Searching for Axion-Like Particles from Core-Collapse Supernovae with Fermi LAT's Low Energy Technique

Abstract

Light axion-like particles (ALPs) are expected to be abundantly produced in core-collapse supernovae (CCSNe), resulting in a $\sim$10-second long burst of ALPs. These particles subsequently undergo conversion into gamma-rays in external magnetic fields to produce a long gamma-ray burst (GRB) with a characteristic spectrum peaking in the 30--100-MeV energy range. At the same time, CCSNe are invoked as progenitors of {\it ordinary} long GRBs, rendering it relevant to conduct a comprehensive search for ALP spectral signatures using the observations of long GRB with the \textit{Fermi} Large Area Telescope (LAT). We perform a data-driven sensitivity analysis to determine CCSN distances for which a detection of an ALP signal is possible with the LAT's low-energy (LLE) technique which, in contrast to the standard LAT analysis, allows for a a larger effective area for energies down to 30~MeV. Assuming an ALP mass $m_a\lesssim 10^{-10}$~eV and ALP-photon coupling $g_{a\gamma }=5.3\times 10^{-12}$ GeV${}^{-1}$, values considered and deduced in ALP searches from SN1987A, we find that the distance limit ranges from $\sim 0.5$ to $\sim 10$~Mpc, depending on the sky location and the CCSN progenitor mass. Furthermore, we select a candidate sample of twenty-four GRBs and carry out a model comparison analysis in which we consider different GRB spectral models with and without an ALP signal component. We find that the inclusion of an ALP contribution does not result in any statistically significant improvement of the fits to the data. We discuss the statistical method used in our analysis and the underlying physical assumptions, the feasibility of setting upper limits on the ALP-photon coupling, and give an outlook on future telescopes in the context of ALP searches.

arXiv comment15 pages, 8 figures, accepted by Physical Review D

References in corpus (69)

• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• The Large Area Telescope on the Fermi Gamma-ray Space Telescope Mission
• Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
• Asymptotic formulae for likelihood-based tests of new physics
• The Zwicky Transient Facility: System Overview, Performance, and First Results
• Axion Cosmology
• Discovery of the peculiar supernova 1998bw in the error box of GRB980425
• The Man Behind the Curtain: X-rays Drive the UV through NIR Variability in the 2013 AGN Outburst in NGC 2617
• The Physics of Gamma-Ray Bursts
• The Supernova -- Gamma-Ray Burst Connection
• The Fermi Gamma-Ray Burst Monitor
• First Results from the Catalina Real-time Transient Survey
• The Palomar Transient Factory: System Overview, Performance and First Results
• Short-Duration Gamma-Ray Bursts
• Neutrino emission from the direction of the blazar TXS 0506+056 prior to the IceCube-170922A alert
• The Low-Energy Frontier of Particle Physics
• WISPy Cold Dark Matter
• A New Model of the Galactic Magnetic Field
• Northern Sky Variability Survey (NSVS): Public data release
• Excess Electronic Recoil Events in XENON1T
• Revisiting the bound on axion-photon coupling from Globular Clusters
• The metamorphosis of SN1998bw
• Protoneutron star evolution and the neutrino driven wind in general relativistic neutrino radiation hydrodynamics simulations
• New ALPS Results on Hidden-Sector Lightweights
• Revisiting the SN1987A gamma-ray limit on ultralight axion-like particles
• The Locations of Short Gamma-ray Bursts as Evidence for Compact Object Binary Progenitors
• The Observer's Guide to the Gamma-Ray Burst-Supernova Connection
• A Comprehensive Analysis of Fermi Gamma-Ray Burst Data. I. Spectral Components and Their Possible Physical Origins of LAT/GBM GRBs
• A decade of Gamma-Ray Bursts observed by $Fermi$-LAT: The 2${}^{nd}$ GRB catalog
• Search for Spectral Irregularities due to Photon-Axionlike-Particle Oscillations With the Fermi Large Area Telescope
• Studies of Diffuse Interstellar Bands. V. Pairwise Correlations of Eight Strong DIBs and Neutral Hydrogen, Molecular Hydrogen, and Color Excess
• A High Resolution Search for Dark-Matter Axions
• Cool WISPs for stellar cooling excesses
• First lower limits on the photon-axion-like particle coupling from very high energy gamma-ray observation
• Stellar Recipes for Axion Hunters
• Detection of Neutrinos from Supernovae in Nearby Galaxies
• Gamma Rays from SN1987A due to Pseudoscalar Conversion
• SN 1987A Gamma-Ray Limits on the Conversion of Pseudoscalars
• Failed gamma-ray bursts and orphan afterglows
• A New Bound on Axion-Like Particles
• Impulsive and Long Duration High-Energy Gamma-ray Emission From the Very Bright 2012 March 7 Solar Flares
• The Fermi Large Area Telescope as a Galactic Supernovae Axionscope
• Constraining the Axion-Photon Coupling with Massive Stars
• A 3.55 keV Photon Line and its Morphology from a 3.55 keV ALP Line
• Stochastic conversions of TeV photons into axion-like particles in extragalactic magnetic fields
• X-ray Searches for Axions from Super Star Clusters
• Open statistical issues in particle physics
• Solar axions cannot explain the XENON1T excess
• Searching for a 0.1-1 keV Cosmic Axion Background
• Axion-Like Particles and Recent Observations of the Cosmic Infrared Background Radiation
• Core-Collapse Astrophysics with a Five-Megaton Neutrino Detector
• Re-examining the Solar Axion Explanation for the XENON1T Excess
• Search for Axionlike-Particle-Induced Prompt Gamma-Ray Emission from Extragalactic Core-Collapse Supernovae with the Fermi Large Area Telescope
• The ASAS-SN Bright Supernova Catalog $-$ I. 2013$-$2014
• Soft X-ray Excess in the Coma Cluster from a Cosmic Axion Background
• Early Time Light Curves of Type Ia Supernovae Observed with TESS
• Significance of an excess in a counting experiment: assessing the impact of systematic uncertainties and the case with Gaussian background
• PANGU: A High Resolution Gamma-ray Space Telescope
• Hint at an axion-like particle from the redshift dependence of blazar spectra
• Turbulent axion-photon conversions in the Milky-Way
• Revisiting the analysis of axion-like particles with the Fermi-LAT gamma-ray observation of NGC1275
• Axions in neutron star mergers
• Estimating the Explosion Time of Core-Collapse Supernovae from Their Optical Light Curves
• The e-ASTROGAM gamma-ray space mission
• The connection between Gamma-ray bursts and Supernovae Ib/c
• A Cosmic ALP Background and the Cluster Soft X-ray Excess in A665, A2199 and A2255
• ALP Conversion and the Soft X-ray Excess in the Outskirts of the Coma Cluster
• Photon-photon dispersion of TeV gamma rays and its role for photon-ALP conversion
• A possible blazar spectral irregularity case caused by photon--axionlike-particle oscillations

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