If a star was able to increase its size by 16 times but keep its luminosity the same, what would happen to its surface temperature? Explain. What happens to the core of a high mass star after it runs out of hydrogen? Why don't the...
Correlation between the average prompt neutron multiplicity as a function of the primary mass and the corresponding experimental mass of fragments from 252Cf spontaneous fissiondoi:10.1016/j.rinp.2019.102685Modesto MontoyaCarlos RomeroElsevierResults in Physics...
We discuss the properties of magnetically dominated jetlike outflows from stellar mass black holes surrounded by debris tori resulting from neutron star di... P Mészáros,MJ Rees - 《Astrophysical Journal》 被引量: 380发表: 1997年 Optical control of the magnetic anisotropy of ferromagnetic bilayere...
rotational frame-dragging, the induced changes in the neutron and proton densities and the inertial mass, as well as the change in shape of the star. ... N Andersson,GL Comer - 《Classical & Quantum Gravity》 被引量: 53发表: 2001年 Solid Phase-Solution-Root Interactions in Soils Subjected...
We discuss the properties of magnetically dominated jetlike outflows from stellar mass black holes surrounded by debris tori resulting from neutron star di... P Mészáros,MJ Rees - 《Astrophysical Journal》 被引量: 380发表: 1997年 A Comparative Perspective on Poverty Reduction in Brazil, China,...
A Monte Carlo simulation is performed in order to correlate the average prompt neutron multiplicity as a function of post- and pre-neutron fragment mass (n-(m) and ν-(A), respectively). This is applied for 235,233U(nth,f). The input of the simulation consists of quantities related to...
The average total prompt neutron multiplicity [nu with overbar] of Cf spontaneous fission is investigated as a function of the total kinetic energy and the mass split of the fragments through the code FIFRELIN. This Monte Carlo device, already described in a previous work, aims at simulating ...
X-rays:binaries-binaries:close-stars:neutronWe studied and compared the long term average hard X-ray (>20 keV) spectra of a sample of twelve bright low-mass X-ray binaries hosting a neutron star (NS). Our sample comprises the six well studied Galactic Z sources and six Atoll sources, ...
Measurement of the average cross sections for (n, p) reactions on some light and medium mass nuclei in the 241 Am_Be neutron spectrumdoi:10.1016/0020-708X(79)90045-0R. Vänskä and R. RieppoThe International Journal of Applied Radiation and Isotopes...
Another situation of interest is when only the Hall effect plays a role, so there are then no fluid motions, but just the flow of electrons. This is relevant in neutron star crusts, which are solid, so the ions are immobile. Another application is to the solar wind on scales below the...