High Energy Neutrinos from Astrophysical Sources: An Upper Bound
arXiv:hep-ph/9807282 · doi:10.1103/PhysRevD.59.023002
Abstract
We show that cosmic-ray observations set a model-independent upper bound to the flux of high-energy, > 10^14 eV, neutrinos produced by photo-meson (or p-p) interactions in sources of size not much larger than the proton photo-meson (or pp) mean-free-path. The bound applies, in particular, to neutrino production by either AGN jets or GRBs. This upper limit is two orders of magnitude below the flux predicted in some popular AGN jet models, but is consistent with our predictions from GRB models. We discuss the implications of these results for future km^2 high-energy neutrino detectors.
Added discussion showing bound cannot be evaded by invoking magnetic fields. Accepted Phys Rev D
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- From AMANDA to IceCube
- The status of the ANTARES experiment
- Horizontal Muons and a Search for AGN Neutrinos in Soudan 2
- Extragalactic neutrino background from very young pulsars surrounded by supernova envelopes
- High Energy Neutrino Astronomy
- Ultrahigh Energy Cosmic Rays and Neutrinos
- Status of ANITA and ANITA-lite
- Bayesian Approach for Counting Experiment Statistics applied to a Neutrino Point Source Analysis
- Explanation of IceCube spectrum with neutrino splitting in a 2HDM model
- Results from the IceCube Experiment - Neutrino 2012
- The ANTARES neutrino project: status report
- Lectures on neutrino phenomenology
- The Role and Detectability of the Charm Contribution to Ultra High Energy Neutrino Fluxes
- Neutrino Astronomy - A Review of Future Experiments
- Recent results from the ANTARES neutrino telescope
- PeV neutrinos from wind breakouts of type II supernovae
- Solving the missing GRB neutrino and GRB-SN puzzles
- Constraints and prospects on GW and neutrino emissions using GW150914
- On the observability of high-energy neutrinos from gamma ray bursts
- Unparticle effects in neutrino telescopes
- The Scientific Life Of John Bahcall
- The Gamma-Ray Background Constrains the Origins of the Radio and X-Ray Backgrounds
- Upper Limit on the Diffuse Flux of Cosmic with the ANTARES Neutrino Telescope
- High Energy Neutrino Astrophysics
- Neutrino emission from a GRB afterglow shock during an inner supernova shock breakout
- Constraints and prospects on gravitational wave and neutrino emission using GW150914
- Astrophysical neutrinos: theory
- Neutrino Production Associated with Late Bumps in Gamma-Ray Bursts and Potential Contribution to Diffuse Flux at IceCube
- Neutrino Self-Interactions
- Non-thermal neutrinos from supernovae leaving a magnetar
- The Dawn of Multi-Messenger Astronomy
- Investigating starburst-driven neutrino emission from galaxies in the Great Observatories All-Sky LIRG Survey
- Determining neutrino absorption spectra at Ultra-High Energies
- Ultrahigh Energy Cosmic Rays and Neutrinos
- Probing a Four Flavour vis-a-vis Three Flavour Neutrino Mixing for UHE Neutrino Signals at a 1 Detector
- Neutrinos as a signature of ultrahigh energy photons at high red shift
- Extremely energetic cosmic neutrinos: Opportunities for astrophysics, particle physics, and cosmology
- The sensitivity of cosmic ray air shower experiments for leptoquark detection
- Olber's Paradox for Superluminal Neutrinos: Constraining Extreme Neutrino Speeds at TeV-ZeV Energies with the Diffuse Neutrino Background
- Challenges for Cosmic-ray Experiments
- Randall-Sundrum black holes and strange stars
- A relook at the GZK Neutrino-Photon Connection: Impact of Extra-galactic Radio Background & UHECR properties
- Solar flare observations with the Radio Neutrino Observatory Greenland (RNO-G)
- Neutrino Flux Bounds and Prospects for High Energy and Ultrahigh Energy Neutrino Source Detection
