1 Introduction

Alloy design in the past was limited to either one principal element (e.g., the Ni-based superalloys) or two (e.g., the TiAl-based superalloys). Their properties were optimized by a minor addition of other elements. In 2004, a new concept of alloy design based on multiprincipal elements was introduced independently.[1,2] Cantor et al.[1] prepared the alloys with up to 20 elements in equal atom fraction and reported the CoCrFeNiMn alloy with a single fcc solid-solution phase. In contrast to the general understanding of binary and ternary phase diagrams, in which many intermetallic compounds are formed within the center, Yeh et al.[2] pointed out that the high mixing entropy of alloys with multiprincipal elements might make the solid-solution phases more stable. A high entropy alloy (HEA) was then defined as an alloy containing at least five principal elements, each of which has a composition range between 5 and 35 at. pct and possesses a high mixing entropy at their liquid state or high-temperature solid-solution state.[3]

Nowadays, HEAs play an important role in alloy design, ascribing to their superb properties such as excellent fracture resistance at cryogenic temperatures,[4] exceptional combination of strength and ductility,[5,6] and outstanding wear resistance.[7] Although the terminology of such alloys is under debate (e.g., HEAs[3] followed by the current work, multiprincipal alloys,[1] or complex concentrated alloys[8]), studies have become focused on the center region of phase diagrams where uncountable possible combinations of four, five, six, or even greater numbers of elements are available[9] to obtain potential alloys with desired properties. In this sense, the classical trial and error method becomes challenging because a large number of experimental trials are needed to find appropriate HEAs.[10] This is the reason why designing HEAs becomes important.[8,11,12,13]

According to Gao et al.,[13] there are three main approaches for designing HEAs, i.e., the empirical parameters,[14,15,16,17,18,19,20,21,22,23,24,25,26,27,28,29,30,31,32,33,34,35,36,37,38,39] the CALPHAD method,[9,40,41,42] and the first-principle calculations.[43,44,45,46,47,48,49] The empirical parameters can provide some simple design rules. Their reliability depends on the parameters themselves and the data collection of reported HEAs. The CALPHAD method is the most effective way for calculating the phase diagrams of HEAs, as long as reliable thermodynamic databases are available. The extrapolation of binary and ternary phase diagrams into high order systems, however, is not reliable. Furthermore, there are no thermodynamic databases for all the reported HEAs. The first-principle calculations are able to predict phase equilibria with the atomic number and the crystal structure as the input parameters. Compared with the CALPHAD method and the first-principle calculations, which require significant computing workload, the empirical parameters provide an easy way for designing HEAs and, thus, were studied intensively.[14,15,16,17,18,19,20,21,22,23,24,25,26,27,28,29,30,31,32,33,34,35,36,37,38,39] Furthermore, their combination with other approaches is able to improve the efficiency of alloy design.[10] For the HEAs with five components in an equal atom fraction, the empirical parameters reduced the trials of 1287 alloys to 127 alloys for designing HEAs with a single fcc or bcc phase. Then, the CALPHAD method reduced the number of potential alloys to 10.

Up to now, a number of empirical parameters have been proposed: \( \delta r \), standard deviation of dimensionless atomic radius;[14] \( \delta d \), standard deviation of dimensionless atomic radii in pairs;[27] \( \gamma \), the ratio of two solid angles of atomic packing for the elements with the largest and smallest atomic sizes[27]; \( \varepsilon_{\text{RMS}} \), root-mean-square strain[29]; \( \Delta S_{mix} \), the mixing entropy[2]; \( \Delta H_{\text{mix}} \), the mixing enthalpy[14]; \( \delta H_{\text{mix}} \), standard deviation of dimensionless mixing enthalpy[38]; \( \Omega \) (\( = {{T_{\text{m}} S_{\text{config}} } \mathord{\left/ {\vphantom {{T_{\text{m}} S_{\text{config}} } {\left| {\Delta H_{\text{mix}} } \right|}}} \right. \kern-0pt} {\left| {\Delta H_{\text{mix}} } \right|}} \) with \( T_{\text{m}} \) the melting temperature and \( S_{\text{config}} \) the ideal configurational mixing entropy)[15]; \( \mu \) (\( = {{T_{\text{m}} } \mathord{\left/ {\vphantom {{T_{\text{m}} } {T_{\text{SC}} }}} \right. \kern-0pt} {T_{\text{SC}} }} \) with \( T_{\text{SC}} \) the critical spinodal temperature)[24]; \( \Phi \) (\( = {{\left( {S_{\text{config}} - S_{\text{H}} } \right)} \mathord{\left/ {\vphantom {{\left( {S_{\text{config}} - S_{\text{H}} } \right)} {S_{\text{E}} }}} \right. \kern-0pt} {S_{\text{E}} }} \) with \( S_{\text{H}} \) the entropy due to the mixing enthalpy and \( S_{\text{E}} \) the excessive mixing entropy due to the geometrical mismatch)[32]; \( \Lambda \) (\( = \frac{{S_{\text{config}} }}{\delta }r^{2} \))[30]; \( S_{\text{corr}} \), the nonideal configurational mixing entropy[36]; and \( \Theta \).[39] Despite their great success,[14,15,16,17,18,19,20,21,22,23,24,25,26,27,28,29,30,31,32,33,34,35,36,37,38,39] most of the empirical parameters aim to design HEAs with a single solid-solution phase.

Actually, HEAs with a single fcc phase are ductile but not strong enough, whereas HEAs with a single bcc phase are very strong but brittle.[50] Lu et al.[51,52,53] designed the eutectic HEAs with dual fcc and bcc phases to obtain an excellent balance between strength and ductility. Similarly, a series of (FeCoNiCrMn)100–xAlx (x = 0 to 20 at. pct) HEAs were prepared to show the effects of Al addition on the structure evolution and tensile properties.[54] With the increase of Al addition, the structure changes from a single fcc phase to dual fcc and bcc phases and then to a single bcc phase. The HEAs with a single fcc phase have relatively low strength but high ductility. The HEAs with dual fcc and bcc phases have a sharp increase in strength but decrease in ductility. The HEAs with a single bcc phase are extremely brittle. Moreover, addition of Al into the CoCrCuFeNi HEAs leads to an increase of the volume fraction of bcc phase, thus increasing hardness and wear resistance.[55] Therefore, a combination of fcc and bcc phases is able to optimize the mechanical properties of HEAs, thus highlighting the importance to design HEAs with dual fcc and bcc solid-solution phases.

