Electromagnetically induced transparency (EIT) is a coherent optical nonlinearity, and brings dramatic changes in optical properties such as absorption, emission, refraction etc. The phenomena relate to the quantum mechanical overlapping state created by two different wavelengths of coherent light. Recently, EIT for X-rays has been theoretically predicted. According to the theory, it is possible to make Ne gas, which is normally opaque, transparent by exposing it to laser light of 800 nm with extremely high flux of 1012 W/cm2. The scheme could be used for producing ultra-short X-ray pulses. For more information, see the paper, "Electromagnetically Induced Transparency for X Rays ", C. Buth et al., Phys. Rev. Lett., 98, 253001 (2007). For more about general EIT, see, for example, "Electromagnetically Induced Transparency.", S. Harris, Physics Today, 50, 36-42 (1997).
A research group at the Japan Atomic Energy Agency (Kizugawa, Japan) has recently developed a novel table-top pulsed X-ray source. The source employs a Ti:sapphire laser, emitting 70 fs duration 2 TW pulses of 800 nm wavelength at 10 Hz. The laser beam is focused to the flow of high-density Ar gas. The source was applied to perform phase contrast imaging. For more information, see the paper, "Phase-contrast x-ray imaging with intense Ar Ka radiation from femtosecond-laser-driven gas target", L. M. Chen et al., Appl. Phys. Lett. 90, 211501 (2007).
Recently, some very interesting research on magnetic noise from antiferromagnets has been published. Unlike ferromagnets, the characteristics of which have been studied for many years, antiferromagnets have remained a mystery because their internal structure was too fine to be measured. Their internal order is on the same scale as the wavelength of X-rays, and therefore, X-ray photon correlation spectroscopy, which measures 'speckle' patterns, can give a unique 'fingerprint' of a particular magnetic domain configuration. It was found that the domain wall motion is thermally activated at temperatures above 100 K, but not so at lower temperatures. For more information, see the paper, "Direct measurement of antiferromagnetic domain fluctuations", O. G. Shpyrko, et al., Nature 447, 68 (2007).
Atoms become ions when exposed to extremely intense light. The process is predicted to occur via tunnelling through the binding potential that is suppressed by the light field near the peaks of its oscillations. Professor F. Krausz (Max Planck Institute of Quantum Optics in Garching, Germany) and his collaborators recently reported the real-time observation of this most elementary step in strong-field interactions, i.e., light-induced electron tunnelling. The team used 250-attosecond pulses of UV radiation, and confirmed theoretical predictions about the tunneling process. It was also found that the process lasted for several hundred attoseconds, depleting atomic-bound states. This would suggest that the use of tunneling itself is feasible for probing short-lived, transient states of atoms or molecules, e.g., multi-electron excitation (shake-up) and relaxation (cascaded Auger decay) processes etc. For more information, see the paper, "Attosecond real-time observation of electron tunnelling in atoms", M. Uiberacker et al., Nature, 446, 627 (2007).
The Sub-Picosecond Pulse Source (SPPS) is a prototype X-ray free electron laser built using the 2-mile-long linear accelerator at Stanford Linear Accelerator Center (SLAC), California, United States. To date, ultrafast phenomena have been mainly studied with femtosecond lasers operating at ultraviolet to infrared wavelengths; however, these wavelengths are not short enough for structural studies on atomic distances. Therefore, the emergence of short pulse laser in the hard X-ray region represents a significant challenge. Recently, at Stanford, an international collaborative team from 20 different institutions succeeded in observing the atomic motion of Bismuth crystal, which, although cubic, has a slight elongation along the diagonal called a Peierls distortion. The measurements have brought new fundamental insights into the dynamics of the material, which shows very strong coupling between the electronic and ionic structures. The results could also be used to screen many theoretical calculations made so far. For more information, see the paper, "Ultrafast Bond Softening in Bismuth: Mapping a Solid's Interatomic Potential with X-rays ", D. M. Fritz et al., Science 315, 633 (2007).