- Ultrahigh energy cosmic rays and neutrino flux models
- Bounds on the neutrino flux from cosmic sources of relativistic particles
- High Energy Astroparticle Physics
- Supersymmetry on the Rocks
- Probing New Physics with Astrophysical Neutrinos
- The ANTARES experiment: past, present and future
- Confronting the dark matter capture rate with a continuous gravitational wave probe of local neutron stars
- Probing Physics at Extreme Energies with Cosmic Ultra-High Energy Radiation
- Effects of non-standard interaction on microscopic black holes from ultra-high energy neutrinos
- Report from the Multi-Messenger Working Group at UHECR-2014 Conference
- Multi-messenger Astronomy with Quenched Superradiance
- Neutrino Astronomy with the IceCube Observatory
- Neutrino Astronomy 2017
- High-energy neutrino emission from Gamma-Ray Bursts
- Multi-Messenger Astrophysics with THESEUS in the 2030s
- Overall Ultra-high Energy Neutrino Emission from GRBs during Jet Expansion
- Probing a Supersymmetric Model for Neutrino Masses at Ultrahigh Energy Neutrino Telescopes
- On the relation between the astrophysical neutrino fluxes and the cosmic ray fluxes
- Observational strategies for ultrahigh-energy neutrinos: the importance of deep sensitivity for detection and astronomy
- Obscured -channel neutrino sources
- First search for neutrinos in correlation with gamma-ray bursts with the ANTARES neutrino telescope
- Detectors for Cosmic Rays on Ground and in Space
- Little Red Dots as Hidden Neutrino Sources
- IceCube and Searches for Astrophysical Sources
- High Energy Neutrinos: Sources and Fluxes
- Neutrino Astronomy (Rapporteur Talk)
- Radiowave Neutrino Detection
- Observe Gamma-Rays and Neutrinos Associated with Ultra-High Energy Cosmic Rays
- Implications of cosmic ray results for UHE neutrinos
- High Energy Neutrinos as a Probe for New Physics and Astrophysics
- Particle Physics in the Sky and Astrophysics Underground: Connecting the Universe's Largest and Smallest Scales
- The starburst-GRB connection
- Closing in on the sources of Galactic and extragalactic cosmic rays
- Selected results from IceCube
- Status and Perspectives of Neutrino Physics
- IceCube: Neutrino Physics from GeV - PeV
- High Energy Neutrinos and Cosmic Rays
- SUSY at the Pole
- Neutrino Astronomy at High Energies - An Experimental Review
- Constraining Galactic Interactions with Cosmic Ray Electron and Positron Spectra
- Prospects for GMRT to Observe Radio Waves from UHE Particles Interacting with the Moon
- High Energy Neutrinos with a Mediterranean Neutrino Telescope
- Neutrino Detection with the Surface Array of the Pierre Auger Observatory
- Common origin of the diffuse high energy backgrounds of gamma rays, neutrinos and cosmic ray positrons?
- Aspects of astrophysical particle production and beyond the Standard Model phenomenology
- Strongly Interacting Neutrinos as the Highest Energy Cosmic Rays: A Quantitative Analysis
- Indirect Probes of Supersymmetry Breaking in the JEM-EUSO Observatory
- Search for neutrino emission from gamma-ray sources with the Antares Telescope
- Astrophysical neutrino results
- The Relevance of Mediterranean Neutrino Telescope Sites on Earth-skimming tau neutrino detection
- Event rates vs. cross sections at neutrino telescopes
- ANTARES and other Neutrino Telescopes in the Northern Hemisphere
- Search for Ultra High-Energy Neutrinos with AMANDA-II
- Theory of high-energy messengers
- MeV, GeV and TeV neutrinos from binary-driven hypernovae
- Particle Reacceleration by Turbulence and Radio Constraints on Multi-Messenger High-Energy Emission from the Coma Cluster
- Echoes of the past: ultra-high energy cosmic rays accelerated by radio galaxies, scattered by starburst galaxies