Results 71 to 80 of about 622,972 (290)

On the Progenitors of Core-Collapse Supernovae

open access: yes, 2010
Theory holds that a star born with an initial mass between about 8 and 140 times the mass of the Sun will end its life through the catastrophic gravitational collapse of its iron core to a neutron star or black hole. This core collapse process is thought
A. Gal-Yam   +42 more
core   +1 more source

On the Lightweight Potential of Laser Additive Manufactured NiTi Triply Periodic Minimal Sheet Lattices

open access: yesAdvanced Engineering Materials, EarlyView.
This study explores the lightweight potential of laser additive‐manufactured NiTi triply periodic minimal surface sheet lattices. It systematically investigates the effects of relative density and unit cell size on surface quality, deformation recovery, compression behavior, and energy absorption.
Haoming Mo   +3 more
wiley   +1 more source

SN 2024abfl: A Low-luminosity Type IIP Supernova at the Low-mass End of Core Collapse

open access: yesThe Astrophysical Journal
We present optical photometric and spectroscopic observations of the low-luminosity (LL) Type IIP supernova SN 2024abfl. The distance to its host galaxy is highly uncertain, with independent estimates of $9.{5}_{-2.4}^{+2.3}$ Mpc and $15.{0}_{-1.9}^{+8.9}
Luhan Li   +10 more
doaj   +1 more source

Preliminary Results from the Caltech Core-Collapse Project (CCCP) [PDF]

open access: yes, 2006
We present preliminary results from the Caltech Core-Collapse Project (CCCP), a large observational program focused on the study of core-collapse SNe.
Cenko, S. B.   +6 more
core   +2 more sources

Core-collapse supernovae

open access: yes
This is a pre-print of a chapter for the Encyclopedia of Astrophysics (edited by I. Mandel, section editor F.R.N.
Jerkstrand, Anders   +2 more
openaire   +2 more sources

Understanding Core-Collapse Supernovae

open access: yesNuclear Physics A, 2010
Our understanding of core-collapse supernovae continues to improve as better microphysics is included in increasingly realistic neutrino-radiationhydrodynamic simulations. Recent multi-dimensional models with spectral neutrino transport, which slowly develop successful explosions for a range of progenitors between 12 and 25 solar mass, have motivated ...
W.R. Hix   +8 more
openaire   +2 more sources

Multimessenger asteroseismology of core-collapse supernovae [PDF]

open access: yesPhysical Review D, 2019
25 pages, 16 figures. Version accepted to PRD.
John Ryan Westernacher-Schneider   +6 more
openaire   +4 more sources

Interaction of Ladle Slag With Varying SiO2 Content and Recyclate‐Based MgO–C Refractories

open access: yesAdvanced Engineering Materials, EarlyView.
Ladle slags (CaO/Al2O3 = 1) with 1–20 wt% SiO2 were investigated in contact with industrial MgO–C refractories fabricated from fresh magnesia and 50 wt% recyclate. The sessile drop method at 1600°C reveals intensive gas formation, delayed slag infiltration in recyclate‐based samples, and, under high‐SiO2 slag, formation of a dense MgAl2O4‐rich ...
Anton Yehorov   +6 more
wiley   +1 more source

Turbulence in Core-collapse Supernovae

open access: yesThe Astrophysical Journal
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

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