
Attosecond science based on high harmonic generation from gases and solids
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ABSTRACT Recent progress in high power ultrafast short-wave and mid-wave infrared lasers has enabled gas-phase high harmonic generation (HHG) in the water window and beyond, as well as the
demonstration of HHG in condensed matter. In this Perspective, we discuss the recent advancements and future trends in generating and characterizing soft X-ray pulses from gas-phase HHG and
extreme ultraviolet (XUV) pulses from solid-state HHG. Then, we discuss their current and potential usage in time-resolved study of electron and nuclear dynamics in atomic, molecular and
condensed matters. SIMILAR CONTENT BEING VIEWED BY OTHERS ULTRAFAST HIGH-HARMONIC SPECTROSCOPY OF SOLIDS Article 10 October 2024 HOW TO OPTIMIZE HIGH-ORDER HARMONIC GENERATION IN GASES
Article 13 October 2022 BRIGHT CONTINUOUSLY TUNABLE VACUUM ULTRAVIOLET SOURCE FOR ULTRAFAST SPECTROSCOPY Article Open access 11 January 2024 INTRODUCTION Tabletop attosecond light sources in
the soft X-ray (SXR) spectral region based on high-harmonic generation are highly desirable in chemical and material sciences since they can spectroscopically identify specific elements, as
well as the oxidation states, charge states and even the spin states of those elements1. One of the important spectral regions is the “water window” (282–533 eV), which covers the atomic
K-shell excitation of carbon and oxygen. Although high harmonics in the water window were first generated with Ti:Sapphire lasers centered at 800 nm more than 20 years ago2,3, the X-ray
photon flux was too low for time-resolved applications. The mechanism of HHG in gases can be explained by the semiclassical three-step model4,5,6. When driving laser-field strength reaches
~108 V m−1, the bound electron in the atomic gas can tunnel through the Coulomb potential barrier and become a free electron. In the oscillating laser field, the free-electron wave packet
may return to its parent ion with the right time of birth. At recombination, the interference between the wave packets of the returning and bound electrons produces an oscillating dipole
that emits attosecond radiation. Returning electrons with various kinetic energy will recombine at different times giving rise to the chirp in the attosecond radiation7. This process repeats
twice for every optical cycle. The temporal beating of attosecond pulses results in the high-harmonic combs in the spectral domain. Empowered by the advances in driving lasers with center
wavelengths around 1.8 μm, soft X-ray high harmonics can be generated with a moderate intensity of 1014 W cm−2 (see Box 1 for details). Significant progress has recently been made in
developing attosecond light within the water window8. By spectrally broadening pulses from an Optical Parametric Amplifier (OPA) using a gas-filled hollow-core fiber9 or by broadband phase
matching in an Optical Parametric Chirped Pulse Amplifier (OPCPA)10, two-cycle, mJ-level pulses centered with 1 kHz repetition rate are now generated in many laboratories8. Seed pulses for
such light source can be produced by intra-pulse difference frequency generation (DFG)11 with stable carrier–envelope phase. In 2010 HHG has also been realized in condensed matter systems
using mid-infrared laser fields12. Since then, there has been significant attention on this field in investigating the underlying microscopic mechanism of solid-state HHG. Its promises
include stable attosecond light sources in compact forms and the possibility of attosecond metrology in solid-state materials13,14. A string of experimental surprises in solid-state HHG
include anomalous ellipticity dependence15, observation of a multiple plateau feature16 and orthogonally polarized high harmonics17. XUV harmonics from certain solid materials such as SiO2
crystals were found to be immune to fluctuations in the driving pump laser, providing a novel path toward stable attosecond pulses18. There are many exciting initiatives involving the
exploitation of microscopic generation processes in high-harmonic spectroscopy (HHS) of materials, including all-optical probing of the valence charge density in the real space15,19 and
electronic band structure in the reciprocal space20. Other unique features include the use of engineered materials at the nanometer scale to enhance, control, and manipulate the generation
process. HHS provides a novel approach to probe active electrons on nanoscale devices and on the surface state of quantum materials such as topological insulators. In this perspective, we
will first discuss the recent progress, challenges, and future trends in the development of gas-phase attosecond X-ray sources in the water window, followed by an extensive discussion on
their applications in molecular systems and condensed matter. Then, we will briefly review novel microscopic dynamics underlying solid-state HHG and discuss their applications in
high-harmonic spectroscopy of condensed matter systems both in and out-of-equilibrium. BOX 1 PHOTON ENERGY OF THE HIGH-HARMONIC SPECTRUM The highest photon energy (cutoff photon energy) from
gas-phase HHG can be estimated by $$\hbar \omega _{\mathrm{c}}\left[ {eV} \right] = I_{\mathrm{p}} + 3 \times 10^{ - 13}I_0\lambda _{\mathrm{L}}^2,$$ (1) where _I_p is the ionization
potential of the gas atom expressed in eV. The peak laser intensity \(I_0\) is in W cm−2, and the driving laser wavelength, \(\lambda _{\mathrm{L}}\), is in μm. Due to quantum diffusion, the
