Relic neutrino background from cosmological supernovae
arXiv:astro-ph/0410061 · doi:10.1088/1367-2630/6/1/170
Abstract
Present and future observations of supernova relic neutrinos (SRNs), i.e., a cosmological neutrino background from past core-collapse supernova explosions, potentially give us useful information concerning various fields of astrophysics, cosmology and particle physics. We review recent progress of theoretical and observational studies of SRNs, particularly focusing on the detectability and also on implications for cosmic star formation history and neutrino physics.
29 pages, 8 figures, minor revision; review article accepted by New Journal of Physics, focus issue on neutrino physics
References in corpus (48)
- First Results from KamLAND: Evidence for Reactor Anti-Neutrino Disappearance
- High Redshift Galaxies in the Hubble Deep Field. Color Selection and Star Formation History to z=4
- New Insight on Galaxy Formation and Evolution from Keck Spectroscopy of the Hawaii Deep Fields
- The Star Formation History of Field Galaxies
- Unveiling Dust-enshrouded Star Formation in the Early Universe: a Sub-mm Survey of the Hubble Deep Field
- The CANADA-FRANCE REDSHIFT SURVEY XIII: The luminosity density and star-formation history of the Universe to z ~ 1
- Measurement of the Total Active 8B Solar Neutrino Flux at the Sudbury Neutrino Observatory with Enhanced Neutral Current Sensitivity
- Determination of Solar Neutrino Oscillation Parameters using 1496 Days of Super-Kamiokande-I Data
- The Nature of High-Redshift Galaxies
- Monte Carlo Study of Supernova Neutrino Spectra Formation
- Measurement of the flux and zenith-angle distribution of upward through-going muons by Super-Kamiokande
- Identifying the neutrino mass spectrum from a supernova neutrino burst
- GADZOOKS! Antineutrino Spectroscopy with Large Water Cerenkov Detectors
- The Evolution of the Global Star Formation History as Measured from the Hubble Deep Field
- On the Association of Gamma-ray Bursts with Massive Stars: Implications for Number Counts and Lensing Statistics
- Atmospheric neutrino flux above 1 GeV
- Calculation of the Flux of Atmospheric Neutrinos
- A three-dimensional calculation of atmospheric neutrinos
- Constraints on a Universal IMF from UV to Near-IR Galaxy Luminosity Densities
- Evolution of the Galaxy Population Based on Photometric Redshifts in the Hubble Deep Field
- Decay of High-Energy Astrophysical Neutrinos
- A New calculation of the atmospheric neutrino flux in a 3-dimensional scheme
- Search for Supernova Relic Neutrinos at Super-Kamiokande
- On the Evolution of the Cosmic Supernova Rates
- An Ultraviolet-Selected Galaxy Redshift Survey: New Estimates of the Local Star Formation Rate
- Do solar neutrinos decay?
- Measurement of Star-Formation Rate from H-alpha in field galaxies at z=1
- Reactor-based Neutrino Oscillation Experiments
- Neutrinoless Universe
- Bounds on the Coupling of the Majoron to Light Neutrinos from Supernova Cooling
- A High Sensitivity Search for 's from the Sun and Other Sources at KamLAND
- Supernova Bounds on Majoron-emitting decays of light neutrinos
- A brute force analysis of the COBE DMR data
- Detectability of the Supernova Relic Neutrinos and Neutrino Oscillation
- Three-generation flavor transitions and decays of supernova relic neutrinos
- Spectrum of the Supernova Relic Neutrino Background and Evolution of Galaxies
- The Supernova Relic Neutrino Background
- The Ultraviolet Luminosity Density of the Universe from Photometric Redshifts of Galaxies in the Hubble Deep Field
- M/String Theory, S-branes and Accelerating Universe
- Decaying neutrinos and implications from the supernova relic neutrino observation
- Spectrum of the relic neutrino background from past supernovae and cosmological models
- The Sloan Digital Sky Survey: The Cosmic Spectrum and Star-Formation History
- Supernova relic neutrinos and observational implications for neutrino oscillation
- Appearance of neutronization peak and decaying supernova neutrinos
- Geomagnetic Effects on Atmospheric Neutrinos
- Three-generation study of neutrino spin-flavor conversion in supernova and implication for neutrino magnetic moment
- The IMF Revisited: A Case for Variations
