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| Main Authors: | , , , , |
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| Format: | Preprint |
| Published: |
2025
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| Subjects: | |
| Online Access: | https://arxiv.org/abs/2503.22053 |
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| _version_ | 1866912298780590080 |
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| author | Otero, Oswaldo López, Jesús E. Tsygankov, P. Páez-González, Carlos J. Orozco, E. A. |
| author_facet | Otero, Oswaldo López, Jesús E. Tsygankov, P. Páez-González, Carlos J. Orozco, E. A. |
| contents | This study investigates the autoresonant acceleration of electrons using the GYRAC mechanism in a cylindrical cavity excited in the TE$_{011}$ microwave mode, under a slowly increasing external magnetic field. The acceleration process is driven by the interaction between electrons and the right-hand circularly polarized (RHP) component of the electric field, maintained in phase through electron cyclotron resonance (ECR). A simplified single-particle model and numerical simulations based on the relativistic Newton-Lorentz equation were employed to evaluate particle dynamics under different values of the magnetic field growth parameter $ α$.
The results demonstrate that efficient trapping and energy transfer can be achieved for appropriate values of $ α$, and that the spatial non-uniformity of the TE$_{011}$ mode introduces critical sensitivity to initial particle positioning. The study further identifies a ring-shaped region in which electrons are consistently captured in the GYRAC regime, and shows how the evolution of the Larmor radius, phase shift, and energy distribution depends on the electromagnetic configuration.
Simulations involving disk-like and ring-like electron clouds reveal the fraction of captured, escaped, and uncaptured particles, confirming that precise control of the magnetic field variation is essential to optimize the efficiency of the acceleration process. These findings provide a basis for future self-consistent plasma simulations and support the development of compact radiation sources based on GYRAC-TE$_{011}$ acceleration. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2503_22053 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Electron Acceleration by the Axisymmetric TE$_{011}$ Mode in a Slowly Varying External Magnetic Field Otero, Oswaldo López, Jesús E. Tsygankov, P. Páez-González, Carlos J. Orozco, E. A. Accelerator Physics This study investigates the autoresonant acceleration of electrons using the GYRAC mechanism in a cylindrical cavity excited in the TE$_{011}$ microwave mode, under a slowly increasing external magnetic field. The acceleration process is driven by the interaction between electrons and the right-hand circularly polarized (RHP) component of the electric field, maintained in phase through electron cyclotron resonance (ECR). A simplified single-particle model and numerical simulations based on the relativistic Newton-Lorentz equation were employed to evaluate particle dynamics under different values of the magnetic field growth parameter $ α$. The results demonstrate that efficient trapping and energy transfer can be achieved for appropriate values of $ α$, and that the spatial non-uniformity of the TE$_{011}$ mode introduces critical sensitivity to initial particle positioning. The study further identifies a ring-shaped region in which electrons are consistently captured in the GYRAC regime, and shows how the evolution of the Larmor radius, phase shift, and energy distribution depends on the electromagnetic configuration. Simulations involving disk-like and ring-like electron clouds reveal the fraction of captured, escaped, and uncaptured particles, confirming that precise control of the magnetic field variation is essential to optimize the efficiency of the acceleration process. These findings provide a basis for future self-consistent plasma simulations and support the development of compact radiation sources based on GYRAC-TE$_{011}$ acceleration. |
| title | Electron Acceleration by the Axisymmetric TE$_{011}$ Mode in a Slowly Varying External Magnetic Field |
| topic | Accelerator Physics |
| url | https://arxiv.org/abs/2503.22053 |