single-atom efficiency decreases with the driving laser wavelength (~\(\lambda _{\mathrm{L}}^{ - 6}\))41. The peak laser intensity is set for phase matching the HHG process to achieve high
photon flux, where the negative plasma dispersion is balanced by the unionized portion of the target gas. The calculated cutoff photon energy for noble gases at different laser wavelengths
is depicted in the figure below. This shows that the HHG spectrum can cover the water window by using short-wave infrared (SWIR) lasers144,145. Ionization induced plasma defocusing tends to
clamp laser intensity and reshape the radius profile146,147. The achievable SXR spectrum is therefore a collaborative result of atomic response and coherent buildup of high-harmonic
strength. WAVELENGTH SCALING OF HHG CUTOFF PHOTON ENERGY. Calculated cutoff photon energy of HHG under the phase-matching condition from various inert gases driven by lasers at different
center wavelengths. The purple square, blue dot, and red triangle indicate the achievable cutoff photon energy by using a 0.8 μm, 1.6 μm, and 2.5 μm driving laser, respectively. ISOLATED
WATER WINDOW X-RAY ATTOSECOND PULSES Single isolated attosecond pulses (IAP) are needed for conducting pump–probe measurements, such as attosecond streaking and attosecond
transient-absorption spectroscopy21,22,23,24. Various gating techniques have been developed to obtain such pulses (Table 1), and some of them have been implemented to generate isolated water
window X-ray bursts. SUBCYCLE GATING TECHNIQUES The simplest method to isolate a single attosecond burst from a few-cycle driving field is the amplitude gating (AG)25. In AG, with a proper
carrier–envelope phase value, the strongest half-cycle of the driving field will produce the attosecond burst with the broadest spectrum that exceeds all other bursts. By selecting a
suitable filter that transmits only this cutoff spectrum, an IAP can be achieved. AG has been adapted for the few-cycle short-wave infrared laser to demonstrate water window IAP10,26,27,28.
The width of the continuum near the cutoff can be estimated by $${\mathrm{\Delta }}\hbar \omega _{\mathrm{c}}[eV] = 3 \times 10^{ - 13}{\mathrm{\Delta }}I_{\mathrm{L}}\lambda
_{\mathrm{L}}^2,$$ (2) where \({\mathrm{\Delta }}I_{\mathrm{L}}\) is the intensity difference between the most intense half-cycle and the neighboring half-cycles of the driving laser field.
Future efforts will be made to increase this intensity by reducing the SWIR driving laser-pulse duration from the current state-of-the-art, ~two cycle, to just a single cycle. It is clear
from Eq. (2) that a much broader continuum can be obtained by using a longer wavelength driving laser for a given intensity difference. Highly efficient Chirped Pulse Amplification lasers
based on gain media such as Cr:ZnSe at 2.5 μm and Fe:ZnSe at 4 μm may extend the attosecond spectrum to O K-edge29,30,31. Spectral filtering methods, such as AG and ionization gating (IG)32,
can only isolate IAPs near the HHG spectrum cutoff. Techniques based on the temporal gating of the HHG process can generate an attosecond supercontinuum that covers both the plateau and
cutoff spectrum portion. The most common temporal gating method is polarization gating (PG)33,34. The influence of field ellipticity on HHG suppression increases as the driving wavelength
increases35. PG has the potential for generating ultra-broadband SXR pulses36, which may support even shorter attosecond sources in the future. Unfortunately, in PG, a substantial amount of
laser energy is wasted37. To reduce loss, the double optical gating (DOG) technique was proposed38. In DOG, a second harmonic field is added to break the fundamental field’s symmetry in a
process known as two-color gating39. A stronger IAP in the water window can be expected by applying the DOG40. CHARACTERIZATION OF ATTOSECOND PULSES Due to the low conversion efficiency
(~10−6) in gas-phase41 high-harmonic generation, attosecond pulse metrology relies on the photon ionization of the gas media by a weak IAP in the presence of a perturbative infrared (IR)
pulse. The photoelectron will gain (lose) energy by absorbing (emitting) one or more IR photons, depending on their relative delay. This technique, named attosecond streaking24, can
characterize an IAP after its birth. The unknown attosecond spectral phase information is encoded in the perturbed photoelectron energy spectrogram and can now be retrieved using the
frequency-resolved optical gating for complete reconstruction of attosecond bursts (FROG-CRAB) technique42, which is suitable for narrowband pulses. Alternative techniques are available for
characterizing broadband pulses43,44,45,46. Statistical noise in the streaking traces pose a challenge to reliable phase retrieval. For instance, large discrepancies are found in the pulse
duration and spectral phase when different phase retrieval schemes are applied47. Previous attosecond phase-retrieval schemes are based on time-consuming iterative algorithms. It is expected
that deep neuron network (DNN) algorithms will significantly cut down retrieval time46. Streaking measurements are affected by space charge effects. SWIR OPA/OPCPA lasers based on
high-average-power diode-pumped thin disc/slab Yb lasers48 provide a promising approach to deliver high-repetition-rate and high-flux attosecond pulses in the water window. This will
significantly improve the signal to noise ratio of streaking traces. ATTO-CHIRP COMPENSATION In HHG experiments, usually the short quantum pass survives through the macroscopic phase
