A solid-state template method in Fig. 1a is used to prepare 2D RP. Firstly, the precursor PI3 is coated on the surface of the L-ascorbic acid (L-ASA) template by solvent evaporation. A large amount of interface effectively limits the growth of materials in the two dimensions. In order to avoid reactions in the liquid phase, the evaporating temperature needs to be sufficiently low (~ 25°C), which can be estimated by the non-existence of purple iodine in the collection bottle. Afterwards, the coated mixture is heated at a relatively high temperature (~ 70°C) to bring about thermal decomposition on the interface. The reaction is controlled by temperature, as the color difference of reactants can be observed between the high-temperature reaction vessel edge and the low-temperature center (brown at the edge, orange at the center). Finally, the template and unreacted precursor are easily removed by dissolving and washing.
The morphology of 2D RP is characterized by transmission electron microscopy (TEM). The layered structure is detected, which is the distinct characteristic of 2D materials (Fig. 1b). The high-resolution TEM (HRTEM) image and selected area electron diffraction pattern in Fig. 1c give direct evidence of the amorphous structure and disordered atomic arrangement of 2D RP. As shown in Fig. 1d, the homogeneous morphologies and size uniformities are observed from the scanning electron microscopy (SEM) images. The size of 2D RP is about 115 nm (Fig. S4). The atomic force microscopy (AFM) result proves the average height of 2D RP is 1.62 ± 0.09 nm (Fig. 1e). Elemental mapping of energy dispersive spectroscopy (EDS) is used to study the chemical composition of 2D RP (Fig. 1f). Three kinds of elements of P, O, and C are detected, among which P is the most significant. The existence of O is due to the oxidation of the surface to stabilize the edge structure of 2D RP.
To figure out the molecular vibration of 2D RP, the sample is characterized by Raman spectroscopy in Fig. 2a. These three characteristic peaks of 2D RP at 356.7, 385.0, and 445.0 cm− 1, which are also observed in commercial amorphous RP, are attributed to B1 fundamental mode, A1 symmetric stretching modes, and E1 degenerate mode, respectively29. In the group theory analysis, B1, A1, and E1 modes are the irreducible symmetric types of point groups. X-ray diffraction (XRD) spectra are presented in Fig. 2b. The sharp diffraction peak at 2θ = 15.5° can be ascribed to a medium-range ordered structure matching with commercial amorphous RP. The wide diffraction peak from 20.0 to 39.0° suggests a long-range disordered structure30. Taking use of Fourier transform infrared (FT-IR) spectroscopy, functional groups in 2D RP are detected in Fig. 2c. The peaks located at 1637, 1158, and 1042 cm− 1 can be ascribed to P = O, P-O, and P-P-O stretching vibration, respectively31. In addition, the peaks at 3440 and 1644 cm− 1 can be attributed to the stretching vibration and the bending vibration of the hydroxyl group of water absorbed on the surface of the sample. The peak at 2364 cm− 1 is caused by the bending vibration of the attached CO2. X-ray photoelectron spectroscopy (XPS) is used to probe the surface chemical composition and state of 2D RP. As shown in Fig. 2d, the strong peaks in XPS survey spectra from left to right are O 1s, N 1s, C 1s, P 1s, and P 2p of 2D RP and commercial amorphous RP. For comparison, the O content in 2D RP is lower than that in commercial RP. The high-resolution XPS spectra at the binding energy of the P element are differentiated and fitted to analyze the chemical states (Fig. 2e). The peaks centered at 134, 133, 132, 131, and 130 eV can be assigned to P2O5, O-P = O, P-O-P, P 2p1/2, and P 2p3/2, respectively. The peaks of O can be divided into oxidation states of P and C (Fig. 2f). Compared with commercial RP, the oxidation state of 2D RP is lower.
