Fourth order perturbative expansion for the Casimir energy with a slightly deformed plate
We apply a perturbative approach to evaluate the Casimir energy for a massless real scalar field in 3+1 dimensions, subject to Dirichlet boundary conditions on two surfaces. One of the surfaces is assumed to be flat, while the other corresponds to a small deformation, described by a single function...
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2012
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| Acceso en línea: | Registro en Scopus DOI Handle Registro en la Biblioteca Digital |
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| LEADER | 04880caa a22005297a 4500 | ||
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| 001 | PAPER-23293 | ||
| 003 | AR-BaUEN | ||
| 005 | 20250327092357.0 | ||
| 008 | 190411s2012 xx ||||fo|||| 00| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-84871060913 | |
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| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 100 | 1 | |a Fosco, César Daniel | |
| 245 | 1 | 0 | |a Fourth order perturbative expansion for the Casimir energy with a slightly deformed plate |
| 260 | |c 2012 | ||
| 270 | 1 | 0 | |m Fosco, C.D.; Centro Atómico Bariloche, Comisión Nacional de Energía Atómica, R8402AGP Bariloche, Argentina |
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| 504 | |a Wu, H.Y., Schaden, M., (2012) Phys. Rev. D, 85, p. 045008. , PRVDAQ 1550-7998 10.1103/PhysRevD.85.045008 | ||
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| 504 | |a Fosco, C.D., Lombardo, F.C., Mazzitelli, F.D., (2011) Phys. Rev. D, 84, p. 105031. , PRVDAQ 1550-7998 10.1103/PhysRevD.84.105031 | ||
| 504 | |a Fosco, C.D., Lombardo, F.C., Mazzitelli, F.D., (2012) Phys. Rev. D, 85, p. 125037. , PRVDAQ 1550-7998 10.1103/PhysRevD.85.125037 | ||
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| 504 | |a Fosco, C.D., Lombardo, F.C., Mazzitelli, F.D., (2012) Phys. Rev. D, 86, p. 045021. , PRVDAQ 1550-7998 10.1103/PhysRevD.86.045021 | ||
| 506 | |2 openaire |e Política editorial | ||
| 520 | 3 | |a We apply a perturbative approach to evaluate the Casimir energy for a massless real scalar field in 3+1 dimensions, subject to Dirichlet boundary conditions on two surfaces. One of the surfaces is assumed to be flat, while the other corresponds to a small deformation, described by a single function η, of a flat mirror. The perturbative expansion is carried out up to the fourth order in the deformation η, and the results are applied to the calculation of the Casimir energy for corrugated mirrors in front of a plane. We also reconsider the proximity force approximation within the context of this expansion. © 2012 American Physical Society. |l eng | |
| 593 | |a Centro Atómico Bariloche, Comisión Nacional de Energía Atómica, R8402AGP Bariloche, Argentina | ||
| 593 | |a Instituto Balseiro, Universidad Nacional de Cuyo, R8402AGP Bariloche, Argentina | ||
| 593 | |a Departamento de Física Juan José Giambiagi, IFIBA CONICET-UBA, Ciudad Universitaria, Pabellón I, 1428 Buenos Aires, Argentina | ||
| 700 | 1 | |a Lombardo, F.C. | |
| 700 | 1 | |a Mazzitelli, F.D. | |
| 773 | 0 | |d 2012 |g v. 86 |k n. 12 |p Phys Rev D Part Fields Gravit Cosmol |x 15507998 |t Physical Review D - Particles, Fields, Gravitation and Cosmology | |
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| 856 | 4 | 0 | |u https://doi.org/10.1103/PhysRevD.86.125018 |y DOI |
| 856 | 4 | 0 | |u https://hdl.handle.net/20.500.12110/paper_15507998_v86_n12_p_Fosco |y Handle |
| 856 | 4 | 0 | |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_15507998_v86_n12_p_Fosco |y Registro en la Biblioteca Digital |
| 961 | |a paper_15507998_v86_n12_p_Fosco |b paper |c PE | ||
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