matching resulting in attosecond pulses with a positive chirp49. Such chirp can be compensated by the negative group delay dispersion (GDD) of thin foils or neutral gases50. Recently,
isolated 53-as X-ray pulses whose spectra cover the 100–300 eV range have been characterized by attosecond streaking36. It is, however, difficult to compensate atto-chirp above the carbon
K-edge (282 eV) due to the lack of materials that exhibiting negative group velocity dispersion and low loss. It was illustrated theoretically that atto-chirp in the 300–1000 eV range can be
reduced by hydrogen gas or plasma with the proper pressure–length product given that the transmission of the gas or plasma is higher than 10%51,52. The GDD of neutral molecular hydrogen gas
at the photon energy \(\hbar \omega _{\mathrm{x}}\) can be expressed $$GDD_{{\mathrm{H}}_2}\left( {\hbar \omega _{\mathrm{x}}} \right) = 1.509 \times 10^9\frac{{PL}}{{\left( {\hbar \omega
_{\mathrm{x}}} \right)^3}},$$ (3) where pressure, _P_, is in atm, length, _L,_ is in cm, and photon energy, ℏ_ω_x, is in eV. As an example, to compensate a 1600 as2 chirp at 365 eV, the
required pressure–length product is 54-atm cm, which is experimentally feasible. Hydrogen is preferred because of its low absorption in the SXR region compared with other materials. Uranium
foil also exhibits negative GDD beyond 300 eV53, but its absorption is much higher than H2, as shown in Fig. 1. Their dispersion values are the same at 350 eV. The peak transmission of U
foil is <10−3 to compensate a 290 as2 atto-chirp, where the transmission of H2 is 80%. The transmission of ionized H2 is even better. Single-atom simulations based on the strong-field
approximation54,55,56,57,58 of high-harmonic generation have been performed to demonstrate feasibility of the atto-chirp compensation in the 300–500 eV51 and 530–1000 eV52 photon energy
regions. It has been shown that isolated attosecond pulses as short as 25-as are achievable when high-harmonic generation in helium is driven by single-cycle lasers centered at 1.7 μm or 3.2
μm. The effectiveness of the chirp compensation by H2 plasma has been validated by simulations that account for phase macroscopic effects59. Experimental demonstration of such a chirp
compensation scheme may yield milestone results. Efforts need to be made to find schemes that can compensate the third-order phase error. Atto-chirp can also be reduced in the HHG process by
reshaping the driving field waveform using a multicolor synthesizer with controlled CEP and delay. Simulation has shown that nearly 60 pulses can be achieved in the 300–500 eV energy range
without atto-chirp compensation53. This technique is also promising for atto-chirp suppression in keV range. APPLICATIONS OF ATTOSECOND X-RAY SOURCES Attosecond XUV sources driven by
Ti:Sapphire lasers have been extensively used to study dynamics of electrons with less than 150 eV binding energy60. Femtosecond transient-absorption experiments with HHG sources at the
carbon K-edge have recently been reported, revealing molecular structural deformation processes that happen on a 50–100-fs timescale61,62. Attosecond water window X-ray sources have recently
enabled the observation of electronic processes in Ar atom at the L-edge (~250 eV)63, and in TiS2 films at the Ti L-edge (~460 eV)64. Ionization, vibration, and rotation dynamics have been
resolved in NO molecules using attosecond transient-absorption spectroscopy at the Nitrogen K-edge (~400 eV)65, as shown in Fig. 2. It is anticipated that more experiments will be conducted
to study charge dynamics in molecules and materials whose absorption edges are in the water window region66. Here, we discuss a few important applications. CHARGE MIGRATION IN MOLECULES AND
WAVE-PACKAGE DYNAMICS AT CONICAL INTERSECTIONS Comprehensive numerical simulations of electron dynamics in polyatomic molecules have predicted that when an electron is suddenly removed from
one end of a chain molecule, the hole can move to the other end in a few fs, often before electron–nuclear coupling sets in refs. 67,68. This purely electronic ultrafast dynamic process is
termed charge migration, a convention introduced in ref. 67, which should be distinguished from charge transfer, a slower spatial redistribution of electronic charge involving nuclear motion
that leads to charge relocation permanently from a donor to an acceptor. Charge migration is the first step in the fundamental process of electron transfer, which plays a role in
photochemistry, biology, and photovoltaics. Due to the coupling between the electron and nuclear motion, it may be possible to control the chemical reactivity of molecules by manipulating
their electronic motion as in the subfield dubbed attochemistry69. Observation of charge migration requires the preparation of a coherent superposition of electronic states and experimental
tools with sufficient temporal resolution to follow charge dynamics occurring on electronic timescales. This remains a grand challenge. Only a few experimental observations of charge motion
in molecules have so far been reported70,71. Numerical simulations predicted that charge migration occurs in many complex organic molecules67,68,72,73,74,75. However, almost none of them
have been verified experimentally due to the lack of experimental tools. The attosecond water window X-ray sources and transient-absorption spectroscopy provide a unique opportunity to
verify these predictions. They would allow probing charge migration in molecules containing C, N, and O atoms, the halogen atoms such as Cl, Br, and I, with attosecond time resolution.