The NLO performance of 2D RP is measured by an Nd: YAG laser with a wavelength of 532 nm, a repetition frequency of 10 Hz, and a pulse duration of 6 ns. The open-aperture (OA), closed-aperture (CA), and nonlinear scattering Z-scan are equipped with the optical settings in Fig. 3a and b. The waist radius of the lens is 13.55 µm. The transmittance of all samples in different solvents are ~ 60% (at 532 nm). The OA Z-scan results of the blank samples (without the 2D RP) are shown in Fig. S16. By using the OA Z-scan, the solvent-dependent NLO phenomenon of 2D RP is observed at the same waist power density of incident light (I0, 1.132 GW/cm2) in Fig. 3c. The SA signals are detected in a part of these solvents and RSA signals are in the other part. It is discovered that the imaginary parts of third-order NLO susceptibilities (Imχ(3), calculated by expression 18, obtained by fitting the OA Z-scan curves) of 2D RP show linear correlation with the relative dielectric constants of solvents (Fig. 3g). Among these solvents, PG and GI were selected as the focus of this research. SA and RSA signals of 2D RP are observed in PG and in GI, respectively (Fig. 3d and e). Both their absolute values of modulation depth (MD, defined as the transmittance at Z = 0) increase with the increase of incident light power density. The absorption coefficients (obtained by fitting the OA Z-scan curves) are related to light intensities as well as the susceptibilities and the quality factors (FOM, calculated by expression 19) in Fig. S5 and Table S3. The OA Z-scan curves in Fig. 3f reveal that 2D RP can convert between SA and RSA by adjusting the volume ratios of PG and GI in the mixed solvents. The Imχ(3) and FOM of 2D RP in mixed solvents are calculated in Fig. 3h and Table 1. The Imχ(3) increases with the increase of GI content. When the volume ratio is 1:1, the FOM of 2D RP decreases to the bottom value. By comparing the FOM, the NLO performance of 2D RP in PG is better than that in GI. To demonstrate that the conversion from SA in PG to RSA in GI is not caused by the higher viscosity of GI (800 mPa·s) than PG (61 mPa·s), 2D RP in dimethyl silicone oils with different viscosities is detected by OA Z-scan (Fig. S6). Even when the viscosity of silicone oil (60000 mPa·s) is much higher than that of GI (800 mPa·s), there is no conversion between SA and RSA, indicating that the viscosity is not the reason for the different signals in PG and in GI. Besides, CA Z-scan properties of 2D RP in PG and in GI are investigated in Fig. S7a. No self-focusing or self-defocusing signal (up-to-down or down-to-up oriented centrosymmetric shape) is found. With the sample placed in focus, laser power densities at both front and rear of the sample are detected and converted into the laser transmittance spectra (Fig. S7c and d). The transmittance of 2D RP in PG increases with the increase of incident power density, as opposed to GI.
To confirm whether nonlinear scattering is the main reason for the convertible orientation of OA Z-scan curves in PG and in GI, the optical devices behind the sample are rotated by 10 degrees around the focus to receive the scattering signals (Fig. 3b). As shown in Fig. S7b, nonlinear scattering Z-scan results of 2D RP in different solvents are both downward signals. Additionally, the intensities of the nonlinear scattering signals are smaller than those of the OA signals by about two orders of magnitude. Therefore, the nonlinear scattering just slightly influences the intensity of the OA Z-scan curves and does not change the curve orientations. According to the laser spot images in Fig. 3i and j, these downward nonlinear scattering signals are caused by the expansion of scattered laser spots and the decrease of light intensity received by the detector. Because the light expands outside the detector when the sample is near Z = 0. This is reflected in the nonlinear scattering Z-scan curve as a decrease in transmittance (i.e. the signals are both downward signals) because the transmittance is obtained by the ratio of light intensity value received by detector A to B. However, the OA Z-scan curves of 2D RP are upward in PG and downward in GI (Fig. 3d and e). Even if the nonlinear scattering can slightly influence the OA Z-scan signals due to the range of scattering spots exceeding the size of the detector, the intensities of nonlinear scattering signals are too weak to dominate the orientations of these curves. At the waist (Z = 0) and the Gaussian laser center parts, the light intensity of 2D RP in GI is weak. While in PG, it is strong. Together with the fact that the sizes of the Gaussian light spots are not visibly reduced or enlarged, the difference at the center part of the Gaussian laser can be explained by the nonlinear absorption.
