Results 41 to 50 of about 6,857,496 (360)
Scientific Reports, 2020 Stacking fault energies (SFE) were determined in additively manufactured (AM) stainless steel (SS 316 L) and equiatomic CrCoNi medium-entropy alloys. AM specimens were fabricated via directed energy deposition and tensile loaded at room temperature.
W. Woo +8 more
doaj +1 more source
On the deconfinement phase transition in neutron-star mergers [PDF]
European Physical Journal A, 2019 We study in detail the nuclear aspects of a neutron-star merger in which deconfinement to quark matter takes place. For this purpose, we make use of the Chiral Mean Field (CMF) model, an effective relativistic model that includes self-consistent chiral ...
E. Most +8 more
semanticscholar +1 more source
The entrainment matrix of a superfluid neutron-proton mixture at a finite temperature [PDF]
, 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]
Physical 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.
Fantoni, S., Sarsa, A., Schmidt, K. E.
openaire +2 more sources
The energy-resolved neutron imaging system, RADEN.
Review of Scientific Instruments, 2020 The energy-resolved neutron imaging system, RADEN, has been installed at the pulsed neutron source in the Materials and Life Science Experimental Facility of the Japan Proton Accelerator Research Complex.
T. Shinohara +15 more
semanticscholar +1 more source
Neutron stars in a chiral model with finite temperature [PDF]
Journal 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 ...
Dexheimer, V., Schramm, S., Stoecker, H.
openaire +2 more sources
Magnetic, thermal and rotational evolution of isolated neutron stars [PDF]
Living Reviews in Computational Astrophysics, 2019 The strong magnetic field of neutron stars is intimately coupled to the observed temperature and spectral properties, as well as to the observed timing properties (distribution of spin periods and period derivatives).
J. Pons, D. Viganò
semanticscholar +1 more source
Design of a high-temperature neutron irradiation container [PDF]
Nuclear Instruments and Methods, 1973 Abstract The design and construction of a neutron irradiation container in which all samples receive the same total neutron dose and the temperature is controlled to ±0.5° C in the 25°C to 200°C range is reported.
Fee, Darrell C., Markowitz, Samuel S.
openaire +2 more sources
Applied Sciences, 2021 Polychromatic and wavelength-selective neutron transmission radiography were applied during bead-on-plate welding on 5 mm thick sheets on the face side of martensitic low transformation temperature (LTT) steel plates using gas tungsten arc welding (GTAW).
Axel Griesche +3 more
doaj +1 more source
Constraints on axion-like particles and nucleon pairing in dense matter from the hot neutron star in HESS J1731-347 [PDF]
Physical Review C, 2018 If the thermal evolution of the hot young neutron star in the supernova remnant HESS J1731-347 is driven by neutrino emission, it provides a stringent constraint on the coupling of light (mass $\ll 10$ keV) axion-like particles to neutrons.
M. Beznogov +3 more
semanticscholar +1 more source