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New refractory MAB phases and their 2D derivatives: insight into the effects of valence electron concentration and chemical composition

Yinqiao Liu, Zhou Jiang, Xue Jiang* and Jijun Zhao
Key Laboratory of Material Modification by Laser, Ion and Electron Beams (Dalian University of Technology), Ministry of Education, Dalian, 116024, China. E-mail: jiangx@dlut.edu.cn

Received 16th May 2020 , Accepted 25th June 2020

First published on 8th July 2020


Abstract

Since MAB (where M is a transition metal, A is an groups 13–16 element, and B is boron) phases possess good electrical conductivity, high-temperature oxidation and shock resistance, it is meaningful to develop a database to help us figure out optimal compositions and further promote their applications. In this paper, we screened and studied all the available MABs with the M-site being one of the 3d, 4d, or 5d transition metals by using an ab initio method. Among them, 23 MAB phases of M2Al2B2 (222-MAB phases with M = Ti, V, Nb, Ta, Cr, Mo, W, Mn, and Tc) and M2AlB2 (212-MAB phases with M = Sc, Ti, Zr, Hf, V, Nb, Cr, Mo, W, Mn, Tc, Fe, Co, and Ni) stand out in terms of structural stability and their electronic, mechanical, optical and thermodynamic properties have been investigated. For both types of MAB phases early transition elements are more feasible to synthesize than post transition elements, because of the lower number of valence electrons and lower formation energy. The effect of valence electron concentration and composition of MAB compounds could also enable fine tuning of their mechanical properties. The bulk modulus, shear modulus, and Young's modulus of the 222-MAB phases are in the range of 145–233 GPa, 101–145 GPa, and 252–361 GPa, respectively, while they are 152–262 GPa, 91–177 GPa, and 237–422 GPa for the 212-MAB phases, respectively. Their mechanical ductilities also show strong valence electron number dependency, with their maximum value occurring at Ni2AlB2 and Co2AlB2, respectively. More interestingly, a low thermal expansion coefficient and good high temperature strength have also been found in those MAB phases, which are favorable for their potential applications as refractory materials. In addition, the possibility of forming new two-dimensional (2D) materials from layered MAB phases, termed MBenes, is predicted by investigating the interplay of the tensile strain, complex chemical bonding and exfoliation energy.


1. Introduction

“MAX phases”, originally studied in the 1960s,1–4 are a family of 80+ ternary carbides and nitrides that share a common type of layered structure. They are named “MAX” because of their chemical formula: Mn+1AXn, where n = 1, 2, or 3, M is a transition metal, A is an A-group element (specifically, the subset of group 13–16 elements), and X is either carbon or nitrogen. MAX phases have some outstanding properties and behave like both metals and ceramics.5 Like metals, they have good thermal and electrical conductivity, thermal shock resistance, machinability, and damage tolerance. Like ceramics, they are light weight, stiff, refractory, and oxidation resistant. Owing to this unique combination of properties, MAX phases are well developed as high temperature foil bearings, heating elements, and sputtering targets for electrical contact deposition.

Another group of compounds, MAB phases, as boron analog of MAX phases, contain stacked M–B blocks and interleaved with A-atom planes. The first MAB-type phase, MoAlB, was synthesized in 1942 by Halla and Thury.6 Soon afterward, the Mo–Al–B ternary phase diagram has been determined using cold compress and weld. In experiment at 1000 °C, MoAlB is indeed stable with a relatively narrow stoichiometric range.7 Meanwhile, X-ray diffraction data indicated that this MoAlB compound crystallized with an orthorhombic structure (Cmcm space group).8 Although MoAlB has been successfully synthesized, MAB phases as a class of compounds were not widely investigated until recently. Benefited from the development of synthesis technique, MAB phases have recovered to be an interesting topic now. The number of pure MAB phases as well as their solid solutions continues to expand. For example, an isostructural member of MoAlB with transition metal element W has been reported.9,10 A new series competing phase, 212-MAB phases have been successfully prepared, such as Fe2AlB2 and Cr2AlB2.10,11 In addition, solid-solution single-crystals, (Mox, M1−x)AlB with M = Cr and W12 and (Fe2, M2−x)AlB2 with M = Cr and Mn, have been also synthesized recently.13

The discovery of the versatile structures endows MAB phases many interesting properties, such as near room-temperature (RT) magnetocaloric properties,14 high-temperature oxidation resistance,15 shock resistance,16 and electrocatalytic properties.17,18 Ke et al. investigated the intrinsic magnetic properties of Fe2AlB2-related compounds and their alloys.19 They found Mn2AlB2 to be ferromagnetic within the basal ab plane and antiferromagnetic along the c axis. All 3d transition metal doping will decrease the magnetization and Curie temperature in Fe2AlB2. At ground-states and high temperatures, the mechanical and thermal properties of MAB (M = Mo and W) were thoroughly calculated by Xiang et al.,20 which confirm their high-temperature stability. The nature of bonding and mechanical properties in some MAB (M = Cr, W, Mo) compounds has been studied.21–23 Bai et al.21 found that, similar to Mo2AlC, MoAlB also have good mechanic properties for the potential engineering applications. Dai et al.22 and Zhou et al.23 discussed the potential impacts of strong B–B/M–B bonds and the weaker Al–Al/M–Al bonds on high elastic modulus and damage tolerance of MAlB. The optical conductivity of MoAlB has been further investigated by Li et al., and they found high reflectivity in the visible-ultraviolet region up to ∼19 eV region,24 which make it possible to use as coating material. By combining theory with experiments, Kádas et al.11 studied the mechanical properties of AlM2B2 (M = Cr, Mn, Fe, Co and Ni) and predicted their brittle or ductile behavior with different M metals. They further presented evidences of delamination phenomena and discussed the mechanism.