In order to evaluate the NLO performance of 2D RP, the OA Z-scan of 2D BP is examined and the nonlinear absorption coefficients of other materials are investigated. Similar to 2D RP, SA and RSA are also observed on 2D BP in PG and in GI, respectively (Fig. S9). Compared with 2D BP, 2D RP has much better RSA performance, whether in terms of the starting NLO threshold (\({F}_{on}^{5\%}\), defined as the power density when the linear transmittance is increased or decreased by 5%, Fig. S10b) or MD (Fig. S11b). For SA performance, the RP also exhibits a better MD and FOM (Fig. S11a and 13a) despite the lager \({F}_{on}^{5\%}\) (Fig. S10a). Consequently, the significance lies in the point that RP is more capable and suitable for the practical application scenario of a wider-ranged NLO modulation. Table 2 compares other materials with 2D RP on the nonlinear absorption coefficients32–39. It can be concluded that 2D RP has excellent NLO performance.
Ultraviolet-visible-near infrared (UV-vis-NIR) diffuse reflectance spectra (DRS) are obtained to explore the intrinsic absorption properties and band gap of 2D RP (Fig. 4b). Compared with bulk commercial RP, the absorption band of 2D RP is blue-shifted. Based on the Kubelka–Munk theory40,41 \([F\left(R\right)={\left(1-R\right)}^{2}/2R]\) and the Tauc plot Eq. 42,43 \(\left[{\left(ah\nu \right)}^{2}=A\left(h\nu -{E}_{g}\right)\right]\), the band gap of 2D RP is confirmed to be about 1.93 eV, as shown in the inset of Fig. 4b. UV-vis-NIR absorption spectra in Fig. 4c show that the GSA of 2D RP in PG is slightly stronger than that in GI at 532 nm. Femtosecond ultrafast carrier dynamics of 2D RP are pumped at 320 nm and probed from 420 nm to 620 nm. Their optical setting is shown in Fig. S14. The laser generated by the resonant cavity is divided into two beams through a splitter. One of the 800 nm lasers is converted to a 320 nm pump light through the optical parametric amplifier. The other is converted into a supercontinuum white light (350~800 nm) through a CaF2 crystal. The ground state electrons of the sample absorb the pump light energy and rise to the excited state. The excited state electrons absorb the probe light energy and the detector collects the absorption spectra. The TAS at different time scales are obtained by an optical delay device. 2D mapping of TAS in Fig. 4d and g provide direct and visible proof of the stronger ESA of 2D RP in GI. The positive absorption peaks centered at 580 nm decrease with the increase of probe delay time in Fig. 4e and h. Excited electrons at 580 nm have the largest number of transition electrons and the slowest de-excitation velocity, indicating that the upper-level bandwidth matches the corresponding energy of this wavelength (Fig. 4f and i). Therefore, the simplified two- and three-level models of 2D RP in PG and in GI are established to explain its SA and RSA in OA Z-scan results (Fig. 4a). In addition, the characteristic of the intermolecular energy or charge transfer on TAS is that the positive absorption signal must be accompanied proportionally by a bleaching signal nearby. No intermolecular charge transfer signal (the positive absorption signal accompanied proportionally by a negative bleaching signal nearby) is found in the TAS (Fig. 4e and h), indicating that the dielectric polarizations of the solvents affect the nonlinear absorption.
Two-level model44 is developed to facilitate the fitting of SA signals. The rate equations can be expressed as:
\(\frac{d{N}_{0}}{dt}=-\frac{{\sigma }_{01}\bullet I\bullet {N}_{0}}{h\nu }+\frac{{N}_{1}}{{\tau }_{10}}\) | (1) |
\(\frac{d{N}_{1}}{dt}=\frac{{\sigma }_{01}\bullet I\bullet {N}_{0}}{h\nu }-\frac{{N}_{1}}{{\tau }_{10}}\) | (2) |
\(N={N}_{0}+{N}_{1}\) | (3) |
where \(N={N}_{0}+{N}_{1}\) is the total population density. \({N}_{i}\) are the population densities of levels \({S}_{i}\). \({\sigma }_{ij}\) are the absorption cross sections of level \({S}_{i}\). \({\tau }_{ji}\) are the lifetimes of electrons relaxing from level \({S}_{j}\) to level \({S}_{i}\).
Because the width of the incident laser pulse is much longer than the lifetimes (\({\tau }_{L}\gg {\tau }_{ji}\)), the steady-state approximation can be brought into the rate equations to calculate the population densities of each level, i.e., \(d{N}_{i}/dt=0\). This results in:
$${N}_{0}=\frac{N}{1+I/{I}_{s}}$$
4
Where \({I}_{s}\) is the saturated absorption intensity, \({I}_{s}=h\nu /\left({\sigma }_{01}\bullet {\tau }_{10}\right)\).
