Multi-dimensional fluid flow plays a paramount role in the explosions of massive stars as
core-collapse supernovae. In recent years, three-dimensional (3D) simulations of these …

Gravitational-wave emission from stellar collapse has been studied for nearly four decades.
Current state-of-the-art numerical investigations of collapse include those that use …

We present three-dimensional hydrodynamic simulations of the evolution of core-collapse
supernovae (SN) from blast-wave initiation by the neutrino-driven mechanism to shock …

Asymmetry is required by most numerical simulations of stellar core-collapse explosions, but
the form it takes differs significantly among models. The spatial distribution of radioactive …

No supernova (SN) in the Milky Way has been observed since the invention of the optical
telescope, instruments for other wavelengths, neutrino detectors, or gravitational wave …

Abstract We discuss Monte Carlo techniques for addressing the three-dimensional time-
dependent radiative transfer problem in rapidly expanding supernova atmospheres. The …

Abstract e-ASTROGAM ('enhanced ASTROGAM') is a breakthrough Observatory space
mission, with a detector composed by a Silicon tracker, a calorimeter, and an …

I review studies of core collapse supernovae (CCSNe) and similar transient events that
attribute major roles to jets in powering most CCSNe and in shaping their ejecta. I start with …

In core-collapse supernovae, titanium-44 (44Ti) is produced in the innermost ejecta, in the
layer of material directly on top of the newly formed compact object. As such, it provides a …

Core-collapse explosions of massive stars leave behind neutron stars, with a known
diversity that includes the 'Central Compact Objects'(CCOs). Typified by the neutron star …