Abstract
We calculate the flux from a spherical mirror which is expanding or contracting with nearly uniform acceleration. The flux at an exterior point (which could in principle be a functional of the mirror’s past history) is actually found to be a local function, depending on the first and second time derivatives of acceleration at the retarded time.
- Received 20 April 1999
DOI:https://doi.org/10.1103/PhysRevD.60.084003
©1999 American Physical Society
