free-electron lasers\(\def\hfill{\hskip 5em}\def\hfil{\hskip 3em}\def\eqno#1{\hfil {#1}}\)

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775

Combining THz laser excitation with resonant soft X-ray scattering at the Linac Coherent Light Source

CROSSMARK_Color_square_no_text.svg

aLinac Coherent Light Source, SLAC National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, CA 94025, USA, bDepartment of Chemistry, Massachusetts Institute of Technology, Cambridge, MA 02139, USA, cSwiss Light Source, Paul Scherrer Institut, 5232 Villigen, Switzerland, and dETH Zurich, Institute for Quantum Electronics, Wolfgang-Pauli-Strasse 16, 8093 Zurich, Switzerland
*Correspondence e-mail: joshuat@slac.stanford.edu

Edited by I. Schlichting, Max Planck Institute for Medical Research, Germany (Received 11 November 2014; accepted 24 March 2015; online 11 April 2015)

This paper describes the development of new instrumentation at the Linac Coherent Light Source for conducting THz excitation experiments in an ultra high vacuum environment probed by soft X-ray diffraction. This consists of a cantilevered, fully motorized mirror system which can provide 600 kV cm−1 electric field strengths across the sample and an X-ray detector that can span the full Ewald sphere with in-vacuum motion. The scientific applications motivated by this development, the details of the instrument, and spectra demonstrating the field strengths achieved using this newly developed system are discussed.

1. Introduction

The recent development of the X-ray free-electron laser (FEL) has opened up numerous new scientific opportunities, paving the way for many scientific breakthroughs in its short history. For example, FEL experiments have offered new insights in structural biology enabling a better understanding of African sleeping sickness (Redecke et al., 2013[Redecke, L. et al. (2013). Science, 339, 227-230.]) and of the proteins responsible for photosynthesis at room temperature (Kern et al., 2013[Kern, J. et al. (2013). Science, 340, 491-495.]). The soft X-ray range affords further unique opportunities in an array of scientific fields, including astrophysics (Bernitt et al., 2012[Bernitt, S. et al. (2012). Nature (London), 492, 225-228.]), planetary science (Vinko et al., 2012[Vinko, S. M. et al. (2012). Nature (London), 482, 59-62.]) and surface chemistry (Dell'Angela et al., 2013[Dell'Angela, M. et al. (2013). Science, 339, 1302-1305.]). One area, however, which has shown increased potential is in the area of understanding materials. In particular, resonant soft X-ray diffraction has proven to be a valuable tool to look at long-range ordering of different order parameters. An adaptation of this tool has allowed researchers to gain time-resolved information of relevant order parameters in condensed matter systems in response to dynamic stimuli in materials such as CuO (Johnson et al., 2012[Johnson, S. L. et al. (2012). Phys. Rev. Lett. 108, 037203.]), manganites (Tobey et al., 2012[Tobey, R. I. et al. (2012). Phys. Rev. B, 86, 064425.]) and nickelates (Caviglia et al., 2013[Caviglia, A. D. et al. (2013). Phys. Rev. B, 88, 220401.]; Chuang et al., 2013[Chuang, Y. D. et al. (2013). Phys. Rev. Lett. 110, 127404.]). Recent work has even utilized pulsed pumping schemes at specialized photon energies to exclusively excite phonons (Först et al., 2011[Först, M. et al. (2011). Phys. Rev. B, 84, 241104.], 2013[Först, M., Mankowsky, R., Bromberger, H., Fritz, D. M., Lemke, H., Zhu, D., Chollet, M., Tomioka, Y., Tokura, Y., Merlin, R., Hill, J., Johnson, S. & Cavalleri, A. (2013). Solid State Commun. 169, 24-27.]) as a route to material control. However, using low-photon-energy excitation to study the intricate workings of quantum materials (Kubacka et al., 2014[Kubacka, T. et al. (2014). Science, 343, 1333-1336.]) is an area which has so far been under-utilized, but remains quite promising.

