Annihilating Mini BHs: Difference between revisions
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|Progenitor = Annihilating Mini BHs | |Progenitor = Annihilating Mini BHs | ||
|Type = Single | |Type = Single | ||
|EnergyMechanism = | |EnergyMechanism = - | ||
|EmissionMechanism = | |EmissionMechanism = - | ||
|LFRadioCounterpart = | |LFRadioCounterpart = - | ||
|HFRadioCounterpart = | |HFRadioCounterpart = - | ||
|MicrowaveCounterpart = | |MicrowaveCounterpart = - | ||
|THzCounterpart = | |THzCounterpart = - | ||
|OIRCounterpart = | |OIRCounterpart = - | ||
|XrayCounterpart = | |XrayCounterpart = - | ||
|GammarayCounterpart = | |GammarayCounterpart = - | ||
|GWCounterpart = | |GWCounterpart = - | ||
|NeutrinoCounterpart = | |NeutrinoCounterpart = - | ||
|References = https://arxiv.org/pdf/1206.4135.pdf | |References = https://arxiv.org/pdf/1206.4135.pdf | ||
|Comments = None | |Comments = None | ||
Revision as of 08:13, 9 October 2018
| Category | Progenitor | Type | Energy Mechanism | Emission Mechanism | Counterparts | References | Brief Comments | ||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| LF Radio | HF Radio | Microwave | Terahertz | Optical/IR | X-rays | Gamma-rays | Gravitational Waves | Neutrinos | |||||||
| Void | Annihilating Mini BHs | Single | - | - | - | - | - | - | - | - | - | - | - | https://arxiv.org/pdf/1206.4135.pdf | None |
Definitions: LF Radio (3 MHz to 3 GHz); HF Radio (3 GHz to 30 GHz); Microwave (30 to 300 GHz)
Model Description
When a BH evaporates to some critical mass, a fireball of e+− pairs can be created. The relativistic pairs expand into the magnetic field of the surrounding ISM, which, for a sufficiently low mass BH, could produce a emission consistent with an FRB.
Observational Constraints
In this scenario the inferred distance to the Lorimer burst is calculated to be 200 kpc -- far too little, thus making this theory inviable.