Interacting supernovae as high-energy multimessenger transients
arXiv:2312.17239 · doi:10.1103/PhysRevD.109.103020
Abstract
Multiwavelength observations have revealed that dense, confined circumstellar material (CCSM) commonly exists in the vicinity of supernova (SN) progenitors, suggesting enhanced mass losses years to centuries before their core collapse. Interacting SNe, which are powered or aided by interaction with the CCSM, are considered to be promising high-energy multimessenger transient sources. We present detailed results of broadband electromagnetic emission, following the time-dependent model proposed in the previous work on high-energy SN neutrinos [K. Murase, New prospects for detecting high-energy neutrinos from nearby supernovae, Phys. Rev. D 97, 081301(R) (2018)]. We investigate electromagnetic cascades in the presence of Coulomb losses, including inverse-Compton and synchrotron components that significantly contribute to MeV and high-frequency radio bands, respectively. We also discuss the application to SN 2023ixf.
20 pages, 10 figures, 1 table, version published in PRD, multimessenger spectral templates available on Github at https://github.com/pegasuskmurase/ModelTemplates/tree/main/SNHEMM
References in corpus (26)
- Pulsational pair instability as an explanation for the most luminous supernovae
- Confined Dense Circumstellar Material Surrounding a Regular Type II Supernova: The Unique Flash-Spectroscopy Event of SN 2013fs
- Parametrization of gamma-ray production cross-sections for pp interactions in a broad proton energy range from the kinematic threshold to PeV energies
- Parameterization of Gamma, e^+/- and Neutrino Spectra Produced by p-p Interaction in Astronomical Environment
- Shell-shocked diffusion model for the light curve of SN2006gy
- Unifying Type II Supernova Light Curves with Dense Circumstellar Material
- The Pacific Ocean Neutrino Experiment
- Swift and Chandra Detections of Supernova 2006jc: Evidence for Interaction of the Supernova Shock with a Circumstellar Shell
- The All-sky Medium Energy Gamma-ray Observatory eXplorer (AMEGO-X) Mission Concept
- From Discovery to the First Month of the Type II Supernova 2023ixf: High and Variable Mass Loss in the Final Year before Explosion
- Time-resolved hadronic particle acceleration in the recurrent Nova RS Ophiuchi
- Early Spectroscopy and Dense Circumstellar Medium Interaction in SN 2023ixf
- Bolometric Light Curves for 33 Type II-Plateau Supernovae
- A Nova Outburst Powered by Shocks
- Gamma-Ray and Hard X-Ray Emission from Pulsar-Aided Supernovae as a Probe of Particle Acceleration in Embryonic Pulsar Wind Nebulae
- Far-Ultraviolet to Near-Infrared Observations of SN 2023ixf: A high energy explosion engulfed in complex circumstellar material
- Early hard X-rays from the nearby core-collapse supernova SN2023ixf
- Modelling the Type Ic SN 2004aw: a Moderately Energetic Explosion of a Massive C+O Star without a GRB
- Search for Early Gamma-ray Production in Supernovae Located in a Dense Circumstellar Medium with the Fermi LAT
- Time-dependent high-energy gamma-ray signal from accelerated particles in core-collapse supernovae: the case of SN 1993J
- An Analytical Density Profile of Dense Circumstellar Medium in Type II Supernovae
- Modelling type IIP/IIL supernovae interacting with recent episodic mass ejections from their presupernova stars with MESA & SNEC
- Core-collapse supernovae in dense environments -- particle acceleration and non-thermal emission
- Optically Informed Searches of High-Energy Neutrinos from Interaction-Powered Supernovae
- The first days of type II-P core collapse supernovae in the gamma-ray range
- Detecting High-Energy Neutrinos from Galactic Supernovae with ATLAS
Cited by in corpus (7)
- Search for gravitational waves emitted from SN 2023ixf
- On the diversity of strongly-interacting Type IIn supernovae
- Probing superheavy dark matter through lunar radio observations of ultrahigh-energy neutrinos and the impacts of neutrino cascades
- Multi-messenger connection in high-energy neutrino astronomy
- Towards Multi Energy Neutrino Astronomy: Diagnosing Enhanced Circumstellar Material around Stripped-Envelope Supernovae
- Hadronic Processes, Plasma Evolution and Neutrino Emission in Magnetic Towers of Neutron-Star Merger Remnants
- Constraining the TeV gamma-ray emission of SN 2024bch, a possible type IIn-L from a red supergiant progenitor. Multiwavelength observations and analysis of the progenitor