Guo et al.[18] studied the relationship between the average valence electron concentration (VEC) and the structure transition from a single fcc phase to a single bcc phase in HEAs. It was found that the fcc phase is stable for large values of VEC (≥ 8), while the bcc phase is stable for small values of VEC (≤ 6.87). Poletti and Battezzati[24] found that the HEAs with a single fcc (bcc) phase are stable when VEC > 7.5 and 1.6 < e/a < 1.8 (VEC < 7.5 and 1.8 < e/a < 2.3). Here, e/a is the average itinerant electron concentration (Section II–C).

Tripathy et al.[37] found that the product of \( S_{\text{E}} \) and the electronegativity difference \( \Delta \chi \) (or \( \delta r \)) is also able to describe phase selection between the fcc and bcc phases. Regarding that a large value of VEC is inclined to form an fcc phase and improve ductility while a small value of VEC tends to form a bcc phase and increase strength, VEC was adopted to modulate the strength and ductility of HEAs.[56] The validity of this proposal was proved by adding the Ni (Mo) element with a large (small) value of VEC 10 (6) to the AlCoCrFeNi (CoCrCuFeNi) with a small (large) value of VEC 7.2 (8.8). The study performed by Chen et al.,[56] however, did not provide quantitative design rules for HEAs with desired mechanical properties. Tian et al.[22] collected the HEAs with a single fcc and a single bcc phase, based on which they found that maximum hardness is achieved when VEC ≈ 6.8.

The current work aims to provide quantitative design rules for HEAs from structures (e.g., a single fcc phase, dual fcc and bcc phases, or a single bcc phase) to mechanical properties (e.g., hardness HV, yield strength \( \sigma_{\text{y}} \), and plastic strain \( \varepsilon_{\text{p}} \)). This study is based on the latest data collection of reported HEAs with a single fcc phase, with dual fcc and bcc phases, and with a single bcc phase (Supplementary Tables S-I and S-II). The preparation states of HEAs include as-cast (AC), as-homogenized (AH), as-deformed (AD), and mechanically alloyed (MA). First, the empirical parameters, including those for the atomic size difference \( \delta r \), \( \delta d \), \( \gamma \), and \( S_{\text{E}} \), the electronegativity difference \( \Delta \chi \) and \( \delta \chi \), the electron concentration VEC (or \( e/a \)) and its standard deviation \( \delta {\text{VEC}} \) (or \( \delta e/a \)), and the chemical bond mismatch \( \Delta H_{\text{mix}} \), \( \delta H_{\text{mix}} \), and \( \delta H_{\text{mix}}^{0} \), and those based on thermodynamic models \( \Omega \), \( \Phi \), and \( \Theta \), are described in Section II. After that, the relationships between the empirical parameters and the structures (the mechanical properties) are studied (Section III). It was found that VEC and δVEC are the parameters that can describe quantitatively phase selection between the fcc and bcc phases in HEAs. \( \delta r \) and \( S_{E} \) relate almost linearly with the mechanical properties. The relationship between VEC (δVEC) and the mechanical properties follows approximately a quadratic (cubic) function. The validity of current design rules is tested by application to some typical HEA systems (Section IV).

2 Empirical Parameters

The empirical parameters were generally proposed from the Hume–Rothery rules[57] and the thermodynamic model of Takeuchi and Inoue.[58,59,60] For the former, the stability of a solid-solution phase is controlled by the atomic size difference, the electronegativity difference, and the electron concentration. For binary alloys, a solid-solution phase is primarily formed when the atomic size difference is less than 15 pct, the electronegativity difference is small, and the electron concentration is within a proper range. For the latter, the difference between the Gibbs free energy of solid and liquid phases is assumed to be proportional to the mixing Gibbs free energy:

$$ \Delta G_{\text{mix}} = \Delta H_{\text{mix}} - T\Delta S_{\text{mix}} $$
(1)

A solid-solution phase is stable when the mixing entropy is able to restrain the tendencies of ordering and segregation. This means that a solid-solution phase is stable when the chemical bond mismatch is small or its effect can be offset by other factors.

2.1 Atomic Size Difference

The atomic size difference is a key factor for designing HEAs, e.g., a small value indicates a high possibility for the formation of a single solid-solution phase, a large value tends to form the amorphous phase, and otherwise HEAs with multiphases are formed.[14,38] To describe the comprehensive effect of atomic size difference, a standard deviation of dimensionless atomic radius \( \delta r \) was introduced by Zhang et al.[14] For an HEA with n components,

$$ \delta r = \sqrt {\mathop \sum \limits_{i = 1}^{n} c_{i} \left( {1 - \frac{{r_{i} }}{{\overline{r} }}} \right)^{2} } $$
(2)

where \( r_{i} \) is the atomic radius of component i and \( \overline{r} = \mathop \sum \limits_{i = 1}^{n} c_{i} r_{i} \) is the average atomic radius. Similar to \( \delta r \), the standard deviation of the dimensionless atomic radius in pairs \( \delta d \) was adopted by Wang et al.[27]:

$$ \delta d = \sqrt {\mathop \sum \limits_{i = 1}^{n} \mathop \sum \limits_{j > i}^{n} c_{i} c_{j} \left( {1 - \frac{{r_{i} + r_{j} }}{{2\overline{r} }}} \right)^{2} } $$
(3)

Further, the solid angles of atomic packing for the elements with the largest and smallest atomic sizes (\( \omega_{\text{L}} \), \( \omega_{\text{S}} \)) were introduced. Their ratio \( \gamma \) was chosen to describe the geometrical mismatch and topological instability in atomic packing:

$$ \gamma = \frac{{\omega_{\text{S}} }}{{\omega_{\text{L}} }} = \frac{{\left( {1 - \sqrt {\frac{{\left( {r_{\text{S}} + \overline{r} } \right)^{2} - \overline{r}^{2} }}{{\left( {r_{\text{S}} + \overline{r} } \right)^{2} }}} } \right)}}{{\left( {1 - \sqrt {\frac{{\left( {r_{\text{L}} + \overline{r} } \right)^{2} - \overline{r}^{2} }}{{\left( {r_{\text{L}} + \overline{r} } \right)^{2} }}} } \right)}} $$
(4)

where \( r_{\text{L}} \) and \( r_{\text{S}} \) are the radius of the largest and smallest atoms. Thermodynamically, the atomic size difference can be described by the geometrical mismatch entropy \( S_{\text{E}} \).

