dark-matter admixed neutron stars [PDF]
Physical Review D, 2011 We study the hydrostatic equilibrium configuration of an admixture of degenerate dark matter and normal nuclear matter by using a general relativistic two-fluid formalism. We consider non- self-annihilating dark matter particles of mass ~ 1 GeV. The mass-radius relations and moments of inertia of these dark-matter admixed neutron stars are investigated
Leung, S. -C., Chu, M. -C., Lin, L. -M.
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