It is expected that the growing family of MAB phases and their properties would have significant applications like MAX phases. However, a large number of MAB compounds are still unexplored by considering the diverse elements combinations. As for just 211-M2AX compounds, the possible stable phases have 1080 candidate structures. Moreover, the constructed structure maps will help us understand the stability trends and give the guideline to experimental synthesis of new MAB phases. Therefore, in this paper, we mainly focus on constructing a structure map for MAB compounds with compositions of 2[thin space (1/6-em)]:[thin space (1/6-em)]2[thin space (1/6-em)]:[thin space (1/6-em)]2 and 2[thin space (1/6-em)]:[thin space (1/6-em)]1[thin space (1/6-em)]:[thin space (1/6-em)]2, respectively. We start from the possible compositions of MAB phases with the M-site metal being one of the 3d, 4d and 5d transition metals and A site being generally accepted Al element. By high-throughput DFT calculations, 23 stable MAB phases: nine 222-MAB phases (M = Ti, V, Nb, Ta, Cr, Mo, W, Mn, and Tc) and fourteen 212-MAB phases (M = Sc, Ti, Zr, Hf, V, Nb, Cr, Mo, W, Mn, Tc, Fe, Co and Ni) have been identified by rigorous structural stability analysis. Along with the calculations of electronic structure, mechanical properties, chemical bonding, delamination properties, thermal and optical conductivities, the effects of valence electron number and compositions have been further discussed. Although the sparse data of electronic structure and mechanical properties have already reported for few MAB phases,11,13,14,19,21 a comprehensive study using an unified computational method would be helpful for deep understanding of the overall trend relationship between stability/properties and chemical compositions.

2. Theoretical methods

The electronic structures of the MAB phases were calculated using density functional theory (DFT)25 implemented in the VASP code.26,27 We employed the projected augmented wave (PAW) method28,29 to treat outermost electrons as valence electrons for atoms in MAB phases, respectively. The Perdew–Burke–Ernzerh of (PBE) parameterization30 within the generalized gradient approximation (GGA) was adopted to describe the exchange and correlation interactions. Integrations over the Brillouin zone were performed using Monkhorst–Pack grids31 with uniform spacing of 2π × 0.03 Å−1. The plane-wave cutoff energy was set to 500 eV. The optical conductivities were calculated by using CASTEP program.32 The dynamic stability of the constructed structures was assessed by phonon dispersion, which were computed using a supercell approach as implemented in the PHONOPY code.33

For the equilibrium crystal structure, its second-order elastic constants (Cij) were determined using a finite strain technique,34 and bulk and shear moduli were thus derived from the elastic constants using the Voigt–Reuss–Hill averaging scheme.35 The calculations of stress–strain relations were performed using the method in ref. 36. This approach with a relaxed loading path has been successfully applied to the calculation of the strength of several strong solids. Hardness were estimated based on the empirical formula developed by Jiang et al.37 The quasi-harmonic Debye model38 implemented in the Gibbs2 program38 was employed to determine the thermodynamic properties at ambient conditions and elevated temperatures and pressures.

3. Results and discussions

Based on experimental confirmations,8,10,39 the crystal structures of two types of MAB phases with stoichiometry of 2[thin space (1/6-em)]:[thin space (1/6-em)]2[thin space (1/6-em)]:[thin space (1/6-em)]2 and 2[thin space (1/6-em)]:[thin space (1/6-em)]1[thin space (1/6-em)]:[thin space (1/6-em)]2 are displayed in Fig. 1(a). According to the compositions, they are named as 222-MAB and 212-MAB phases, respectively. Here, we only focus on the generally accepted Al containing MAB phases. On one hand, the number of MAB phases is much smaller in comparison to that of the MAX-phases. The reason is that the variation of the transition metal and especially the main group metal “A” is much more restricted. Up to now, mostly MAB-phases are characterized only for A = Al.10 On the other hand, only the Al containing MAX-phases and MAB-phases are identified experimentally as the likely precursors to achieve a high-yield synthesis of two-dimensional MXene40 and MBene.41–44 As seen from the Fig. 1(a), the difference between 222-MAB and 212-MAB phases is the thickness of the Al layers, that is, the binary M–B boride are separated by single and double Al layers, respectively. In addition, both types of MAB phases are crystallized in orthorhombic lattices but with different atomic arrangements, i.e., space group of Cmcm for 222-MAB phases and space group of Cmmm for 222-MAB. To obtain the potentially unreported MAB phases, transition metals in 3d (Ti, V, Cr, Mn, Fe, Co, Ni, Cu and Zn), 4d (Zr, Nb, Mo, Tc, Ru, Rh, Pd, Ag and Cd) and 5d (Hf, Ta, W, Re, Os, Ir, Pt, Au and Hg) series are systematically investigated by first-principles calculations.
image file: d0ra04385k-f1.tif
Fig. 1 (a) Crystal structure of (left) 222-MAB compounds and (right) 212-MAB compounds. (b) Transition metal element table of the structure stabilities in MAB, the orange/blue color means stable and the grey color means unstable, while the upper and lower parts in an element grid are correspond to 222-MAB type and 212-MAB typed phases, respectively.

