Superheavy dark matter from the natural inflation in light of the highest-energy astroparticle events
arXiv:2504.15272 · doi:10.1088/1475-7516/2025/10/109
Abstract
Superheavy dark matter has been attractive as a candidate of particle dark matter. We propose a ``natural" particle model, in which the dark matter serves as the inflaton in natural inflation, while decaying to high-energy particles at energies of from the prediction of the inflation. A scalar field responsible for diluting the dark matter abundance revives the natural inflation either with or without the recent data from the Atacama Cosmology Telescope (ACT) and baryon acoustic oscillation results from Dark Energy Spectroscopic Instrument. Since the dark matter must be a spin-zero scalar, we carefully study the galactic dark matter 3-body decay into fermions and two body decays into a gluon pair, and point out relevant multi-messenger bounds that constrain these decay modes. Interestingly, the predicted energy scale may coincide with the AMATERASU event and/or the KM3NeT neutrino event, KM3-230213A. We also point out particle models with dark baryon to further alleviate -ray bounds. This scenario yields several testable predictions for the UHECR observations, including the highest-energy neutrons that are unaffected by magnetic fields, the tensor-to-scalar ratio, the running of spectral indices, , and the existence of light new colored particles that could be accessible at future collider experiments. Further measurements of high-energy cosmic rays, including their components and detailed directions, may provide insight into not only the origin of the cosmic rays but also inflation.
arXiv comment37 pages, 5 figures
References in corpus (77)
- A Universal Density Profile from Hierarchical Clustering
- Planck 2018 results. X. Constraints on inflation
- The Inner Structure of LambdaCDM Halos III: Universality and Asymptotic Slopes
- DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
- BICEP / Keck XIII: Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season
- Primordial Black Holes - Perspectives in Gravitational Wave Astronomy -
- Natural Inflation: Particle Physics Models, Power Law Spectra for Large Scale Structure, and Constraints from COBE
- Thermal Inflation and the Moduli Problem
- Superheavy dark matter
- The Astrophysics of Ultrahigh Energy Cosmic Rays
- Mission design of LiteBIRD
- The IceCube high-energy starting event sample: Description and flux characterization with 7.5 years of data
- Ultra-high energy cosmic rays without GZK cutoff
- The Milky Way total mass profile as inferred from Gaia DR2
- MeV-scale reheating temperature and thermalization of oscillating neutrinos by radiative and hadronic decays of massive particles
- Nonthermal Supermassive Dark Matter
- Trans-Planckian Censorship and the Swampland
- Differential limit on the extremely-high-energy cosmic neutrino flux in the presence of astrophysical background from nine years of IceCube data
- Probing Planckian physics: resonant production of particles during inflation and features in the primordial power spectrum
- Improved Characterization of the Astrophysical Muon-Neutrino Flux with 9.5 Years of IceCube Data
- On the gravitational production of superheavy dark matter
- Mirror particles and mirror matter: 50 years of speculation and search
- Extremely high energy cosmic rays from relic particle decays
- Mirror World and its Cosmological Consequences
- Neutrinos at IceCube from Heavy Decaying Dark Matter
- Detection of a particle shower at the Glashow resonance with IceCube
- Neutrino Constraints on the Dark Matter Total Annihilation Cross Section
- Ultra-High Energy Cosmic Rays, Superheavy Long-Living Particles, and Matter Creation after Inflation
- Gamma-ray Constraints on Decaying Dark Matter and Implications for IceCube
- Features of the energy spectrum of cosmic rays above eV using the Pierre Auger Observatory
- Ultra-High-Energy Cosmic Rays
- Testing the Dark Matter Scenario for PeV Neutrinos Observed in IceCube
- Are IceCube neutrinos unveiling PeV-scale decaying dark matter?
- Inflaton Decay and Heavy Particle Production with Negative Coupling
- Dark Matter Spectra from the Electroweak to the Planck Scale
- Depth of Ultra High Energy Cosmic Ray Induced Air Shower Maxima Measured by the Telescope Array Black Rock and Long Ridge FADC Fluorescence Detectors and Surface Array in Hybrid Mode
- The ALP miracle: unified inflaton and dark matter
- Constraining Very Heavy Dark Matter Using Diffuse Backgrounds of Neutrinos and Cascaded Gamma Rays
- Ultra High Energy Cosmic Rays and Inflation Relics
- Post--Sphaleron Baryogenesis
- Detection of the Keplerian decline in the Milky Way rotation curve
- Classical inflaton field induced creation of superheavy dark matter
- Multi-Natural Inflation
- Probing the stability of superheavy dark matter particles with high-energy neutrinos
- The ALP miracle revisited
- Heavy decaying dark matter and IceCube high energy neutrinos
- Model-independent dark matter annihilation bound from the diffuse gamma ray flux
- Flavourful Production at Hadron Colliders
- An extremely energetic cosmic ray observed by a surface detector array
- Multi-Natural Inflation in Supergravity and BICEP2
- Super Heavy Dark Matter in light of BICEP2, Planck and Ultra High Energy Cosmic Rays Observations
- Multi-Natural Inflation in Supergravity
- KASCADE-Grande Limits on the Isotropic Diffuse Gamma-Ray Flux between 100 TeV and 1 EeV
- Trans-Planckian censorship and other swampland bothers addressed in warm inflation
- Superheavy scalar dark matter from gravitational particle production in -attractor models of inflation
- Probing heavy dark matter decays with multi-messenger astrophysical data
- Super-Heavy Dark Matter - Towards Predictive Scenarios from Inflation
- Trans-Planckian wimpzillas
- High-energy Neutrinos from Multi-body Decaying Dark Matter
- A search for photons with energies above eV using hybrid data from the low-energy extensions of the Pierre Auger Observatory
- Axion monodromy inflation with multi-natural modulations
- Implications of an Improved Neutron-Antineutron Oscillation Search for Baryogenesis: A Minimal Effective Theory Analysis
- Search for Extremely-High-Energy Neutrinos and First Constraints on the Ultrahigh-Energy Cosmic-Ray Proton Fraction with IceCube
- Hybrid natural inflation from non Abelian discrete symmetry
- Revisiting ultrahigh-energy constraints on decaying super-heavy dark matter
- Boosted Neutrinos and Relativistic Dark Particles as Messengers from Reheating
- Hybrid Natural Low Scale Inflation
- Super heavy dark matter origin of the PeV neutrino event: KM3-230213A
- Hybrid Natural Inflation
- The Spectrum of Dark Radiation as a Probe of Reheating
- Direct baryogenesis in the broken phase
- Dark sectors in neutron-shining-through-a-wall and nuclear absorption signals
- High Energy Sphalerons for Baryogenesis at Low Temperatures
- Indirect detection of unstable heavy dark matter
- Probing superheavy dark matter through lunar radio observations of ultrahigh-energy neutrinos and the impacts of neutrino cascades
- Shining ALP Dark Radiation
- The past and future 20-years endeavor for discovering origins of ultra-high energy cosmic rays -- Rapporteur's summary of cosmic ray indirect --
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- Cosmogenic Origin of KM3-230213A: Delayed Gamma-Ray Emission from A Cosmic-Ray Transient
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- Exploring ultra-high energy neutrino experiments through the lens of the transport equation
- Linking the KM3-230213A Neutrino Event to Dark Matter Decay and Gravitational Wave signals
- Beyond the Local Void: A data-driven search for the origins of the Amaterasu particle