According to Mansoori et al.,[61]

$$ \frac{{S_{\text{E}} }}{{k_{\text{B}} }} = \frac{{F - F^{\text{id}} }}{{k_{\text{B}} T}} - \ln Z - \left( {3 - 2\xi } \right)\left( {1 - \xi } \right)^{ - 2} + 3 + \ln \left[ {\left( {1 + \xi + \xi^{2} - \xi^{3} } \right)\left( {1 - \xi } \right)^{ - 3} } \right] $$
(5)

where

$$ \frac{{F - F^{\text{id}} }}{{k_{\text{B}} T}} = - \frac{3}{2}\left( {1 - y_{1} + y_{2} + y_{3} } \right) + \left( {3y_{2} + 2y_{3} } \right)\left( {1 - \xi } \right)^{ - 1} + \frac{3}{2}\left( {1 - y_{1} + y_{2} - \frac{1}{3}y_{3} } \right)\left( {1 - \xi } \right)^{ - 2} + \left( {y_{3} - 1} \right)\ln \left( {1 - \xi } \right) $$
(6)
$$ Z = \left[ {\left( {1 + \xi + \xi^{2} } \right) - 3\xi \left( {y_{1} + y_{2} \xi } \right) - \xi^{3} y_{3} } \right]\left( {1 - \xi } \right)^{ - 3} $$
(7)
$$ y_{1} = \mathop \sum \limits_{i = 1}^{n} \mathop \sum \limits_{j > i}^{n} \Delta_{ij} \left( {d_{i} + d_{j} } \right)\left( {d_{i} d_{j} } \right)^{ - 1/2} $$
(8)
$$ y_{2} = \mathop \sum \limits_{i = 1}^{n} \mathop \sum \limits_{j > i}^{n} \Delta_{ij} \mathop \sum \limits_{k = 1}^{n} \frac{{\xi_{k} }}{\xi }\frac{{\left( {d_{i} d_{j} } \right)^{ - 1/2} }}{{d_{k} }} $$
(9)
$$ y_{3} = \left[ {\mathop \sum \limits_{i = 1}^{n} \left( {\frac{{\xi_{i} }}{\xi }} \right)^{2/3} c_{i}^{1/3} } \right]^{3} $$
(10)
$$ \Delta_{ij} = \frac{{\left( {\xi_{i} \xi_{j} } \right)^{1/2} }}{\xi }\frac{{\left( {d_{i} + d_{j} } \right)^{2} }}{{d_{i} d_{j} }}\left( {c_{i} c_{j} } \right)^{1/2} $$
(11)
$$ \xi = \mathop \sum \limits_{i = 1}^{n} \xi_{i} = \mathop \sum \limits_{i = 1}^{n} \frac{1}{6}\pi \rho c_{i} d_{i}^{3} $$
(12)

Here, \( d_{i} \) is the atomic diameter of component \( i \), \( \rho \) is the number density, \( \xi \) is the overall atomic packing fraction for a given \( \rho \), and \( k_{\text{B}} \) is the Boltzmann constant.

2.2 Electronegativity Difference

Electronegativity χ is a chemical property that describes the tendency of an atom to attract a shared pair of electrons toward itself. The electronegativity difference can be described by the standard deviation of electronegativity[17]:

$$ \Delta \chi = \sqrt {\mathop \sum \limits_{{i = 1}}^{n} c_{i} \left( {\chi _{i} - \bar{\chi }} \right)^{2} } $$
(13)

where \( \chi_{i} \) is the Pauling electronegativity of component \( i \) and \( \bar{\chi } = \mathop \sum \limits_{i = 1}^{n} c_{i} \chi_{i} \) is the average electronegativity. Similarly, the electronegativity difference can be described by standard deviation of dimensionless electronegativity; i.e.,

$$ \delta \chi = \sqrt {\mathop \sum \limits_{i = 1}^{n} c_{i} \left( {1 - \frac{{\chi_{i} }}{{\bar{\chi }}}} \right)^{2} } $$
(14)

The electronegativity difference was found to be able to describe phase selection between the fcc and bcc phases,[24] but it was not given much attention.[17,37]

2.3 Electron Concentration and Its Standard Deviation

The electron concentration can be defined by either the average number of itinerant electrons per atom, e/a, or the number of total electrons including the d-electrons accommodated in the valence band, VEC. For the former, we have

$$ e/a = \mathop \sum \limits_{i = 1}^{n} c_{i} \left( {e/a} \right)_{i} $$
(15)

For the latter, we have

$$ {\text{VEC}} = \mathop \sum \limits_{i = 1}^{n} c_{i} \left( {\text{VEC}} \right)_{i} $$
(16)

Here, \( \left( {e/a} \right)_{i} \) and \( \left( {\text{VEC}} \right)_{i} \) are the itinerant and the VEC of component \( i \). (A detailed description of e/a and VEC is available in References 1718, and 24 and the references therein.) In the present work, the standard deviation of dimensionless electron concentration is introduced:

$$ \delta e/a = \sqrt {\mathop \sum \limits_{i = 1}^{n} c_{i} \left( {1 - \frac{{\left( {e/a} \right)_{i} }}{e/a}} \right)^{2} } $$
(17)
$$ \delta {\text{VEC}} = \sqrt {\mathop \sum \limits_{i = 1}^{n} c_{i} \left( {1 - \frac{{\left( {\text{VEC}} \right)_{i} }}{\text{VEC}}} \right)^{2} } $$
(18)

In this way, both the average electron concentration and the electron concentration difference are considered to design HEAs.

