ASCERTAINING THE CORE COLLAPSE SUPERNOVA MECHANISM: The State of the Art and the Road Ahead

By A. Mezzacappa. 2005

159 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/db23a5277c963e8972bc53d8b46fc7105904f8cb

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Citations in the corpus

Progenitor mass constraints for core-collapse supernovae from correlations with host galaxy star formation⋆ (2012, background): “…aided by copious neutrino fluxes is thought to produce a shock wave that expels the star’s envelope generating the transients we observe (see Mezzacappa 2005 for a review of the latter stages of stellar evolution that lead to CC and SN).1 The immense temperatures, densities and energies…”
The Spherical Accretion Shock Instability in the Linear Regime (2005, unknown): “(For a review, see Mezzacappa (2005).)”
Three-dimensional simulations of neutrino-driven core-collapse supernovae from low-mass single and binary star progenitors (2018, background): “…is arguably the neutrinodriven mechanism, which relies on the partial reabsorption of neutrinos emitted from the young proto-neutron star (PNS) and the accretion layer at its surface to revive the shock and power the explosion (for reviews, see Mezzacappa 2005; Janka 2012; Burrows et al. 2012).”
The GMRT Epoch of Reionization experiment: a new upper limit on the neutral hydrogen power spectrum at z≈ 8.6 (2010, background): “However, the mechanism of and factors affecting core-collapse are not known and most numerical models appear to generically not result in SNe at all (Mezzacappa 2005).”
The Supernova Gamma-Ray Burst Connection (2006, background): “Models for ordinary core-collapse supernovae have been extensively reviewed by Woosley and Weaver (1986); Bethe (1990); Burrows (2000); Woosley et al. (2002); Buras et al. (2003, 2006); Woosley and Janka (2005); Janka et al. (2005); Mezzacappa (2005).”
Colloquium: Perspectives on core-collapse supernova theory (2012, background): “There are many papers on the computational issues specific to core collapse, but the papers by Arnett (1966,1967,1977), Imshennik & Nadëzhin (1973), Bowers & Wilson (1982), Bruenn (1985), Mayle & Wilson (1988), Liebendörfer et al. (2001), Liebendörfer, Rampp, Janka, & Mezzacappa (2005), Burrows e”
How much H and He is ‘hidden’ in SNe Ib/c? – I. Low-mass objects (2012, background): “Stripped core-collapse supernovae of types IIb, Ib and Ic (SNe IIb, Ib and Ic) are increasingly well observed, and long-standing issues about the explosion physics (Mezzacappa 2005; Janka etal.”