On quantum resonances in stationary geometries

Lettere al Nuovo Cimento (1971-1985) - Tập 15 - Trang 257-262 - 2007
T. Damour1,2, N. Deruelle3, R. Ruffini4,2
1Joseph Henry Physical Laboratories, Princeton
2Physics Department, University of Western Australia, Nedlands
3Institute of Theoretical Astronomy, Cambridge, England
4Institute for Advanced Study, Princeton

Tài liệu tham khảo

See,e. g., Proceeding of the Marcel Grossman Meeting, edited byR. Ruffini (Amsterdam, 1976).

See,e. g.,J. A. Wheeler:Transcending the law of conservation of leptons, inQuaderno No. 157, Accademia Nazionale dei Lincei (Roma, 1971), p. 133.

N. Deruelle andR. Ruffini:Phys. Lett.,52 B, 437 (1974); in this paper the positive- and negative-root solutions introduced byD. Christodoulou andR. Ruffini:Phys. Rev. D,4, 3552 (1971), are identified with the classical limits of the positive- and negative-energy states of a relativistic quantized field. Sce alsoT. Damour:Lett. Nuovo Cimento,12, 315 (1975), where this correspondence is made manifest by a suitable choice of the co-ordinates.

See,e. g.,T. Damour andR. Ruffini:Phys. Rev. Lett.,35, 463 (1975);N. Deruelle andR. Ruffini:Phys. Lett.,58 B, (1975) and references mentioned there.

See,e.g.,B. Carter:Comm. Math. Phys.,10, 280 (1968);D. Brill, P. M. Chrzanowski, C. M. Pereira, E. D. Fackerell andJ. R. Ipser:Phys. Rev. D,5, 1913 (1972).

J. Meixner andF. W. Schärfke:Mathieusche Funktionen und Sphäroidfunktionen (Berlin, 1954).

G. Gamow:Zeits. Phys.,51 204 (1928). See alsoG. Gamow:Structure of Atomic Nuclei and Nuclear Transformations (Oxford, 1937).

There is one important difference between the study of the resonances of a nucleus and the resonances of a quantized field around a collapsed object: the leakage in the case of a nucleus occurs always toward spatial infinity (r→∞) while in the case of a collapsed object occurs toward the horizon (r→r + orx→−∞).

D. Christodoulou andR. Ruffini:On the electrodynamics of collapsed objects, inBlack Holes, edited byB. de Witt andC. de Witt (London, 1973).

B. Carter: inBlack Holes, edited byB. de Witt andC. de Witt (London, 1973).

See,e.g.,G. Breit andF. L. Yost:Phys. Rev.,48, 203 (1935).