Induced Gravitational Waves probing Primordial Black Hole Dark Matter with Memory Burden

Abstract

Quantum evaporation of a black hole is conventionally studied semiclassically by assuming self-similarity of the black hole throughout the evaporation process. However, its validity was recently questioned, and the lifetime of a black hole is conjectured to be much extended by the memory burden effect. It gives rise to the possibility that the primordial black holes (PBHs) lighter than $10^{10}$ grams are the dark matter in the Universe. To probe such PBH dark matter, we study gravitational waves (GWs) induced by primordial curvature perturbations that produced the PBHs. We find ${\Omega }_{\text{GW}}(f_{\text{peak}})h^2=7\times 10^{-9}$ with the peak frequency $f_{\text{peak}}=1\times 10^3(M_{\text{PBH}}/(10^{10}\mathrm{g}){)}^{-1/2}\mathrm{Hz}$, and the induced GWs associated with the PBH dark matter whose initial mass is greater than about $10^7$ grams can be tested by future observations such as Cosmic Explorer. Furthermore, the scenario can be in principle confirmed by detecting another GW signal from the mergers of PBHs, which leads to high-frequency GWs with $f_{\text{peak}}=2\times 10^{27}(M_{\text{PBH, ini}}/(10^{10}\mathrm{g}){)}^{-1}\mathrm{Hz}$. On the other hand, the induced GW signals stronger than expected would contradict the dark matter abundance and exclude the memory burden effect.

23 pages, 5 figures; published version

References in corpus (103)