Moreover, they would allow experimentalists to monitor the interplay of charge migration and nuclear motion on femtosecond timescales76. X-ray spectroscopy is element-specific and oxidation-
and charge-state sensitive77. Thus, SXR provide a powerful means to measure the charge states and charge migration between atoms. The individual atoms within a molecule exhibit X-ray energy
shifts, which depend on either the local chemical bonding environment or the electronic coherences themselves as charges migrate around a molecule. It is necessary to validate new
experimental tools by observing charge migration in simple molecules first and then to demonstrate their unique advantages by comparing them to previous methods. Charge migration in an
iodoacetylene cation has been observed in C2HI+ using high-harmonic spectroscopy71, where the high-harmonic XUV spectrum itself is measured as a function of pump–probe time delay after a
strong ionizing pulse. High-harmonic spectroscopy is based on the predictions of the semiclassical model of HHG that relate photon energy of a harmonic peak to the time difference between
the tunneling ionization (pump) and the photon emission (probe)78. When C2HI is ionized within a fraction of an optical cycle by the electric field of an intense infrared laser pulse, a
coherent electronic superposition state is created that can be expressed as an orbital mixture of the HOMO and HOMO-1 ground-state orbitals of the neutral molecule. $${\mathrm{\Psi
}}_{{\mathrm{MIX}}}\left( {{\mathbf{r}},t} \right) = \frac{1}{{\sqrt 2 }}\left[ {\phi _{{\mathrm{HOMO}}}\left( {\mathbf{r}} \right)e^{ - iE_{{\mathrm{HOMO}}}t/\hbar } + \phi
_{{\mathrm{HOMO}} - 1}\left( {\mathbf{r}} \right)e^{ - iE_{{\mathrm{HOMO}} - 1}t/\hbar }} \right].$$ (3) Numerical simulations show that ionization from the HOMO/HOMO-1 superposition of
states leads to characteristic charge oscillations with a period of ~2 fs. The dynamics of the electron hole reconstructed from the HHG measurements is shown in Fig. 3a71. By definition,
charge migration is periodic in the absence of dephasing or relaxation. Permanent charge transfer, on the other hand, requires electronic dephasing. One of the most important questions in
the study of charge migration is the lifetime of the electronic coherence that drives charge migration especially in the presence of vibrational motion. Numerical simulations suggest that
the charge migration induced by strong-field ionization lasts for at least 28 fs in C2HI+, as shown in Fig. 3b79. Such a prediction has not been confirmed by high-harmonic spectroscopy
measurements due to the limited time range of the measurements. The temporal window of the measurement is determined by the optical cycle of the driving lasers. This deficiency can be
addressed by X-ray transient absorption. Charge migration in C2HCl+, C2HBr+, and C2HI+ can be investigated using HHG-based attosecond water window X-rays. The scheme is shown in Fig. 3c.
