Prospects for Observing Astrophysical Transients with GeV Neutrinos
arXiv:2412.05087 · doi:10.3847/1538-4357/adb716
Abstract
Although Cherenkov detectors of high-energy neutrinos in ice and water are often optimized to detect TeV-PeV neutrinos, they may also be sensitive to transient neutrino sources in the 1-100~GeV energy range. A wide variety of transient sources have been predicted to emit GeV neutrinos. In light of the upcoming IceCube-Upgrade, which will extend the IceCube detector's sensitivity down to a few GeV, as well as improve its angular resolution, we survey a variety of transient source models and compare their predicted neutrino fluences to detector sensitivities, in particular those of IceCube-DeepCore and the IceCube Upgrade. We consider the ranges of neutrino fluence from transients powered by non-relativistic shocks, such as novae, supernovae, fast blue optical transients, and tidal disruption events. We also consider fast radio bursts and relativistic outflows of high- and low-luminosity gamma-ray bursts. Our study sheds light on the prospects of observing GeV transients with existing and upcoming neutrino facilities.
References in corpus (98)
- A bright millisecond radio burst of extragalactic origin
- The Physics of Gamma-Ray Bursts
- Gamma-Ray Bursts
- Nearby Supernova Rates from the Lick Observatory Supernova Search. II. The Observed Luminosity Functions and Fractions of Supernovae in a Complete Sample
- A fast radio burst associated with a Galactic magnetar
- Nearby Supernova Rates from the Lick Observatory Supernova Search. III. The Rate-Size Relation, and the Rates as a Function of Galaxy Hubble Type and Colour
- Simulations of Ion Acceleration at Non-relativistic Shocks. I. Acceleration Efficiency
- V1309 Scorpii: merger of a contact binary
- An ultraviolet-optical flare from the tidal disruption of a helium-rich stellar core
- A Continuum of H- to He-Rich Tidal Disruption Candidates With a Preference for E+A Galaxies
- Fast radio bursts as synchrotron maser emission from decelerating relativistic blast waves
- Particle Acceleration in Relativistic Magnetized Collisionless Electron-Ion Shocks
- Rates of Stellar Tidal Disruption as Probes of the Supermassive Black Hole Mass Function
- Collisional mechanism for GRB emission
- Rapidly-Evolving and Luminous Transients from Pan-STARRS1
- Parameterization of Gamma, e^+/- and Neutrino Spectra Produced by p-p Interaction in Astronomical Environment
- PTF11kx: A Type-Ia Supernova with a Symbiotic Nova Progenitor
- The luminosity function and the rate of Swift's Gamma Ray Bursts
- Atmospheric neutrino flux calculation using the NRLMSISE00 atmospheric model
- A flaring magnetar in FRB 121102?
- An embedded X-ray source shines through the aspherical AT2018cow: revealing the inner workings of the most luminous fast-evolving optical transients
- Observing the Next Galactic Supernova
- Weighing Black Holes using Tidal Disruption Events
- High Energy Neutrinos and Cosmic-Rays from Low-Luminosity Gamma-Ray Bursts?
- The Cow: discovery of a luminous, hot and rapidly evolving transient
- Gamma-Ray Emission Concurrent with the Nova in the Symbiotic Binary V407 Cygni
- The Fast, Luminous Ultraviolet Transient AT2018cow: Extreme Supernova, or Disruption of a Star by an Intermediate-Mass Black Hole?
- The X-ray through Optical Fluxes and Line Strengths of Tidal Disruption Events
- Fermi Establishes Classical Novae as a Distinct Class of Gamma-Ray Sources
- Optical-Ultraviolet Tidal Disruption Events
- Rates of Superluminous Supernovae at z~0.2
- A unified picture for low-luminosity and long gamma-ray bursts based on the extended progenitor of llgrb 060218/SN 2006aj
- On the mass and luminosity functions of tidal disruption flares: rate suppression due to black hole event horizons
- Implications of a "Fast Radio Burst" from a Galactic Magnetar
- Prompt Radiation and Mass Outflows from the Stream-Stream Collisions of Tidal Disruption Events
- Superluminous supernovae
- 5-10 GeV Neutrinos from Gamma-Ray Burst Fireballs
- Low-Luminosity Gamma-Ray Bursts as a Distinct GRB Population:A Firmer Case from Multiple Criteria Constraints
- Failed Supernovae Explain the Compact Remnant Mass Function
- A mildly relativistic outflow from the energetic, fast-rising blue optical transient CSS161010 in a dwarf galaxy
- High-Energy Neutrino Emission from Short Gamma-Ray Bursts: Prospects for Coincident Detection with Gravitational Waves
- Shock-powered light curves of luminous red novae as signatures of pre-dynamical mass loss in stellar mergers
- Gamma-ray novae as probes of relativistic particle acceleration at non-relativistic shocks
- The Galactic Nova Rate Revisited
- Can tidal disruption events produce the IceCube neutrinos?