We first assess the dynamic, thermodynamically, and mechanical stabilities of totally 58 MAB phases in terms of the phonon dispersions, formation energy, and elastic constants. Among them, nine 222-MAB phases (M = Ti, V, Nb, Ta, Cr, Mo, W, Mn, and Tc) and fourteen 212-MAB phases (M = Sc, Ti, Zr, Hf, V, Nb, Cr, Mo, W, Mn, Tc, Fe, Co, and Ni) stand out (Fig. 1(b)). The lattice parameters, mass densities per formula unit obtained for those MAB phases are listed in Tables 1 and 2. For comparison, the previous experimental and theoretical results of 222-MABs with M = Mo, W and 212-MABs with M = Cr, Mn, Fe, Co and Ni are also presented in this paper.10,11,21 The current lattice parameters and cell volumes for the MAB compounds are in good agreement with previous experimental and theoretical values,10,11,21 validating our methodology of DFT calculations. Generally, as the valence electron number increases in one row of periodic table, the atomic radius decreases. Thus, for 222-MABs with M = Ti, V and Cr, and 212-MABs with M = Sc, Ti, V, Cr and Mn, the increasing valence electron number directly reduce the lattice parameters and cell volumes.

Table 1 Theoretical and experimental unit cell parameters a, b, and c (in Å), mass density ρ (in gcm−3) and formation energy ΔE (in eV) of nine stable 222-MAB typed phases
M2Al2B a (Å) b (Å) c (Å) ρ (g cm−3) ΔE (eV)
Ti2Al2B2 3.049 3.297 14.641 3.87 −1.933
V2Al2B2 3.009 3.084 14.235 4.46 −1.649
Nb2Al2B2 3.124 3.359 14.675 5.64 −1.486
Ta2Al2B2 3.107 3.351 14.576 9.57 −1.453
Cr2Al2B2 2.968 3.001 13.886 4.82 −1.183
Mo2Al2B2 3.109 3.217 14.040 6.33 −1.357
Mo2Al2B2, expt.10 3.094 3.199 13.922 6.45
W2Al2B2 3.118 3.217 13.985 10.50 −0.929
W2Al2B2, expt.10 3.102 3.202 13.906 10.66
Mn2Al2B2 3.011 2.821 14.137 5.13 −0.937
Tc2Al2B2 3.162 3.024 14.111 6.73 −1.089


Table 2 Theoretical and experimental unit cell parameters a, b, and c (in Å), mass density ρ (in g cm−3) and formation energy ΔE (in eV) of fourteen stable 212-MAB typed phases
M2AlB2 a (Å) b (Å) c (Å) ρ (g cm−3) ΔE (eV)
Sc2AlB2 3.185 3.613 11.745 3.40 −3.410
Ti2AlB2 3.046 3.308 11.3203 4.20 −4.034
Zr2AlB2 3.190 3.572 12.067 5.58 −3.674
Hf2AlB2 3.165 3.549 11.819 10.15 −3.441
V2AlB2 3.009 3.084 11.141 4.46 −3.043
Nb2AlB2 3.161 3.341 11.626 6.34 −2.471
Cr2AlB2 2.923 2.932 11.042 5.36 −2.447
Cr2AlB2, expt.10 2.937 2.968 11.051 5.26
Mo2AlB2 3.076 3.147 11.538 7.15 −2.333
W2AlB2 3.088 3.139 11.566 12.33 −1.466
Mn2AlB2 2.893 2.821 11.063 5.83 −2.373
Mn2AlB2, expt.10 2.918 2.893 11.038 5.65
Tc2AlB2 3.048 3.021 11.519 7.72 −2.316
Fe2AlB2 2.913 2.847 11.021 5.82 −2.064
Fe2AlB2, expt.10 2.923 2.870 11.034 5.75
Co2AlB2 2.959 2.694 11.323 6.13 −2.178
Ni2AlB2 3.000 2.784 11.107 5.94 −1.284


Phonon dispersions, formation energy and elastic constants are shown in Fig. S1, Tables 3 and 4. There are no negative frequencies throughout the entire Brillouin zone for these MAB phases, and all independent elastic constants satisfy the well-known Born stability criteria.35 These results confirm that the studied structures are dynamically and mechanically stable at ambient conditions. Considering the specific experimental reactants and products,10 the formation energies (ΔE) are further computed by ΔE = E(MAB) − E(M) − E(B) − E(Al). Among them, E(MAB) is the per MAB formula total energy of MAB crystal compound, where E(M), E(B) and E(Al) are the total energies of M, B and Al crystal, respectively. By definition, a negative ΔE means that the formation of this system is exothermic. Noted from Fig. 2(a) and (b) that the formation energies are negative and decrease with valence electron number of M atom increasing. For example, first-principles calculations show that formation energy of 212-MABs with M = Cr, Mn, Fe, Co and Ni are −2.447 eV, −2.373 eV, −2.064 eV, −2.178 eV and −1.284 eV, respectively. Such tendency is in accordance with the results of previous work,11 which show that MAB compounds are indeed more feasible to crystallize in lower valence electron number of M metal component. The 212-MABs with M = Cr, Mn, Fe, Co and Ni and 222-MABs with M = Mo and W have already been produced in the laboratory now.10,11 Based on the favorable formation energy, we can infer that Ti2Al2B2, V2Al2B2, Sc2AlB2, Ti2AlB2, Zr2AlB2, Hf2AlB2 are most likely to be identified in experiments.

