A constraint on light primordial black holes from the interstellar medium temperature
arXiv:2007.07739 · doi:10.1093/mnras/stab1222
Abstract
Primordial black holes are a viable dark matter candidate. They decay via Hawking evaporation. Energetic particles from the Hawking radiation interact with interstellar gas, depositing their energy as heat and ionization. For a sufficiently high Hawking temperature, fast electrons produced by black holes deposit a substantial fraction of energy as heat through the Coulomb interaction. Using the dwarf galaxy Leo T, we place an upper bound on the fraction of primordial black hole dark matter. For , our bound is competitive with or stronger than other bounds.
arXiv comment10 pages, 5 figures; discussion extended, minor typos/numerical error corrected, conclusion unchanged, matches the version accepted for publication in MNRAS
References in corpus (50)
- The chemical composition of the Sun
- The Aquarius Project: the subhalos of galactic halos
- An atomic and molecular database for analysis of submillimetre line observations
- Radiative transfer in a clumpy universe: IV. New synthesis models of the cosmic UV/X-ray background
- New cosmological constraints on primordial black holes
- A Unified Representation of Gas-Phase Element Depletions in the Interstellar Medium
- The Universal Stellar Mass-Stellar Metallicity Relation for Dwarf Galaxies
- Gas-to-Dust mass ratios in local galaxies over a 2 dex metallicity range
- The Evolution of the Elemental Abundances in the Gas and Dust Phases of the Galaxy
- The Faintest Dwarf Galaxies
- Multi-Element Abundance Measurements from Medium-Resolution Spectra. III. Metallicity Distributions of Milky Way Dwarf Satellite Galaxies
- Discovery of an Unusual Dwarf Galaxy in the Outskirts of the Milky Way
- The delay-time distribution of type-Ia supernovae from Sloan II
- Primordial black holes as a dark matter candidate are severely constrained by the Galactic Center 511 keV gamma-ray line
- Uncertainties in H2 and HD Chemistry and Cooling and their Role in Early Structure Formation
- INTEGRAL constraints on primordial black holes and particle dark matter
- Delay Time Distribution Measurement of Type Ia Supernovae by the Subaru/XMM-Newton Deep Survey and Implications for the Progenitor
- Voyager 1 Further Constrain Primordial Black Holes as Dark Matter
- BlackHawk v2.0: A public code for calculating the Hawking evaporation spectra of any black hole distribution
- Neutrino and Positron Constraints on Spinning Primordial Black Hole Dark Matter
- Constraining primordial black hole abundance with the Galactic 511 keV line
- The Fate of the First Galaxies. I. Self-Consistent Cosmological Simulations with Radiative Transfer
- Constraints on primordial black holes from Galactic gamma-ray background
- 21cm Limits on Decaying Dark Matter and Primordial Black Holes
- The Local Group dwarf Leo T: HI on the brink of star formation
- Connecting the first galaxies with ultra faint dwarfs in the Local Group: chemical signatures of Population~III stars
- Atomic Hydrogen Gas in Dark-Matter Minihalos and the Compact High Velocity Clouds
- Planck Constraint on Relic Primordial Black Holes
- Secondary ionization and heating by fast electrons
- Magnetic fields in Local Group dwarf irregulars
- Constraining primordial black hole masses with the isotropic gamma ray background
- The Distribution of Alpha Elements in Ultra-Faint Dwarf Galaxies
- Exotic energy injection with ExoCLASS: Application to the Higgs portal model and evaporating black holes
- The structural properties and star formation history of Leo T from deep LBT photometry
- CMB and BBN constraints on evaporating primordial black holes revisited
- Thermal Phases of the Neutral Atomic Interstellar Medium -- from Solar Metallicity to Primordial Gas
- X-ray and gamma-ray limits on the primordial black hole abundance from Hawking radiation
- The Star Formation History of Leo T from Hubble Space Telescope Imaging
- Electron-impact excitation of neutral oxygen
- Galactic Center Gas Clouds and Novel Bounds on Ultra-Light Dark Photon, Vector Portal, Strongly Interacting, Composite, and Super-Heavy Dark Matter
- Constraining Primordial Black Holes with Dwarf Galaxy Heating
- Calorimetric Dark Matter Detection With Galactic Center Gas Clouds
- Deep neutral hydrogen observations of Leo T with the Westerbork Synthesis Radio Telescope
- Ultra-Compact High Velocity Clouds as Minihalos and Dwarf Galaxies
- Constraining Primordial Black Hole Fraction at the Galactic Centre using radio observational data
- Stout: Cloudy's Atomic and Molecular Database
- Star Formation in Ultrafaint Dwarfs: Continuous or Single-age Bursts?
