Energetics and energy scaling of quasi-monoenergetic protons in laser radiation pressure acceleration
Creators
- 1. University of Maryland, College Park, Maryland 20742 (United States)
- 2. Ruhr-University Bochum, D-44780 Bochum (Germany)
- 3. Indian Institute of Technology, New Delhi 110016 (India)
Description
Theoretical and computational studies of the ion energy scaling of the radiation pressure acceleration of an ultra-thin foil by short pulse intense laser irradiation are presented. To obtain a quasi-monoenergetic ion beam with an energy spread of less than 20%, two-dimensional particle-in-cell simulations show that the maximum energy of the quasi-monoenergetic ion beam is limited by self-induced transparency at the density minima caused by the Rayleigh-Taylor instability. For foils of optimal thickness, the time over which Rayleigh-Taylor instability fully develops and transparency occurs is almost independent of the laser amplitude. With a laser power of about one petawatt, quasi-monogenetic protons with 200 MeV and carbon ions with 100 MeV per nucleon can be obtained, suitable for particle therapy applications.
Additional details
Identifiers
- DOI
- 10.1063/1.3672515;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 18
- Journal Issue
- 12
- Journal Page Range
- p. 123105-123105.7
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 44006610
- Subject category
- S43: PARTICLE ACCELERATORS; S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- ACCELERATION; BEAM PRODUCTION; CARBON IONS; FOILS; ION BEAMS; LASER-PRODUCED PLASMA; LASERS; MEV RANGE; OPACITY; PETAWATT POWER RANGE; PLASMA DENSITY; PLASMA SIMULATION; PROTON BEAMS; PULSES; RADIATION PRESSURE; RAYLEIGH-TAYLOR INSTABILITY
- Descriptors DEC
- BEAMS; CHARGED PARTICLES; ENERGY RANGE; INSTABILITY; IONS; NUCLEON BEAMS; OPTICAL PROPERTIES; PARTICLE BEAMS; PHYSICAL PROPERTIES; PLASMA; POWER RANGE; SIMULATION
Optional Information
- Notes
- (c) 2011 American Institute of Physics