What differentiates the outcome of a Direct Collapse scenario from a standard Supernova event regarding the visible explosion?
Answer
The entire stellar envelope falls directly onto the core, resulting in no massive explosion.
While the supernova path involves the core collapsing and then violently rebounding the outer layers in a spectacular explosion, the Direct Collapse scenario bypasses this rebound entirely. This occurs either due to the star being exceptionally massive or specific configurations in the progenitor system. Instead of generating a visible shockwave, the outer layers simply continue falling inward onto the already collapsing core, crushing it immediately into a black hole without the characteristic bright flash associated with a typical supernova explosion. This leaves behind a different observational signature.
Related Questions
What is the fundamental energetic characteristic of fusing Iron within the core of a supermassive star?What speed do the infalling outer layers of a massive star reach during the core's rapid implosion phase?Where are elements heavier than iron synthesized during the explosion of a supermassive star?What specific pressure mechanism is responsible for halting the gravitational collapse to form a Neutron Star?What is the critical remnant core mass, related to the Tolman-Oppenheimer-Volkoff limit, that determines if a black hole forms instead of a Neutron Star?In terms of energy output, how does the energy released during a core-collapse supernova compare to the Sun's expected total lifetime production?What intense energetic phenomenon is often generated and observed as narrow beams accompanying a Hypernova explosion?What differentiates the outcome of a Direct Collapse scenario from a standard Supernova event regarding the visible explosion?For a star that is twenty times the mass of the Sun, how does the duration of its entire active life cycle compare to the lifespan of our Sun?What element sits at the center of the massive star's internal, onion-like fusion structure just before the core loses its thermal pressure support?