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Effective photon mass from black-hole formation

Emelyanov, Slava

We compute the value of effective photon mass mγ at one-loop level in QED in the background of small (1010 g≲M≪1016 g) spherically symmetric black hole in asymptotically flat spacetime. This effect is associated with the modification of electron/positron propagator in presence of event horizon. Physical manifestations of black-hole environment are compared with those of hot neutral plasma. We estimate the distance to the nearest black hole from the upper bound on mγ obtained in the Coulomb-law test. We also find that corrections to electron mass me and fine structure constant α at one-loop level in QED are negligible in the weak gravity regime.

Zugehörige Institution(en) am KIT Institut für Theoretische Physik (ITP)
Publikationstyp Zeitschriftenaufsatz
Jahr 2017
Sprache Englisch
Identifikator DOI: 10.1016/j.nuclphysb.2017.03.016
ISSN: 0550-3213, 1873-1562
URN: urn:nbn:de:swb:90-689948
KITopen ID: 1000068994
Erschienen in Nuclear physics <Amsterdam> / B
Band 919
Seiten 110-122
Lizenz CC BY 4.0: Creative Commons Namensnennung 4.0 International
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