Explosion mechanism, neutrino burst and gravitational wave in core-collapse supernovae

2005/09/16 by Kei Kotake, Katsuhiko Sato, Keitaro Takahashi · 313 citations
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #COSMIC cancer database #Cosmic ray #Gamma-ray burst #Gamma-ray bursts and supernovae #Gravitational wave #Neutrino #Neutrino Physics Research #Neutrino oscillation #Supernova #Type II supernova #astro-ph

paper · pdf · doi:10.1088/0034-4885/69/4/r03

published in Reports on Progress in Physics 69(4), 971-1143 (IOP Publishing) · 195 pages, 132 figures, submitted to Reports on Progress in Physics, A paper with higher-resolution figures available at http://www.heap.phys.waseda.ac.jp/kkotake/IOP_paper.html

arxiv created 2005/09/16 · openalex publication_date 2006/03/08 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Core-collapse supernovae are among the most energetic explosions in the universe marking the catastrophic end of massive stars. In spite of rigorous studies for several decades, we still do not understand the explosion mechanism completely. Since they are related to many astrophysical phenomena such as nucleosynthesis, gamma-ray bursts and acceleration of cosmic rays, understanding of their physics has been of wide interest to the astrophysical community. In this paper, we review recent progress in the study of core-collapse supernovae focusing on the explosion mechanism, supernova neutrinos and the gravitational waves. Regarding the explosion mechanism, we present a review paying particular attention to the roles of multidimensional aspects, such as convection, rotation and magnetic fields, on the neutrino heating mechanism. Next, we discuss supernova neutrino, which is a powerful tool to probe not only deep inside the supernovae but also the intrinsic properties of neutrinos. For this purpose, it is necessary to understand neutrino oscillation which has been established recently by many experiments. Gravitational astronomy is also now becoming a reality. We present an extensive review on the physical foundations and the emission mechanism of gravitational waves in detail and discuss the possibility of their detections.

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• Low-Frequency Gravitational Waves in Three-Dimensional Core-Collapse Supernova Models
• Dedicated-frequency analysis of gravitational-wave bursts from core-collapse supernovae with minimal assumptions
• Impacts of axion cooling on the direct detection of supernova axions
• Rotating Proto-Neutron Stars Admixed with Mirror Dark Matter: A two fluid approach
• Search for gravitational waves emitted from SN 2023ixf
• Neutrino spectrum from SN 1987A and from cosmic supernovae
• Relativistic stars with purely toroidal magnetic fields
• EFFECTS OF ROTATION ON STANDING ACCRETION SHOCK INSTABILITY IN NONLINEAR PHASE FOR CORE-COLLAPSE SUPERNOVAE
• Neutrino oscillations in magnetically driven supernova explosions
• Search method for coincident events from LIGO and IceCube detectors
• Quasinormal modes of black holes and black branes
• PLANE GRAVITATIONAL RADIATION FROM NEUTRINOS SOURCE WITH KALB-RAMOND COUPLING
• Improved analysis of SN1987A antineutrino events
• Diffuse supernova neutrino background is detectable in Super-Kamiokande
• Stability of Accretion Flows with Stalled Shocks in Core‐Collapse Supernovae
• Features of the Acoustic Mechanism of Core‐Collapse Supernova Explosions
• Effects of QCD phase transition on gravitational radiation from two-dimensional collapse and bounce of massive stars
• Detection of supernova neutrinos at spallation neutron sources
• A GENERAL RELATIVISTIC RAY-TRACING METHOD FOR ESTIMATING THE ENERGY AND MOMENTUM DEPOSITION BY NEUTRINO PAIR ANNIHILATION IN COLLAPSARS
• Post-Newtonian corrections to the gravitational-wave memory for quasicircular, inspiralling compact binaries
• Impact of binary interactions on the diffuse supernova neutrino background
• Pasta phases in neutron stars under strong magnetic fields
• Neutrino quantum kinetic equations: The collision term
• The transient gravitational-wave sky
• Three-dimensional simulation of a core-collapse supernova for a binary star progenitor of SN 1987A
• Estimating the core compactness of massive stars with Galactic supernova neutrinos
• Determination of the angular momentum distribution of supernovae from gravitational wave observations
• Gravitational waves from supernova matter
• MULTI-DIMENSIONAL FEATURES OF NEUTRINO TRANSFER IN CORE-COLLAPSE SUPERNOVAE
• Alfvén Wave–Driven Supernova Explosion
• Relativistic hybrid stars with super-strong toroidal magnetic fields: an evolutionary track with QCD phase transition
• Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects
• Gravitational-wave astronomy [wikipedia]
• Phil Plait [wikipedia]

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