- Resonant spin-flavor conversion of supernova neutrinos: Dependence on presupernova models and future prospects
Cited by in corpus (104)
- On the normalisation of the cosmic star formation history
- Neutrino Physics with JUNO
- The Diffuse Supernova Neutrino Background
- The Diffuse Supernova Neutrino Background is detectable in Super-Kamiokande
- High Energy Neutrino Emission and Neutrino Background from Gamma-Ray Bursts in the Internal Shock Model
- Neutrino and Positron Constraints on Spinning Primordial Black Hole Dark Matter
- Muonic Boson Limits: Supernova Redux
- Detection of Neutrinos from Supernovae in Nearby Galaxies
- Grand Unified Neutrino Spectrum at Earth: Sources and Spectral Components
- Supernova Neutrino Light Curves and Spectra for Various Progenitor Stars: From Core Collapse to Proto-neutron Star Cooling
- Theia: An advanced optical neutrino detector
- Stochastic Gravitational Wave Background from Cosmological Supernovae
- Search for extraterrestrial antineutrino sources with the KamLAND detector
- Probing supernova shock waves and neutrino flavor transitions in next-generation water-Cherenkov detectors
- High Energy Neutrinos from the Tidal Disruption of Stars
- Gravitational Radiation from Standing Accretion Shock Instability in Core-Collapse Supernovae
- Diffuse neutrino flux from failed supernovae
- Diffuse supernova neutrinos at underground laboratories
- Measuring the supernova unknowns at the next-generation neutrino telescopes through the diffuse neutrino background
- The Concordance Cosmic Star Formation Rate: Implications from and for the Supernova Neutrino and Gamma Ray Backgrounds
- Impact of form factor uncertainties on interpretations of coherent elastic neutrino-nucleus scattering data
- Magnetorotational Collapse of Population III Stars
- Stellar Collapse Diversity and the Diffuse Supernova Neutrino Background
- Gravitational Waves from the First Stars
- Diffuse Supernova Neutrino Background from extensive core-collapse simulations of - progenitors
- Diffuse supernova neutrinos: oscillation effects, stellar cooling and progenitor mass dependence
- Hierarchical Growth and Cosmic Star Formation: Enrichment, Outflows and Supernova Rates
- Dips in the Diffuse Supernova Neutrino Background
- The diffuse supernova neutrino flux, supernova rate and SN1987A
- Developing the MeV potential of DUNE: Detailed considerations of muon-induced spallation and other backgrounds
- Spectrum of the Supernova Relic Neutrino Background and Metallicity Evolution of Galaxies
- Detection potential for the diffuse supernova neutrino background in the large liquid-scintillator detector LENA
- Synoptic Sky Surveys and the Diffuse Supernova Neutrino Background: Removing Astrophysical Uncertainties and Revealing Invisible Supernovae
- Diffuse neutrinos from luminous and dark supernovae: prospects for upcoming detectors at the O(10) kt scale
- Neutrino Spectrum from SN 1987A and from Cosmic Supernovae
- Detecting the QCD phase transition in the next Galactic supernova neutrino burst
- Probing secret interactions of eV-scale sterile neutrinos with the diffuse supernova neutrino background
- Oscillation and Future Detection of Failed Supernova Neutrinos from Black Hole Forming Collapse
- Prospects for Detecting the Diffuse Supernova Neutrino Background with JUNO
- Shockwaves in Supernovae: New Implications on the Diffuse Supernova Neutrino Background
- Direct Measurement of Supernova Neutrino Emission Parameters with a Gadolinium-Enhanced Super-Kamiokande Detector
- Imprint of Explosion Mechanism on Supernova Relic Neutrinos
- New analysis of the SN 1987A neutrinos with a flexible spectral shape
- Effect of Collective Flavor Oscillations on the Diffuse Supernova Neutrino Background
- Diffuse Cosmic Neutrino Background from Population III Stars
- Resonant Neutrino Self-Interactions
- Discovery potential for supernova relic neutrinos with slow liquid scintillator detectors
- Neutrinos from failed supernovae at future water and liquid argon detectors
- Detecting the Diffuse Supernova Neutrino Background with LENA
- Neutral-current background induced by atmospheric neutrinos at large liquid-scintillator detectors: I. model predictions
