Revisiting the Contributions of Supernova and Hypernova Remnants to the Diffuse High-Energy Backgrounds: Constraints on Very-High-Redshift Injections

Abstract

Star-forming and starburst galaxies are considered as one of the viable candidate sources of the high-energy cosmic neutrino background detected in IceCube. We revisit contributions of supernova remnants (SNRs) and hypernova remnants (HNRs) in such galaxies to the diffuse high-energy neutrino and gamma-ray backgrounds, in light of the latest Fermi data above 50GeV. We also take into account possible time dependent effects of the cosmic-ray (CR) acceleration during the SNR evolution. CRs accelerated by the SNR shocks can produce high-energy neutrinos up to $\sim 100$ TeV energies, but CRs from HNRs can extend the spectrum up to PeV energies. We show that, only if HNRs are dominant over SNRs, the diffuse neutrino background above 100 TeV can be explained without contradicting the gamma-ray data. However, the neutrino data around 30 TeV remain unexplained, which might suggest a different population of gamma-ray dark CR sources. Alternatively, we consider possible contributions of Pop-III HNRs up to $z\lesssim 10$, and show that they are not constrained by the gamma-ray data, and thus could contribute to the diffuse high-energy backgrounds if their explosion energy reaches ${\mathcal{E}}_{\mathrm{POP}-\mathrm{III}}\sim \mathrm{a}\mathrm{few}\times 10^{53}$erg. More conservatively, our results suggest that the explosion energy of POP-III HNRs is ${\mathcal{E}}_{\mathrm{POP}-\mathrm{III}}\lesssim 7\times {10}^{53}$erg.

9 pages, 8 figures, ApJ in press

References in corpus (27)

• The spectrum of isotropic diffuse gamma-ray emission between 100 MeV and 820 GeV
• On the Rates of Gamma Ray Bursts and Type Ib/c Supernovae
• Magnetic Fields in Starburst Galaxies and The Origin of the FIR-Radio Correlation
• Star-forming galaxies as the origin of diffuse high-energy backgrounds: Gamma-ray and neutrino connections, and implications for starburst history
• Photohadronic origin of $\gamma$-ray BL Lac emission: implications for IceCube neutrinos
• Simulations and Theory of Ion Injection at Non-relativistic Collisionless Shocks
• High-energy Cosmic Rays and Neutrinos from Semi-relativistic Hypernovae
• A Galactic Halo Origin of the Neutrinos Detected by IceCube
• Extragalactic Zeeman Detections in OH Megamasers
• Neutrino Spectra from Low and High Luminosity Populations of Gamma Ray Bursts
• Gamma-Ray and Neutrino Backgrounds as Probes of the High-Energy Universe: Hints of Cascades, General Constraints, and Implications for TeV Searches
• What IceCube data tell us about neutrino emission from star-forming galaxies (so far)
• Does the Milky Way Produce a Nuclear Galactic Wind?
• Extragalactic star-forming galaxies with hypernovae and supernovae as high-energy neutrino and gamma-ray sources: the case of the 10 TeV neutrino data
• The diffuse gamma-ray flux associated with sub-PeV/PeV neutrinos from starburst galaxies
• Prompt TeV neutrinos from dissipative photospheres of gamma-ray bursts
• [Fe II] and H2 filaments in the Supernova Remnant G11.2-0.3: Supernova Ejecta and Presupernova Circumstellar Wind
• Shock Speed, Cosmic Ray Pressure, and Gas Temperature in the Cygnus Loop
• Star-forming galaxies as the origin of the IceCube PeV neutrinos
• Gamma-ray bursts and Population III stars
• Ultra-high Energy Cosmic Rays and Neutrinos from Gamma-Ray Bursts, Hypernovae and Galactic Shocks
• Neutrino Emission in Jet Propagation Process
• High Energy Neutrino Emission from the Earliest Gamma-Ray Bursts
• TeV-PeV Neutrino Oscillation of Low-luminosity Gamma-ray Bursts
• Parametric studies of cosmic ray acceleration in supernova remnants
• Origin of Galactic Cosmic Rays from Supernova Remnants
• Supernovae at the cosmic dawn

Cited by in corpus (29)

• High-Energy Neutrinos from Magnetized Coronae of Active Galactic Nuclei and Prospects for Identification of Seyfert Galaxies and Quasars in Neutrino Telescopes
• High-Energy Neutrino Flares From X-Ray Bright and Dark Tidal Disruptions Events
• Astrophysical Sources of High Energy Neutrinos in the IceCube Era
• Contribution of starburst nuclei to the diffuse gamma-ray and neutrino flux
• New constraints on the origin of medium-energy neutrinos observed by IceCube
• The TeV Diffuse Cosmic Neutrino Spectrum and the Nature of Astrophysical Neutrino Sources
• Starburst galaxies strike back: a multi-messenger analysis with Fermi-LAT and IceCube data
• Can winds driven by active galactic nuclei account for the extragalactic gamma-ray and neutrino backgrounds?
• Multi-messenger tests of cosmic-ray acceleration in radiatively inefficient accretion flows
• Constraints on the models of the origin of high-energy astrophysical neutrinos
• High-energy gamma-ray and neutrino production in star-forming galaxies across cosmic time: Difficulties in explaining the IceCube data
• Multi-PeV Signals from a New Astrophysical Neutrino Flux Beyond the Glashow Resonance
• High-Energy Neutrino Emission from White Dwarf Mergers
• Are starburst galaxies a common source of high energy neutrinos and cosmic rays?
• Cumulative Neutrino and Gamma-Ray Backgrounds from Halo and Galaxy Mergers
• IceCube Neutrinos from Hadronically Powered Gamma-Ray Galaxies
• High-energy neutrino emission subsequent to gravitational wave radiation from supermassive black hole mergers
• Origin and Impacts of the First Cosmic Rays
• Near-future discovery of point sources of ultra-high-energy neutrinos
• High-Energy Gamma Rays and Neutrinos from Nearby Radio Galaxies
• Neutrino production in Population III microquasars
• Cosmic rays, neutrinos and GeV-TeV gamma rays from Starburst Galaxy NGC 4945
• Cosmic rays escaping from Galactic starburst-driven superbubbles
• Secondary Radio and X-ray Emissions from Galaxy Mergers
• Gamma-Rays from Star Forming Activity Appear to Outshine Misaligned Active Galactic Nuclei
• On the non-detection of Glashow resonance in IceCube
• Investigating starburst-driven neutrino emission from galaxies in the Great Observatories All-Sky LIRG Survey
• First Search for High-Energy Neutrino Emission from Galaxy Mergers
• Little Red Dots as Hidden Neutrino Sources