We report on a method, PUSH, for triggering core-collapse supernova (CCSN) explosions of massive stars in spherical symmetry. This method provides a framework to study many important aspects of core collapse supernovae: the effects of the shock passage through the star, explosive supernova nucleosynthesis and the progenitor-remnant connection. Here we give an overview of the method, compare the results to multi-dimensional simulations and investigate the effects of the progenitor and the equation of state on black hole formation.
from #AlexandrosSfakianakis via Alexandros G.Sfakianakis on Inoreader http://ift.tt/2lb4161
via IFTTT
Εγγραφή σε:
Σχόλια ανάρτησης (Atom)
Δημοφιλείς αναρτήσεις
-
ACS Nano DOI: 10.1021/acsnano.7b04100 from #AlexandrosSfakianakis via Alexandros G.Sfakianakis on Inoreader http://ift.tt/2h0ZFyU via...
-
Molecules, Vol. 24, Pages 2837: Bioavailability and Bioactivity of Encapsulated Phenolics and Carotenoids Isolated from Red Pepper Waste Mol...
-
Whether to wear a pollution filter Development of air quality forecasting system in Macedonia, based on WRF-Chem model Abstract Urban air qu...
-
Abstract Background Henoch–Schönlein purpura is the most common vasculitis in children. Its long-term prognosis depends on renal involve...
-
Denotation as Complex and Chronologically Extended: anvitābhidhāna in Śālikanātha's Vākyārthamātṛkā - I Abstract The two theories of ve...
-
UM-Chor1: establishment and characterization of the first validated clival chordoma cell line. J Neurosurg. 2017 Apr 21;:1-9 Authors:...
-
Abstract Cerebral and systemic organ microvascular pathologies coexist with human Alzheimer’s disease (AD) neuropathology. In this study, w...
-
Tetracycline Repressors (TetRs) modulate multi-drug efflux pathways in several pathogenic bacteria. In Streptomyces, they additionally regul...
-
A descriptive study of clinical and radiological profile of longitudinal extensive myelitis in a tertiary hospital in Rajasthan, India Publi...
Δεν υπάρχουν σχόλια:
Δημοσίευση σχολίου