Long-term evolution of non-thermal emission from Type Ia and core-collapse supernova remnants in a diversified circumstellar medium

Abstract

The contribution of galactic supernova remnants (SNRs) to the origin of cosmic rays (CRs) is an important open question in modern astrophysics. Broadband non-thermal emission is a useful proxy for probing the energy budget and production history of CRs in SNRs. We conduct hydrodynamic simulations to model the long-term SNR evolution from explosion all the way to the radiative phase (or $3\times 10^5$ yrs at maximum), and compute the time evolution of the broadband non-thermal spectrum to explore its potential applications on constraining the surrounding environments as well as the natures and mass-loss histories of the SNR progenitors. A parametric survey is performed on the ambient environments separated into two main groups, namely a homogeneous medium with a uniform gas density and one with the presence of a circumstellar structure created by the stellar wind of a massive red-supergiant (RSG) progenitor star. Our results reveal a highly diverse evolution history of the non-thermal emission closely correlated to the environmental characteristics of a SNR. Up to the radiative phase, the roles of CR re-acceleration and ion-neutral wave damping on the spectral evolution are investigated. Finally, we make an assessment of the future prospect of SNR observations by the next-generation hard X-ray space observatory FORCE and predict what we can learn from their comparison with our evolution models.

arXiv comment27 pages, 15 figures, 2 tables, accepted for publication in ApJ

References in corpus (111)