Table 3 Calculated elastic constants (Cij), bulk modulus (B), shear modulus (G), Young modulus (E), Poisson's ratio (ν) and ratio of B/G of 9 stable 222-MAB typed phases
M2Al2B2 C11 C12 C13 C23 C22 C33 C44 C55 C66 B G E ν B/G
Ti2Al2B2 352 74 83 92 273 202 122 130 158 145 116 274 0.18 1.25
V2Al2B2 354 102 118 110 310 244 181 145 179 173 133 317 0.19 1.30
Nb2Al2B2 352 125 104 123 298 271 173 152 165 180 130 315 0.21 1.38
Ta2Al2B2 369 131 116 138 321 278 187 163 181 192 138 333 0.21 1.39
Cr2Al2B2 395 112 119 131 339 262 173 192 160 189 140 338 0.20 1.35
Mo2Al2B2 390 146 129 142 349 326 168 191 162 210 143 350 0.22 1.47
W2Al2B2 405 189 143 160 365 349 183 195 171 233 145 361 0.24 1.60
Mn2Al2B2 318 108 143 125 292 181 145 159 132 167 101 252 0.25 1.65
Tc2Al2B2 349 154 172 162 375 287 169 111 144 220 114 292 0.28 1.92


Table 4 Calculated elastic constants (Cij), bulk modulus (B), shear modulus (G), Young modulus (E), Poisson's ratio (ν) and ratio of B/G of 14 stable 212-MAB typed phases
M2AlB2 C11 C12 C13 C23 C22 C33 C44 C55 C66 B G E ν B/G
Sc2AlB2 497 147 122 146 453 380 129 118 168 238 142 356 0.25 1.67
Ti2AlB2 406 91 80 108 307 270 176 165 204 170 150 347 0.16 1.13
Zr2AlB2 344 99 84 124 267 185 144 134 178 152 112 270 0.20 1.36
Hf2AlB2 371 109 87 113 294 246 160 140 190 168 132 314 0.19 1.27
V2AlB2 414 102 116 128 336 315 115 110 200 195 129 317 0.23 1.51
Nb2AlB2 366 160 136 139 292 276 125 116 168 199 110 279 0.27 1.80
Cr2AlB2 521 118 107 113 444 428 165 160 215 229 177 422 0.19 1.29
Mo2AlB2 497 147 122 146 453 380 129 118 168 238 142 356 0.25 1.67
W2AlB2 511 187 154 179 474 365 147 115 163 262 139 354 0.28 1.89
Mn2AlB2 488 102 173 120 504 381 160 174 200 239 169 411 0.21 1.42
Tc2AlB2 473 135 203 187 505 333 130 129 163 260 132 339 0.28 1.97
Fe2AlB2 421 116 147 129 323 369 131 132 168 209 133 329 0.24 1.58
Co2AlB2 374 173 182 165 268 292 111 83 157 216 92 242 0.31 2.34
Ni2AlB2 362 157 140 162 241 296 107 114 110 200 91 237 0.30 2.20



image file: d0ra04385k-f2.tif
Fig. 2 (a) and (b) Formation energies, (c) and (d) ratio of B/G, (e) and (f) bond stiffness versus increasing valence electron filings of M atom for 222-MAB compounds (left) and 212-MAB (right) compounds, respectively.

To further evaluate the stabilities and examine the electronic structure, Fig. S2 shows the total and partial density of state (DOS) of the predicted 23 MAB phases. The finite DOS at the Fermi energy for all those MABs reveal their metallic character. The total density of states near the Fermi level are dominated by transition metal atoms, while the lower lying states are dominated by B and Al atoms. As the valence electron number of M metal increases, the number of states lower than Fermi level increases because of valance electron filling, which push the total density of states to lower energy and are mainly responsible for the stability. As suggested in pervious literature,11 the stability of the metallic materials is roughly relative to the pseudogap formation. That is to say, a local minimum (dip) at Fermi energy level (Ef) for metals implies higher structural stability, while a local maximum Ef is usually a sign of structural instability. Among our predicted 23 MABs, Cr2Al2B2, Mo2Al2B2 and W2Al2B2 have their Ef located at a local minimum in the total density of state (TDOS), suggesting their higher level of stability. These results are indirectly supported by the experimental findings of Mo2Al2B2 and W2Al2B2 phases. Meanwhile, we demonstrated again that Cr2Al2B2 is a very promising candidate for experimental synthesis. In addition, V2Al2B2, V2AlB2 and Nb2AlB2 show a peak in the TDOS at the Fermi level, suggesting a relative lower stability than Cr2Al2B2, Mo2Al2B2 and W2Al2B2. However, they might show better conductive performance than the other MABs systems reported here (Fig. S2).

To promote their practical engineering applications, we have also investigated the mechanical properties of 222-MAB and 212-MAB phases. The theoretical single crystal elastic constants Cij are shown in Tables 3 and 4. The corresponding bulk modulus (B), shear modulus (G), Young modulus (E), and Poisson's ratio (ν) are also obtained on basis of the Voigt–Reuss–Hill approximation.35 Clearly, our present elastic constants coincide with the previous theoretical values.11,21 As the Al concentration decreases, the modulus of MABs are strengthened. For instance, the theoretical bulk modulus, shear modulus, and Young modulus of 222-MAB phases are in the range of 145–233 GPa, 101–145 GPa, and 252–361 GPa, while those values of 212-MAB phases are 152–262 GPa, 91–177 GPa, and 237–422 GPa, respectively. It is noticeable that these values of MAB phases are comparable to or even higher than the corresponding MAX compounds.45 We further predict the Vickers hardness (Hv) of those MAB phases. The average Hv from the empirical formula developed by ourselves37 are 12–26 GPa (Tables S1 and S2), which is consistent with experimental value of 7.0–21.7 GPa.46 Among them, Ta2Al2B2, Cr2Al2B2, Mo2Al2B2, W2Al2B2, Sc2AlB2, Cr2AlB2, Mo2AlB2, W2AlB2, Mn2AlB2 possess higher modulus and hardness than other MAB phases. Moreover, we examined the universal anisotropy index, Au.47 Au accounts for both compressibility and shear contributions and it can be positive or zero, zero Au value represents an isotropic crystal. In Tables S1 and S2, it is seen that most MAB compounds have high elastic anisotropies, except Cr2AlB2, Mo2AlB2 W2AlB2 and Fe2AlB2, which have notably low anisotropies (Au = 0.08, 0.13, 0.15 and 0.12, respectively) than the other compounds. Thus, Cr2AlB2, Mo2AlB2 W2AlB2 with high modulus, high hardness and low elastic anisotropies are highly anticipated for future material applications.