Radiation in the THz regime (∼0.4–40 meV) (Kampfrath et al., 2013[Kampfrath, T., Tanaka, K. & Nelson, K. A. (2013). Nat. Photon. 7, 680-690.]; Hwang et al., 2014[Hwang, H. Y., Fleischer, S., Brandt, N. C., Perkins, B. G., Liu, M., Fan, K., Sternbach, A., Zhang, X., Averitt, R. D. & Nelson, K. A. (2014). J. Mod. Opt., doi:10.1080/09500340.2014.918200.]) lies in a unique photon energy range for potential investigations in deciphering the nature of competing interactions in a material at nearly degenerate energies. The low photon energies are associated with many low-energy excitations in solids (Basov et al., 2011[Basov, D. N., Averitt, R. D., van der Marel, D., Dressel, M. & Haule, K. (2011). Rev. Mod. Phys. 83, 471-541.]). The combination of strong THz excitation sources and the advent of fourth-generation light sources has enabled the study of long-range order at atomic length scales and ultrafast timescales (Hoffmann & Turner, 2012[Hoffmann, M. C. & Turner, J. J. (2012). Synchrotron Radiat. News, 25, 17-24.]) and is one of the motivations for the developments discussed in this paper.

One challenge with measuring soft X-ray diffraction in an ultra high vacuum environment is the incorporation of an in-vacuum diffractometer. Doing so enlarges the vacuum chamber, especially when the chamber volume is designed to span the full range of the Ewald sphere with a large area detector. Furthermore, a large optical element very close to the sample is needed to strongly focus the low-photon-energy pump pulses near the diffraction limit, thus maximizing the intensity at the sample. Typically a small-diameter vacuum chamber is used with the optical element outside the chamber. THz pump/soft X-ray probe experiments have been quite challenging because of the competing needs of a large vacuum chamber volume for the diffractometer and small chamber volume for strong focusing of the excitation pulse.

We have solved this problem by designing a focusing system inside a large-diameter vacuum chamber. By cantilevering a 2 inch-diameter optic from the side of the vacuum chamber, we have allowed for full control of six degrees of freedom for the focusing system alignment. As a result, we can now provide THz pumping at electric field strengths of up to 600 kV cm−1 (corresponding to magnetic field strengths of up to 200 mT) on a sample for resonant soft X-ray scattering experiments. The chamber has also been designed to prevent interference from the movement of an avalanche photodiode (APD) detector assembly with the optics. The assembly can move over a hemisphere about the sample to measure all possible diffraction angles at a distance of 14 cm [\pm] 3.8 cm. This new design allows for THz pump/soft X-ray diffraction probe experiments with probing in any Bragg geometry. The angular range of detection is limited only by the size of the shadow of the focusing mirror placed in front of the sample onto the detector plane.

2. Resonant scattering at FELs

The promise offered by using resonant scattering at soft X-ray energies for FEL research is astounding. X-ray scattering has been used to understand distinct types of long-range ordering by using resonant enhancement. This is especially useful in the soft X-ray range because many of the L-edges for important materials, such as transition metal oxides, lie in the soft X-ray range. The L-edges in these types of materials are important because they give access to types of order that involve the d-electrons, those relevant for emergent behavior arising from interactions of the orbital, charge or magnetic degrees of freedom. Furthermore, what makes this technique interesting for FEL research is the large degree of coherence (Vartanyants et al., 2011[Vartanyants, I. A. et al. (2011). Phys. Rev. Lett. 107, 144801.]), which means coherent scattering methods could also be used to study dynamics for these types of materials, such as in magnetic or orbital domain fluctuations (Konings et al., 2011[Konings, S., Schüssler-Langeheine, C., Ott, H., Weschke, E., Schierle, E., Zabel, H. & Goedkoop, J. B. (2011). Phys. Rev. Lett. 106, 077402.]; Seu et al., 2010[Seu, K. A., Roy, S., Turner, J. J., Park, S., Falco, C. & Kevan, S. D. (2010). Phys. Rev. B, 82, 012404.]; Turner et al., 2008[Turner, J. J., Thomas, K. J., Hill, J. P., Pfeifer, M. A., Chesnel, K., Tomioka, Y., Tokura, Y. & Kevan, S. D. (2008). New J. Phys. 5, 053023.]).