- Strong late-time circumstellar interaction in the peculiar supernova iPTF14hls
- Neutrino Spectra from Low and High Luminosity Populations of Gamma Ray Bursts
- Observational properties of extreme supernovae
- Time-resolved hadronic particle acceleration in the recurrent Nova RS Ophiuchi
- High-Energy Neutrino and Gamma-Ray Emission from Tidal Disruption Events
- The Core Collapse Supernova Rate from the SDSS-II Supernova Survey
- A Nova Outburst Powered by Shocks
- Subphotospheric Neutrinos from Gamma-Ray Bursts: The Role of Neutrons
- Ultra-High Energy Cosmic Rays and Neutrinos from Tidal Disruptions by Massive Black Holes
- High-Energy Neutrinos from Millisecond Magnetars formed from the Merger of Binary Neutron Stars
- Fermi LAT Gamma-ray Detections of Classical Novae V1369 Centauri 2013 and V5668 Sagittarii 2015
- Luminosity function and jet structure of Gamma Ray Bursts
- Electron acceleration in non-relativistic quasi-perpendicular collisionless shocks
- On Computing Upper Limits to Source Intensities
- Physics of radiation mediated shocks and its applications to GRBs, supernovae, and neutron star mergers
- Proton acceleration in thermonuclear nova explosions revealed by gamma rays
- Luminous Red Novae: population models and future prospects
- Orbital Periods for Three Recurrent Novae
- Energy spectra of secondaries in proton-proton interactions
- High-Energy Neutrinos and Gamma-Rays from Non-Relativistic Shock-Powered Transients
- High-Energy Emission from Interacting Supernovae: New Constraints on Cosmic-Ray Acceleration in Dense Circumstellar Environments
- Heavy Nuclei Synthesized in Gamma-Ray Burst Outflows as the Source of UHECRs
- Limits on Neutrino Emission from GRB 221009A from MeV to PeV using the IceCube Neutrino Observatory
- Particle acceleration and non-thermal emission during the V407 Cygni nova outburst
- Neutrinos from the Brightest Gamma-Ray Burst?
- X-ray Emission from SN 2012ca: A Type Ia-CSM Supernova Explosion in a Dense Surrounding Medium
- Detection Prospects for GeV Neutrinos from Collisionally Heated Gamma-ray Bursts with IceCube/DeepCore
- AAfrag: Interpolation routines for Monte Carlo results on secondary production in proton-proton, proton-nucleus and nucleus-nucleus interactions
- A population of heavily reddened, optically missed novae from Palomar Gattini-IR: Constraints on the Galactic nova rate
- Light Curve Model for Luminous Red Novae and Inferences about the Ejecta of Stellar Mergers
- Multimessenger Implications of AT2018cow: High-Energy Cosmic Ray and Neutrino Emissions from Magnetar-Powered Super-Luminous Transients
- Interpretation of the observed neutrino emission from three Tidal Disruption Events
- The Multi-Dimensional Structure of Radiative Shocks: Suppressed Thermal X-rays and Relativistic Ion Acceleration
- Fermi-LAT Gamma-ray Detection of the Recurrent Nova RS Ophiuchi during its 2021 Outburst
- The B & V Light Curves for Recurrent Nova T CrB From 1842--2022, the Unique Pre- and Post-Eruption High-States, the Complex Period Changes, and the Upcoming Eruption in 2025.51.3
- A Light Curve Analysis of Recurrent and Very Fast Novae in our Galaxy, Magellanic Clouds, and M31
- Search for Early Gamma-ray Production in Supernovae Located in a Dense Circumstellar Medium with the Fermi LAT
- The role of jet-cocoon mixing, magnetization and shock breakout in neutrino and cosmic-ray emission from short GRBs
- Time-dependent high-energy gamma-ray signal from accelerated particles in core-collapse supernovae: the case of SN 1993J
- Volumetric rates of Luminous Red Novae and Intermediate Luminosity Red Transients with the Zwicky Transient Facility
- Evidence for multiple shocks from the -ray emission of RS Ophiuchi
- Search for gamma-ray emission from super-luminous supernovae with the Fermi-LAT
- Search for 10--1000 GeV neutrinos from Gamma Ray Bursts with IceCube
- Neutrino Counterparts of Fast Radio Bursts
- Particle Acceleration in Mildly Relativistic Outflows of Fast Energetic Transient Sources
- Search for sub-TeV Neutrino Emission from Novae with IceCube-DeepCore
- A Search for IceCube sub-TeV Neutrinos Correlated with Gravitational-Wave Events Detected By LIGO/Virgo
- Systematic exploration of heavy element nucleosynthesis in protomagnetar outflows
- Detection prospects for multi-GeV neutrinos from collisionally heated GRBs
- First all-flavor search for transient neutrino emission using 3-years of IceCube DeepCore data
- Search for Transient Astrophysical Neutrino Emission with IceCube-DeepCore
- KM3NeT/ORCA: status and perspectives for neutrino oscillation and mass hierarchy measurements
- Quasithermal GeV neutrinos from neutron-loaded magnetized outflows in core-collapse supernovae: spectra and light curves