The bulk modulus to shear modulus ratio, B/G, is an important measure of elasticity of a material. Materials with a B/G < 1.75 are expected to be brittle, while materials with B/G > 1.75 are ductile. The ratios B/G are also summarized in Tables 3, 4, Fig. 2(c) and (d). It can be seen that the ratio of B/G for most 222-MAB compounds are in the range from 1.30 to 1.65, implying that they are brittle-like ceramics. For the 212-MAB compounds, the values of B/G are in the range from 1.27 to 2.34. The ductile materials are predicted for Tc2Al2B2, Nb2AlB2, W2AlB2, Tc2AlB2, Co2AlB2 and Ni2AlB2 with B/G values of 1.92, 1.79, 1.89, 1.97, 2.34 and 2.20, respectively. In orthorhombic materials, the Cauchy pressure can be defined for the three different crystal directions: Pa = C23C44, Pb = C13C55, and Pc = C12C66, while is also an indicator of ductile behavior. As listed in Tables S1 and S2, the Cauchy pressure of W2AlB2, Co2AlB2 and Ni2AlB2 are positive in all the three directions. In short, a strong dependence of the elasticity with valence electron number is observed from Fig. 2(c) and (d). The B/G ratio of MABs increases with the increasing valence electron number. By substitute different M element, these MAB phases can be tune from inductile to ductile. For example, the ductility of 212-MAB compounds can be improved by alloying it with Tc, W, Co and Ni, or a combination of them.

The mechanical properties can be understood by their bond stiffness, tensile–stress curve, the work of separation, and the effective charge, respectively. Based on the bond stiffness values listed in Fig. 2(e), (f) and Table S3, we can summarize several findings. Firstly, the bond stiffness values show the trend as B–B > M–B > M–Al > Al–B > Al–Al. That is to say, the bond stiffnesses for intralayer B–B and B–M bonds are much larger than those for interlayer Al–M (Al–B/Al–Al) bonds. Secondly, the high bond stiffnesses of B–B and B–M bonds mainly determine their mechanical properties. One can observe relation of intralayer B–B, B–M bond stiffness as Mo2Al2B2 < W2Al2B2, which coincide with the tendency of experimental hardness value Hv (13.6 GPa10) of W2Al2B2 being lower than Hv (21.7 GPa10) of Mo2Al2B2. Moreover, there is relation of intralayer B–B, B–M bond stiffness as Cr2AlB2 < Mn2AlB2 < Fe2AlB2, which also agrees with the relation of experimental Hv of three 212-MAB phases Cr2AlB2 (7.0 GPa) < Mn2AlB2 (9.6 GPa) < Fe2AlB2 (14.7 GPa).10 Analogously, some hypothetical compounds of Tc2Al2B2, Tc2AlB2 and W2AlB2 probably possess higher Hv value due to their higher bond stiffness of B–B and B–M bonds. Thirdly, the mechanical properties of MAB phases are also affected by the ratio of the bond stiffness of the weakest bond to that of the strongest bond. As listed in Tables S3 and S4, Mn2Al2B2, Sc2AlB2, Zr2AlB2 and Nb2AlB2 have lower ratios, suggesting the contributions from interlayer weak M–Al, Al–B, Al–Al bonds to mechanical properties are also important, which will weaken the modulus and hardness to some extent.

The relatively weak bond stiffness of the M–Al and Al–B bonds can be related to the delamination properties and the production mechanism of 2D derivatives. The tensile–strain relationships along the [001] stacking direction are illustrated in Fig. 3. The highest points on the stress–strain curves can be defined as ideal tensile strengths at the critical fractural strain. The ideal tensile strength for 222-MAB are about 11–16 GPa from c axis, and the ideal tensile strength of 212-MAB compounds are 13–39 GPa, respectively. Such big difference in ideal strength is mainly attributed to their atomic arrangements. The failure of 212-MAB is characterized by an abrupt stretch of the M–Al bonds, which is very similar to that of MAX phases.48 However, the failure of 222-MAB is characterized by an abrupt stretching of the Al–Al bonds (Fig. 3).


image file: d0ra04385k-f3.tif
Fig. 3 (a) Calculated stress versus tensile strain along c axis for (a) 222-MAB compounds and (b) 212-MAB compounds. The inset photograph shows the deformation at free strain, at critical fractural strains and at strain after critical point, respectively.