Therefore, the absorption coefficient of the medium is:
$$\alpha ={\sigma }_{0}{\bullet N}_{0}=\frac{{\sigma }_{0}\bullet N}{1+I/{I}_{s}}=\frac{{\alpha }_{0}}{1+I/{I}_{s}}$$
5
Where \({\alpha }_{0}\) is the linear absorption coefficient of the medium.
Three-level model45 is developed to facilitate the fitting of RSA signals. The rate equations can be expressed as:
\(\frac{d{N}_{0}}{dt}=-\frac{{\sigma }_{01}\bullet I\bullet {N}_{0}}{h\nu }+\frac{{N}_{1}}{{\tau }_{10}}\) | (6) |
\(\frac{d{N}_{1}}{dt}=\frac{{\sigma }_{01}\bullet I\bullet {N}_{0}}{h\nu }-\frac{{\sigma }_{12}\bullet I\bullet {N}_{1}}{h\nu }-\frac{{N}_{1}}{{\tau }_{10}}+\frac{{N}_{2}}{{\tau }_{21}}\) | (7) |
\(\frac{d{N}_{2}}{dt}=\frac{{\sigma }_{12}\bullet I\bullet {N}_{1}}{h\nu }-\frac{{N}_{2}}{{\tau }_{21}}\) | (8) |
\(\frac{d{N}_{0}}{dt}=-\frac{{\sigma }_{01}\bullet I\bullet {N}_{0}}{h\nu }+\frac{{N}_{1}}{{\tau }_{10}}\) | (9) |
The steady-state approximation can be brought into the rate equations to calculate the population densities of each level, i.e., \(d{N}_{i}/dt=0\). This results in:
$${N}_{0}=\frac{N\bullet {h}^{2}\bullet {\nu }^{2}}{{I}^{2}\bullet {\sigma }_{01}\bullet {\sigma }_{12}\bullet {\tau }_{10}\bullet {\tau }_{21}+{I\bullet \sigma }_{01}\bullet {\tau }_{10}\bullet h\nu +{h}^{2}\bullet {\nu }^{2}}$$
10
$${N}_{1}=\frac{N\bullet {\sigma }_{01}\bullet {\tau }_{10}\bullet h\nu \bullet I}{{I}^{2}\bullet {\sigma }_{01}\bullet {\sigma }_{12}\bullet {\tau }_{10}\bullet {\tau }_{21}+{I\bullet \sigma }_{01}\bullet {\tau }_{10}\bullet h\nu +{h}^{2}\bullet {\nu }^{2}}$$
11
Define the parameters of saturated absorption intensities of ground and excited states as:
$${I}_{{s}_{0}}=\frac{h\nu }{{\sigma }_{01}\bullet {\tau }_{10}}$$
12
$${I}_{{s}_{1}}=\frac{h\nu }{{\sigma }_{12}\bullet {\tau }_{21}}$$
13
Hence:
$${N}_{0}=\frac{N\bullet {I}_{{s}_{0}}\bullet {I}_{{s}_{1}}}{{I}^{2}+I\bullet {I}_{{s}_{1}}+{I}_{{s}_{0}}\bullet {I}_{{s}_{1}}}$$
14
$${N}_{1}=\frac{N\bullet {I}_{{s}_{1}}\bullet I}{{I}^{2}+I\bullet {I}_{{s}_{1}}+{I}_{{s}_{0}}\bullet {I}_{{s}_{1}}}$$
15
Therefore, the absorption coefficient of the medium is:
$$\alpha ={\sigma }_{01}\bullet {N}_{0}+{\sigma }_{12}\bullet {N}_{1}=\frac{{\alpha }_{0}\bullet {I}_{{s}_{1}}\bullet \left({I}_{{s}_{0}}+{\sigma }_{12}/{\sigma }_{01}\bullet I\right)}{{I}^{2}+I\bullet {I}_{{s}_{1}}+{I}_{{s}_{0}}\bullet {I}_{{s}_{1}}}$$
16
Adding a perturbation \({\eta }_{NLS}\) caused by nonlinear scattering, its normalized transmittance can be approximated as:
$$T=\frac{1-\alpha \bullet l-{\eta }_{NLS}\bullet l}{1-{\alpha }_{0}\bullet l}$$
17
Where \(l\) is the sample thickness.