• Detection of the Characteristic Pion-Decay Signature in Supernova Remnants
• Nucleosynthesis and Evolution of Massive Metal-Free Stars
• The Expulsion of Stellar Envelopes in Core-Collapse Supernovae
• The H.E.S.S. Galactic plane survey
• Broad-band nonthermal emission from molecular clouds illuminated by cosmic rays from nearby supernova remnants
• The 1st Fermi Lat Supernova Remnant Catalog
• A Census of High-Energy Observations of Galactic Supernova Remnants
• A revised catalogue of 294 Galactic supernova remnants
• Chandra Detection of the Forward and Reverse Shocks in Cassiopeia-A
• Search for Spatial Extension in High-Latitude Sources Detected by the Fermi Large Area Telescope
• Gamma-ray Emission from Crushed Clouds in Supernova Remnants
• Rayleigh-Taylor Instabilities in Young Supernova Remnants Undergoing Efficient Particle Acceleration
• Escape-limited Model of Cosmic-ray Acceleration Revisited
• Dynamical Feedback of Self-generated Magnetic Fields in Cosmic Ray Modified Shocks
• An Exact Integration Scheme for Radiative Cooling in Hydrodynamical Simulations
• H.E.S.S. observations of RX J1713.7-3946 with improved angular and spectral resolution; evidence for gamma-ray emission extending beyond the X-ray emitting shell
• Proper Motions and Brightness Variations of Nonthermal X-ray Filaments in the Cassiopeia A Supernova Remnant
• Search for extended sources in the Galactic Plane using 6 years of Fermi-Large Area Telescope Pass 8 data above 10 GeV
• Expansion Velocity of Ejecta in Tycho's Supernova Remnant Measured by Doppler Broadened X-ray Line Emission
• X-Ray Measured Dynamics of Tycho's Supernova Remnant
• Mechanism for spectral break in cosmic ray proton spectrum from Supernova remnant W44
• Investigation of the large-scale neutral hydrogen near the supernova remnant W28
• On the Expansion Rate, Age, and Distance of the Supernova Remnant G266.2-1.2 (Vela Jr.)
• Enhanced abundances in three large-diameter mixed-morphology supernova remnants
• A Near-Infrared and X-ray Study of W49B: A Wind Cavity Explosion
• Universal behaviour of shock precursors in the presence of efficient cosmic-ray acceleration
• Non-linear diffusive shock acceleration with free escape boundary
• Magnetic field amplification in nonlinear diffusive shock acceleration including resonant and non-resonant cosmic-ray driven instabilities
• Expansion of the Youngest Galactic Supernova Remnant G1.9+0.3
• Gamma-ray observations of Tycho's SNR with VERITAS and Fermi
• The Kinematics of Kepler's Supernova Remnant as revealed by Chandra
• Supernova Remnants Interacting with Molecular Clouds: X-ray and Gamma-ray Signatures
• Population study of Galactic supernova remnants at very high $\gamma$-ray energies with H.E.S.S.
• VLA and XMM-Newton observations of the SNR W41/TeV Gamma-ray source HESS J1834-087
• Radio Spectrum and Distance of the SNR HB9
• Evolution of high-energy particle distribution in Supernova Remnants
• Revisiting the distance, environment and supernova properties of SNR G57.2+0.8 that hosts SGR 1935+2154
• On magnetic field amplification and particle acceleration near non-relativistic astrophysical shocks: Particles in MHD Cells simulations
• A Generalized Model of Nonlinear Diffusive Shock Acceleration Coupled to an Evolving Supernova Remnant
• Detailed Investigation of the Gamma-Ray Emission in the Vicinity of SNR W28 with FERMI-LAT
• Proper Motions of H-alpha filaments in the Supernova Remnant RCW 86
• Deeper H.E.S.S. observations of Vela Junior (RX J0852.0$-$4622): Morphology studies and resolved spectroscopy
• Comparison of Different Methods for Nonlinear Diffusive Shock Acceleration
• Distance of three Supernova Remnants from HI line observations in a complex region: G114.3+0.3, G116.5+1.1, and CTB 1 (G116.9+0.2)
• Supernova remnants in clumpy media: particle propagation and gamma-ray emission
• The supernova remnant W44: a case of cosmic-Ray reacceleration
• Modeling Bright Gamma-ray and Radio Emission at Fast Cloud Shocks
• Are Models for Core-Collapse Supernova Progenitors Consistent with the Properties of Supernova Remnants?
• Radio and X-ray Profiles in Supernova Remnants Undergoing Efficient Cosmic Ray Production
• Long-term TeV and X-ray Observations of the Gamma-ray Binary HESS J0632+057
• Hi Shells and Supershells in the I-GALFA Hi 21-cm Line Survey: I. Fast-Expanding Hi Shells Associated with Supernova Remnants
• A Spatially Resolved Study of the Synchrotron Emission and Titanium in Tycho's Supernova Remnant with NuSTAR
• Cosmic-ray acceleration and escape from post-adiabatic Supernova remnants
• The supernova remnant W49B as seen with H.E.S.S. and Fermi-LAT
• The Cygnus Loop's Distance, Properties, and Environment Driven Morphology
• Supernova remnant W49B and its environment
• A high resolution HI study towards the supernova remnant Puppis A and its environments
