Creation of fermions by rotating charged black-holes

When studying the problem of linear stability, such growing modes therefore cannot appear as the asymptotic behavior of a gravitational wave; in fact, one can argue, as we shall do

This text is based on notes (taken by R. Thangadurai) of three courses given at Goa University on December 15 and 16, 2014, on Algebraic independence of Periods of Elliptic

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In the case of massless fields, we prove the existence and asymptotic completeness of classical wave operators at the horizon of the Black-Hole and at infinity.. On

tational waves are conveniently studied by means of the null tetrad formalism introduced by Newman and Penrose [19].. 165 SCATTERING OF A PLANE GRAVITATIONAL WAVE BY A