Clocking femtosecond X rays

Linear-accelerator-based sources will revolutionize ultrafast x-ray science due to their unprecedented brightness and short pulse duration. However, time-resolved studies at the resolution of the x-ray pulse duration are hampered by the inability to precisely synchronize an external laser to the acc...

Full description

Saved in:
Bibliographic Details
Published in:Physical review letters Vol. 94; no. 11; pp. 114801.1 - 114801.4
Main Authors: CAVALIERI, A. L, FRITZ, D. M, SIDDONS, D. P, LOWNEY, D. P, MACPHEE, A. G, WEINSTEIN, D, FALCONE, R. W, PAHL, R, ALS-NIELSEN, J, BLOME, C, DÜSTERER, S, ISCHEBECK, R, LEE, S. H, SCHLARB, H, SCHULTE-SCHREPPING, H, TSCHENTSCHER, Th, SCHNEIDER, J, HIGNETTE, O, SETTE, F, SOKOLOWSKI-TINTEN, K, CHAPMAN, H. N, LEE, R. W, HANSEN, T. N, BUCKSBAUM, P. H, SYNNERGREN, O, LARSSON, J, TECHERT, S, SHEPPARD, J, WARK, J. S, BERGH, M, CALEMAN, C, HULDT, G, VAN DER SPOEL, D, TIMNEANU, N, REIS, D. A, HAJDU, J, AKRE, R. A, BONG, E, EMMA, P, KREJCIK, P, ARTHUR, J, BRENNAN, S, GAFFNEY, K. J, LINDENBERG, A. M, LUENING, K, RUDATI, J, HASTINGS, J. B, MILLS, D. M, FUOSS, P. H, STEPHENSON, G. B, KAO, C. C
Format: Journal Article
Language:English
Published: Ridge, NY American Physical Society 25-03-2005
Subjects:
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary:Linear-accelerator-based sources will revolutionize ultrafast x-ray science due to their unprecedented brightness and short pulse duration. However, time-resolved studies at the resolution of the x-ray pulse duration are hampered by the inability to precisely synchronize an external laser to the accelerator. At the Sub-Picosecond Pulse Source at the Stanford Linear-Accelerator Center we solved this problem by measuring the arrival time of each high energy electron bunch with electro-optic sampling. This measurement indirectly determined the arrival time of each x-ray pulse relative to an external pump laser pulse with a time resolution of better than 60 fs rms.
Bibliography:ObjectType-Article-1
SourceType-Scholarly Journals-1
ObjectType-Feature-2
content type line 23
ISSN:0031-9007
1079-7114
1079-7114
DOI:10.1103/PhysRevLett.94.114801