Central to FEL experiments on materials is the pump–probe technique, where ordering is enabled/disrupted by a pump pulse, and then the change of that order is monitored by a probe pulse – in this case an ultrafast soft X-ray pulse. This enables the study of distinct charge, orbital and spin order following an excitation mechanism, allowing for a full study of long-range-ordering dynamics. Comparing different types of interaction strengths in non-equilibrium conditions is the real strength of this method because it allows one to unravel the different ordering mechanisms by separating them in the time domain, offering prospects for their control. Though much excellent work has been done using non-selective optical pump methods (Staub et al., 2014[Staub, U. et al. (2014). Phys. Rev. B, 89, 220401.]; de Jong et al., 2013[Jong, S. de et al. (2013). Nat. Mater. 12, 882-886.]; Lee et al., 2012[Lee, W. S. et al. (2012). Nat. Commun. 3, 838.]), recent work has shown the importance of selective excitation to clarify the physics of the mechanisms being studied (Fausti et al., 2011[Fausti, D., Tobey, R. I., Dean, N., Kaiser, S., Dienst, A., Hoffmann, M. C., Pyon, S., Takayama, T., Takagi, H. & Cavalleri, A. (2011). Science, 331, 189-191.]). For instance, the lattice of a superconductor can be resonantly pumped while observing the response of the charge density wave state (Först et al., 2014a[Först, M., Frano, A., Kaiser, S., Mankowsky, R., Hunt, C. R., Turner, J. J., Dakovski, G. L., Minitti, M. P., Robinson, J., Loew, T., Le Tacon, M., Keimer, B., Hill, J. P., Cavalleri, A. & Dhesi, S. S. (2014a). Phys. Rev. B, 90, 184514.]), or of the charge order and of the crystal lattice structure itself (Först et al., 2014b[Först, M. et al. (2014b). Phys. Rev. Lett. 112, 157002.]). In the case of quantum materials many of the interactions compete on even lower energy scales, on the order of tens of meV. This motivates the use of lower-energy laser sources because resonant pumping can be performed to separate these mechanisms. By tuning to different types of modes, the physics in complex systems can be unraveled on ultrafast timescales such as in the recent study of electromagnons (Kubacka et al., 2014[Kubacka, T. et al. (2014). Science, 343, 1333-1336.]).

3. Instrumentation

The instrumental developments addressed in this paper were made to an existing diffraction chamber (Doering et al., 2011[Doering, D. et al. (2011). Rev. Sci. Instrum. 82, 073303.]) which is now permanently located at the Linac Coherent Light Source (LCLS). The system incorporates a 3+2-circle diffractometer which can move a detector anywhere along the surface of the Ewald sphere. Currently, APDs are being used to detect the soft X-ray photons; however, we plan on improving the setup by utilizing a multi-channel plate (MCP) as well.