• Advanced Virgo: a 2nd generation interferometric gravitational wave detector
• Advanced LIGO
• Planck 2018 results. X. Constraints on inflation
• The NANOGrav 15-year Data Set: Evidence for a Gravitational-Wave Background
• Exploring the Sensitivity of Next Generation Gravitational Wave Detectors
• Did LIGO detect dark matter?
• Search for an isotropic gravitational-wave background with the Parkes Pulsar Timing Array
• Science Case for the Einstein Telescope
• Searching for the nano-Hertz stochastic gravitational wave background with the Chinese Pulsar Timing Array Data Release I
• New cosmological constraints on primordial black holes
• Sensitivity Studies for Third-Generation Gravitational Wave Observatories
• Gravitational Wave Experiments and Early Universe Cosmology
• Interferometer design of the KAGRA gravitational wave detector
• The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals
• BICEP / Keck XIII: Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season
• Possibility of Direct Measurement of the Acceleration of the Universe Using 0.1 Hz Band Laser Interferometer Gravitational Wave Antenna in Space
• Primordial Black Hole Scenario for the Gravitational-Wave Event GW150914
• Detector configuration of KAGRA - the Japanese cryogenic gravitational-wave detector
• A Covariant Entropy Conjecture
• Primordial Black Holes - Perspectives in Gravitational Wave Astronomy -
• The NANOGrav 15-year Data Set: Search for Signals from New Physics
• Primordial Black Holes as Dark Matter: Recent Developments
• Gravitational Wave Spectrum Induced by Primordial Scalar Perturbations
• Detecting a stochastic background of gravitational radiation: Signal processing strategies and sensitivities
• Beyond LISA: Exploring Future Gravitational Wave Missions
• The cosmological gravitational wave background from primordial density perturbations
• Primordial Black Holes as a dark matter candidate
• Inspiral-merger-ringdown waveforms for black-hole binaries with non-precessing spins
• The clustering of massive Primordial Black Holes as Dark Matter: measuring their mass distribution with Advanced LIGO
• Semianalytic Calculation of Gravitational Wave Spectrum Nonlinearly Induced from Primordial Curvature Perturbations
• Model Independent Properties and Cosmological Implications of the Dilaton and Moduli Sectors of 4-d Strings
• Scientific Objectives of Einstein Telescope
• Cosmological Implications of Dynamical Supersymmetry Breaking
• KAGRA: 2.5 Generation Interferometric Gravitational Wave Detector
• Detecting the Cosmic Gravitational Wave Background with the Big Bang Observer
• Detector configuration of DECIGO/BBO and identification of cosmological neutron-star binaries
• Thermal Inflation and the Moduli Problem
• Upper Limits on the Isotropic Gravitational-Wave Background from Advanced LIGO's and Advanced Virgo's Third Observing Run
• Relativistic second-order perturbations of the Einstein-de Sitter Universe
• A template bank for gravitational waveforms from coalescing binary black holes: non-spinning binaries
• Gravitational wave background as a probe of the primordial black hole abundance
• Cosmological Constraints on Late-time Entropy Production
• Gravitational Waves from Coalescing Black Hole MACHO Binaries
• The NANOGrav 15-year Data Set: Constraints on Supermassive Black Hole Binaries from the Gravitational Wave Background
• A Cosmological Signature of the SM Higgs Instability: Gravitational Waves
• Challenges and Opportunities of Gravitational Wave Searches at MHz to GHz Frequencies
• Formation and Evolution of Primordial Black Hole Binaries in the Early Universe
• Black Hole Remnants and the Information Loss Paradox
• New Sensitivity Curves for Gravitational-Wave Signals from Cosmological Phase Transitions
• General Relativistic Dynamics of Irrotational Dust: Cosmological Implications
• Improved limits on the tensor-to-scalar ratio using BICEP and Planck
• Primordial gravitational waves, precisely: The role of thermodynamics in the Standard Model
• Inflationary Primordial Black Holes as All Dark Matter
• Gravitational waves from a universe filled with primordial black holes
• Quantum Compositeness of Gravity: Black Holes, AdS and Inflation
• Constraints on the Primordial Black Hole Abundance from the First Advanced LIGO Observation Run Using the Stochastic Gravitational-Wave Background
• Universal infrared scaling of gravitational wave background spectra
• Solar-Mass Primordial Black Holes Explain NANOGrav Hint of Gravitational Waves
• Multiband Gravitational-Wave Astronomy: Observing binary inspirals with a decihertz detector, B-DECIGO
• Dark Radiation and Superheavy Dark Matter from Black Hole Domination
• Gravitational Wave Production right after a Primordial Black Hole Evaporation
• Detecting High-Frequency Gravitational Waves with Microwave Cavities
• Gravitational-Wave Constraints on the Abundance of Primordial Black Holes
• Black Hole Binary Formation in the Expanding Universe --- Three Body Problem Approximation ---
• Gravitational Waves Induced by Scalar Perturbations with a Lognormal Peak
• Enhancement of Gravitational Waves Induced by Scalar Perturbations due to a Sudden Transition from an Early Matter Era to the Radiation Era
• Gravitational Waves Induced by Scalar Perturbations during a Gradual Transition from an Early Matter Era to the Radiation Era
• The primordial black hole formation criterion re-examined: parameterisation, timing, and the choice of window function
• Gravitational waves induced from primordial black hole fluctuations: The effect of an extended mass function
• Upper limits on the amplitude of ultra-high-frequency gravitational waves from graviton-photon mixing
• Black Hole Metamorphosis and Stabilization by Memory Burden
• Gravitational wave constraints on the primordial black hole dominated early universe
• Log-dependent slope of scalar induced gravitational waves in the infrared regions
• Potential of radio telescopes as high-frequency gravitational wave detectors
• Hunt for Light Primordial Black Hole Dark Matter with Ultra-High-Frequency Gravitational Waves
• Primordial Black Holes
• Probing GHz Gravitational Waves with Graviton-magnon Resonance
• Breakdown of Hawking Evaporation opens new Mass Window for Primordial Black Holes as Dark Matter Candidate
• The Detected Stochastic Gravitational Waves and Subsolar-Mass Primordial Black Holes
• Electromagnetic Antennas for the Resonant Detection of the Stochastic Gravitational Wave Background
• Gravitational waves from dark matter isocurvature
• Detecting Planetary-mass Primordial Black Holes with Resonant Electromagnetic Gravitational Wave Detectors
• Conversion of relic gravitational waves into photons in cosmological magnetic fields
• First cryogenic test operation of underground km-scale gravitational-wave observatory KAGRA
• Evaporation of Primordial Black Holes in the Early Universe: Mass and Spin Distributions
• Non-Thermal Corrections to Hawking Radiation Versus the Information Paradox
• Planck and BICEP/Keck Array 2018 constraints on primordial gravitational waves and perspectives for future B-mode polarization measurements
• Quantum effects on the evaporation of PBHs: contributions to dark matter
• A formalism for magnon gravitational wave detectors
• Probing modified Hawking evaporation with gravitational waves from the primordial black hole dominated universe
• Eluding the BBN constraints on the stable gravitino
• Exploring High Frequency Gravitational Waves with Magnons
• Memory burden effect mimics reheating signatures on SGWB from ultra-low mass PBH domination
• Comparing Instrument Spectral Sensitivity of Dissimilar Electromagnetic Haloscopes to Axion Dark Matter and High Frequency Gravitational Waves
• Gravitational wave hints black hole remnants as dark matter
• The Primordial Black Hole Abundance: The Broader, the Better
• Black Holes as Brains: Neural Networks with Area Law Entropy
• Limits on High-Frequency Gravitational Waves in Planetary Magnetospheres
• Gravitational wave search through electromagnetic telescopes
• Area Law Micro-State Entropy from Criticality and Spherical Symmetry
• Finding Critical States of Enhanced Memory Capacity in Attractive Cold Bosons
• The Timescales of Quantum Breaking
• Electromagnetic field in a cavity induced by gravitational waves

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• High-energy gamma-ray emission from memory-burdened primordial black holes
• Can a Breakdown of Hawking Evaporation Open a New Mass Window for Primordial Black Holes as Dark Matter?
• Primordial black holes save $R^2$ inflation
• Theoretical Radio Signals from Radio-Band Gravitational Waves Converted from the Neutron Star Magnetic Field
• Memory burden effect of regular primordial black holes