2.4 Chemical Bond Mismatch

For an HEA with n elements, the mixing enthalpy \( \Delta H_{\text{mix}} \) is given by[58]

$$ \Delta H_{\text{mix}} = \mathop \sum \limits_{i = 1}^{n} \mathop \sum \limits_{j > i}^{n} \Omega_{ij} c_{i} c_{j} = \mathop \sum \limits_{i = 1}^{n} \mathop \sum \limits_{j > i}^{n} 4H_{\text{mix}}^{ij} c_{i} c_{j} $$
(19)

where \( H_{\text{mix}}^{ij} \) is the mixing enthalpy between components i and j. The mixing enthalpy actually describes the tendencies of ordering and segregation; e.g., a negative \( \Delta H_{\text{mix}} \) makes different components combine to form intermetallic compounds, while a positive \( \Delta H_{\text{mix}} \) makes a mix of different components difficult and leads to segregation in solids.[15] In this sense, a small value of \( \left| {\Delta H_{\text{mix}} } \right| \) results in the formation of HEAs with solid-solution phases. However, this is not always the case because a negligible \( \left| {\Delta H_{\text{mix}} } \right| \) does not guarantee that the mixing enthalpy of each atomic pair is negligibly small.[38] Furthermore, it was found that both the chemical bond mismatch between different atomic pairs and the geometrical mismatch between different components induce energy fluctuations in an alloy and make the mixing entropy change from an ideal to a nonideal one.[36] Similar to the standard deviation of the dimensionless atomic radius \( \delta r \) that characterizes the atomic size difference, the standard deviation of dimensionless mixing enthalpy was introduced to describe the chemical bond mismatch[38]:

$$ \delta H_{\text{mix}} = \frac{{\sqrt {\mathop \sum \nolimits_{i = 1}^{n} \mathop \sum \nolimits_{j > i}^{n} c_{i} c_{j} \left( {H_{\text{mix}}^{ij} - \Delta H_{\text{mix}} } \right)^{2} } }}{{{\text{k}}_{\text{B}} T_{m} }} $$
(20)

The relationship between the normalized energy fluctuation by He et al.,[36] \( x_{c} \), at the melting temperature and the standard deviation of dimensionless mixing enthalpy is \( x_{c} \left| {T = T_{m} } \right. = 2\sqrt {\delta H_{\text{mix}} } \). Because it is the difference between \( H_{\text{mix}}^{ij} \) and 0 but not between \( H_{\text{mix}}^{ij} \) and \( \Delta H_{\text{mix}} \) that characterizes the tendencies of ordering and segregation, the standard deviation of dimensionless mixing enthalpy was redefined as[38]

$$ \delta H_{\text{mix}}^{0} = \frac{{\sqrt {\mathop \sum \nolimits_{i = 1}^{n} \mathop \sum \nolimits_{j > i}^{n} c_{i} c_{j} \left( {H_{\text{mix}}^{ij} - 0} \right)^{2} } }}{{{\text{k}}_{\text{B}} T_{m} }} $$
(21)

Both \( \delta H_{\text{mix}} \) and \( \delta H_{\text{mix}}^{0} \) (or \( 2\sqrt {\delta H_{\text{mix}} } \) and \( 2\sqrt {\delta H_{\text{mix}}^{0} } \)) were found to be able to separate reasonably HEAs with a single solid-solution phase, with multiphases and with an amorphous phase; the latter predicts a little bit better than the former.[38]

2.5 Parameters Based on Thermodynamic Models

In the thermodynamic model of Takeuchi and Inoue[58,59,60] (Eq. [1]), \( \left| {\Delta H_{\text{mix}} } \right| \) is the driving force for ordering or segregation whereas \( \Delta S_{\text{mix}} \) is the resistant force. In the case that \( \Delta S_{\text{mix}} \) is given by \( S_{\text{config}} \), the competition between \( {\text{TS}}_{\text{config}} \) and \( \left| {\Delta H_{\text{mix}} } \right| \) determines the formation of solid-solution phases; i.e., a larger value of \( \Omega \) corresponds to a higher possibility for the formation of HEAs with solid-solution phases.[15] It should be mentioned that at the liquid state, the configurational entropy dominated over the enthalpy. If \( \Delta S_{\text{mix}} \) is given by \( S_{\text{config}} + S_{\text{E}} \),[58] Eq. [1] can be rewritten as \( \Delta G_{\text{mix}} = \Delta H_{\text{mix}} - T\left( {S_{\text{config}} + S_{\text{E}} } \right) \). When \( \Delta G_{\text{mix}} \) is dominated by \( \Delta S_{\text{mix}} \), we have \( \frac{{\left| {\Delta H_{\text{mix}} } \right|}}{{T\Delta S_{\text{mix}} }} < < 1 \) and \( {{\left| {S_{\text{E}} } \right|} \mathord{\left/ {\vphantom {{\left| {S_{\text{E}} } \right|} {S_{\text{config}} }}} \right. \kern-0pt} {S_{\text{config}} }} + {{S_{\text{H}} } \mathord{\left/ {\vphantom {{S_{\text{H}} } {S_{\text{config}} }}} \right. \kern-0pt} {S_{\text{config}} }} < < 1 \), indicating that both the atom size difference and the mixing enthalpy should be near zero for the formation of HEAs with single solid-solution phases. This is equivalent to the \( \Phi \) parameter, for which a large value indicates a high possibility for the formation of HEAs with a single solid-solution phase.[32]

