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Short-pulse Laser Capability on the Mercury Laser System
R. Campbell
B. Stuart
J. Crane
R. Cross
P. Armstrong
S. Sutton
B. Chai
Y. Fei
B. Freitas
J. Britten
K. Schaffers
C. Bibeau
C. Ebbers
A. Bayramian
I. Jovanovic
C. J. Barty
Z. Liao
A. Erlandson
J. Caird
S. Telford
E. Utterback
T. Ladran
B. Molander
P. Thelin
出版
United States. Department of Energy
, 2006
URL
http://books.google.com.hk/books?id=yS_sjwEACAAJ&hl=&source=gbs_api
註釋
Applications using high energy ''petawatt-class'' laser drivers operating at repetition rates beyond 0.01 Hz are only now being envisioned. The Mercury laser system is designed to operate at 100 J/pulse at 10 Hz. We investigate the potential of configuring the Mercury laser to produce a rep-rated, ''petawatt-class'' source. The Mercury laser is a prototype of a high energy, high repetition rate source (100 J, 10 Hz). The design of the Mercury laser is based on the ability to scale in energy through scaling in aperture. Mercury is one of several 100 J, high repetition rate (10 Hz) lasers sources currently under development (HALNA, LUCIA, POLARIS). We examine the possibility of using Mercury as a pump source for a high irradiance ''petawatt-class'' source: either as a pump laser for an average power Ti:Sapphire laser, or as a pump laser for OPCPA based on YCa{sub 4}O(BO{sub 3}){sub 3} (YCOB), ideally producing a source approaching 30 J /30 fs /10 Hz--a high repetition rate petawatt. A comparison of the two systems with nominal configurations and efficiencies is shown in Table 1.