Large ideal strengths are observed in the Mo2Al2B2, W2Al2B2, W2AlB2, Mn2AlB2, Tc2AlB2 and Co2AlB2 phases, which means that those compounds have strong delamination resistance. While for Mn2Al2B2, Sc2AlB2, Zr2AlB2, and Hf2AlB2, the ideal tensile strengths are less than 15 GPa due to the weak Al–Al or Al–B bond, which suggest the corresponding 2D derivatives could be synthesized through mechanical exfoliation. In those compounds, Al atoms donate less electrons (0.5–1.2e) to B atoms forming weaker Al–B and Al–Al bonds (Fig. 4). Indeed, the corresponding 2D Hf2B2, V2B2, Nb2B2, Cr2B2, Mn2B2 and Co2B2 sheets are dynamically stable by our phonon calculations (Fig. S3). Interestingly, 2D MBenes, such as MoB, CrB, FeB, TiB have already been synthesized by chemical stepwise etching.41–44 The works of separation of them are further studied and shown in Fig. 5. The corresponding works of separation of Hf2AlB2, V2AlB2, Nb2AlB2, Cr2AlB2, Mn2AlB2 and Co2AlB2 are 3.148 J m−2, 3.929 J m−2, 3.509 J m−2, 5.095 J m−2, 4.861 J m−2 and 3.986 J m−2, respectively, which are comparable to the value of monolayer Ti2C MXene (∼5 J m−2).49


image file: d0ra04385k-f4.tif
Fig. 4 Charge transfers versus increasing valence electron filings of M atoms for (a) 222-MAB compounds and (b) 212-MAB compounds.

image file: d0ra04385k-f5.tif
Fig. 5 Work of separation for 222-MAB compounds and 212-MAB compounds.

We have also calculated the interband dielectric function ε(ω) for the MAB phases in the frequency range from 0 to 30 eV using CASTEP code. Then, the optical conductivities and reflectivity are extracted from the obtained dielectric function. The optical conductivities resolved into axial components (X, Y, Z) are displayed in Fig. S4(a) and (b). Several interesting observations can be made from these plots. The X, Y, Z components of optical conductivities show distinctly isotropic property, except in the energy range of 1 eV. For 222-MAB compounds, the conductivity shows a sharp increase to reach the maximum value in the energy in range from 4.5 to 5.0 eV in the ultraviolet region and then decreases to the minimum. While for 212-MAB compounds, the conductivity reaches the maximum value in the energy range from 6 to 8 eV. In generally, both 222-MABs and 212-MABs should be more conductive for the incident photon energy ranges from 4.5 eV to 8.0 eV. The reflectivity is the ratio of the energy of a wave reflected from a surface to the energy of the wave incident on the surface. The reflectivity spectra of MAB as a function of incident light energy are presented in Fig. S5(a) and (b). For M = Ti, Cr, Mo, W, Mn, Tc of 222-MAB and M = Ti, Zr, W, Mn, Tc of 212-MAB, the reflectivities increase to reach the maximum value of about 80% in the ultraviolet region, i.e., in the range of 15 and 20 eV, then decrease drastically to reach the minimum, which mean optical properties of MAB changes from metallic to dielectric after about 20 eV. For others studied compounds, the values of reflectivity are almost above 44% (in the range of 0 and 20 eV). These MAB compounds will be capable of reducing solar heating if it has reflectivity >44%50 in the visible light region. Therefore, we may conclude MAB compounds are also candidate materials for coating to reduce solar heating.

The thermodynamic properties such as thermal expansion coefficient α and bulk modulus are evaluated in the temperature range from 0 to 1500 K (Fig. 6 and 7), where the quasi-harmonic approximate (QHA) remains fully valid. As seen in Fig. 6, the temperature dependence of volume thermal expansion coefficient α can be divided into two regions: in the first region, the α increases sharply with increasing temperature up to 300 K, whereas in the second region (300–1500 K), the α increases slowly with a nearly constant volume thermal expansion coefficient. With the exception of Mn2Al2B2, the values of them are 1.8–4.5 × 10−5 K−1 in 300–1500 K, which are comparable to α of MAX phases (1.5–3 × 10−5 K−1 (ref. 46)), and are relatively low as expected for refractory solids.51 Our predicted thermal expansion coefficient of Mo2Al2B2 is 2.88 × 10−5 K−1 in 1270 K, which is in good agreement with the experimental value that of 2.85 × 10−5 K−1 at 1000 °C.15 The temperature dependent bulk modulus are shown in Fig. 7. One can see that they are nearly a constant (140–260 GPa) in the temperature range of 0 and 100 K. When temperature exceeds 100 K, it starts to decrease linearly with increasing temperature. However, the bulk modulus of most MAB compounds decreases by only 10% (∼20 GPa) from 100 K to 1500 K, showing the temperature driven softening of modulus. In a word, we propose MAB possess temperature insensitive elastic modulus, meanwhile they have low thermal expansion in high temperature region. We propose the good thermodynamic properties MAB compounds make them applicable for potential ultra-high temperature ceramics applications.


image file: d0ra04385k-f6.tif
Fig. 6 (a) Thermal expansion α for the (a) 222-MAB phases and (b) 212-MAB phase, respectively.

image file: d0ra04385k-f7.tif
Fig. 7 (a) The bulk modulus B versus temperature for studied (a) 222-MAB phases and (b) 212-MAB phases, respectively.

