Abstract
A black hole can carry quantum numbers that are not associated with massless gauge fields, contrary to the spirit of the no-hair theorems. In the Higgs phase of a gauge theory, electric charge on a black hole generates a nonzero electric field outside the event horizon. This field is nonperturbative in Latin small letter h with stroke and is exponentially screened far from the hole. It arises from the cloud of virtual cosmic strings that surround the black hole. In the confinement phase, a magnetic charge on a black hole generates a classical field that is screened at long range by nonperturbative effects. Despite the sharp difference in their formal descriptions, the electric and magnetic cases are closely similar physically.
Original language | English (US) |
---|---|
Pages (from-to) | 1975-1978 |
Number of pages | 4 |
Journal | Physical Review Letters |
Volume | 67 |
Issue number | 15 |
DOIs | |
State | Published - 1991 |
Externally published | Yes |
ASJC Scopus subject areas
- Physics and Astronomy(all)