Noting that the parameters \( \Omega \) and \( \Phi \) are based on the average properties of constituent elements, significant deviation of individual properties might make them inapplicable; a \( \Theta \) parameter that includes not only the average properties (e.g., \( S_{\text{config}} \), \( \Delta H_{\text{mix}} \), and \( S_{\text{E}} \)) but also the individual properties (e.g., the highest negative (positive) mixing enthalpy \( \Delta H_{\text{mix}}^{{ij,{ \hbox{min} }}} \) (\( \Delta H_{\text{mix}}^{{ij,{ \hbox{max} }}} \))) was proposed[39]:

$$ \Theta = \frac{{\left| {\Delta H_{\text{mix}} } \right|}}{{T_{\text{m}} S_{\text{config}} }} + \frac{{\left| {\Delta H_{\text{mix}}^{{ij,{ \hbox{min} }}} } \right|}}{{T_{\text{m}} S_{\text{config}} }}\frac{{\left| {\Delta H_{\text{mix}}^{{ij,{ \hbox{max} }}} } \right|}}{{T_{\text{m}} S_{\text{config}} }}\frac{{\left| {S_{\text{E}} } \right|}}{{S_{\text{config}} }} $$
(22)

The first, second, and third terms on the right-hand side of Eq. [22] characterize the tendencies for the formation of intermetallic compounds and segregation in solids, while the fourth term stands for the atomic size difference. In other words, both the chemical and geometrical mismatches are integrated into the \( \Theta \) parameter. For each of four terms, a small value corresponds to a high possibility for the formation of HEAs with a single solid-solution phase.

3 Design Rules

In this section, the relationship between the empirical parameters and the structures (the mechanical properties) is studied based on the current data collection of reported HEAs.

3.1 Predicting the Structures

Figure 1 shows the one-dimensional (1-D) maps for \( \delta r \), \( \delta d \), \( \gamma \), and \( S_{\text{E}} \). From Figure 1(a), HEAs with a single fcc phase, with dual fcc and bcc phases, and with a single bcc phase are found when 0.1 pct < δr < 5.6 pct, 3.1 pct < δr < 6.9 pct, and 2.2 pct < δr < 7.6 pct, respectively, even though the evolution tendency could be that a small (large) value of δr corresponds to a high possibility for the formation of HEAs with a single fcc (bcc) phase. The region of HEAs with dual fcc and bcc phases is totally within the region of HEAs with a single bcc phase. Different from Tripathy et al.,[37] the current work with more data collection of reported HEAs demonstrates that the standard deviation of dimensionless atomic radius is not able to separate reasonably the three regions. For \( \delta d \), \( \gamma \), and \( S_{\text{E}} \), the same evolution tendency can be found, i.e., a relatively small (large) atomic size difference corresponds to a high possibility for the formation of HEAs with a single fcc (bcc) phase. Because \( S_{\text{E}} \sim \left( {\delta r} \right)^{2} \) holds,[31] the prediction of \( S_{\text{E}} \) is similar to \( \delta r \); e.g., HEAs with a single fcc phase, with dual fcc and bcc phases, and with a single bcc phase are found when \( 0 < S_{\text{E}} < 0.11 \) (J mol−1 K−1), \( 0.03 < S_{\text{E}} < 0.17 \), and \( 0.01 < S_{\text{E}} < 0.20 \), respectively.

Fig. 1
figure 1

Effect of atomic size difference on phase selection between the fcc and the bcc phase in HEAs: (a) \( \delta r \times 100 \), (b) \( \delta d \), (c) \( \gamma \), and (d) \( S_{\text{E}} \)

Figure 2 shows the 1-D maps for the electronegativity difference \( \Delta \chi \) and \( \delta \chi \). It is obvious that for both \( \Delta \chi \) and \( \delta \chi \), regions of HEAs with dual fcc and bcc phases and with a single bcc phase are within the region of HEAs with a single fcc phase. Even though \( \delta \chi \) is able to separate the regions of HEAs with a single solid-solution phase, with a dual solid-solution phase and intermetallic compound,[24] it is insensitive to the crystal structure of solid-solution phase and, thus, is not able to describe phase selection between the fcc and bcc phases, consistent with Tripathy et al.[37]

Fig. 2
figure 2

Effect of electronegativity difference on phase selection between the fcc and bcc phases in HEAs: (a) \( \Delta \chi \) and (b) \( \delta \chi \)

Figure 3 show the 1-D maps for \( {\text{VEC}} \), \( \delta {\text{VEC}} \), \( e/a \), and \( \delta e/a \). One can see that \( {\text{VEC}} \) (\( \delta {\text{VEC}} \)) is able to separate the three regions; i.e., HEAs with a single fcc phase, with dual fcc and bcc phases, and with a single bcc phase are found when \( 7.7 < {\text{VEC}} < 8.9 \) (\( 0.17 < \delta {\text{VEC < 0}} . 3 2 \)), \( 6.8 < {\text{VEC}} < 8.5 \) (\( 0.21 < \delta {\text{VEC < 0}} . 4 6 \)), and \( 4.2 < {\text{VEC}} < 8.2 \) (\( 0.07 < \delta {\text{VEC < 0}} . 2 2 \) or \( 0.31 < \delta {\text{VEC < 0}} . 5 4 \)), respectively. These results are comparable with Guo et al.,[18] according to which an fcc (bcc) phase is stable for large (small) values of \( {\text{VEC}} \). For \( e/a \), the region of HEAs with dual fcc and bcc phases is within the region of HEAs with a single bcc phase. For \( \delta e/a \), the region of HEAs with a single fcc phase is within the region of HEAs with a single bcc phase. Therefore, phase selection between the fcc and bcc phases is insensitive to the itinerant electron concentration as well as its standard deviation.

Fig. 3
figure 3

Effects of electron concentration and electron concentration difference on phase selection between the fcc and bcc phases in HEAs: (a) \( {\text{VEC}} \), (b) \( \delta {\text{VEC}} \), (c) \( \frac{e}{a} \), and (d) \( \delta \frac{e}{a} \)

Figure 4 shows the effects of mixing enthalpy and chemical bond mismatch on phase selection between the fcc and bcc phases in HEAs. For the former, the region of HEAs with a single bcc (fcc) phase locates at small (large) values and the region of HEAs with dual fcc and bcc phases is totally within the region of HEAs with a single bcc region (Figure 4(a)). Similar results are found for \( 2\sqrt {\delta H_{\text{mix}} } \) and \( 2\sqrt {\delta H_{\text{mix}}^{0} } \), as shown in Figures 4(b) and (c). In contrast to the fact that the chemical bond mismatch plays an important role in the design of HEAs with a single solid-solution phase,[36,38,39] it seems to be irrelevant to the design of HEAs with dual fcc and bcc phases.