The sample goniometer has three-axis linear motion, and all three angular degrees of freedom (θ, χ and φ) available for adjustment. In addition, the sample is attached to a liquid-helium-flow cryostat to adjust the temperature of the sample from 15 to 350 K. The whole diffraction chamber is mounted to a six-strut system for alignment and includes a load lock for interchanging samples without venting the system. The chamber can maintain pressures of 10-9 Torr without cooling. The entire system has been integrated with an operating system to fully control all aspects of the system while taking measurements remotely from outside the enclosed X-ray hutch. The system is one of the endstations for use by the general user community at the SXR instrument (Schlotter et al., 2012[Schlotter, W. F. et al. (2012). Rev. Sci. Instrum. 83, 043107.]). This SXR instrument delivers pulses up to about 1 mJ per pulse to the endstation, depending on the photon energy range of 285 eV–2 keV (Tiedtke et al., 2014[Tiedtke, K. et al. (2014). Opt. Express, 22, 21214-21226.]). The degree of monochromaticity can be tuned (Heimann et al., 2011[Heimann, P. et al. (2011). Rev. Sci. Instrum. 82, 093104.]) with pulse durations ranging from less than 10 fs up to a few hundred fs, and the instrument includes an array of timing diagnostics (Krupin et al., 2012[Krupin, O. et al. (2012). Opt. Express, 20, 11396-11406.]; Beye et al., 2012[Beye, M. et al. (2012). Appl. Phys. Lett. 100, 121108.]), absolute pulse energy calibration (Moeller et al., 2015[Moeller, S., Brown, G., Dakovski, G., Hill, B., Holmes, M., Loos, J., Maida, R., Paiser, E., Schlotter, W., Turner, J. J., Wallace, A., Jastrow, U., Kreis, S., Sorokin, A. A. & Tiedtke, K. (2015). J. Synchrotron Rad. 22, 606-611.]), and a KB optical system to adjust the X-ray spot size down to a few microns (Chalupsky et al., 2011[Chalupsky, J., Bohacek, P., Hajkova, V., Hau-Riege, S., Heimann, P., Juha, L., Krzywinski, J., Messerschmidt, M., Moeller, S., Nagler, B., Rowen, M., Schlotter, W., Swiggers, M. & Turner, J. (2011). Nucl. Instrum. Methods Phys. Res. Sect. A, 631, 130-133.]). For more information on the capabilities of the SXR instrument and an overview of some of the experiments that have been carried out using it, cf. Dakovski et al. (2015[Dakovski, G. L., Heimann, P., Holmes, M., Krupin, O., Minitti, M. P., Mitra, A., Moeller, S., Rowen, M., Schlotter, W. F. & Turner, J. J. (2015). J. Synchrotron Rad. 22, 498-502.]).

The newly developed instrument is shown in Figs. 1[link] and 2[link]. The main focus of the current setup is the positioning and control of a large THz focusing mirror assembly very close to the sample in-vacuum. We address this by mounting a 2 inch parabolic mirror with a 2 inch effective focal length nominally 2.25 inches from the sample to optimize a slightly diverging beam at the center of the chamber. This directs a strong THz excitation pulse onto the sample for a pump–probe experimental geometry. Using a short-focal-length optic very close to the sample enables near-diffraction-limited THz spot sizes, as small as 300 µm for DSTMS crystal THz generation (see below), and has increased the available THz field strength by a factor of 20 compared with previous measurements where the focusing optics were located outside the vacuum chamber. The focal distance, as well as the two directions transverse to the beam, can all be optimized remotely by three orthogonal, in-vacuum linear stages (Micos VT-80, custom). The focusing optic has a small hole through the center, approximately 3 mm in diameter, to allow the X-ray beam to illuminate the sample in a collinear geometry with the THz excitation. The in-vacuum linear stages allow for alignment of the hole to the beam, as well as optimization of the focal distance from the optic to the sample. All three stages have a range of 100 mm (P/N 6230Z018), except for the vertical motion which has a range of 25 mm (Micos VT-80 custom, P/N 62305050), limited by the chamber height. The mirror system is cantilevered off the side of the chamber to place the mirror near the center of the chamber and the focus axis collinear to the incoming X-ray beam.

[Figure 1]
Figure 1
Photograph showing the new in-vacuum optics and motorization together with the cryostat and sample manipulator with the detector arm. This view is in the middle of the two incoming beams, 45° from both the incoming THz beam as well as to the incoming X-ray beam which travels through the small hole in the back of the cantilevered focusing mirror. The view is parallel to the support which cantilevers the setup from the wall of the vacuum chamber in the center of the interaction region. Also seen are the detectors on the support arm and the timing crystals which hang below the sample.
[Figure 2]
Figure 2
The model of the upgrade for the new THz excitation instrument. The blue components are the mechanisms designed to move the mirror in three dimensions and adjust the angle of the mirror with three angular degrees of freedom with respect to the incoming THz beam (shown in blue). The red components show the X-ray detectors, both the APDs and the MCP (future), used to detect scattered X-rays (shown in red).

