Propagating parabolic rotational beams, new family of accelerated beams
A novel class of structured propagating waves with parabolic rotational symmetry is introduced for the first time. These are described by exact solutions of the non-paraxial Helmholtz equation. As a result of the separability of the Helmholtz equation, the intensity of these wavefields remains invar...
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| Format: | Article |
| Language: | English |
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EDP Sciences
2024-01-01
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| Series: | EPJ Web of Conferences |
| Online Access: | https://www.epj-conferences.org/articles/epjconf/pdf/2024/19/epjconf_eosam2024_01013.pdf |
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| _version_ | 1846139398225133568 |
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| author | Espíndola-Ramos Ernesto Gómez-Correa Jesús Emmanuel Hernández-Nolasco José Adán Chávez-Cerda Sabino |
| author_facet | Espíndola-Ramos Ernesto Gómez-Correa Jesús Emmanuel Hernández-Nolasco José Adán Chávez-Cerda Sabino |
| author_sort | Espíndola-Ramos Ernesto |
| collection | DOAJ |
| description | A novel class of structured propagating waves with parabolic rotational symmetry is introduced for the first time. These are described by exact solutions of the non-paraxial Helmholtz equation. As a result of the separability of the Helmholtz equation, the intensity of these wavefields remains invariant while propagating along parabolic trajectories, thus exhibiting apparent acceleration. We will show that superposition of the fundamental traveling waves can present parabolic, spherical or even rectilinear propagation. |
| format | Article |
| id | doaj-art-3fd7adbef33d427288e892dda5fd0b03 |
| institution | Kabale University |
| issn | 2100-014X |
| language | English |
| publishDate | 2024-01-01 |
| publisher | EDP Sciences |
| record_format | Article |
| series | EPJ Web of Conferences |
| spelling | doaj-art-3fd7adbef33d427288e892dda5fd0b032024-12-06T10:18:44ZengEDP SciencesEPJ Web of Conferences2100-014X2024-01-013090101310.1051/epjconf/202430901013epjconf_eosam2024_01013Propagating parabolic rotational beams, new family of accelerated beamsEspíndola-Ramos Ernesto0Gómez-Correa Jesús Emmanuel1Hernández-Nolasco José Adán2Chávez-Cerda Sabino3Instituto Nacional de Astrofísica, Óptica y Electrónica, Calle Luis Enrique Erro 1, Santa María TonantzintlaInstituto Nacional de Astrofísica, Óptica y Electrónica, Calle Luis Enrique Erro 1, Santa María TonantzintlaAcademic Division of Sciences and Information Technology, Juarez Autonomous University of TabascoInstituto Nacional de Astrofísica, Óptica y Electrónica, Calle Luis Enrique Erro 1, Santa María TonantzintlaA novel class of structured propagating waves with parabolic rotational symmetry is introduced for the first time. These are described by exact solutions of the non-paraxial Helmholtz equation. As a result of the separability of the Helmholtz equation, the intensity of these wavefields remains invariant while propagating along parabolic trajectories, thus exhibiting apparent acceleration. We will show that superposition of the fundamental traveling waves can present parabolic, spherical or even rectilinear propagation.https://www.epj-conferences.org/articles/epjconf/pdf/2024/19/epjconf_eosam2024_01013.pdf |
| spellingShingle | Espíndola-Ramos Ernesto Gómez-Correa Jesús Emmanuel Hernández-Nolasco José Adán Chávez-Cerda Sabino Propagating parabolic rotational beams, new family of accelerated beams EPJ Web of Conferences |
| title | Propagating parabolic rotational beams, new family of accelerated beams |
| title_full | Propagating parabolic rotational beams, new family of accelerated beams |
| title_fullStr | Propagating parabolic rotational beams, new family of accelerated beams |
| title_full_unstemmed | Propagating parabolic rotational beams, new family of accelerated beams |
| title_short | Propagating parabolic rotational beams, new family of accelerated beams |
| title_sort | propagating parabolic rotational beams new family of accelerated beams |
| url | https://www.epj-conferences.org/articles/epjconf/pdf/2024/19/epjconf_eosam2024_01013.pdf |
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