Spectrum of the Supernova Relic Neutrino Background and Metallicity Evolution of Galaxies

Abstract

The spectrum of the supernova relic neutrino (SRN) background from past stellar collapses including black hole formation (failed supernovae) is calculated. The redshift dependence of the black hole formation rate is considered on the basis of the metallicity evolution of galaxies. Assuming the mass and metallicity ranges of failed supernova progenitors, their contribution to SRNs is quantitatively estimated for the first time. Using this model, the dependences of SRNs on the cosmic star formation rate density, shock revival time and equation of state are investigated. The shock revival time is introduced as a parameter that should depend on the still unknown explosion mechanism of core collapse supernovae. The dependence on equation of state is considered for failed supernovae, whose collapse dynamics and neutrino emission are certainly affected. It is found that the low-energy spectrum of SRNs is mainly determined by the cosmic star formation rate density. These low-energy events will be observed in the Super-Kamiokande experiment with gadolinium-loaded water.

arXiv comment14 pages, 14 figures, accepted for publication in ApJ. The supernova relic neutrino data computed in this study are available at http://asphwww.ph.noda.tus.ac.jp/srn/

References in corpus (59)

• Stellar population synthesis at the resolution of 2003
• The Origin of the Mass--Metallicity Relation: Insights from 53,000 Star-Forming Galaxies in the SDSS
• The physical properties of star forming galaxies in the low redshift universe
• On the normalisation of the cosmic star formation history
• UV Star Formation Rates in the Local Universe
• Explosion Mechanisms of Core-Collapse Supernovae
• A fundamental relation between mass, SFR and metallicity in local and high redshift galaxies
• The 'Forbidden' Abundance of Oxygen in the Sun
• AMAZE. I. The evolution of the mass-metallicity relation at z>3
• Black Hole Formation in Failing Core-Collapse Supernovae
• Identifying the neutrino mass spectrum from a supernova neutrino burst
• GADZOOKS! Antineutrino Spectroscopy with Large Water Cerenkov Detectors
• Perspectives on Core-Collapse Supernova Theory
• Precise quasielastic neutrino/nucleon cross section
• Revealing the High-Redshift Star Formation Rate with Gamma-Ray Bursts
• The Supernova Channel of Super-AGB Stars
• A Finite Difference Representation of Neutrino Radiation Hydrodynamics in Spherically Symmetric General Relativistic Space-Time
• Missing Black Holes Unveil The Supernova Explosion Mechanism
• Postbounce evolution of core-collapse supernovae: Long-term effects of equation of state
• Super and massive AGB stars - IV. Final fates - Initial to final mass relation
• The Diffuse Supernova Neutrino Background
• The stellar mass function of galaxies to z ~ 5 in the Fors Deep and GOODS-S fields
• Search for Supernova Relic Neutrinos at Super-Kamiokande
• The Cosmic Core-collapse Supernova Rate does not match the Massive-Star Formation Rate
• On the Collapsar Model of Long Gamma-Ray Bursts: Constraints from Cosmic Metallicity Evolution
• Supernova Relic Neutrino Search at Super-Kamiokande
• The neutrino signal from protoneutron star accretion and black hole formation
• The metallicity of the long GRB hosts and the Fundamental Metallicity Relation of low-mass galaxies
• The FMOS-Cosmos Survey of Star-Forming Galaxies at z~1.6 II. The Mass-Metallicity Relation and the Dependence on Star Formation Rate and Dust Extinction
• Supernova Neutrino Light Curves and Spectra for Various Progenitor Stars: From Core Collapse to Proto-neutron Star Cooling
• Relic neutrino background from cosmological supernovae
• Supernova Relic Neutrino Search with Neutron Tagging at Super-Kamiokande-IV
• No collective neutrino flavor conversions during the supernova accretion phase
• The contribution of star formation and merging to stellar mass buildup in galaxies
• A Spectroscopic Study of Type Ibc Supernova Host Galaxies from Untargeted Surveys
• Search for extraterrestrial antineutrino sources with the KamLAND detector
• Neutrino signals from the formation of black hole: a probe of equation of state of dense matter
• NIR Spectroscopy of Star-Forming Galaxies at z~1.4 with Subaru/FMOS: The Mass-Metallicity Relation
• The Role of Collective Neutrino Flavor Oscillations in Core-Collapse Supernova Shock Revival
• Diffuse neutrino flux from failed supernovae
• An Implicit Lagrangean Code for Spherically Symmetric General Relativistic Hydrodynamics with an Approximate Riemann Solver
• The red supergiant and supernova rate problems: implications for core-collapse supernova physics
• The mass-metallicity relation at z~1.4 revealed with Subaru/FMOS
• First Study of Neutron Tagging with a Water Cherenkov Detector
• Spectrum of the Supernova Relic Neutrino Background and Evolution of Galaxies
• A Search for Neutrinos from the Solar hep Reaction and the Diffuse Supernova Neutrino Background with the Sudbury Neutrino Observatory
• Diffuse supernova neutrinos: oscillation effects, stellar cooling and progenitor mass dependence
• Metallicity in the GRB 100316D/SN 2010bh Host Complex
• Supernova Relic Neutrinos and the Supernova Rate Problem: Analysis of Uncertainties and Detectability of ONeMg and Failed Supernovae
• Synoptic Sky Surveys and the Diffuse Supernova Neutrino Background: Removing Astrophysical Uncertainties and Revealing Invisible Supernovae
• A metallicity study of 1987A-like supernova host galaxies
• Shockwaves in Supernovae: New Implications on the Diffuse Supernova Neutrino Background
• Imprint of Explosion Mechanism on Supernova Relic Neutrinos
• Post-shock-revival evolutions in the neutrino-heating mechanism of core-collapse supernovae
• Gravitational Collapse and Neutrino Emission of Population III Massive Stars
• Exploring Hadron Physics in Black Hole Formations: a New Promising Target of Neutrino Astronomy
• Revisiting the Cosmic Star Formation History: Caution on the Uncertainties in Dust Correction and Star Formation Rate Conversion
• The Redshift Evolution of the Relation between Stellar Mass, Star Formation Rate, and Gas Metallicity of Galaxies
• Neutrino oscillation and expected event rate of supernova neutrinos in adiabatic explosion model