The instrument also has a control system to change the angles of the THz focusing mirror assembly remotely. The most important rotation is the degree of freedom that translates the THz focus vertically across the sample, because it must be set such that the collinear X-rays are unobstructed to the sample as well as ensuring spatial overlap between the THz and X-ray beams. This motion is controlled via a 2 inch-diameter in-vacuum rotary stage (Newport Agilis Piezo rotation stage: P/N AG-PR100V6). The degree of freedom that rotates the focus across the sample, horizontally, is controlled by a picomotor (NewFocus picomotor: P/N 8301-UHV). The adjustment to this motion is not as critical and is typically set at the start of the experiment and not moved as frequently. The third angle is the roll of the focusing mirror and is set manually.

There are a number of ways to generate high-field THz pulses (Hwang et al., 2014[Hwang, H. Y., Fleischer, S., Brandt, N. C., Perkins, B. G., Liu, M., Fan, K., Sternbach, A., Zhang, X., Averitt, R. D. & Nelson, K. A. (2014). J. Mod. Opt., doi:10.1080/09500340.2014.918200.]), including using the LCLS itself (Daranciang et al., 2011[Daranciang, D., Goodfellow, J., Ghimire, S., Loos, H., Reis, D., Fisher, A. S. & Lindenberg, A. M. (2011). CLEO: 2011 - Laser Applications to Photonic Applications. OSA Technical Digest (CD), p. CMW7. Optical Society of America.]). We use a nonlinear organic crystal, 4-N,N-dimethylamino-4-N-methyl-stilbazolium 2,4,6-trimethylbenzenesulfonate (DSTMS), as a medium for nonlinear frequency conversion (Yang et al., 2007[Yang, Z., Mutter, L., Stillhart, M., Ruiz, B., Aravazhi, S., Jazbinsek, M., Schneider, A., Gramlich, V. & Günter, P. (2007). Adv. Funct. Mater. 17, 2018-2023.]). Strong THz pulses are achieved via optical rectification of mJ-level pulses centered around 1.5 µm in wavelength (Hauri et al., 2011[Hauri, C. P., Ruchert, C., Vicario, C. & Ardana, F. (2011). Appl. Phys. Lett. 99, 161116.]). A Ti:sapphire-based ultrafast laser system synchronized to the FEL delivers up to 15 mJ of 50 fs (FWHM) pulses centered at 800 nm to a high-power optical parametric amplifier (OPA) (Minitti et al., 2015[Minitti, M. P. et al. (2015). J. Synchrotron Rad. 22, 526-531.]). The signal of the OPA was tuned to 1.5 µm at 50 fs with a maximum output of 2.0 mJ per pulse to enable efficient THz generation in a 400 µm-thick DSTMS crystal. This produces nearly single cycle THz pulses with energies of a few µJ and peak brightness at 2 THz.

The THz-generation crystal is situated in a nitrogen-purged environment outside the main vacuum chamber. The THz beam is transported into the chamber through a polymer window that is transparent for both THz and visible light (Topas Advanced Polymers, part 6013S-04: Cyclic Olefin Copolymer), simplifying the alignment procedure. The field strength is measured by electro-optical sampling using an additional 800 nm probe beam overlapped with both the X-rays and the THz beam at the sample position. The polarization optics and detection for the 800 nm probe beam are located on the downstream end of the chamber, outside the vacuum system as in Kubacka et al. (2014[Kubacka, T. et al. (2014). Science, 343, 1333-1336.]). For more information on the general laser capabilities at the LCLS, cf. Minitti et al. (2015[Minitti, M. P. et al. (2015). J. Synchrotron Rad. 22, 526-531.]).

