Results 1 to 10 of about 250,180 (275)
Decoupling of a Neutron Interferometer from Temperature Gradients [PDF]
Review of Scientific Instruments, 2016 Neutron interferometry enables precision measurements that are typically operated within elaborate, multi-layered facilities which provide substantial shielding from environmental noise.
A. R. Young +16 more
core +7 more sources
Neutron matter at finite temperature [PDF]
Nuclear 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
Structure Factors of Neutron Matter at Finite Temperature [PDF]
Physical Review Letters, 2021 5 pages, 3 figures, data included in submission; further experimental data ...
Andrei Alexandru +3 more
openaire +4 more sources
Discovery of a correlation between the frequency of the mHz quasi-periodic oscillations and the neutron-star temperature in the low-mass X-ray binary 4U 1636-53 [PDF]
, 2014 We detected millihertz quasi-periodic oscillations (QPOs) in an XMM-Newton observation of the neutron-star low-mass X-ray binary 4U 1636-53. These QPOs have been interpreted as marginally-stable burning on the neutron-star surface.
Altamirano, Diego +2 more
core +13 more sources
Transition density and pressure in hot neutron stars [PDF]
, 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
Temperature Distribution in Magnetized Neutron Star Crusts [PDF]
Astronomy & Astrophysics, 2004 We investigate the influence of different magnetic field configurations on the temperature distribution in neutron star crusts. We consider axisymmetric dipolar fields which are either restricted to the stellar crust, ``crustal fields'', or allowed to penetrate the core, ``core fields''. By integrating the two-dimensional heat transport equation in the
Ulrich Geppert, Dany Page, M. Kueker
openaire +5 more sources
Radiation of Neutron Stars Produced by Superfluid Core [PDF]
, 2002 We find that neutron star interior is transparent for collisionless electron sound, the same way as it is transparent for neutrinos. In the presence of magnetic field the electron sound is coupled with electromagnetic radiation and form the fast ...
Amundsen L. +17 more
core +2 more sources
Pairing correlations in N~Z pf-shell nuclei [PDF]
, 1996 We perform Shell Model Monte Carlo calculations to study pair correlations in the ground states of $N=Z$ nuclei with masses A=48-60. We find that $T=1$, $J^{\pi}=0^+$ proton-neutron correlations play an important, and even dominant role, in the ground ...
Alhassid +28 more
core +2 more sources
Forecasting Neutron Star Temperatures: Predictability and Variability [PDF]
Physical Review Letters, 2013 5 pages, 3 figures. Submitted to Phys.
Dany Page, Sanjay Reddy
openaire +4 more sources