Table 1
NLO parameters of 2D RP in mixed solvents.
Mixed solvents VPG:VGI | I0 (GW/cm2) | IS0 (GW/cm2) | IS1 (GW/cm2) | σ12/σ01 | MD | αNL (cm/GW) | Imχ(3) (10− 11 esu) | FOM (10− 12 esu cm) |
1:0 | 1.132 | 0.270 | - | - | 1.620 | -524.822 | -3.536 | 5.440 |
3:1 | 1.132 | 0.541 | - | - | 1.328 | -439.809 | -2.963 | 4.559 |
1:1 | 1.132 | 15.296 | - | - | 1.074 | -44.789 | -0.302 | 0.464 |
1:3 | 1.132 | 1.922 | 27.354 | 1.594 | 0.701 | 131.130 | 0.884 | 1.359 |
0:1 | 1.132 | 0.230 | 58.010 | 1.600 | 0.453 | 308.594 | 2.079 | 3.199 |
The rate equations are used to solve the transmittance expressions in different solvents. The transmittance expressions are then used to fit the OA Z-scan curves to further obtain the nonlinear absorption coefficients \({\alpha }_{NL}\) and other relevant NLO parameters. The expression for the imaginary part of the third-order nonlinear susceptibility is as follows:
$$Im{\chi }^{\left(3\right)}=\frac{{c}^{2}\bullet {n}_{0}^{2}}{240\bullet {\pi }^{2}\bullet \omega }\bullet {\alpha }_{NL}$$
18
Where \(c\) is the light velocity, \({n}_{0}\) is the linear refraction, \(\omega\) is the angular frequency of light, and \({\alpha }_{NL}\) is the nonlinear absorption coefficient, \(\alpha ={\alpha }_{0}+{\alpha }_{NL}\).
The FOM is the abbreviation of figures of merit for evaluating the NLO performance of materials, and is expressed as follows:
$$FOM=\left|\frac{Im{\chi }^{\left(3\right)}}{{\alpha }_{0}}\right|$$
19
Table 2
Nonlinear absorption coefficients of different materials at 532 nm.
Sample | Wavelength (nm) | Pulse width | α (cm/GW) | References |
GO (DMF) | 532 | 6 ns | 30.22 | 32 |
GO–PcZn (DMF) | 532 | 6 ns | 51.16 | 32 |
TiS2 | 532 | 7 ns | 62 | 33 |
MoSe2/GO | 532 | 5 ns | 580 | 34 |
GDY | 532 | 6 ns | 1.7 | 35 |
PDPP-TTzPt | 532 | 6 ns | 36 | 36 |
Carboxyl-GO | 532 | 30 ps | 0.17 | 37 |
Cd0.5Zn0.5S | 532 | 40 ps | 120 | 38 |
2D Cr | 532 | 230 ps | 3.12 | 39 |
2D RP (PG) | 532 | 6–7 ns | 328.8 | This work |
2D RP (GI) | 532 | 6–7 ns | 578.5 | This work |
TD-DFT is used to calculate the GSA and ESA of 2D RP in PG and in GI. So far, the exact structure of amorphous RP is still unclear, and we only know it is composed of the possible linear-chain polymer8. In many researches, calculations have chosen a section of the structure proposed by Pauling in 1952, which is formed by P4 molecules after opening a covalent bond and bond-connecting each other46–48. Therefore, the structure in Fig. S17a is taken as the input configuration. Geometric optimization is performed to minimize the energy. In PG, the GSA of 2D RP at 532 nm is larger than the ESA (Fig. 5a). It is the reason for the SA of 2D RP in PG. In GI, the absorption property is just the opposite, which leads to the RSA (Fig. 5b). Compared with the experimental results, the positions of the absorption lines in theoretical molar extinction coefficient spectra show a blue-shift to some degrees, which may be caused by the inadequate size of the atomic system or the uncertainty of the optimized configuration. Non-electrostatic terms are not considered in the implicit solvent model, and the solvent environments are simply treated as the polarizable continuous medium because the sample does not have strong bonding or hydrogen bonding with the solvents. With the static and dynamic dielectric constants of solvents as variables, the ESA of 2D RP exhibits a significant change in these two solvents.