Like in the HHG spectroscopy experiments, the electronic superposition state can be formed by ionization of the molecules with a strong IR laser pulse. However, here the hole motion will be
monitored by an X-ray probe using the transient-absorption method. Thanks to the broad X-ray supercontinuum from the HHG source, absorptions at the C K-edge and the I N-edge, Br M-edge, or
Cl L-edge can be measured simultaneously. Since the adjacent atoms of the two carbons are different, the absorption due to the core-to-valence transition should also be different. The motion
of the hole from one carbon to another carbon, and then to the iodine or chlorine will be monitored by the temporal variation of these absorptions. The temporal window in the X-ray
transient-absorption measurements can easily cover 100 fs or longer65. Therefore, the femtosecond decoherence process may be observed as well. The Born–Oppenheimer approximation is commonly
used in quantum chemistry to separate fast electronic dynamics from slow nuclear motions. However, it breaks down at conical intersections where two or more potential energy surfaces are
degenerate. Consequently, the coupling between electronic and nuclear motion must be considered in simulating the processes. Understanding charge dynamics around the conical intersections is
important for studying photosynthesis and other photon-initiated processes. Although energy surface crossings are ubiquitous in photochemistry80, material science81, and biology82, direct
observation of non-adiabatic dynamics at conical intersections with water window X-rays remains experimentally challenging. Neville et al. reported numerical simulations that show attosecond
transient absorption at the carbon K-edge is a powerful tool to study wave-package dynamics at a conical intersection of C2H2 molecules83. Experimental validation of theoretical predictions
of such simple molecules will pave the way to the investigation of more complex biological systems. PROBING CHARGE TRANSFER IN ORGANIC PHOTOVOLTAIC MATERIALS Organic photovoltaic materials
have received extensive research attention due to low fabrication cost, large area production, light weight, and flexibility. One type of organic solar cell consists of two different organic
molecules, namely donor and acceptor, that are mixed on the molecular level in a bulk-heterojunction structure. The most well-studied materials are poly(3-hexylthiophene-2,5-diyl) (P3HT) as
a donor, and [6,6]-phenyl-C61-butyric acid methyl ester (PC61BM) as an acceptor. The electron transfer from donor to acceptor needs to be fast to compete with lossy processes, such as
radiative and nonradiative recombination. Another important photovoltaic device is the dye-sensitized solar cell in which organic dyes such as N3, N719, and 2-picolinic acid are adsorbed
onto the electron transport layer such as TiO2 to enhance the charge transfer84,85, as illustrated in Fig. 4a. In a strongly coupled system, the charge injection from the organic dye
molecules to TiO2 takes place in 3–30 fs86,87, exceeding the instrument limit of femtosecond lasers that are the primary tool to time-resolve these processes at present88,89. Attosecond
pulses are poised to become a powerful technique to better understand such ultrafast dynamic processes involved in improving the efficiency and functionality of solar cell materials and
devices. Attosecond X-ray absorption spectroscopy can probe resonant transitions between core electrons and unoccupied states in the valence shells of molecules, as well as the valence and
conduction band of semiconductors. By utilizing a visible/UV pump with an attosecond soft X-ray probe, the electron transfer on timescales commensurate with electron and nuclei motion can be
investigated. For molecules adsorbed onto TiO2, a few-fs UV or visible pulse can be used as the pump. During the excitation, the absorption of LUMO at the C or N K-edges (~285 eV or ~400
eV) should decrease. When the electrons move to the TiO2, the absorption in the conduction band probed by the Ti L-edge (~460 eV) should decrease. At the same time, the absorption of the
LUMO at the C or N K-edges should increase, as shown in Fig. 4. The attosecond X-ray transient absorption at the C, N, and Ti edges could be a unique tool to measure the electron-transfer
time of the strongly coupled system. The spatial localization of the 1s shell of C and N or the 2p shell of Ti means that excitation of electrons from these shells by attosecond X-ray pulses
to valence electronic states provides an atomic-site-specific probe of transient valence electron/hole populations. Similar pump–probe scheme can be applied to study charge transfer between
donors and acceptors in organic bulk-heterojunction solar cells. CONTROLLING DIELECTRIC PROPERTIES OF SOLIDS The electronic properties of matter can be modified drastically from its
equilibrium state by intense laser pulses. In 2011, a substantial redshift on the band-edge (>10% of the bandgap) was reported in bulk ZnO crystals subjected to intense mid-infrared laser
fields90. The shift was measured using a broadband ultraviolet light source in a pump–probe transient-absorption setting. In other independent studies, attosecond XUV pulses were used to
probe the dynamical absorption, on the subcycle timescale of the driving laser field, using thin Si91 as well as diamond92. Reversible semi-metallization of insulating materials has been
demonstrated in 2013, when SiO2 was illuminated with intense few-cycle near-infrared Ti:Sapphire-laser pulses93. A semi-metallization model was proposed to explain the transient-absorption
experiments at the Si L-edge (100–110 eV) that was covered by the spectral range of the Ti:Sapphire-laser-driven attosecond pulses. The attosecond water window X-ray source will allow
simultaneous measurements at both the Si L-edge and the O K-edge (533 eV) in transient-absorption experiments. This could provide the evidence of correlated charge motion at the Si and O
sites to deepen the understanding of the physical mechanism. Other materials such as diamond, BN, and Si3N4 can also be investigated in the similar manner. Controlling electrical
conductivity of solids at the timescale of an optical cycle allows a way to extend the speed of optoelectronics into the petahertz (1015 Hz) domain94, far exceeding the limit of current
field-effect transistor-based semiconductor electronics. This is critical to applications of high-speed all-optical signal processing and to the development of optical-field-effect
devices95,96. HIGH-HARMONIC SPECTROSCOPY OF CONDENSED MATTER High-harmonic spectroscopy has been widely used in atomic and molecular systems97, but that knowledge cannot be directly
implemented in condensed matter systems because underlying microscopic dynamics are different. In solid-state materials, the laser field-driven electrons are in the proximity of the periodic
Coulomb potential, so the usual strong-field approximation98, which is the foundation of the three-step re-collision model4,5, becomes qualitatively invalid. Recently, a real-space electron
trajectory model has been developed that considers the role of the periodic potential on the semiclassical motion of the electron and includes the possibility of coherent collisions with
the neighboring atomic sites15,19. In this picture, harmonic emission becomes stronger (weaker) when electron trajectories strike (miss) the atomic cores of nearest-neighbor atoms. A typical
experimental setup for such spectroscopy is shown in Fig. 5a. In this particular example, a wide-bandgap MgO crystal is pumped with a NIR laser pulse, and XUV harmonics are analyzed as a
function of crystal orientation and laser ellipticity. The real-space electron trajectory model describes the observed crystal orientation dependence, ellipticity dependence, and therefore
provides the opportunity to probe the valence charge density distributions inside bulk materials in all-optical settings15,19. Because the electron trajectories can be controlled by laser
parameters (field strength, polarization, and wavelength), the real-space picture provides a powerful, all-optical, and tabletop approach to probe valence charge density distributions in
bulk materials. Dynamics in solid-state materials are often described in reciprocal or momentum space. In this framework, non-perturbative high-order harmonics originate mainly from two
channels, namely the intraband nonlinear current and the interband polarization, as shown schematically represented by simple cosine bands of opposite mass across a direct bandgap in Fig.