With the current setup, we can produce a measured peak THz electric field of 0.6 MV cm−1 using the new optical in-vacuum setup shown in Fig. 3[link], comparable with what is generated on a traditional optical setup (Yeh et al., 2007[Yeh, K.-L., Hoffmann, M. C., Hebling, J. & Nelson, K. A. (2007). Appl. Phys. Lett. 90, 171121.]). This was using a gold-coated aluminium mirror with a numerical aperture of 1/6. Field-strength calibration was performed via electro-optical sampling by inserting a 100 µm-thick (110)-cut GaP crystal in-vacuum mounted on the cryostat. We are currently developing methods to further increase the field strength by using different materials for THz generation (Hoffmann & Fülöp, 2011[Hoffmann, M. C. & Fülöp, J. A. (2011). J. Phys. D, 44, 083001.]).

[Figure 3]
Figure 3
Temporal electric field profile (a) of the THz pump pulse, measured by electro-optic sampling in gallium phosphide. The peak electric field is 0.6 MV cm−1 corresponding to a peak magnetic field of 200 mT. (b) The amplitude spectrum of the THz pump pulse in (a), showing the frequency content of the pulse.

An additional challenge with such a setup can be to measure the diffracted X-ray beam intensity adequately at the requisite point in reciprocal space without interfering with the focusing optics. Currently, two APDs are used for detection and are built in a custom-designed encasement which prevents unwanted optical and radio frequency signals. With a newly designed detector arm, the full range of motion can be explored with two adjacent APD detectors which can incorporate a slit or filter to block optical radiation. The distance to the sample can be adjusted from 10.2 cm to 17.8 cm depending on the nature of the experiment. The new design (see Fig. 2[link]) places the detector in the plane behind the focusing optic such that it can move freely behind the optical system with no interference. A fast area detector is being developed at the SLAC National Accelerator Laboratory (Blaj et al., 2015[Blaj, G. et al. (2015). J. Synchrotron Rad. 22, 577-583.]), which will have 0.5 megapixels over 2 cm2, and a readout frame rate of 120 Hz with 20 electrons of readout noise. With this technology, we will be developing a specific detector to incorporate into this setup for two-dimensional measurements, such as time-resolved coherent diffraction measurements in materials. Additionally, we are planning to have an MCP mounted on the detector stage for low-photon-count experiments.

4. Conclusion

New instrumentation has recently been commissioned at the SXR instrument to perform low-photon-energy THz pump/resonant soft X-ray diffraction probe measurements. With fully motorized in-vacuum optics, THz electric field strengths were improved by a factor of 20. The design has been developed to produce a versatile, general-purpose instrument for different excitation sources. Diffraction peaks can be measured at large angle without interference of the large optical elements close to the sample. The system described here has been commissioned and is now open to the general user community at the LCLS.

Acknowledgements

We would like to acknowledge Aymeric Robert and Bill White for careful reading of the manuscript. We would especially like to thank Greg Stewart for his help with the figures and Andy Freeberg for his photography. The SXR instrument is funded by a consortium whose membership includes the LCLS, Stanford University through the Stanford Institute for Materials Energy Sciences (SIMES), Lawrence Berkeley National Laboratory (LBNL), the University of Hamburg through the BMBF priority program FSP 301, and the Center for Free Electron Laser Science (CFEL). HYH would like to acknowledge support from the NSF, grant No. CHE-1111557. This research was carried out at the Linac Coherent Light Source (LCLS) at the SLAC National Accelerator Laboratory. LCLS is an Office of Science User Facility operated for the US Department of Energy Office of Science by Stanford University.

