Bulletin of the American Physical Society
2018 Annual Meeting of the APS Mid-Atlantic Section
Volume 63, Number 20
Friday–Sunday, November 9–11, 2018; College Park, Maryland
Session B01: Poster Session (Day 1)
8:00 PM,
Friday, November 9, 2018
Edward St. John
Room: Lounge
Chair: Wendell T. Hill, III, University of Maryland, College Park
Abstract ID: BAPS.2018.MAS.B01.11
Abstract: B01.00011 : Towards an in situ, full-power intensity profiler for petawatt-class lasers
Presenter:
Calvin Z He
(University of Maryland, College Park)
Authors:
Calvin Z He
(University of Maryland, College Park)
Wendell Talbot Hill
(Univ of Maryland-College Park)
Collaboration:
Calvin Z He, Wendell T Hill III, Luis Roso, Jose Perez-Hernández, Giancarlo Gatti, Massimo De Marco, Robert Fedojesevs, Andrew Longman
A technique to measure the intensity profile of a focused laser pulse at full power is a long-standing desire. Nearly 40 years ago, Sarachik and Schappert suggested an approach, and worked out many of the details, to measure the intensity that is based on relativistic Thomson scattering (RTS), which consists of a rich spectrum of Doppler shifted radiation of the laser light, and its harmonics. It is straightforward to show that intensities can be extracted from the nth-order RTS harmonic spectrum from: I(λ,θ;n)=2πmec3/[r0λ02(1-cos2θ)](nλ/λ0-1), where λ0, λ, me, r0, θ, n and c are the laser wavelength, nth harmonic wavelength, the electron mass, classical electron radius, angle of observation, harmonic order and speed of light respectively. This expression was recently used to measure the intensity of VEGA 2, 200 TW pulses generated at the Centro de Láseres Pulsados (CLPU) facility in Salamanca, Spain. Specifically, 30 fs pulses with energies between 1 and 2.5 J were focused to w0 ~ 20 μm and captured by microscope objectives and dispersed by an Andor iStar spectrometer. This presentation will include a description of the apparatus, our initial results and a discussion of prospects for exploiting RTS to develop an in situ intensity profiler for intensities above 1018 W/cm2.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.MAS.B01.11
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