From the 1 of 5 linked papers with an AI index.
5 papers
Core-Collapse Supernovae and their Gravitational Wave Signals: The Status of Theory and Modeling
Bernhard Müller
The paper reviews the current theoretical understanding of core‑collapse supernovae and describes how their gravitational‑wave signals can reveal details about the explosion mechan…
Angular momentum transport in the convection zone of a 3D MHD simulation of a rapidly rotating core-collapse progenitor
Ryota Shimada, Lucy O. McNeill, Vishnu Varma +3
Rotation and magnetic fields in the cores of evolved massive stars in their final phase are thought to play an important role in the subsequent supernova explosion and the formatio…
The Impact of Initial Mass Dependent Convective Boundary Mixing on the Structure and Fates of Massive Stars
Emily E. Whitehead, Raphael Hirschi, Vishnu Varma +4
While convection has been known to play a key role in stars for many decades, its implementation in one-dimensional stellar evolution codes still represents a major uncertainty tod…
Gravitational waves from core-collapse supernovae with no electromagnetic counterparts
Jade Powell, Bernhard Müller
Core-collapse supernovae (CCSNe) are regularly observed electromagnetically, prompting targetted searches for their gravitational-wave emission. However, there are scenarios where…
Effects of multidimensional treatment of gravity in simulations on supernova gravitational waves
Hajime Sotani, Bernhard Müller, Tomoya Takiwaki
Supernova explosions are expected as one of the promising candidates for gravitational wave sources. In this study, we examine the supernova gravitational waves, focusing on the mu…