Bright Supernovae from Magnetar Birth

Abstract

Following an initial explosion that might be launched either by magnetic interactions or neutrinos, a rotating magnetar radiating according to the classic dipole formula could power a very luminous supernova. While some 56Ni might be produced in the initial explosion, the peak of the light curve in a Type I supernova would not be directly related to its mass. In fact, the peak luminosity would be most sensitive to the dipole field strength of the magnetar. The tail of the light curve could resemble radioactive decay for some time but, assuming complete trapping of the pulsar emission, would eventually be brighter. Depending on the initial explosion energy, both high and moderate velocities could accompany a very luminous light curve.

submitted to Astrophysical Journal Letters

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• Persistent X-ray emission from ASASSN-15lh: massive ejecta and pre-SLSN dense wind?
• SN 2018gk Revisited: the Photosphere, the Central Engine, And the Putative Dust
• A magnetar powers the luminous supernova 2023pel, associated with a long gamma-ray burst
• Prospects for Time-Domain and Multi-Messenger Science with eXTP
• A Population Study on the Radio Emission of Fast Blue Optical Transients
• The bright long-lived Type II SN 2021irp powered by aspherical circumstellar material interaction (I): Revealing the energy source with photometry and spectroscopy
• A puzzle solved after two decades: SN 2002gh among the brightest of superluminous supernovae
• Eruptive mass loss less than a year before the explosion of superluminous supernovae: I. The cases of SN 2020xga and SN 2022xgc
• Special supernova signature from BH-NS/BH progenitor systems
• Effects of nucleon-nucleon short-range correlation and symmetry energy on the evolution of newly born magnetars
• Exploring GRBs and supernovae connection: does a superluminous hypernova population exist?
• The supernova remnant CTB 37B and its associated magnetar CXOU J171405.7-381031: evidence for a magnetar-driven remnant
• Dynamics and observational signatures of core-collapse supernovae with central engines: hydrodynamics simulations with Monte Carlo post-processing
• Hard X-ray Observations of the Hydrogen-poor Superluminous Supernova SN 2018hti with NuSTAR
• Modeling the Light Curves of the Luminous Type Ic Supernova 2007D
• An axisymmetric shock breakout indicated by prompt polarized emission from the type II supernova 2024ggi
• Modeling the fast optical transient SN 2019bkc/ATLAS19dqr with a central engine and implication for its origin
• Quasithermal GeV neutrinos from neutron-loaded magnetized outflows in core-collapse supernovae: spectra and light curves
• On the initial spin periods of magnetars born in weak supernova explosions and their gravitational wave radiation
• A powerful e^{+-} outflow driven by a proto-strange quark star
• The restframe ultraviolet of superluminous supernovae -- I. Potential as cosmological probes
• Magnetic Fields in Stars: Origin and Impact
• On the Binary Nature of the Progenitor of SN2015ap: Insights from Its Light Curve and Spectral Evolution
• Constraints on Explosion Timescale of Core-Collapse Supernovae Based on Systematic Analysis of Light Curves
• Rotational Dynamics in Pulsational Pair-Instability Supernovae: Implications for Mass-Loss and Transient Events
• Observed Consequences of Presupernova Instability in Very Massive Stars
• JWST Detection of Hydrocarbon Ices and Methane Gas on Makemake
• Studying newborn neutron stars by the transient emission after stellar collapses and compact binary mergers
• Optical Observations and Modeling of the Superluminous Supernova 2018lfe
• Candidate strongly lensed type Ia supernovae in the Zwicky Transient Facility archive
• A search for hard X-ray bursts occurring simultaneously to fast radio bursts in the repeating FRB 121102
• Evidence for GeV emission of the superluminous supernova SN 2017egm
• Late-Time Hubble Space Telescope Observations of a Hydrogen-Poor Superluminous Supernova Reveal the Power-Law Decline of a Magnetar Central Engine
• Two years of optical and NIR observations of the superluminous supernova UID 30901 discovered by the UltraVISTA SN survey
• ASASSN-13dn: A Luminous and Double-Peaked Type II Supernova
• Unveiling the nature of the unidentified gamma-ray sources 4FGL J1908.6+0915e, HESS J1907+089/HOTS J1907+091, and 3HWC J1907+085 in the sky region of the magnetar SGR 1900+14
• VLBI Observations of SN 2012au Reveal a Compact Radio Source a Decade Post Explosion
• Spectroscopic Modeling of Luminous Transients Powered by H-Rich and He-Rich Circumstellar Interaction
• The nearby He-rich superluminous supernova SN 2021bnw during photospheric phases
• Large $\mathrm{Pm}$ small-scale kinematic dynamo in protoneutron stars
• A VLA Survey of Late-time Radio Emission from Superluminous Supernovae and the Host Galaxies
• Fluid Instabilities of Magnetar-Powered Supernovae
• SN 2017ati: A luminous type IIb explosion from a massive progenitor
• The Fast Radio Burst-emitting magnetar SGR 1935+2154 -- proper motion and variability from long-term Hubble Space Telescope monitoring
• Estimating Transient Rates from Cosmological Simulations and BPASS
• The maximum mass and rotational kinetic energy of rapidly rotating neutron stars
• Discovering Supernovae at Epoch of Reionization with Nancy Grace Roman Space Telescope