Regularization parameters for the self-force in Schwarzschild spacetime. II. Gravitational and electromagnetic cases

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 67, Issue 2, 2003, Pages

  Barack, Leor ^a   Ori, Amos ^b  

^a ALBERT EINSTEIN INSTITUT   (Germany)

^b TECHNION ISRAEL INSTITUTE OF TECHNOLOGY   (Israel)

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; CALCULATION; ELECTROMAGNETIC FIELD; ELEMENTARY PARTICLE; GRAVITY; MATHEMATICAL ANALYSIS; PHYSICS;

EID: 0037437917     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.67.024029     Document Type: Article

References (20)

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4. Phys. Rev. DL. Barack, 62, 084027 (2000).
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11. An alternative, elegant formulation of the self force was recently introduced in S. Detweiler and B. F. Whiting, Phys. Rev. D (to be published), gr-qc/0202086.
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13. A closely related calculation scheme, also employing a mode- sum decomposition (but relying on a different regularization scheme, based on the zeta-function regularization technique), was introduced in C. O. Lousto, Phys. Rev. Lett. 84, 5251 (2000).
14. A full implementation of the mode-sum scheme for the scalar self force is demonstrated in L. M. Burko, Phys. Rev. Lett. 84, 4529 (2000);
15. L. Barack and L. M. Burko, Phys. Rev. D 62, 084040 (2000);
16. Phys. Rev. DL. M. Burko, Y.-T. Liu, and Y. Soen, 63, 024015 (2001);
17. Phys. Rev. DL. M. Burko and Y.-T. Liu, 64, 024006 (2001). The mode-sum scheme has also been implemented in the gravitational case for radial 5 and circular 14 trajectories around a Schwarzschild black hole.
18. L. Barack and C. O. Lousto (work in progress).
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