Fig. 4
figure 4

Effects of mixing enthalpy and the chemical bond mismatch on phase selection between the fcc and bcc phases in HEAs: (a) \( \Delta H_{\text{mix}} \), (b) \( 2\sqrt {\delta {\text{H}}_{\text{mix}} } \), and (c) \( 2\sqrt {\delta H_{\text{mix}}^{0} } \)

Figure 5 shows the predictions of \( \Omega \), \( \Phi \), and \( \Theta \). Such empirical parameters derived from the thermodynamic models include either the chemical effect of mixing enthalpy (i.e., \( \Omega \)) or the effects of both chemical band mismatch and atomic size difference (i.e., \( \Phi \) and \( \Theta \)). Similar to the results represented in Figures 1 and 4, the region of HEAs with dual bcc and fcc phases is totally within the region of HEAs with a single bcc phase; thus, all of these empirical parameters fail to predict phase selection between the fcc and bcc phases in HEAs.

Fig. 5
figure 5

Effects of (a) \( \Omega \), (b) \( \Phi \), and (c) \( \Theta \) on phase selection between the fcc and bcc phases in HEAs

From Figures 1 through 5, phase selection is insensitive to the atomic size difference, the electronegativity difference, the average itinerant electron concentration and its standard deviation, the chemical bond mismatch, as well as a combination of these effects. This is also the case for the empirical parameter \( S_{\text{E}} \Delta \chi \) (\( S_{\text{E}} \delta r \)) adopted by Tripathy et al.[42] (not shown here), which is a combination of the atomic size difference and the electronegativity difference (different empirical parameters for the atomic size difference). The average VEC and its standard deviation are the only parameters that are sensitive to the crystal structure of solid-solution phase. According to Chen et al.,[56] a larger (smaller) value of \( {\text{VEC}} \) induces higher (lower) atomic bonding forces, so that the alloy tends to form an fcc (bcc) structure with a larger (smaller) atomic packing density. Therefore, \( \delta {\text{VEC}} \) might characterize the difference (fluctuation) in the atomic bonding forces. Accordingly, either a smaller or a larger difference (or value of fluctuation) in the atomic bonding forces tends to form a single bcc phase in HEAs, while an intermediate value indicates the formation of HEAs with a single fcc phase. In the current work, the sufficient condition for designing HEAs with a single fcc phase is \( {\text{VEC}} > 8.5 \). For the HEAs with dual bcc and fcc phases (a single bcc phase), it is \( \delta {\text{VEC}} > 0.32 \) (\( \delta {\text{VEC < 0}} . 1 7 \) or \( \delta {\text{VEC > 0}} . 4 6 \)). Such rules for designing HEAs with dual bcc and fcc phases are so rigorous that they may lose most of the potential HEAs. Therefore, it is more sensible to design first an HEA with a single fcc (bcc) phase by the necessary condition \( {\text{VEC > 7}} . 7 \) or \( 0.17 < \delta {\text{VEC < 0}} . 3 2 \) (\( {\text{VEC}} < 8.2 \), \( \delta {\text{VEC < 0}} . 2 2 \), or \( \delta {\text{VEC > 0}} . 3 1 \)) and then add other elements with lower (higher) values of VEC.[5]

It should be pointed out that Zhang et al.[62] studied the effect of nitrogen addition on the structure and mechanical properties of (Al0.5CrFeNiTi0.25)Nx high-entropy films by magnetron sputtering (MS). The film is amorphous when x = 0 and is transformed to a single fcc phase with increasing addition of nitrogen. The Al0.5CrFeNiTi0.25 HEA prepared by casting is a single bcc phase. If these results are included, e.g., as stars in Figures 3(a) and (b), one can see that they are out of the region with a single fcc phase. Indeed, films prepared by MS are quite different from bulk alloys prepared by AC, AH, AD, and MA. Predicting their phase constitution is outside the scope of the current work.

3.2 Predicting the Mechanical Properties

In the work of Tian et al.,[22] which aimed to design HEAs with high hardness, \( {\text{VEC}} \) and \( \delta r \) were adopted. The former determines the structures and affects the mechanical properties. The latter characterizes the atomic size difference. It is highly related to the atomic stress state in solids and, hence, the mechanical properties. In the current work, the geometrical mismatch entropy, \( S_{\text{E}} \), that is frequently used and the standard deviation of VEC, \( \delta {\text{VEC}} \), that is introduced currently are adopted further to predict the mechanical properties of HEAs.

Figure 6 shows the effects of the atomic size difference, the average VEC, and its standard deviation on hardness HV. Despite its large scatter, hardness HV increases continuously with \( \delta r \) and \( S_{\text{E}} \) (Figures 6(a) and (b)). If a linear function is adopted, the relationship between HV and \( \delta r \) (\( S_{\text{E}} \)) is \( {\text{HV}} = 97.1 + 65.2\delta r \times 100 \) (\( {\text{HV}} = 206.0 + 2191.3S_{\text{E}} \)). With the increase of \( {\text{VEC}} \), HV increases first and then decreases, as shown in Figure 6(c). The relationship between HV and \( {\text{VEC}} \) can be well predicted by the quadratic function \( {\text{HV}} = - 2177.4 + 888.56{\text{VEC }} - 7 1. 6 {\text{VEC}}^{2} \), according to which a critical value of \( {\text{VEC = 6}} . 2 \) is found at which hardness is a maximum. With the increase of \( \delta {\text{VEC}} \), HV decreases first and then increases (Figure 6(d)). If a cubic function is adopted to fit the relationship, \( {\text{HV}} = 986.3 - 8592.6\delta {\text{VEC + 29470}} . 8\delta {\text{VEC}}^{2} - 26771.1{\text{VEC}}^{3} \) results according to which a critical value of \( \delta {\text{VEC = 0}} . 2 \) is predicted at which hardness is a minimum.

