Evaporating black holes: constraints on anomalous emission mechanisms
arXiv:2107.14244 · doi:10.1103/PhysRevD.104.124024
Abstract
Hawking radiation of astrophysical black holes is minute and thought to be unobservable. However, different mechanisms could contribute to an anomalously high emission rate: extra dimensions, new "dark" families of bosons or fermions, or a lower fundamental Planck scale. Do black holes flood the Universe with gravitational waves via mass loss? Here, we show that the formation of black hole binaries and the absence of a stochastic background of gravitational waves can limit the emission rate to , seven orders of magnitude more stringent than bounds from resolvable inspiralling binaries.
arXiv comment5 pages, 2 figures, 1 table
References in corpus (50)
- A Large Mass Hierarchy from a Small Extra Dimension
- The Hierarchy Problem and New Dimensions at a Millimeter
- New Dimensions at a Millimeter to a Fermi and Superstrings at a TeV
- String Axiverse
- Characterization of the LIGO detectors during their sixth science run
- Exploring the Sensitivity of Next Generation Gravitational Wave Detectors
- Science Case for the Einstein Telescope
- Compact Remnant Mass Function: Dependence on the Explosion Mechanism and Metallicity
- A Comprehensive Study of Binary Compact Objects as Gravitational Wave Sources: Evolutionary Channels, Rates, and Physical Properties
- The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars
- On the properties of massive Population III stars and metal-free stellar populations
- Detecting a stochastic background of gravitational radiation: Signal processing strategies and sensitivities
- Black holes, gravitational waves and fundamental physics: a roadmap
- Tests of General Relativity with GW170817
- The history of star formation in a LCDM universe
- Sensitivity curves for searches for gravitational-wave backgrounds
- Spectroscopy of the quantum black hole
- Black Holes and Large N Species Solution to the Hierarchy Problem
- Interacting Spin-2 Fields
- Stochastic and resolvable gravitational waves from ultralight bosons
- Essentials of Blackfold Dynamics
- Neutron Star Extreme Matter Observatory: A kilohertz-band gravitational-wave detector in the global network
- Limits on the number of spacetime dimensions from GW170817
- Instability and new phases of higher-dimensional rotating black holes
- New experimental limits on non-Newtonian forces in the micrometer-range
- X-Rays from Isolated Black Holes in the Milky Way
- The Impact of Star Formation and Gamma-Ray Burst Rates at High Redshift on Cosmic Chemical Evolution and Reionization
- Gravitational wave production by Hawking radiation from rotating primordial black holes
- Gravity and large black holes in Randall-Sundrum II braneworlds
- Probing Fundamental Physics with Gravitational Waves: The Next Generation
- A first search for a stochastic gravitational-wave background from ultralight bosons
- Potential gravitational-wave signatures of quantum gravity
- Eccentricity evolution of compact binaries and applications to gravitational-wave physics
- Modeling and searching for a stochastic gravitational-wave background from ultralight vector bosons
- The coupling to matter in Massive, Bi- and Multi-Gravity
- Probing the size of extra dimension with gravitational wave astronomy
- Nonviolent unitarization: basic postulates to soft quantum structure of black holes
- Astronomical tests for quantum black hole structure
- Gravitational waves and higher dimensions: Love numbers and Kaluza-Klein excitations
- Large Randall-Sundrum II Black Holes
- Probing ultralight dark matter with future ground-based gravitational-wave detectors
- Ultralight Fermionic Dark Matter
- New solar metallicity measurements
- Constraining the braneworld with gravitational wave observations
- Constraints on Braneworld Gravity Models from a Kinematic Limit on the Age of the Black Hole XTE J1118+480
- Shrinking the Braneworld: Black Hole in a Globular Cluster
- A Precision Test for an Extra Spatial Dimension Using Black Hole--Pulsar Binaries
- Spherically symmetric vacuum solutions arising from trace dynamics modifications to gravitation
- Composition of an Emission Line System in Black Hole Host Globular Cluster RZ2109
- Upper limits on the temperature of inspiraling astrophysical black holes