References

First citationBasov, D. N., Averitt, R. D., van der Marel, D., Dressel, M. & Haule, K. (2011). Rev. Mod. Phys. 83, 471–541.  Web of Science CrossRef CAS Google Scholar
First citationBernitt, S. et al. (2012). Nature (London), 492, 225–228.  Web of Science CrossRef CAS PubMed Google Scholar
First citationBeye, M. et al. (2012). Appl. Phys. Lett. 100, 121108.  Web of Science CrossRef Google Scholar
First citationBlaj, G. et al. (2015). J. Synchrotron Rad. 22, 577–583.  Web of Science CrossRef CAS IUCr Journals Google Scholar
First citationCaviglia, A. D. et al. (2013). Phys. Rev. B, 88, 220401.  Web of Science CrossRef Google Scholar
First citationChalupsky, J., Bohacek, P., Hajkova, V., Hau-Riege, S., Heimann, P., Juha, L., Krzywinski, J., Messerschmidt, M., Moeller, S., Nagler, B., Rowen, M., Schlotter, W., Swiggers, M. & Turner, J. (2011). Nucl. Instrum. Methods Phys. Res. Sect. A, 631, 130–133.  Web of Science CrossRef CAS Google Scholar
First citationChuang, Y. D. et al. (2013). Phys. Rev. Lett. 110, 127404.  Web of Science CrossRef PubMed Google Scholar
First citationDakovski, G. L., Heimann, P., Holmes, M., Krupin, O., Minitti, M. P., Mitra, A., Moeller, S., Rowen, M., Schlotter, W. F. & Turner, J. J. (2015). J. Synchrotron Rad. 22, 498–502.  CrossRef IUCr Journals Google Scholar
First citationDaranciang, D., Goodfellow, J., Ghimire, S., Loos, H., Reis, D., Fisher, A. S. & Lindenberg, A. M. (2011). CLEO: 2011 – Laser Applications to Photonic Applications. OSA Technical Digest (CD), p. CMW7. Optical Society of America.  Google Scholar
First citationDell'Angela, M. et al. (2013). Science, 339, 1302–1305.  Web of Science CAS PubMed Google Scholar
First citationDoering, D. et al. (2011). Rev. Sci. Instrum. 82, 073303.  Web of Science CrossRef PubMed Google Scholar
First citationFausti, D., Tobey, R. I., Dean, N., Kaiser, S., Dienst, A., Hoffmann, M. C., Pyon, S., Takayama, T., Takagi, H. & Cavalleri, A. (2011). Science, 331, 189–191.  Web of Science CrossRef CAS PubMed Google Scholar
First citationFörst, M., Frano, A., Kaiser, S., Mankowsky, R., Hunt, C. R., Turner, J. J., Dakovski, G. L., Minitti, M. P., Robinson, J., Loew, T., Le Tacon, M., Keimer, B., Hill, J. P., Cavalleri, A. & Dhesi, S. S. (2014a). Phys. Rev. B, 90, 184514.  Google Scholar
First citationFörst, M., Mankowsky, R., Bromberger, H., Fritz, D. M., Lemke, H., Zhu, D., Chollet, M., Tomioka, Y., Tokura, Y., Merlin, R., Hill, J., Johnson, S. & Cavalleri, A. (2013). Solid State Commun. 169, 24–27.  Google Scholar
First citationFörst, M. et al. (2011). Phys. Rev. B, 84, 241104.  Google Scholar
First citationFörst, M. et al. (2014b). Phys. Rev. Lett. 112, 157002.  Web of Science PubMed Google Scholar
First citationHauri, C. P., Ruchert, C., Vicario, C. & Ardana, F. (2011). Appl. Phys. Lett. 99, 161116.  Web of Science CrossRef Google Scholar
First citationHeimann, P. et al. (2011). Rev. Sci. Instrum. 82, 093104.  Web of Science CrossRef PubMed Google Scholar
First citationHoffmann, M. C. & Fülöp, J. A. (2011). J. Phys. D, 44, 083001.  Web of Science CrossRef Google Scholar
First citationHoffmann, M. C. & Turner, J. J. (2012). Synchrotron Radiat. News, 25, 17–24.  CrossRef Google Scholar
First citationHwang, H. Y., Fleischer, S., Brandt, N. C., Perkins, B. G., Liu, M., Fan, K., Sternbach, A., Zhang, X., Averitt, R. D. & Nelson, K. A. (2014). J. Mod. Opt., doi:10.1080/09500340.2014.918200.  Google Scholar