At Brookhaven National Laboratory, United States, researchers have recently found a novel way to generate a very short controllable free electron laser (FEL) pulse, which usually depends on the length of the electron pulse. The main idea is the use of a Ti:Sapphire laser that combines a 150 femtosecond (FWHM) pulse of light with the much longer electron beam. This leads to a femtosecond FEL pulse that keeps growing in intensity and shortening in time duration, which is attributed to a phenomenon called superradiance (for details, see, R. H. Dicke, Phys. Rev. 93, 99 (1954)). The present research is the first to experimentally observe the effects of superradiance in a FEL setup. The output FEL pulse duration was measured to be as short as 81 femtoseconds, a roughly 50% reduction compared to the input seed laser. Understanding how to produce these intense, ultrafast pulses of light could help scientists around the world as they begin to construct the next generation of light source facilities. For more information, see the paper, "Experimental Characterization of Superradiance in a Single-Pass High-Gain Laser-Seeded Free-Electron Laser Amplifier ", T. Watanabe et al., Phys. Rev. Lett. 98, 034802 (2007).
In January 2006, the Stardust spacecraft brought back a number of tiny particles from comet Wild 2, which is believed to have originated within a cloud of comets just beyond the orbit of Neptune called the Kuiper Belt. The particles have been analyzed by X-rays at six synchrotron radiation facilities around the world, ESRF (France), APS (Argonne, USA), SSRL(Stanford, USA), ALS (Berkeley, USA), NSLS (Brookhaven, USA) and SPring-8 (Japan). The particles from this comet are important because they are believed to be close to the starting material of the solar system, which is now about 4.5 billion years old. The particles were found to contain a wide variety of minerals and organic materials that look similar to those seen in primitive meteorites found on earth, but the samples also revealed the presence of new materials not previously found in meteorites. It was also discovered that the samples contained minerals similar to Calcium Aluminum-rich inclusions (CAIs), which can be formed at high temperatures, i.e., in the innermost part of the solar nebula, well inside the orbit of Mercury. For more information on the Stardust mission, visit http://stardust.jpl.nasa.gov/home/index.html. Some interesting results have been published as part of a special series of papers in the Dec. 15, 2006, edition of the journal Science.
By combining coherent X-ray scattering with a method of direct phase recovery called over-sampling, lens-free microscopy in the X-ray region becomes a realistic technique. The latest hot topic is the extension of the technique from two to three dimensions. One of the most promising ways of applying this technique is the recently reported combination of (i) ab initio phase retrieval of 2D coherent diffraction patterns with a guided hybrid input-output algorithm and (ii) 3D image reconstruction with equally sloped tomography. The scheme was applied to quantitative 3D imaging of a heat-treated GaN particle with each voxel corresponding to 17×17×17 nm3. The internal GaN-Ga2O3 core shell structure was successfully captured in three dimensions. For more information about the analysis, see the paper, "Three-Dimensional GaN-Ga2O3 Core Shell Structure Revealed by X-Ray Diffraction Microscopy", J. Miao et al., Phys. Rev. Lett. 97, 215503 (2006).
At the FLASH free-electron laser facility at DESY in Hamburg, an international team of scientists recently published the first data on diffraction imaging of a non-crystalline sample. Theoretically, a single X-ray pulse, if it is extremely bright and perfectly coherent, can produce a diffraction pattern from a large macromolecule, a virus or a cell (for example, see, "Potential for biomolecular imaging with femtosecond X-ray pulses", R. Neutze et al., Nature, 406, 752-757 (2000)). In the present experiment, the team tested a laser pulse with 25 fs, 41013 W/cm2/pulse, containing 1012 photons at 32 nm wavelength, and obtained a coherent diffraction pattern from a nanostructured non-periodic object before this exploded into a plasma at ca. 60,000 K. They employed a novel X-ray camera assured of single-photon detection sensitivity by filtering out parasitic scattering and plasma radiation. For more information, see the paper, "Femtosecond diffractive imaging with a soft-X-ray free-electron laser", H. N. Chapman et al., Nature Physics, published online 12 November 2006.