4. Summary

We have performed a systematic first-principles calculation of the 222-MABs and 212-MABs compounds with the M-site being one of 3d, 4d, and 5d transition metal elements. We final assess 23 dynamicaly and mechanically stable MAB phases. According to our calculations, the dynamic stabilities, electronic structure, tendency of hardness and the thermal expansion of Mo2Al2B2, W2Al2B2, Cr2AlB2, Mn2AlB2, Fe2AlB2, Co2AlB2 and Ni2AlB2 coincide with those reported by previous work. Furthermore, we found many interesting properties in unreported MAB phases. For example, Ti2Al2B2, Sc2AlB2, Ti2AlB2, Zr2AlB2 and Hf2AlB2 are energetically more favorable and Cr2Al2B2 is more stable provided by analysis of their formation energy and DOS. V2Al2B2, V2AlB2 and Nb2AlB2 could show better conductive performance as well. The ductile materials are Tc2Al2B2, Nb2AlB2, W2AlB2, Tc2AlB2, Co2AlB2 and Ni2AlB2, while high modulus and low elastic anisotropies compounds are Mo2AlB2 W2AlB2 revealed by elastic modulus exploration. The Tc2Al2B2, Tc2AlB2 and W2AlB2 could possess high hardness provided by bond stiffness calculation. By correlating with the interlayer strength, work of separation and phonon dispersion curve, 2D structures of Hf2B2, V2B2, Nb2B2, Cr2B2, Mn2B2 and Co2B2 are found to be stable. For M = Ti, Cr, Mo, W, Mn, Tc of 222-MAB and M = Ti, Zr, W, Mn, Tc of 212-MAB, the ultraviolet reflectivities are as high as 90% showing attractive coating applications to reduce solar heating. Finally, the temperature dependence of volume thermal expansion coefficient and bulk modulus are investigated, the results show they have low thermal expansion as transition metal borides in 300–1500 K and the desired bulk modulus decreases by only 10% in 100–1500 K.

With a much enlarged database and comprehensive discussion of electronic structure, mechanical properties, chemical bonding, delamination properties, thermodynamic and optical properties, this study may eventually provide a theoretical fundamental property as guide to experimental work in MAB phases. These results enrich the family of MAB phases, and make the deep understanding of the overall trend relationship between stability/properties and chemical compositions, which are surely more beneficial for future material applications.

Conflicts of interest

There are no conflicts to declare.

Acknowledgements

This work was supported by the National Natural Science Foundation of China (11874097) and the Fundamental Research Funds for the Central Universities of China (DUT19LK12). We acknowledge the Xinghai Scholar project of Dalian University of Technology and the project of Dalian Youth Science and Technology Star (2017RQ012). We also acknowledge the Supercomputing Center of Dalian University of Technology for providing the computing resource.