614. Initially, the valence band is full, and the conduction band is empty. Upon photoexcitation, an electron–hole pair is created at the zone center (_k_ = 0) by tunneling across the
minimum bandgap. Then, both the electron and the hole are accelerated by the electric field towards the zone edge. At high-enough peak-field strength, the electrons can reach the zone edge
(_k_ = π/a, where a is the lattice constant) and be Bragg diffracted, even multiple times every half-cycle. For nonparabolic bands such intraband current can radiate at much higher
frequencies than the fundamental driving frequency. Similarly, the electron and hole can recombine at later time at higher crystal momentum locations, as shown by the dashed arrow, releasing
a high-energy photon99,100. Often at high peak fields these dynamics get coupled. Through the intraband channel, the dispersion of a responsible conduction band can be probed, as proposed
by Ghimire et al. 12 and implemented in detail by Luu et al. using quartz crystal recently101. In contrast, the interband channel involves intrinsic atto-chirp because there are unique
recombination paths at different energies and momenta corresponding to different harmonic orders99,100. Therefore, by measuring the atto-chirp of high harmonics from the interband channel,
the momentum-dependent bandgap can be deduced, as shown in ZnO crystal20. At sufficient high-harmonic peak intensities, transitions to higher-lying conduction bands is possible and that
could lead to secondary plateau in high-harmonic spectrum, as observed in rare-gas solids16 and in room temperature solids, such as MgO and SiO2 crystal102. Similarly, depending on the
system, lower-lying valence bands may also contribute, as understood by analysing the terahertz-field driven harmonics in GaSe crystal103,104. Therefore, in the momentum-space framework,
high-harmonic spectroscopy also presents a novel, all-optical approach for probing electronic band structure, including away from the zone center. For these measurements it may be essential
to separate propagation effects. DIPOLE PHASE AND PROPAGATION EFFECTS One of the unique challenges in probing atto-chirp, and for HHS in general, is separating the strong propagation
effects. This is because in bulk samples, the intense pump laser pulse accumulates a significant nonlinear phase as it propagates from the entrance to the exit end from where the above
bandgap harmonics are typically emitted from. Modeling the effects of the nonlinear phase, such as the effects from \(\chi ^{\left( 3 \right)}\) on to the fundamental laser field and
consequently to high-order harmonics, is complex. Recently, non-perturbative high harmonics were also observed in the backward reflection geometry, which avoids propagation effects105. In
the following passage, we briefly discuss the results of attosecond interferometry in a homodyne configuration that was performed in both a reflection and a transmission geometry106. The
experimental setup is shown in Fig. 7. Here, the main idea is that XUV harmonics are generated in two spatially separated foci, but harmonics overlap in the far field and self-referenced
interferometry is performed. The measured fringe shifts in the reflected harmonics were reproduced by separating the interband polarization in a strongly driven two-level system. The fringe
shifts in transmission are overwhelmed by propagation effects, as the shifts are much larger than the predictions from microscopic model and are opposite in direction. Intriguingly, the
measured fringe shifts in reflection mode are source material-dependent, as XUV harmonics from MgO crystal show much larger shifts compared with those from SiO2. This is in contrast to the
gas-phase HHG where, for high-enough photon energies, the dipole phase is independent of the target atom107. While it is not immediately clear what specific features of the electronic
structure make the dipole phase shift differently in these materials, the experimental results clearly show the sensitivity of high-harmonic spectroscopy. Along this line, future experiments
can utilize this platform in many ways; for example, by referencing novel high-harmonics sources such as from solids, nanostructures, or liquid media with respect to that from well-studied
gas-phase sources in a heterodyne configuration. HHS could also be used to probe impurities in semiconductors with high spatial resolution. COMPACT XUV LIGHT SOURCE BASED ON SOLID-STATE HHG
Recent results have shown that solid-state HHG has the following main advantages when compared with HHG from dilute gas targets: (i) lower prerequisite on driving peak intensity because
solid-state HHG threshold on dielectrics is around 1012 W cm−216, (ii) the XUV waveform produced by some solid-state materials are found largely immune to fluctuations in the driving
fields18, and (iii) the use of tailored nanostructures, such as metal–sapphire bow tie108, or the use of heterostructures, such as epsilon-near-zero materials, improves the HHG efficiency
substantially109. The use of zone plates as a source material has provided the ability to focus the high-harmonic beams directly without the use of additional optics110 that could be
