| TYC, Tomáš, H L DAO a Aaron James DANNER. Absolute optical instruments without spherical symmetry. Phys. Rev. A. USA: The American Phys. Society, 2015, roč. 92, č. 5, s. "nestránkováno", 6 s. ISSN 1050-2947. Dostupné z: https://dx.doi.org/10.1103/PhysRevA.92.053827. |
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@article{1336245,
author = {Tyc, Tomáš and Dao, H L and Danner, Aaron James},
article_location = {USA},
article_number = {5},
doi = {http://dx.doi.org/10.1103/PhysRevA.92.053827},
keywords = {absolute optical instruments; refractive index; Cartesian coordinates},
language = {eng},
issn = {1050-2947},
journal = {Phys. Rev. A},
title = {Absolute optical instruments without spherical symmetry},
url = {http://journals.aps.org/pra/abstract/10.1103/PhysRevA.92.053827},
volume = {92},
year = {2015}
}
TY - JOUR
ID - 1336245
AU - Tyc, Tomáš - Dao, H L - Danner, Aaron James
PY - 2015
TI - Absolute optical instruments without spherical symmetry
JF - Phys. Rev. A
VL - 92
IS - 5
SP - "nestránkováno"
EP - "nestránkováno"
PB - The American Phys. Society
SN - 10502947
KW - absolute optical instruments
KW - refractive index
KW - Cartesian coordinates
UR - http://journals.aps.org/pra/abstract/10.1103/PhysRevA.92.053827
L2 - http://journals.aps.org/pra/abstract/10.1103/PhysRevA.92.053827
N2 - Until now, the known set of absolute optical instruments has been limited to those containing high levels of symmetry. Here, we demonstrate a method of mathematically constructing refractive index profiles that result in asymmetric absolute optical instruments. The method is based on the analogy between geometrical optics and classical mechanics and employs Lagrangians that separate in Cartesian coordinates. In addition, our method can be used to construct the index profiles of most previously known absolute optical instruments, as well as infinitely many different ones.
ER -
TYC, Tomáš, H L DAO a Aaron James DANNER. Absolute optical instruments without spherical symmetry. \textit{Phys. Rev. A}. USA: The American Phys. Society, 2015, roč.~92, č.~5, s.~''nestránkováno'', 6 s. ISSN~1050-2947. Dostupné z: https://dx.doi.org/10.1103/PhysRevA.92.053827.
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