Fred Hartemann
Lawrence Livermore National Laboratory
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Featured researches published by Fred Hartemann.
Physics of Plasmas | 2004
D. J. Gibson; S. G. Anderson; C. P. J. Barty; S. M. Betts; Rex Booth; Winthrop J. Brown; John K. Crane; Robert R. Cross; D. N. Fittinghoff; Fred Hartemann; Jaroslav Kuba; Gregory Peter Le Sage; Dennis R. Slaughter; A. Tremaine; Alan Wootton; Edward P. Hartouni; P. T. Springer; J. B. Rosenzweig
The PLEIADES (Picosecond Laser-Electron Inter-Action for the Dynamical Evaluation of Structures) facility has produced first light at 70 keV. This milestone offers a new opportunity to develop laser-driven, compact, tunable x-ray sources for critical applications such as diagnostics for the National Ignition Facility and time-resolved material studies. The electron beam was focused to 50 μm rms, at 57 MeV, with 260 pC of charge, a relative energy spread of 0.2%, and a normalized emittance of 5 mm mrad horizontally and 13 mm mrad vertically. The scattered 820 nm laser pulse had an energy of 180 mJ and a duration of 54 fs. Initial x rays were captured with a cooled charge-coupled device using a cesium iodide scintillator; the peak photon energy was approximately 78 keV, with a total x-ray flux of 1.3×106 photons/shot, and the observed angular distribution found to agree very well with three-dimensional codes. Simple K-edge radiography of a tantalum foil showed good agreement with the theoretical divergence-...
Archive | 2010
Miro Shverdin; Fred Hartemann; Felicie Albert; Mike Messerly; D. J. Gibson; C. W. Siders; Chris Barty
Compton-scattering is a well-known process, observed and described by Arthur H. Compton in 1924, where the energy of an incident photon is modified by an inelastic scatter with matter (Compton, 1923). In 1948, Feenberg and Primakoff presented a theory of Compton backscattering, where photons can gain energy through collisions with energetic electrons (Feenberg & Primakoff, 1948). In 1963, Milburn and Arutyanyan and Tumanyan developed a concept for Compton-scattering light sources based on colliding an accelerated, relativistic electron beam and a laser (Arutyunyan & Tumanyan, 1964; Milburn, 1963). When an infrared photon scatters off a relativistic electron beam, its wavelength can be Doppler-upshifted to X-rays. Under properly designed conditions, we can generate high brightness, high flux, MeV-scale photons by colliding an intense laser pulse with a high quality, electron beam accelerated in a Linac. Despite being incoherent, the Compton-generated gamma-rays sharemany of the laser light characteristics: low divergence, high flux, narrow-bandwidth, and polarizability. Traditional laser sources operate in a 0.1−10 eV range, overlapping most of the molecular and atomic transitions. Transitions inside the nucleus have energies greater than 0.1MeV. Bymatching the gamma-ray energy to a particular nuclear transition, we can target a specific isotope, akin to using a laser to excite a particular atomic or molecular transition. Narrow-bandwidth gamma-ray sources enable high impact technological and scientific missions such as isotope-specific nuclear resonance fluorescence (NRF) (Bertozzi & Ledoux, 2005; Pruet et al., 2006), radiography of low density materials (Albert et al., 2010), precision nuclear spectroscopy (Pietralla et al., 2002), medical imaging and treatment (Carroll et al., 2003; Bech et al., 2009), and tests of quantum chromodynamics (Titov et al., 2006). In traditional X-ray radiography, the target must have a higher atomic number than the surrounding material. Hence, one could conceal an object by shielding with a higher Z-number material. In NRF gamma-ray imaging, the MeV class photons have very long absorption lengths and will transmit through meter lengths of material unless resonantly absorbed by a specific isotope. Some applications of NRF tuned gamma-rays include nuclear waste imaging and assay, monitoring of special nuclear material for homeland security, and tumor detection for medical treatment. Compton-based sources are attractive in the 100 keV and higher energy regime because they are highly compact and can be more than 15 orders of magnitude brighter than alternative methods for producing photons in this energy regime: Bremsstrahlung radiation 3
quantum electronics and laser science conference | 2009
Felicie Albert; S. G. Anderson; Gerald Anderson; S. M. Betts; D. J. Gibson; C. Hagmann; Micah Johnson; Mike Messerly; Miroslav Y. Shverdin; A. Tremaine; Fred Hartemann; B. Rusnak; C. W. Siders; Dennis Paul McNabb; C. P. J. Barty
We report detailed spectral and spatial characterization of a 0.1-MeV-0.8 MeV tunable ultra-bright laser-based Compton scattering source. Nuclear Resonance Fluorescence experiments with the source are also presented.
Nonlinear Optics: Materials, Fundamentals and Applications (2007), paper FA4 | 2007
Miroslav Y. Shverdin; Igor Jovanovic; D. J. Gibson; Fred Hartemann; S. Anderson; Curtis G. Brown; S. M. Betts; Jose Hernandez; Micah Johnson; Mike Messerly; Jason Pruet; A. Tremaine; Dennis Paul McNabb; Craig W. Siders; Chris Barty
We designed and constructed a nonlinear crystal-based short pulse recirculation cavity that traps the second harmonic of an incident high power laser. This scheme aims to increase the efficiency of Compton-scattering based light sources.
Ultramicroscopy | 2007
Michael R. Armstrong; Ken Boyden; Nigel D. Browning; Jeffrey D. Colvin; William J. DeHope; Alan M. Frank; D. J. Gibson; Fred Hartemann; Judy S. Kim; Wayne E. King; Thomas LaGrange; Ben J. Pyke; Bryan W. Reed; Richard M. Shuttlesworth; Brent C. Stuart; Ben Torralva
Physical Review Letters | 2016
E. L. Dewald; Fred Hartemann; P. Michel; J. L. Milovich; M. Hohenberger; A. Pak; O. L. Landen; L. Divol; H. F. Robey; O. A. Hurricane; T. Döppner; Felicie Albert; B. Bachmann; N. B. Meezan; A. J. Mackinnon; D. A. Callahan; M. J. Edwards
Conf.Proc.C110328:133-135,2011 | 2012
C. Limborg-Deprey; C. Adolphsen; T S Chu; M. Dunning; R.K. Jobe; Erik Jongewaard; C. Hast; A.E. Vlieks; Faya Wang; D. Walz; Roark Marsh; S.G. Anderson; Fred Hartemann; T.L. Houck; Livermore Llnl
Physical Review Letters | 2013
Fred Hartemann; Sheldon Wu
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2011
S.G. Anderson; Felicie Albert; A. Bayramian; G. Beer; R.E. Bonanno; R.R. Cross; G.A. Deis; Chris Ebbers; D. J. Gibson; Fred Hartemann; T.L. Houck; R. A. Marsh; Dennis Paul McNabb; Michael J. Messerly; R.D. Scarpetti; Miroslav Y. Shverdin; C. W. Siders; S.S. Wu; Chris Barty; Chris Adolphsen; T.S. Chu; Erik Jongewaard; Zenghai Li; C. Limborg; Sami Tantawi; A.E. Vlieks; Faya Wang; J.W. Wang; F. Zhou; T. Raubenheimer
bipolar/bicmos circuits and technology meeting | 2003
James Boyce; D. Douglas; Hiroyuki Toyokawa; Winthrop J. Brown; Fred Hartemann