Fig. 6
figure 6

Hardness HV as a function of (a) \( \delta r \times 100 \), (b) \( S_{\text{E}} \), (c) \( {\text{VEC}} \), and (d) \( \delta {\text{VEC}} \) for HEAs with a single fcc phase, with dual fcc and bcc phases, and with a single bcc phase

Figure 7 shows the yield strength \( \sigma_{\text{y}} \) as a function of \( \delta r \times 100 \), \( S_{\text{E}} \), \( {\text{VEC}} \), and \( \delta {\text{VEC}} \). The relationship between \( \sigma_{\text{y}} \) and \( \delta r \times 100 \) (\( S_{\text{E}} \), \( {\text{VEC}} \), and \( \delta {\text{VEC}} \)) is completely consistent with that between HV and \( \delta r \times 100 \) (\( S_{\text{E}} \), \( {\text{VEC}} \), and \( \delta {\text{VEC}} \)). \( \sigma_{\text{y}} \) increases almost linearly with the atomic size difference and the relationships are \( \sigma_{\text{y}} = 199.2 + 194.3\delta r \times 100 \) and \( \sigma_{\text{y}} = 571.7 + 5924.1S_{\text{E}} \). \( \sigma_{y} \) increases first with VEC and then decreases, whereas it decreases first with \( \delta {\text{VEC}} \) and then increases. The relationships fitted by the quadratic and the cubic function are \( \sigma_{\text{y}} = - 7486.7 + 3075.0{\text{VEC }} - 2 5 5. 2 {\text{VEC}}^{2} \) and \( \sigma_{\text{y}} = 1665.5 - 3724.2\delta {\text{VEC}} - 8 7 8 2. 4\delta {\text{VEC}}^{2} + 46957.2\delta {\text{VEC}}^{3} \), respectively. The maximum and minimum \( \sigma_{\text{y}} \) are found at \( {\text{VEC = 6}} . 1 \) and \( \delta {\text{VEC = 0}} . 2 3 \), respectively.

Fig. 7
figure 7

Yield strength \( \sigma_{\text{y}} \) as a function of (a) \( \delta r \times 100 \), (b) \( S_{\text{E}} \), (c) \( {\text{VEC}} \), and (d) \( \delta {\text{VEC}} \) for HEAs with a single fcc phase, with dual fcc and bcc phases, and with a single bcc phase

Figure 8 summarizes the effects of the atomic size difference, the average VEC, and its standard deviation on the plastic strain. It is quite obvious that the relationships between the empirical parameters and the plastic strain are completely opposite to those between the empirical parameters and hardness as well as the yield strength. With the increase of atomic size difference, the plastic strain \( \varepsilon_{\text{p}} \) decreases almost linearly and the relationships are \( \varepsilon_{\text{P}} = 46.6 - 4.6\delta r \times 100 \) and \( \varepsilon_{\text{P}} = 35.6 - 119.4S_{\text{E}} \) (Figures 8(a) and (b)). \( \varepsilon_{\text{p}} \) decreases (increases) first with \( {\text{VEC}} \) (\( \delta {\text{VEC}} \)) and then increases (decreases) (Figures 8(c) and (d)). \( \sigma_{\text{y}} = 224.8 - 72.2{\text{VEC + 6VEC}}^{2} \,(\sigma_{\text{y}} = - 101.6 + 1750.7\delta {\text{VEC}} - 6 9 7 4. 2\delta {\text{VEC}}^{2} + 8334.5\delta {\text{VEC}}^{3} ) \) holds. Accordingly, the minimum and maximum plastic strains are achieved at \( {\text{VEC = 6}} . 1 \) and \( \delta {\text{VEC = 0}} . 1 9 \), respectively.

Fig. 8
figure 8

Plastic strain \( \varepsilon_{\text{p}} \) as a function of (a) \( \delta r \times 100 \), (b) \( S_{\text{E}} \), (c) \( {\text{VEC}} \), and (d) \( \delta {\text{VEC}} \) for HEAs with a single fcc phase, with dual fcc and bcc phases, and with a single bcc phase

From Figures 6(c) through 8(c), maximum hardness, maximum strength, and lowest ductility are obtained at almost the same value of average VEC, which is \( {\text{VEC}}^{*} \approx 6.13 \) if the three critical values are averaged. It is not far away from \( {\text{VEC = }}6.8 \) at which hardness is maximum in the work of Tian et al.[22] According to Figure 3(a), the structure of HEAs at \( {\text{VEC}} \approx 6.13 \) is a single bcc phase, indicating that the strongest but brittle HEA should be the HEA with a single bcc phase and with \( {\text{VEC}} \approx 6.13 \), away from which a sharp decrease (increase) of strength (ductility) is identified. From Figures 6(d) through 8(d), lowest hardness, lowest strength, and maximum ductility are also obtained at similar values of standard deviation of the average VEC, which is \( \delta {\text{VEC}}^{*} \approx 0.207 \), if the three critical values are averaged. According to Figure 3(b), the structure of HEAs at \( \delta {\text{VEC}} \approx 0.207 \) consists of a single fcc phase. This means that the most ductile but weak HEAs should be the HEA with a single fcc phase and with \( \delta {\text{VEC}} \approx 0.207 \), away from which a sharp increase (decrease) of strength (ductility) is revealed. Therefore, a modulation between strength and ductility should be achieved by the HEAs with dual fcc and bcc phases, and \( {\text{VEC}} \) (\( \delta {\text{VEC}} \)) can vary away from 6.13 (0.207) to obtain a large ductility (a high strength).

