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| Content Provider | Springer Nature Link |
|---|---|
| Author | MITTAL, K C MAHESHWARI, K P |
| Copyright Year | 2011 |
| Abstract | Performance of the backward wave oscillator (BWO) is greatly enhanced with the introduction of plasma. Linear theory of the dispersion relation and the growth rate have been derived and analysed numerically for plasma-filled rippled wall rectangular waveguide driven by sheet electron beam. To see the effect of plasma on the TM$_{01}$ cold wave structure mode and on the generated frequency, the parameters used are: relativistic factor γ = 1.5 (i.e. v/c = 0.741), average waveguide height y $_{0}$ = 1.445 cm, axial corrugation period z $_{0}$ = 1.67 cm, and corrugation amplitude ε = 0.225 cm. The plasma density is varied from zero to 2 ×10$^{12}$ cm$^{ − 3}$. The presence of plasma tends to raise the TM$_{01}$ mode cut-off frequency (14 GHz at 2 ×10$^{12}$ cm$^{ − 3}$ plasma density) relative to the vacuum cut-off frequency (5 GHz) which also causes a decrease in the group velocity everywhere, resulting in a flattening of the dispersion relation. With the introduction of plasma, an enhancement in absolute instability was observed. |
| Starting Page | 501 |
| Ending Page | 511 |
| Page Count | 11 |
| File Format | |
| ISSN | 03044289 |
| Journal | Pramana |
| Volume Number | 76 |
| Issue Number | 3 |
| e-ISSN | 09737111 |
| Language | English |
| Publisher | Springer-Verlag |
| Publisher Date | 2011-05-27 |
| Publisher Place | India |
| Access Restriction | One Nation One Subscription (ONOS) |
| Subject Keyword | Sheet electron beam; backward wave oscillator; plasma. Astrophysics and Astroparticles Physics Astronomy, Observations and Techniques |
| Content Type | Text |
| Resource Type | Article |
| Subject | Physics and Astronomy |
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