1. Guiding and Ionization Blueshift in Ablative Capillary Waveguide Accelerators.
- Author
-
McGuffey, Chris, Matsuoka, Takeshi, Levin, Michael, Bulanov, Stepan, Chvykov, Vladimir, Kalintchenko, Galina, Rousseau, Pascal, Yanovsky, Victor, Zigler, Arie, Maksimchuk, Anatoly, and Krushelnick, Karl
- Subjects
IONIZATION (Atomic physics) ,ABLATIVE materials ,ELECTRON accelerators ,PLASMA gases ,RADIO frequency ,PROPERTIES of matter ,ULTRASHORT laser pulses - Abstract
Laser wakefield acceleration (LWFA) in plasmas has been demonstrated with gradients which are orders of magnitude greater than the limit on conventional Radio Frequency accelerators. However, the acceleration length is limited by two factors, the dephasing length and the Rayleigh range of the laser pulse. Dephasing length is the distance in which electrons overtake the laser pulse and can be increased by decreasing plasma density. Alternatively the interaction length can be extended by orders of magnitude by using ablative wall discharge capillary targets, in which a plasma is preformed with a transverse density profile capable of guiding the focused laser. We have demonstrated guiding of high intensity laser pulses from the HERCULES laser over 3 cm for powers up to 35 TW. The quality of the laser spot can be retained and the intensity remains high even at the exit of the capillary. The transmitted laser spectrum shows blueshifting due to field ionization by the laser pulse. This ionization might enhance electron injection at low electron density for LWFA GeV accelerators. The field ionization affects carbon atoms and ions from the ablated capillary, which are not present in hydrogen-filled capillaries. This creates an additional challenge to guiding compared to hydrogen-filled capillaries. However, the setup and materials are easier to come by. The use of these capillary targets may also be of interest to other high intensity laser-plasma interactions requiring long interaction lengths such as high harmonic generation from gases and plasmas, or x-ray lasing in underdense plasmas. [ABSTRACT FROM AUTHOR]
- Published
- 2009
- Full Text
- View/download PDF