Proton acceleration by a relativistic laser frequency-chirp driven
plasma snowplow
plasma snowplow
File(s)1405.4309v1.pdf (535.97 KB)
Published version
Author(s)
Type
Conference Paper
Abstract
We analyze the use of a relativistic laser pulse with a controlled frequency
chirp incident on a rising plasma density gradient to drive an acceleration
structure for proton and light-ion acceleration. The Chirp Induced Transparency
Acceleration (ChITA) scheme is described with an analytical model of the
velocity of the snowplow at critical density on a pre-formed rising plasma
density gradient that is driven by a positive-chirp in the frequency of a
relativistic laser pulse. The velocity of the ChITA-snowplow is shown to depend
upon rate of rise of the frequency of the relativistic laser pulse represented
by $\frac{\epsilon_0}{\theta}$ where, $\epsilon_0 =
\frac{\Delta\omega_0}{\omega_0}$ and chirping spatial scale-length, $\theta$,
the normalized magnetic vector potential of the laser pulse $a_0$ and the
plasma density gradient scale-length, $\alpha$. We observe using 1-D OSIRIS
simulations the formation and forward propagation of ChITA-snowplow, being
continuously pushed by the chirping laser at a velocity in accordance with the
analytical results. The trace protons reflect off of this propagating snowplow
structure and accelerate mono-energetically. The control over ChITA-snowplow
velocity allows the tuning of accelerated proton energies.
chirp incident on a rising plasma density gradient to drive an acceleration
structure for proton and light-ion acceleration. The Chirp Induced Transparency
Acceleration (ChITA) scheme is described with an analytical model of the
velocity of the snowplow at critical density on a pre-formed rising plasma
density gradient that is driven by a positive-chirp in the frequency of a
relativistic laser pulse. The velocity of the ChITA-snowplow is shown to depend
upon rate of rise of the frequency of the relativistic laser pulse represented
by $\frac{\epsilon_0}{\theta}$ where, $\epsilon_0 =
\frac{\Delta\omega_0}{\omega_0}$ and chirping spatial scale-length, $\theta$,
the normalized magnetic vector potential of the laser pulse $a_0$ and the
plasma density gradient scale-length, $\alpha$. We observe using 1-D OSIRIS
simulations the formation and forward propagation of ChITA-snowplow, being
continuously pushed by the chirping laser at a velocity in accordance with the
analytical results. The trace protons reflect off of this propagating snowplow
structure and accelerate mono-energetically. The control over ChITA-snowplow
velocity allows the tuning of accelerated proton energies.
Date Issued
2012-07-31
Date Acceptance
2012-05-20
Citation
Proceedings of IPAC 2012, 2012, pp.2654-2656
ISBN
978-3-95450-115-1
Publisher
IEEE
Start Page
2654
End Page
2656
Journal / Book Title
Proceedings of IPAC 2012
Copyright Statement
© 2012 by IEEE- Creative Commons Attribution 3.0 (CC BY 3.0)
License URL
Identifier
http://arxiv.org/abs/1405.4309v1
Source
IPAC 2012
Subjects
physics.plasm-ph
physics.plasm-ph
physics.acc-ph
Notes
Proceedings of IPAC2012, New Orleans, Louisiana, USA, pp.2654-2656, 07 Accelerator Technology and Main Systems, T25 Lasers, ISBN 978-3-95450-115-1
Publication Status
Published
Start Date
2012-05-20
Finish Date
2012-05-25
Coverage Spatial
New Orleans, Louisiana