Results 11 to 20 of about 250,180 (275)

The entrainment matrix of a superfluid neutron-proton mixture at a finite temperature [PDF]

open access: yes, 2005
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]

open access: yesPhysical Review Letters, 2001
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]

open access: yes, 1995
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]

open access: yesJournal of Physics G: Nuclear and Particle Physics, 2007
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]

open access: yesMonthly Notices of the Royal Astronomical Society, 2006
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

open access: yes, 2019
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]

open access: yesJournal of Magnetism and Magnetic Materials, 2005
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

open access: yes, 2011
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

Temperature Profiles of Accretion Disks around Rapidly Rotating Neutron Stars in General Relativity and Implications for Cygnus X-2

open access: yes, 2000
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

High temperature behavior of Sr-doped layered cobaltites Y(Ba1-xSrx)Co2O5.5: phase stability and structural properties

open access: yes, 2010
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

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