First citationJohnson, S. L. et al. (2012). Phys. Rev. Lett. 108, 037203.  Web of Science CrossRef PubMed Google Scholar
First citationJong, S. de et al. (2013). Nat. Mater. 12, 882–886.  Web of Science PubMed Google Scholar
First citationKampfrath, T., Tanaka, K. & Nelson, K. A. (2013). Nat. Photon. 7, 680–690.  Web of Science CrossRef CAS Google Scholar
First citationKern, J. et al. (2013). Science, 340, 491–495.  Web of Science CrossRef CAS PubMed Google Scholar
First citationKonings, S., Schüssler-Langeheine, C., Ott, H., Weschke, E., Schierle, E., Zabel, H. & Goedkoop, J. B. (2011). Phys. Rev. Lett. 106, 077402.  Web of Science CrossRef PubMed Google Scholar
First citationKrupin, O. et al. (2012). Opt. Express, 20, 11396–11406.  Web of Science CrossRef CAS PubMed Google Scholar
First citationKubacka, T. et al. (2014). Science, 343, 1333–1336.  Web of Science CrossRef CAS PubMed Google Scholar
First citationLee, W. S. et al. (2012). Nat. Commun. 3, 838.  Web of Science CrossRef PubMed Google Scholar
First citationMinitti, M. P. et al. (2015). J. Synchrotron Rad. 22, 526–531.  CrossRef IUCr Journals Google Scholar
First citationMoeller, S., Brown, G., Dakovski, G., Hill, B., Holmes, M., Loos, J., Maida, R., Paiser, E., Schlotter, W., Turner, J. J., Wallace, A., Jastrow, U., Kreis, S., Sorokin, A. A. & Tiedtke, K. (2015). J. Synchrotron Rad. 22, 606–611.  Web of Science CrossRef CAS IUCr Journals Google Scholar
First citationRedecke, L. et al. (2013). Science, 339, 227–230.  Web of Science CrossRef CAS PubMed Google Scholar
First citationSchlotter, W. F. et al. (2012). Rev. Sci. Instrum. 83, 043107.  Web of Science CrossRef PubMed Google Scholar
First citationSeu, K. A., Roy, S., Turner, J. J., Park, S., Falco, C. & Kevan, S. D. (2010). Phys. Rev. B, 82, 012404.  Web of Science CrossRef Google Scholar
First citationStaub, U. et al. (2014). Phys. Rev. B, 89, 220401.  Web of Science CrossRef Google Scholar
First citationTiedtke, K. et al. (2014). Opt. Express, 22, 21214–21226.  Web of Science CrossRef CAS PubMed Google Scholar
First citationTobey, R. I. et al. (2012). Phys. Rev. B, 86, 064425.  Web of Science CrossRef Google Scholar
First citationTurner, J. J., Thomas, K. J., Hill, J. P., Pfeifer, M. A., Chesnel, K., Tomioka, Y., Tokura, Y. & Kevan, S. D. (2008). New J. Phys. 5, 053023.  Web of Science CrossRef Google Scholar
First citationVartanyants, I. A. et al. (2011). Phys. Rev. Lett. 107, 144801.  Web of Science CrossRef PubMed Google Scholar
First citationVinko, S. M. et al. (2012). Nature (London), 482, 59–62.  Web of Science CrossRef CAS PubMed Google Scholar
First citationYang, Z., Mutter, L., Stillhart, M., Ruiz, B., Aravazhi, S., Jazbinsek, M., Schneider, A., Gramlich, V. & Günter, P. (2007). Adv. Funct. Mater. 17, 2018–2023.  Web of Science CSD CrossRef CAS Google Scholar
First citationYeh, K.-L., Hoffmann, M. C., Hebling, J. & Nelson, K. A. (2007). Appl. Phys. Lett. 90, 171121.  Web of Science CrossRef Google Scholar

This is an open-access article distributed under the terms of the Creative Commons Attribution (CC-BY) Licence, which permits unrestricted use, distribution, and reproduction in any medium, provided the original authors and source are cited.

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
Follow J. Synchrotron Rad.
Sign up for e-alerts
Follow J. Synchrotron Rad. on Twitter
Follow us on facebook
Sign up for RSS feeds