Results 101 to 110 of about 3,393,330 (216)
Fragmentation and clustering in star matter
The specificity of the crust-core phase transition in neutron star at zero and finite temperature will be discussed. It will be shown that, as a consequence of the presence of long range Coulomb interactions, the equivalence of statistical ensembles is ...
Gulminelli F.
doaj +1 more source
Three-dimensional Simulations from Supernovae to Their Supernova Remnants: The Dynamical and Chemical Evolution of Supernova 1987A [PDF]
Masaomi Ono +10 more
openaire +1 more source
Spherically symmetric simulations of stellar core collapse and post-bounce evolution are used to test the sensitivity of the supernova dynamics to dierent variations of the input physics. We consider a state-of-the-art description of the neutrino-nucleon
Mar Core-Collapse Supernova, R. Buras
core
Turbulence in Core-collapse Supernovae
It is understood in a general sense that turbulent fluid motion below the shock front in a core-collapse supernova stiffens the effective equation of state of the fluid and aids in the revival of the explosion.
David Calvert +6 more
doaj +1 more source
HD 271791: dynamical versus binary-supernova ejection scenario [PDF]
Abstract The atmosphere of the extremely high-velocity (530–920 km s−1) early B-type star HD 271791 is enriched in α-process elements, which suggests that this star is a former secondary component of a massive tight binary system and that its surface was polluted by the nucleosynthetic products after the primary star exploded in a ...
openaire +2 more sources
Effects of Rotation on 3D Core-collapse Supernova Models for Low-mass Progenitors
We explore the dependence upon rotation rate alone of various supernova observables simulated to their saturation for the explosion of a 9 M _⊙ progenitor.
Adam Burrows +2 more
doaj +1 more source
Late-time acceleration with steep exponential potentials
In this letter, we study the cosmological dynamics of steeper potential than exponential. Our analysis shows that a simple extension of an exponential potential allows to capture late-time cosmic acceleration and retain the tracker behavior.
M. Shahalam +3 more
doaj +1 more source
Optimization of nonlinear function with planar regions using supernova [PDF]
Nowadays, optimization is begun to be use in different fields, e.g. preference algorithms. These new challenges need a robustness meta heuristics to solve them.
Mesa Delgado, Eddy Janneth
core
The Milky Way is a dynamic and evolving system shaped by numerous merger events throughout its history. These mergers bring stars with kinematic and dynamic properties differing from the main stellar population.
Wenlang He +3 more
doaj +1 more source
Inhomogeneous Stellar Mixing in the Final Hours before the Cassiopeia A Supernova
Understanding stars and their evolution is a key goal of astronomical research and has long been a focus of human interest. In recent years, theorists have paid much attention to the final interior processes within massive stars, as they can be essential
Toshiki Sato +12 more
doaj +1 more source