- Energy levels, radiative rates and electron impact excitation rates for transitions in Si II
- Comment on the paper "Calorimetric Dark Matter Detection with Galactic Center Gas Clouds"
- Simulating the formation of massive seed black holes in the early Universe. III: The influence of X-rays
Cited by in corpus (43)
- Constraints on Primordial Black Holes
- Direct Detection of Hawking Radiation from Asteroid-Mass Primordial Black Holes
- Constraining primordial black holes as dark matter using the global 21-cm signal with X-ray heating and excess radio background
- Near future MeV telescopes can discover asteroid-mass primordial black hole dark matter
- Low Mass Black Holes from Dark Core Collapse
- Hunt for Light Primordial Black Hole Dark Matter with Ultra-High-Frequency Gravitational Waves
- Breakdown of Hawking Evaporation opens new Mass Window for Primordial Black Holes as Dark Matter Candidate
- Doubly peaked induced stochastic gravitational wave background : Testing baryogenesis from primordial black holes
- Strong constraints on decay and annihilation of dark matter from heating of gas-rich dwarf galaxies
- Strong constraints on primordial black hole dark matter from 16 years of INTEGRAL/SPI observations
- The Primordial Black Holes that Disappeared: Connections to Dark Matter and MHz-GHz Gravitational Waves
- Gas Heating from Spinning and Non-Spinning Evaporating Primordial Black Holes
- Detecting Composite Dark Matter with Long Range and Contact Interactions in Gas Clouds
- Interstellar Gas Heating by Primordial Black Holes
- Primordial Black Hole Dark Matter evaporating on the Neutrino Floor
- Signatures of primordial black hole dark matter at DUNE and THEIA
- Hunting for Dark Matter and New Physics with GECCO
- Ultra-High-Energy Neutrinos from Primordial Black Holes
- Constraining spinning primordial black holes with global 21-cm signal
- Detecting Axion-Like Particles with Primordial Black Holes
- Primordial Black Hole Dark Matter in the Context of Extra Dimensions
- Constraining axion and compact dark matter with interstellar medium heating
- Constraints on the abundance of primordial black holes with different mass distributions from lensing of fast radio bursts
- Impacts of Jets and Winds From Primordial Black Holes
- Search for boosted keV-MeV light dark matter particles from evaporating primordial black holes at the CDEX-10 experiment
- Future Constraints on Primordial Black Holes from XGIS-THESEUS
- The cosmic coincidences of primordial-black-hole dark matter
- Impact of Primordial Black Hole Dark Matter on Gas Properties at Very High Redshift: A Semi-Analytical Model
- Stronger Constraints on Primordial Black Holes as Dark Matter Derived from the Thermal Evolution of the Intergalactic Medium over the Last Twelve Billion Years
- Significance of soft-scale breaking on primordial black hole production in Coleman-Weinberg type supercooling-phase transition
- Picolensing as a Probe of Primordial Black Hole Dark Matter
- The Milky Way satellite galaxy Leo T: A perturbed cored dwarf
- Constraints on primordial black holes from interstellar dust temperature in the Galaxy
- Linearity: galaxy formation encounters an unanticipated empirical relation
- Limits on primordial black holes detectability with Isatis: A BlackHawk tool
- Supersymmetric Horizons at the Edge of Effective Field Theory
- Physics Beyond the Standard Model with BlackHawk v2.0
- Unified Gas Heating Constraints on Extended Dark Matter Compact Objects
- A new probe of dark matter-baryon interactions in compact stellar systems
- Planck isocurvature constraint on primordial black holes lighter than a kiloton
- Correlating Gravitational Wave and Gamma-ray Signals from Primordial Black Holes
- Sensitivities on non-spinning and spinning primordial black hole dark matter with global 21 cm troughs
- Search for Dark Matter Annihilation and Decay with H Line Emission