Scientists at the Japan Atomic Energy Agency (JAEA) led by Dr W. Utsumi have proved that the formation of bulk metallic glass of elemental Zr and Ti, which was recently reported (see for example, Zhang and Zhao, Nature 430, 332 (2004) and Y. Wang et al., Phys. Rev. Lett. 95, 155501 (2005)) was some sort of phantom. The experiment basically took the form of X-ray diffraction in high-temperature and high-pressure conditions, but in addition to the normal energy-dispersive detector, the research group employed an in situ angular-dispersive X-ray diffractometer equipped with a 2D detector and X-ray transparent anvils. The disappearance of all the Bragg peaks in the one-dimensional energy-dispersive data could be taken as evidence of amorphization. However, the research group found several intense Bragg spots in their angular-dispersive data, even in the exact same conditions where amorphization was reported. This indicates that Zr and Ti do not form glass, but that the grains grow rapidly. The experiments were carried out at BL14B1 and BL22XU, SPring-8, Japan. For more information, see the paper, "Does Bulk Metallic Glass of Elemental Zr and Ti Exist?", T. Hattori et al., Phys. Rev. Lett., 96, 255504 (2006).
The appearance of the ultimate X-ray microscope, with atomic-scale resolution and capable of seeing deep inside objects, has long been awaited. Professor I. Robinson (University College London, UK) and his team recently made a significant step towards realizing this dream, using the technique of coherent X-ray diffraction imaging, the possibility of which was first pointed out by Sayre (Acta Crystallogr. 5, 843 (1952)) but not demonstrated until 1999 by Miao et al (Nature 400, 342 (1999)). They observed the growth of nanometer-sized Pb crystals inside the vacuum chamber. The results showed that asymmetries in the diffraction pattern can be mapped to deformities, providing a detailed 3-D map of their location in the crystal. This new method shows that the interior structure of atomic displacements within single nanocrystals can be obtained by direct inversion of the diffraction pattern. The technique is an attractive alternative to electron microscopy because of the superior penetration of materials of interest by the electromagnetic waves, which are often less damaging to the sample than electrons. The experiments were done at beamline 34-ID-C at the Advanced Photon Source (APS) in the United States. For more information, see the paper, "Three-dimensional mapping of a deformation field inside a nanocrystal", Mark A. Pfeifer et al., Nature 442, 63 (2006).
The mineral silica (SiO2) is a common substance that is a constituent of all of the planets in our solar system. At SPring-8, Harima, Japan, Dr. K. Hirose (Tokyo Institute of Technology; Japan Agency for Marine-Earth Science and Technology) and his co-workers recently found that, above 268 GPa and 1800 K, silica exhibits a novel stable high-pressure form with a pyrite-type structure, which is much denser than other known silica phases. This form of silica could be one of the main constituents of the core of a gas-giant planet such as Uranus or Neptune. For more information, see the paper, "The Pyrite-Type High-Pressure Form of Silica", Y. Kuwayama et al., Science, 309, 923-925 (2005).
An Austrian research group recently succeeded in obtaining highly collimated, spatially coherent X-rays, at a wavelength of about 1 nm and at photon energies extending to 1.3 keV, from high-order harmonic generation in an atomic gas ionized by a 720-nm, 5-fs, 0.2-TW laser pulse. The beam divergence was evaluated as 0.2 mrad for the spectral range above 200 eV from a knife-edge scan, indicating perfect coherence of the atomic dipoles within a macroscopic volume of diameters of 13μm and 4μm at photon energies of 0.3 keV and 1 keV, respectively. The beam seems to be diffraction-limited to within a factor of five. The spectrum of the generated radiation was observed by an energy-dispersive X-ray spectrometer with some filters. The results are really exciting, because they could detect the copper L-edges (~950 eV)! One would notice that the energy of photons produced by laser technologies has been increasing every year - the main idea behind this progress is the creation of time-gradient in the driving pulse, which allows some 25% of the helium atoms to be ionized within half a cycle before the pulse peak. The electrons detached within this time are pushed in the most intense half-cycle back to the atomic core. For more information, see the paper, "Source of coherent kiloelectronvolt X-rays", J. Seres et al., Nature, 433, 596 (2005). C. Streli and P. Wobrauschek (Atominstitut der Osterreichischen Universtitaten, Technische Universitat Wien) were the co-authors of this paper.
So far, it has been difficult to observe nonlinear responses to an optical field in the extreme ultraviolet (XUV) and soft X-ray regions. A research group from the University of Tokyo recently succeeded in generating intense isolated XUV pulses (photon energy 27.9 eV) that were shorter than 1 femtosecond through high-harmonic (9th) generation by using a sub-10-femtosecond blue laser (photon energy 3.1 eV) producing a large dipole moment. For more information, see the paper, "Nonlinear optics in the extreme ultraviolet", T. Sekikawa et al., Nature, 432, 605-608 (2004).