extremely demanding in the XUV wavelength range. Solid-state HHG setups do not require sophisticated high-vacuum pumping systems because of no gas load. Polarization of solid-state harmonics
can be controlled by taking advantage of anisotropy in the electronic band structure111 as well as the Berry phase in non-centrosymmetric crystals, such as SiO2112. Circularly polarized
harmonics have been demonstrated, at least in the visible wavelength range113. One drawback of solid-state HHG when compared with gas-phase HHG is that the high-energy cutoff is limited by
the material’s damage threshold, which in the case of wide-bandgap dielectric, has reached a ceiling of ~40 eV16. Further extension to higher photon energy range might be possible by the use
of ultra-short driving pulses. The rapid development of few-cycle, high-repetition-rate light sources, including optical parametric chirped-pulse amplifiers, can provide suitable pump
sources for solid-state HHG. With field enhancement in nanostructures in wide-gap materials108, high-harmonic XUV light sources based on laser oscillators or OPCPAs operating at
high-repetition rates appear promising. The dispersion of solids in the infrared pump wavelength range can be engineered, for example, by introducing waveguides114, photonic crystal
structures115 and metamaterials116, and by utilizing epsilon-near-zero effects through doping109. The phase matching between pump fields and harmonics in a specific spectral range could be
optimized, which could lead to enhanced generation efficiency. In the high photon energy regime, the absorption of harmonics above a material’s bandgap reduces the effective generation
thickness to the absorption length—usually on the order of ten nanometers for XUV harmonics—thus greatly limiting the HHG efficiency. For sufficiently high photon energy ranges, the
absorption of high-energy photons could be alleviated. For example, for just under 100 eV, silicon’s attenuation length is expected to be around 500 nm. If phase matching can also be
achieved, for example by taking advantage of a tunable refractive index in epsilon-near-zero materials, solid-state HHG could also reach the SXR photon energy range. ALL-OPTICAL PROBING OF
ULTRAFAST DYNAMICS IN MATERIALS There are initiatives aimed at testing the potential of the HHG process in probing structure and ultrafast dynamics in condensed matter systems. Examples of
ultrafast phenomena include insulator to metal phase transitions, strongly correlated electron dynamics117, and topological phase transitions in quantum materials118. Theoretical predictions
are emerging, which includes calculations on one dimensional model systems focusing on how the trivial to topological phase transition dramatically enhances the efficiency of the HHG
process118 and two-dimensional Haldane model system focusing on how HHG could probe topological invariants119,120. This particular aspect, as well as just how phase transitions and
correlations manipulate the HHG process at the microscopic level on novel quantum materials, are outstanding questions at this time121. A nominal experimental setup could be a pump–probe
scheme, wherein an ultrafast pump laser initiates a phase transition, and a strong-field probe pulse produces high harmonics from the active medium as a function of pump–probe. Currently,
angle-resolved photoemission spectroscopy (ARPES) is the standard spectroscopic method to measure the band structure. However, since it is based on the detection of electrons, it has
stringent experimental requirements such as ultra-high-vacuum and ultra-clean sample environments. Its temporal resolution in a pump–probe setting has been demonstrated only down to about
tens of femtoseconds122. Similarly, time-resolved X-ray absorption/diffraction techniques also have limitations, usually >50 fs, because of the temporal jitter between the pump laser and
the X-ray source123. Being an all-optical method, high-harmonic spectroscopy provides unprecedented time resolution and also much of these measurements can be performed in ambient
conditions, i.e., without the need for vacuum apparatus, especially if the pump lasers are in the mid-infrared wavelength range. High harmonics provide a novel approach to probe active
electronics in two-dimensional materials and heterostructures. Finally, we note that so far the solid-state HHG theory is largely based on single active electron approximation, either
through solving time-dependent Schrödinger equations (TDSE)99,100,124 or through semiconductor Bloch equations (SBE)103,125. Many-body effects such as electron-electron correlations and
dephasing are largely ignored while the latter is implemented just phenomenologically. Therefore, more predictive theories that consider correlations and multiple electronic bands are highly
desired. One path forward could be through the ab initio approach based on time-dependent density-functional theory (TDFT), which could in principle consider the full band structure and
joint density of states126. SUMMARY AND OUTLOOK The recent breakthroughs in attosecond “water window” X-ray sources open the door to game-changing applications. The combination of
