Results 11 to 20 of about 250,180 (275)
The entrainment matrix of a superfluid neutron-proton mixture at a finite temperature [PDF]
The entrainment matrix (also termed the Andreev-Bashkin matrix or the mass-density matrix) for a neutron-proton mixture is derived at a finite temperature in a neutron star core. The calculation is performed in the frame of the Landau Fermi-liquid theory
Gusakov, M. E., Haensel, P.
core +1 more source
Spin Susceptibility of Neutron Matter at Zero Temperature [PDF]
The Auxiliary Field Diffusion Monte Carlo method is applied to compute the spin susceptibility and the compressibility of neutron matter at zero temperature. Results are given for realistic interactions which include both a two-body potential of the Argonne type and the Urbana IX three-body potential.
Stefano Fantoni+3 more
openaire +3 more sources
ROSAT HRI Observations of the Crab Pulsar: An Improved Temperature upper limit for PSR 0531+21 [PDF]
ROSAT HRI observations have been used to determine an upper limit of the Crab pulsar surface temperature from the off-pulse count rate. For a neutron star mass of 1.4 \Mo and a radius of 10 km as well as the standard distance and interstellar column ...
A Toor+15 more
core +2 more sources
Neutron stars in a chiral model with finite temperature [PDF]
Proceeding to the conference Nuclear Physics in Astrophysics III Accepted for publication in Journal of Physics G: Nuclear and Particle ...
Veronica Dexheimer+2 more
openaire +4 more sources
Temperature-dependent pulsations of superfluid neutron stars [PDF]
We examine radial oscillations of superfluid neutron stars at finite internal temperatures. For this purpose we generalize the description of relativistic superfluid hydrodynamics to the case of superfluid mixtures. We show that in a neutron star at hydrostatic and beta-equilibrium the red-shifted temperature gradient is smoothed out by neutron ...
Nils Andersson+2 more
openaire +4 more sources
Cooling of the Cassiopeia A neutron star and the effect of diffusive nuclear burning
The study of how neutron stars cool over time can provide invaluable insights into fundamental physics such as the nuclear equation of state and superconductivity and superfluidity.
Beznogov, Mikhail+6 more
core +1 more source
Low-temperature neutron diffraction study of MnTe [PDF]
Appearing in J. Magn.
P. R. Sarode+6 more
openaire +3 more sources
Magnetic Fluctuations and Correlations in MnSi - Evidence for a Skyrmion Spin Liquid Phase
We present a comprehensive analysis of high resolution neutron scattering data involving Neutron Spin Echo spectroscopy and Spherical Polarimetry which confirm the first order nature of the helical transition and reveal the existence of a new spin liquid
A. Murani+12 more
core +2 more sources
We calculate the temperature profiles of (thin) accretion disks around rapidly rotating neutron stars (with low surface magnetic fields), taking into account the full effects of general relativity.
Arun V. Thampan+14 more
core +1 more source
In this article we present a neutron diffraction in-situ study of the thermal evolution and high-temperature structure of layered cobaltites Y(Ba, Sr)Co2 O5+{\delta}.
Aurelio G+6 more
core +1 more source