• A CR-hydro-NEI Model of Multi-wavelength Emission from the Vela Jr. Supernova Remnant (SNR RX J0852.0-4622)
• The Thermal Composite Supernova Remnant Kes 27 as Viewed by CHANDRA: Shock Reflection from a Cavity Wall
• Discovery of Molecular Shells Associated with Supernova Remnants. I. Kesteven 69
• The radio SNR G65.1+0.6 and its associated pulsar J1957+2831
• Detection of two TeV shell-type remnants at GeV energies with Fermi-LAT: HESS J1731-347 and SN 1006
• Expansion measurement of Supernova Remnant RX J1713.7-3946
• Abundances in the Ejecta of Core Collapse Supernova Remnants, G350.1-0.3 and G349.7+0.2
• H.E.S.S. detection of TeV emission from the interaction region between the supernova remnant G349.7+0.2 and a molecular cloud
• Discovery of molecular and atomic clouds associated with the gamma-ray supernova remnant Kesteven 79
• Collisionless shocks in partly ionized plasma with cosmic rays: microphysics of non-thermal components
• Direct Numerical Simulations of Cosmic-ray Acceleration at Dense Circumstellar Medium: Magnetic Field Amplification by Bell Instability and Maximum Energy
• Chandra X-Ray Study of Galactic Supernova Remnant G299.2-2.9
• Supernova Remnant Kes 17: Efficient Cosmic Ray Accelerator inside a Molecular Cloud
• GeV detection of HESS J0632+057
• Suzaku Observations of Thermal and Non-Thermal X-Ray Emission from the Middle-Aged Supernova Remnant G156.2+5.7
• Two New Ejecta-Dominated Galactic Supernova Remnants: G337.2-0.7 and G309.2-0.6
• Expansion and Age of the X-ray Synchrotron-Dominated Supernova Remnant G330.2+1.0
• Revealing the obscured supernova remnant Kes 32 with Chandra
• TeV γ-ray observations of the young synchrotron-dominated SNRs G1.9+0.3 and G330.2+1.0 with H.E.S.S
• Spectral softening in core-collapse supernova remnant expanding inside wind-blown bubble
• NuSTAR Detection of Nonthermal Bremsstrahlung from the Supernova Remnant W49B
• NuSTAR observations of the supernova remnant RX J1713.7$-$3946
• Radio Emission from Supernovae in the Very Early Phase: Implications for the Dynamical Mass Loss of Massive Stars
• Chandrasekhar and sub-Chandrasekhar models for the X-ray emission of Type Ia supernova remnants (I): Bulk properties
• Time evolution of broadband non-thermal emission from supernova remnants in different circumstellar environments
• Cosmic Ray Acceleration during Large Scale Structure Formation
• NuSTAR Detection of a Hard X-ray Source in the Supernova Remnant - Molecular Cloud Interaction Site of IC 443
• Magneto-hydrodynamic simulations of young supernova remnants and their energy-conversion phase
• Exploring the X-ray emission properties of the supernova remnant G67.7+1.8 and its central X-ray sources
• An extreme particle accelerator in the Galactic plane: HESS J1826$-$130
• Infrared and X-ray study of the Galactic SNR G15.9+0.2
• SNR G39.2-0.3, an Hadronic Cosmic Rays Accelerator
• G7.7-3.7: a young supernova remnant probably associated with the guest star in 386 CE (SN 386)
• A Grid of Core-Collapse Supernova Remnant Models I: The Effect of Wind-Driven Mass-Loss
• The high-energy gamma-ray detection of G73.9+0.9, a supernova remnant interacting with a molecular cloud
• XMM-Newton, Chandra, and CGPS observations of the Supernova Remnants G85.4+0.7 and G85.9-0.6
• Ionization age of iron ejecta in the Galactic Type Ia supernova remnant G306.3-0.9
• A multiwavelength study of the supernova remnant G296.8-0.3
• Suzaku study on the Ejecta of the Supernova Remnant G272.2$-$3.2
• Recombining Plasma & Gamma-ray Emission in the Mixed-morphology Supernova Remnant 3C 400.2
• An XMM-Newton Study of the Mixed-Morphology Supernova Remnant G346.6-0.2
• Exploring the supernova remnant G308.4-1.4
• The Important Role of Cosmic-Ray Re-Acceleration
• Evidence for gamma-ray emission from the remnant of Kepler's supernova based on deep H.E.S.S. observations
• Discovery of thermal X-ray emission in the Supernova Remnant G337.8-0.1 (Kes 41)
• Suzaku Analysis of the Supernova Remnant G306.3-0.9 and the Gamma-ray View of Its Neighborhood
• X-Ray Observation of the Galactic Supernova Remnant G355.6-0.0 with Suzaku
• Search for galactic Pevatron candidates in a population of unidentified gamma-ray sources
• Ejecta detection in the middle-aged Galactic supernova remnant G296.1-0.5 observed with Suzaku
• Dark Age of Type II Supernova Remnants
• X-ray and radio studies of SNR CTB 37B hosting the magnetar CXOU J171405.7-381031
• A deep X-ray observation of supernova remnant G304.6+0.1 (Kes 17) with Suzaku
• Spatially decomposed $\gamma$-ray features surrounding SNR Kes 79 & PSR J1853+0056
• Resurrection of Non-thermal Emissions from Type Ib/c Supernova Remnants

Cited by in corpus (3)

• Particle acceleration, escape and non-thermal emission from core-collapse supernovae inside non-identical wind-blown bubbles
• Multiwavelength studies of G298.6$-$0.0: An old GeV supernova remnant interacting with molecular clouds
• How to turn a Supernova into a PeVatron