Fig. 1a shows the synthesis process of the rGO@CoPSe/NC composite. First, Co-NTA nanotubes with an average diameter of 200 nm are synthesized by a facile solvothermal reaction according to the reported report (Fig. S1a in Supporting information) [
22]. Then, the Co-NTA nanotubes are pyrolyzed into Co metal nanoparticles confined in N-doped carbon nanotubes (Co/NC) under an Ar atmosphere (Figs. S1b and S2 in Supporting information). Subsequently, the Co/NC is synchronously phosphorized and selenized to obtain CoPSe/NC nanoparticles in a vacuum quartz tube (
Fig. 1b). Finally, the CoPSe/NC nanotubes are assembled with reduced graphene oxide nanosheets to form rGO@CoPSe/NC composites through strong electrostatic interaction (
Fig. 1c). TEM image in
Fig. 1d shows CoPSe nanoparticles are homogeneously confined in the N-doped carbon nanotubes. TEM-based energy dispersive X-ray spectroscopy mappings show that each element is uniformly distributed throughout the entire nanotube (
Fig. 1e). The high-resolution transmission electron microscopy (HRTEM) image of CoPSe shows well-defined lattice fringe spacings of 2.50 Å point to the (210) plane of the cubic-phase CoPSe (
Fig. 1f) [
21]. The X-ray diffraction (XRD) pattern of rGO@CoPSe/NC in
Fig. 1g can be well indexed to the simulated pattern of cubic-CoPSe. Electron paramagnetic resonance (EPR) analysis is performed to verify the detailed defect and vacancy features for the as-prepared samples. As can be found in
Fig. 1h, a characteristic signal at
g value of 2.003 resulting from anion vacancy. It can be clearly seen that rGO@CoPSe/NC displays the highest vacancy content, which may be caused by two anions coexist in the lattice. The chemical composition and elemental valences of rGO@CoPSe/NC are carried out by X-ray photoelectron spectroscopy (XPS). The survey spectrum indicates the presence of C, N, Co, P, Se O elements (Fig. S3a in Supporting information). The existence of O element derived from absorbed oxygen on the surface of the rGO@CoPSe/NC. High resolution Co 2p XPS spectrum (
Fig. 1i) shows two peaks located at 779.3 and 794.2 eV corresponding to the 2p3/2 and 2p1/2 of Co
3+, respectively. High resolution P 2p XPS spectrum in
Fig. 1j illustrates the two dominating peaks at 130.3 and 129.5 eV are assigned to 2p
3/2 and 2p
1/2 orbitals, respectively. The peak at 133.8 eV is assigned to the P—O bonds [
23]. In addition, the peak located at 138.5 eV is the Se Auger emission line. High resolution Se 3d XPS spectrum in
Fig. 1k shows three peaks located at 56.3, 55.5 and 61.6 eV, corresponding to the Se 3d
3/2, Se 3d
5/2 and Se—O, respectively [
24]. Moreover, the Co 3p
1/2 (60.1 eV) and Co 3p
3/2 (58.9 eV) spectra are detected in the Se 3d XPS spectrum [
25]. High-resolution C 1s spectrum is split into two peaks at 284.5 and 285.6 eV (Fig. S3b in Supporting information), which correspond to C—C, and C═N, respectively [
18]. As for the N 1s spectra (Fig. S3c in Supporting information), four peaks are deconvoluted, which ascribe to the graphitic N (401.5 eV), pyrrolic N (400.9 eV), Co-N2 (399.2 eV), and pyridinic-N (397.8 eV) [
26]. Raman spectra show the two peaks at 1323 and 1578 cm
−1 corresponding to D and G bands with intensity ratio (
ID/
IG) of are 1.14, which are higher than that of rGO@CoP/NC and rGO@CoSe
2/NC (Fig. S4 in Supporting information), suggesting the existence of rich structural defects in rGO@CoPSe/NC. The rGO@CoPSe/NC composite shows a Brunauer–Emmett–Teller surface area of 122.4 m
2/g with a pore volume of 0.39 cm
3/g (Fig. S5 in Supporting information). Moreover, the pore size distribution curve indicates hierarchically porous feature with high proportion of mesopores. Previous studies have shown that the mesopores enable fast ion transport for improving rate capability and alleviate volume expansion for maintaining cycling stability [
27]. For comparison, the rGO@CoSe
2/NC and rGO@CoP/NC are also synthesized. As shown in Figs. S6a and b (Supporting information), their morphologies are the same with that of rGO@CoPSe/NC. The XRD patterns (Figs. S6c and d in Supporting information) and XPS survey spectra (Figs. S6e and g in Supporting information) further confirm their successful preparation of the rGO@CoSe
2/NC and rGO@CoP/NC.