References

  1. W. Jeitschko, H. Nowotny and F. Benesovsky, Monatshefte für Chemie und verwandte Teile anderer Wissenschaften, 1963, 94, 672–676 CrossRef CAS.
  2. W. Jeitschko and H. Nowotny, Monatshefte für Chemie - Chemical Monthly, 1967, 98, 329–337 CrossRef CAS.
  3. H. Wolfsgruber, H. Nowotny and F. Benesovsky, Monatshefte für Chemie und verwandte Teile anderer Wissenschaften, 1967, 98, 2403–2405 CrossRef CAS.
  4. O. Beckmann, H. Boller, H. Nowotny and F. Benesovsky, Monatshefte für Chemie/Chemical Monthly, 1969, 100, 1465–1470 CrossRef CAS.
  5. M. W. Barsoum, Prog. Solid State Chem., 2000, 28, 201–281 CrossRef CAS.
  6. F. Halla and W. Thury, Z. Anorg. Allg. Chem., 1942, 249, 229–237 CrossRef CAS.
  7. W. Rieger, H. Nowotny and F. Benesovsky, Monatshefte für Chemie und verwandte Teile anderer Wissenschaften, 1965, 96, 844–851 CrossRef.
  8. W. Jeitschko, Monatshefte für Chemie und verwandte Teile anderer Wissenschaften, 1966, 97, 1472–1476 CrossRef CAS.
  9. Y. Zhang, S. Okada, T. Atoda, T. Yamabe and I. Yasumori, J. Ceram. Soc. Jpn., 1987, 95, 374–380 CrossRef CAS.
  10. M. Ade and H. Hillebrecht, Inorg. Chem., 2015, 54, 6122–6135 CrossRef CAS PubMed.
  11. K. Kádas, D. Iuşan, J. Hellsvik, J. Cedervall, P. Berastegui, M. Sahlberg, U. Jansson and O. Eriksson, J. Phys.: Condens. Matter, 2017, 29, 155402 CrossRef PubMed.
  12. S. Okada, K. Iizumi, K. Kudaka, K. Kudou, M. Miyamoto, Y. Yu and T. Lundström, J. Solid State Chem., 1997, 133, 36–43 CrossRef CAS.
  13. P. Chai, S. A. Stoian, X. Tan, P. A. Dube and M. Shatruk, J. Solid State Chem., 2015, 224, 52–61 CrossRef CAS.
  14. X. Tan, P. Chai, C. M. Thompson and M. Shatruk, J. Am. Chem. Soc., 2013, 135, 9553–9557 CrossRef CAS PubMed.
  15. S. Kota, E. Zapata-Solvas, A. Ly, J. Lu, O. Elkassabany, A. Huon, W. E. Lee, L. Hultman, S. J. May and M. W. Barsoum, Sci. Rep., 2016, 6, 26475 CrossRef CAS PubMed.
  16. J. Liu, S. Li, B. Yao, J. Zhang, X. Lu and Y. Zhou, Ceram. Int., 2018, 44, 16035–16039 CrossRef CAS.
  17. D. K. Mann, J. Xu, N. E. Mordvinova, V. Yannello, Y. Ziouani, N. González-Ballesteros, J. P. S. Sousa, O. I. Lebedev, Y. V. Kolen'ko and M. Shatruk, Chem. Sci., 2019, 10, 2796–2804 RSC.
  18. L. T. Alameda, C. F. Holder, J. L. Fenton and R. E. Schaak, Chem. Mater., 2017, 29, 8953–8957 CrossRef CAS.
  19. L. Ke, B. N. Harmon and M. J. Kramer, Phys. Rev. B, 2017, 95, 104427 CrossRef.
  20. H. Xiang, Z. Feng, Z. Li and Y. Zhou, J. Alloys Compd., 2018, 738, 461–472 CrossRef CAS.
  21. Y. Bai, X. Qi, A. Duff, N. Li, F. Kong, X. He, R. Wang and W. E. Lee, Acta Mater., 2017, 132, 69–81 CrossRef CAS.
  22. F.-Z. Dai, Z. Feng and Y. Zhou, Comput. Mater. Sci., 2018, 147, 331–337 CrossRef CAS.
  23. Y. Zhou, H. Xiang, F.-Z. Dai and Z. Feng, Mater. Res. Lett., 2017, 5, 440–448 CrossRef CAS.
  24. X. Li, H. Cui and R. Zhang, Sci. Rep., 2016, 6, 39790 CrossRef CAS PubMed.
  25. W. Kohn and L. J. Sham, Phys. Rev., 1965, 140, A1133–A1138 CrossRef.
  26. G. Kresse and J. Furthmüller, Comput. Mater. Sci., 1996, 6, 15–50 CrossRef CAS.
  27. G. Kresse and J. Furthmüller, Phys. Rev. B: Condens. Matter Mater. Phys., 1996, 54, 11169–11186 CrossRef CAS PubMed.
  28. P. E. Blöchl, Phys. Rev. B: Condens. Matter Mater. Phys., 1994, 50, 17953–17979 CrossRef PubMed.
  29. G. Kresse and D. Joubert, Phys. Rev. B: Condens. Matter Mater. Phys., 1999, 59, 1758–1775 CrossRef CAS.
  30. J. P. Perdew, K. Burke and M. Ernzerhof, Phys. Rev. Lett., 1996, 77, 3865–3868 CrossRef CAS PubMed.
  31. H. J. Monkhorst and J. D. Pack, Phys. Rev. B: Solid State, 1976, 13, 5188–5192 CrossRef.
  32. J. Clark Stewart, D. Segall Matthew, J. Pickard Chris, J. Hasnip Phil, I. J. Probert Matt, K. Refson and C. Payne Mike, Z. Kristallogr. – Cryst. Mater., 2005, 220(5–6) DOI: 10.1524/zkri.220.5.567.65075.
  33. K. Parlinski, Z. Q. Li and Y. Kawazoe, Phys. Rev. Lett., 1997, 78, 4063–4066 CrossRef CAS.
  34. Y. Le Page and P. Saxe, Phys. Rev. B: Condens. Matter Mater. Phys., 2002, 65, 104104 CrossRef.
  35. Z.-j. Wu, E.-j. Zhao, H.-p. Xiang, X.-f. Hao, X.-j. Liu and J. Meng, Phys. Rev. B: Condens. Matter Mater. Phys., 2007, 76, 054115 CrossRef.
  36. D. Roundy and M. L. Cohen, Phys. Rev. B: Condens. Matter Mater. Phys., 2001, 64, 212103 CrossRef.
  37. X. Jiang, J. Zhao and X. Jiang, Comput. Mater. Sci., 2011, 50, 2287–2290 CrossRef CAS.
  38. A. Otero-de-la-Roza and V. Luaña, Comput. Phys. Commun., 2011, 182, 1708–1720 CrossRef CAS.
  39. W. Jeitschko, Acta Crystallogr., Sect. B: Struct. Crystallogr. Cryst. Chem., 1969, 25, 163–165 CrossRef CAS.
  40. J.-C. Lei, X. Zhang and Z. Zhou, Front. Phys., 2015, 10, 276–286 CrossRef.
  41. L. T. Alameda, P. Moradifar, Z. P. Metzger, N. Alem and R. E. Schaak, J. Am. Chem. Soc., 2018, 140, 8833–8840 CrossRef CAS PubMed.
  42. H. Zhang, F.-Z. Dai, H. Xiang, X. Wang, Z. Zhang and Y. Zhou, J. Mater. Sci. Nanotechnol., 2019, 35, 1593–1600 CrossRef.
  43. L. T. Alameda, R. W. Lord, J. A. Barr, P. Moradifar, Z. P. Metzger, B. C. Steimle, C. F. Holder, N. Alem, S. B. Sinnott and R. E. Schaak, J. Am. Chem. Soc., 2019, 141, 10852–10861 CrossRef CAS PubMed.
  44. J. Wang, T.-N. Ye, Y. Gong, J. Wu, N. Miao, T. Tada and H. Hosono, Nat. Commun., 2019, 10, 2284 CrossRef PubMed.
  45. W.-Y. Ching, Y. Mo, S. Aryal and P. Rulis, J. Am. Ceram. Soc., 2013, 96, 2292–2297 CrossRef CAS.
  46. S. Kota, M. Sokol and M. W. Barsoum, Int. Mater. Rev., 2019, 1–30,  DOI:10.1080/09506608.2019.1637090.
  47. S. I. Ranganathan and M. Ostoja-Starzewski, Phys. Rev. Lett., 2008, 101, 055504 CrossRef PubMed.
  48. Z. Guo, L. Zhu, J. Zhou and Z. Sun, RSC Adv., 2015, 5, 25403–25408 RSC.
  49. T. Hu, M. Hu, Z. Li, H. Zhang, C. Zhang, J. Wang and X. Wang, Phys. Chem. Chem. Phys., 2016, 18, 20256–20260 RSC.
  50. S. Li, R. Ahuja, M. W. Barsoum, P. Jena and B. Johansson, Appl. Phys. Lett., 2008, 92, 221907 CrossRef.
  51. M. Radovic and M. W. Barsoum, American Ceramics Society Bulletin, 2013, 92, 20–27 CAS.

Footnote

Electronic supplementary information (ESI) available. See DOI: 10.1039/d0ra04385k

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