- Upper limits on the diffuse supernova neutrino flux from the SuperKamiokande data
- Gravitational Collapse and Neutrino Emission of Population III Massive Stars
- New Test of Supernova Electron Neutrino Emission using Sudbury Neutrino Observatory Sensitivity to the Diffuse Supernova Neutrino Background
- Mini Z' Burst from Relic Supernova Neutrinos and Late Neutrino Masses
- Measurement of neutrino-oxygen neutral-current quasi-elastic cross section using atmospheric neutrinos at Super-Kamiokande
- Detecting the Diffuse Supernova Neutrino Background in the future Water-based Liquid Scintillator Detector Theia
- Detecting extra-galactic supernova neutrinos in the Antarctic ice
- Neutrino Signatures from the First Stars
- Constraints on MeV dark matter using neutrino detectors and their implication for the 21-cm results
- Flavour specific neutrino self-interaction: tension and IceCube
- The diffuse supernova neutrino background: Expectations and uncertainties derived from SN1987A
- Probing Late Neutrino Mass Properties with Supernova Neutrinos
- Black Hole Accretion Disk Diffuse Neutrino Background
- The diffuse neutrino flux from supernovae: upper limit on the electron neutrino component from the non-observation of antineutrinos at SuperKamiokande
- On the Observability of Collective Flavor Oscillations in Diffuse Supernova Neutrino Background
- Neutral-current background induced by atmospheric neutrinos at large liquid-scintillator detectors: II. Methodology for in situ measurements
- 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
- Testing neutrino spectra formation in collapsing stars with the diffuse supernova neutrino flux
- SN 2023ixf -- an average-energy explosion with circumstellar medium and a precursor
- Impact of late-time neutrino emission on the diffuse supernova neutrino background
- Neutrino Backgrounds in Future Liquid Noble Element Dark Matter Direct Detection Experiments
- Memory-triggered supernova neutrino detection
- Impact of Rotation on Neutrino Emission and Relic Neutrino Background from Population III Stars
- Ultrahigh-energy neutrino flux as a probe of large extra-dimensions
- JUNO sensitivity to the annihilation of MeV dark matter in the galactic halo
- Diffuse neutrino supernova background as a cosmological test
- Neutrino non-radiative decay and the diffuse supernova neutrino background
- Neutrino production in Population III microquasars
- Stellar Neutrino Emission Across The Mass-Metallicity Plane
- An "archaeological" quest for galactic supernova neutrinos
- Low energy neutrinos from stopped muons in the Earth
- Mimicking diffuse supernova antineutrinos with the Sun as a source
- R-process beta-decay neutrino flux from binary neutron star mergers and collapsars
- Cooling the Shock: New Supernova Constraints on Dark Photons
- Diffuse Neutrino Background from Magnetorotational Stellar Core Collapses
- The Diffuse Supernova Neutrino Background in the Standard and Double Collapse Models
- Upper Limit on the Cosmic Gamma-Ray Burst Rate from High Energy Diffuse Neutrino Background
- The Diffuse Supernova Neutrino Background
- Impacts of Black-Hole-Forming Supernova Explosions on the Diffuse Neutrino Background
- Non-thermal neutrinos from supernovae leaving a magnetar
- Neutron Tagging Can Greatly Reduce Spallation Backgrounds in Super-Kamiokande
- Constraining Chaplygin models using diffuse supernova neutrino background
- The Dark Matter Diffused Supernova Neutrino Background
- Timing coincidence search for supernova neutrinos with optical transient surveys
- Neutrino magnetic moment signatures in the supernova neutrino signal
- Core-collapse supernova neutrinos and neutrino properties
- CNNs for enhanced background discrimination in DSNB searches in large-scale water-Gd detectors
- Limits in late time conversion of cold dark matter into dark radiation
- Searching for MeV-mass neutrinophilic Dark Matter with Large Scale Dark Matter Detectors
- Neutrinos from Diffuse Supernova Background
- Low energy neutrino scattering : from fundamental interaction studies to astrophysics
- The Relic Neutrino Backround from the First Stars
- Prospects for Neutrino Observation and Mass Measurement from Binary Neutron Star Mergers