unprecedented time resolution with element-specific spectroscopy provides a unique opportunity for studying charge and nuclear dynamics in organic molecules and materials containing C, N, O,
and other important elements and may help in understanding the charge transfer mechanism in solar cell materials. So far, transient-absorption spectroscopy measurements have been
demonstrated in the water window with attosecond time resolution. It is expected that attosecond photoelectron spectroscopy127, attosecond coherent diffraction imaging128, attosecond
reflection spectroscopy129, as well as other time-resolved techniques130, such as HHG-based ARPES131 and Cold Target Recoil Ion Momentum Spectroscopy (COLTRIMS) apparatus132 will be
implemented beyond the Carbon K-edge. Currently, the attosecond pulse energy from HHG source is too weak to populate excited state in the atoms or molecules. The benefit of more energetic
attosecond pulses is the possibility to perform true attosecond-pump–attosecond-probe experiments, where excitations are fulfilled through direct core level transition by absorbing a single
XUV/SXR photon. Major efforts towards enhancing HHG efficiency include two-color driving fields as well as the use of MWIR. In the latter, it is easier to individually control the three
steps of the HHG process133 because of the long laser cycles. Recently, a fundamentally different technique for producing attosecond pulses has emerged at X-ray free-electron lasers,
particularly at the Linac Coherent Light Source (LCLS)134,135. Accelerator-based sources typically provide substantial flux so they will enable a new class of experiments, including true
attosecond-pump and attosecond-probe capabilities. Solid-state HHG has been realized in a wide range of materials and harmonic spectrum has reached ~40 eV. These results have shown promises
for stable attosecond pulses in compact experimental setups, along with the novel all-optical method to directly probe the structure and dynamics of the source material. Because of the
modest requirements in the peak intensity (1011–1013 W cm−2) solid-state HHG could possibly be pumped with next-generation high-repetition rate fiber laser systems such that the total flux
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Download references ACKNOWLEDGEMENTS This work was supported by United States Air Force Office of Scientific Research (AFOSR) (FA9550-15-1-0037, FA9550-16-1-0013, FA9550-17-1-0099); Army
Research Office (ARO) (W911NF-14-1-0383, W911NF-19-1-0224); Defense Advanced Research Projects Agency (DARPA) (D18AC00011); Defense Threat Reduction Agency (HDTRA11910026); National Science
Foundation (1806575); Department of Energy; Office of Science; Basic Energy Sciences; Chemical Sciences; Geosciences and Biosciences Division through the Early Career Research Program and
Chinese Academy of Science Pioneer Hundred Talents Program (2018-131-S). AUTHOR INFORMATION AUTHORS AND AFFILIATIONS * Academy of Opto-Electronics, Chinese Academy of Sciences, Beijing,
100094, China Jie Li * Institute for the Frontier of Attosecond Science and Technology, CREOL and Department of Physics, University of Central Florida, Orlando, FL, 32816, USA Jie Li, Andrew
Chew, Seunghwoi Han, Jialin Li, Yi Wu & Zenghu Chang * School of Optoelectronics, University of the Chinese Academy of Sciences, Beijing, 100049, China Jie Li * Stanford PULSE
Institute, SLAC National Accelerator Laboratory, Menlo Park, CA, 94025, USA Jian Lu & Shambhu Ghimire * School of Mechanical Engineering, Chonnam National University, Gwangju, 61186,
Republic of Korea Seunghwoi Han * Department of Physics, University of Miami, Coral Gables, FL, 33146, USA He Wang Authors * Jie Li View author publications You can also search for this
author inPubMed Google Scholar * Jian Lu View author publications You can also search for this author inPubMed Google Scholar * Andrew Chew View author publications You can also search for
this author inPubMed Google Scholar * Seunghwoi Han View author publications You can also search for this author inPubMed Google Scholar * Jialin Li View author publications You can also
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You can also search for this author inPubMed Google Scholar CONTRIBUTIONS Jie Li, A.C., S.H., Jialin Li, Y.W., H.W., and Z.C. drafted the sections of generation and applications of gas-phase
soft X-ray HHG. Jian Lu and S.G. drafted the solid-state HHG with corresponding applications. All authors planned and contributed to the final version of the paper. CORRESPONDING AUTHOR
Correspondence to Zenghu Chang. ETHICS DECLARATIONS COMPETING INTERESTS The authors declare no competing interests. ADDITIONAL INFORMATION PUBLISHER’S NOTE Springer Nature remains neutral
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http://creativecommons.org/licenses/by/4.0/. Reprints and permissions ABOUT THIS ARTICLE CITE THIS ARTICLE Li, J., Lu, J., Chew, A. _et al._ Attosecond science based on high harmonic
generation from gases and solids. _Nat Commun_ 11, 2748 (2020). https://doi.org/10.1038/s41467-020-16480-6 Download citation * Received: 21 December 2018 * Accepted: 05 May 2020 * Published:
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