Casimir energies in light of quantum field theory

Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

Volumn 572, Issue 3-4, 2003, Pages 196-201

  Graham, N ^a   Jaffe, R L ^b   Khemani, V ^b   Quandt, M ^b   Scandurra, M ^b   Weigel, H ^c  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^c UNIVERSITY OF TÜBINGEN   (Germany)

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; CASIMIR ENERGY; DENSITY; ENERGY; FORCE; QUANTUM FIELD THEORY; QUANTUM THEORY; SURFACE PROPERTY; SURFACE TENSION;

EID: 0347076370     PISSN: 03702693     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.physletb.2003.03.003     Document Type: Article

References (25)

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15. The energy density away from S is interesting in its own right, since it can be negative, it may induce interesting effects in general relativity: F.J. Tipler, Phys. Rev. Lett. 37 (1976) 879; S.W. Hawking, Phys. Rev. D 46 (1992) 603; L.H. Ford, T.A. Roman, Phys. Rev. D 51 (1995) 4277; K.D. Olum, Phys. Rev. Lett. 81 (1998) 3567, gr-qc/9805003; K.D. Olum, N. Graham, gr-qc/0205134.
16. The energy density away from S is interesting in its own right, since it can be negative, it may induce interesting effects in general relativity: F.J. Tipler, Phys. Rev. Lett. 37 (1976) 879; S.W. Hawking, Phys. Rev. D 46 (1992) 603; L.H. Ford, T.A. Roman, Phys. Rev. D 51 (1995) 4277; K.D. Olum, Phys. Rev. Lett. 81 (1998) 3567, gr-qc/9805003; K.D. Olum, N. Graham, gr-qc/0205134.
17. The energy density away from S is interesting in its own right, since it can be negative, it may induce interesting effects in general relativity: F.J. Tipler, Phys. Rev. Lett. 37 (1976) 879; S.W. Hawking, Phys. Rev. D 46 (1992) 603; L.H. Ford, T.A. Roman, Phys. Rev. D 51 (1995) 4277; K.D. Olum, Phys. Rev. Lett. 81 (1998) 3567, gr-qc/9805003; K.D. Olum, N. Graham, gr-qc/0205134.
18. The energy density away from S is interesting in its own right, since it can be negative, it may induce interesting effects in general relativity: F.J. Tipler, Phys. Rev. Lett. 37 (1976) 879; S.W. Hawking, Phys. Rev. D 46 (1992) 603; L.H. Ford, T.A. Roman, Phys. Rev. D 51 (1995) 4277; K.D. Olum, Phys. Rev. Lett. 81 (1998) 3567, gr-qc/9805003; K.D. Olum, N. Graham, gr-qc/0205134.
19. The energy density away from S is interesting in its own right, since it can be negative, it may induce interesting effects in general relativity: F.J. Tipler, Phys. Rev. Lett. 37 (1976) 879; S.W. Hawking, Phys. Rev. D 46 (1992) 603; L.H. Ford, T.A. Roman, Phys. Rev. D 51 (1995) 4277; K.D. Olum, Phys. Rev. Lett. 81 (1998) 3567, gr-qc/9805003; K.D. Olum, N. Graham, gr-qc/0205134.
20. For a comprehensive review see: N. Graham, R.L. Jaffe, H. Weigel, Int. J. Mod. Phys. A 17 (2002) 846, hep-th/0201148.
21. E. Farhi, N. Graham, P. Haagensen, R.L. Jaffe, Phys. Lett. B 427 (1998) 334, hep-th/9802015; E. Farhi, N. Graham, R.L. Jaffe, H. Weigel, Phys. Lett. B 475 (2000) 335, hep-th/9912283; E. Farhi, N. Graham, R.L. Jaffe, H. Weigel, Nucl. Phys. B 585 (2000) 443, hep-th/0003144; E. Farhi, N. Graham, R.L. Jaffe, H. Weigel, Nucl. Phys. B 630 (2002) 241, hep-th/0112217.
22. E. Farhi, N. Graham, P. Haagensen, R.L. Jaffe, Phys. Lett. B 427 (1998) 334, hep-th/9802015; E. Farhi, N. Graham, R.L. Jaffe, H. Weigel, Phys. Lett. B 475 (2000) 335, hep-th/9912283; E. Farhi, N. Graham, R.L. Jaffe, H. Weigel, Nucl. Phys. B 585 (2000) 443, hep-th/0003144; E. Farhi, N. Graham, R.L. Jaffe, H. Weigel, Nucl. Phys. B 630 (2002) 241, hep-th/0112217.
23. E. Farhi, N. Graham, P. Haagensen, R.L. Jaffe, Phys. Lett. B 427 (1998) 334, hep-th/9802015; E. Farhi, N. Graham, R.L. Jaffe, H. Weigel, Phys. Lett. B 475 (2000) 335, hep-th/9912283; E. Farhi, N. Graham, R.L. Jaffe, H. Weigel, Nucl. Phys. B 585 (2000) 443, hep-th/0003144; E. Farhi, N. Graham, R.L. Jaffe, H. Weigel, Nucl. Phys. B 630 (2002) 241, hep-th/0112217.
24. E. Farhi, N. Graham, P. Haagensen, R.L. Jaffe, Phys. Lett. B 427 (1998) 334, hep-th/9802015; E. Farhi, N. Graham, R.L. Jaffe, H. Weigel, Phys. Lett. B 475 (2000) 335, hep-th/9912283; E. Farhi, N. Graham, R.L. Jaffe, H. Weigel, Nucl. Phys. B 585 (2000) 443, hep-th/0003144; E. Farhi, N. Graham, R.L. Jaffe, H. Weigel, Nucl. Phys. B 630 (2002) 241, hep-th/0112217.
25. K.A. Milton, hep-th/0210081.