4 Application to Typical HEA Systems

In this section, three typical HEA systems are chosen to study the validity of current design rules of HEAs (Table I). Kao et al.[63] studied the structures and hardness of the AC, AH, and as-deformed AlxCoCrFeNi (0 ≤ x ≤ 2) HEAs. For the AC HEAs, the critical value of x for the transition from HEAs with a single fcc phase (dual fcc and bcc phases) to dual fcc and bcc phases (a single bcc phase) is x = 0.45 (x = 0.88) at which \( {\text{VEC}} = 7.72 \) and \( \delta {\text{VEC}} = 0.27 \) (\( {\text{VEC}} = 7.30 \) and \( \delta {\text{VEC}} = 0.33 \)). One can see that the decrease of VEC from 7.72 to 7.30 (or the increase of \( \delta {\text{VEC}} \) from 0.27 to 0.33) leads to the structure transition being consistent with the necessary condition for the formation of HEAs with dual fcc and bcc phases, i.e., \( 6.8 < {\text{VEC < 8}} . 5 \) and \( 0.21 < \delta {\text{VEC < 0}} . 4 6 \). With the increase of x, the value of VEC decreases continuously from VEC = 8.25 for the CoCrFeNi HEA to VEC = 6.50 for the CoCrFeNiAl2.0 HEA. Their hardness decreases first and then increases. The maximum (minimum) hardness HV = 509 (110) was obtained by the CoCrFeNiAl2.0 (CoCrFeNiAl0.25) HEA. Noting that the values of VEC are always smaller than the critical value \( {\text{VEC}}^{*} \approx 6.13 \) at which hardness should be maximum, the increases of HV from the CoCrFeNiAl0.25 HEA to the CoCrFeNiAl2 HEA with the decrease of VEC are completely consistent with the current design rules. In addition, \( \delta {\text{VEC = 0}} . 2 4 \) of the CoCrFeNiAl0.25 HEA is very near to the critical value \( \delta {\text{VEC}}^{*} \approx 0.207 \) at which hardness should be minimum. Despite the difference in the processing procedures and, thus, hardnesses, the AH and as-deformed AlxCoCrFeNi (0 ≤ x ≤ 2) HEAs follow nearly the same rules (Supplementary Tables S-I and S-II).

Table I Summary of Standard Deviation of Atomic Radius \( \delta r \), the Excessive Mixing Entropy Due to the Geometrical Mismatch \( S_{\text{E}} \) (J mol−1 K−1), the Average VEC and Its Standard Deviation \( \varvec{\delta}{\text{VEC}} \), the Hardness HV (kgf mm−2), the Yield Strength \( \sigma_{\text{y}} \) (MPa), the Plastic Strain \( \varepsilon_{\text{p}} \) (Pct) Under Compressive Tests, and the Structure and Processing for the AlxCoCrFeNi (0 ≤ x ≤ 2),[63] AlxCoCrCuFeNi (x = 0, 0.5, 1, and 2.5),[64] and Ti0.5CrFeCoNiAlxCu1−x (x = 0.25, 0.5, and 0.75)[65] HEAs

Tong et al.[64] studied the mechanical properties of AlxCoCrCuFeNi (x = 0, 0.5, 1, and 2.5) and found that as x increases, hardness (the compressive yield strength) increases from 133 to 550 (230 to 1620 MPa). Meanwhile, VEC decreases continuously from 8.80 to 7.14 and \( \delta {\text{VEC}} \) increases gradually from 0.20 to 0.42. Noting that the minimum value VEC = 7.14 is smaller than \( {\text{VEC}}^{*} \approx 6.13 \) and \( \delta {\text{VEC = 0}} . 2 0 \) for the CoCrCuFeNi HEA with the smallest hardness and the yield strength is very near to \( \delta {\text{VEC}}^{*} \approx 0.207 \), the current design rules are followed by the AlxCoCrCuFeNi HEAs. In another work of Wang et al.,[65] the Ti0.5CrFeCoNiAlxCu1−x HEAs were studied. Ti0.5CoCrFeNiAl0.25Cu0.75 (Ti0.5CoCrFeNiAl0.75Cu0.25) is an HEA with a single fcc (bcc) phase whose yield strength and compressive plastic strain are 750 (1900) MPa and 38.5 pct (12 pct), while the Ti0.5CoCrFeNiAl0.5Cu0.5 HEA with dual fcc and bcc phases has a yield strength and a compressive plastic strain of 1580 MPa and 17.4 pct, respectively. The Ti0.5CoCrFeNiAl0.75Cu0.25 HEA, whose value of VEC (= 7.27) is nearest to \( {\text{VEC}}^{*} \approx 6.13 \), has the highest yield strength. The Ti0.5CoCrFeNiAl0.25Cu0.75 HEA, whose value of \( \delta {\text{VEC}} \) (= 0.29) is closest to \( \delta {\text{VEC}}^{*} \approx 0.207 \), has the best ductility. All these results indicate that the current design rules are effective for designing HEAs with dual fcc and bcc phases.

5 Conclusions

The experimental results reported for HEAs with a single fcc phase, with dual fcc and bcc phases, and with a single bcc phase were collected, based on which the design rules for HEAs with dual fcc and bcc phases were studied from structures to mechanical properties. Phase selection between the fcc and bcc phases in HEAs was found to be insensitive to the atomic size difference, the electronegativity difference, the average itinerant electron concentration and its standard deviation, as well as the chemical bond mismatch. The average VEC and its standard deviation are the only parameters that are sensitive to the crystal structure of solid-solution phase. The current work suggests that it is more sensible to design first an HEA with a single fcc (bcc) phase by the necessary condition \( {\text{VEC > 7}} . 7 \) or \( 0.17 < \delta {\text{VEC < 0}} . 3 2 \) (\( {\text{VEC}} < 8.2 \), \( \delta {\text{VEC < 0}} . 2 2 \) or \( \delta {\text{VEC > 0}} . 3 1 \)) and then add other elements with lower (higher) values of VEC. The mechanical properties were found to relate linearly with the atomic size difference. Highest (lowest) hardness, highest (lowest) strength, and lowest (highest) ductility were obtained at nearly the same critical value \( {\text{VEC}}^{*} \approx 6.13 \) (\( \delta {\text{VEC}}^{*} \approx 0.207 \)), which corresponds to the HEA with a single bcc (fcc) phase. Therefore, a modulation between strength and ductility can be achieved by the HEAs with dual fcc and bcc phases.[66] The validity of the current design rules was tested by application to the AlxCoCrFeNi (0 ≤ x ≤ 2), AlxCoCrCuFeNi (x = 0, 0.5, 1, and 2.5), and Ti0.5CrFeCoNiAlxCu1−x (x = 0.25, 0.5, and 0.75) HEAs.