Cited by in corpus (36)

• Grand Unified Neutrino Spectrum at Earth: Sources and Spectral Components
• Diffuse Supernova Neutrino Background Search at Super-Kamiokande
• Measuring the supernova unknowns at the next-generation neutrino telescopes through the diffuse neutrino background
• Stellar Collapse Diversity and the Diffuse Supernova Neutrino Background
• Neutrino emission characteristics of black hole formation in three-dimensional simulations of stellar collapse
• Fundamental physics with the diffuse supernova background neutrinos
• Diffuse Supernova Neutrino Background from extensive core-collapse simulations of $8$-$100{\mathrm{M}}_{\odot }$ progenitors
• Search for astrophysical electron antineutrinos in Super-Kamiokande with 0.01wt% gadolinium-loaded water
• Diffuse neutrinos from luminous and dark supernovae: prospects for upcoming detectors at the O(10) kt scale
• Limits on astrophysical antineutrinos with the KamLAND experiment
• Impact of binary interactions on the diffuse supernova neutrino background
• Towards Probing the Diffuse Supernova Neutrino Background in All Flavors
• Influence of density dependence of symmetry energy in hot and dense matter for supernova simulations
• Detecting the Diffuse Supernova Neutrino Background in the future Water-based Liquid Scintillator Detector Theia
• Gravitational-Wave Background from Binary Mergers and Metallicity Evolution of Galaxies
• Non-Universal Stellar Initial Mass Functions: Large Uncertainties in Star Formation Rates at $z\approx 2-4$ and Other Astrophysical Probes
• Black Hole Accretion Disk Diffuse Neutrino Background
• Charged-current scattering off ${}^{16}$O nucleus as a detection channel for supernova neutrinos
• Numerical Study of Stellar Core Collapse and Neutrino Emission Using the Nuclear Equation of State Obtained by the Variational Method
• Prospects for the detection of the Diffuse Supernova Neutrino Background with the experiments SK-Gd and JUNO
• Diffuse neutrino background from past core-collapse supernovae
• Impact of late-time neutrino emission on the diffuse supernova neutrino background
• Non-thermal neutrinos created by shock acceleration in successful and failed core-collapse supernova
• Diffuse Neutrino Flux Based on the Rates of Core-collapse Supernovae and Black Hole Formation Deduced from a Novel Galactic Chemical Evolution Model
• Exploring the Fate of Stellar Core Collapse with Supernova Relic Neutrinos
• Diffuse supernova neutrino background with up-to-date star formation rate measurements and long-term multidimensional supernova simulations
• Neutrino non-radiative decay and the diffuse supernova neutrino background
• Dark Matter Pollution in the Diffuse Supernova Neutrino Background
• Neutrino emission from the collapse of $\sim 10^4$ $M_{\odot }$ population III supermassive stars
• Diffuse Neutrino Background from Magnetorotational Stellar Core Collapses
• Neutrino-induced reactions on 18O and implications of 18O mixture in water Cherenkov detectors on supernova neutrino events
• Impacts of Black-Hole-Forming Supernova Explosions on the Diffuse Neutrino Background
• Towards a reconstruction of Supernova Neutrino Spectra in JUNO
• A "nu" look at gravitational waves: The black hole birth rate from neutrinos combined with the merger rate from LIGO
• Neutrinos from Diffuse Supernova Background
• New Insights into Uncertainties in the Relic Neutrino Background and Effects from the Nuclear Equation of State