We report the selective etching mechanism of silicon oxide using a mixture of hydrogen fluoride (HF) and NH4F gases. A damage-free selective removal of native oxide has been used in semiconductor manufacturing by forming and removing the ammonium fluorosilicate [(NH4)2SiF6] salt layer. A downstream plasma of NF3/NH3 or a gas-phase mixture of HF and NH4F was used to form (NH4)2SiF6. We modeled and simulated the fluorination of silicon oxide and the salt formation by density functional theory calculation. First, we simulated the successive fluorination of silicon oxide using SiO2 slab models. The fluorination reactions of SiO2 surfaces by the mixture produced a volatile SiF4 molecule or a surface anion of –OSiF4−* with an NH4+ cation with low activation energies. Unlike HF, NH4F produced surface salt species consisting of a surface anion and an ammonium cation. Next, we simulated the (NH4)2SiF6 formation from the two reaction products on fluorinated SiO2 surfaces. (NH4)2SiF6 can be formed exothermally with low activation energies (0.27 or 0.30 eV). Finally, we compared silicon with SiO2 to demonstrate the inherently selective etching of silicon oxide. The fluorination reactions of silicon by the mixture showed the activation energies significantly higher than the SiO2 cases, 1.22–1.56 eV by HF and 1.94–2.46 eV by NH4F due to the less stable transition state geometries. Therefore, the selective salt formation on silicon oxide, not on silicon, is expected in near-room temperature processing, which enables selective etching of silicon oxide.

In semiconductor manufacturing, removing native oxide on the silicon surface is one of the most critical processes in obtaining low contact resistance. The wet cleaning processes using dilute hydrogen fluoride (HF) solutions have been the most widely used method for removing oxide. However, they cannot completely prevent the formation of native oxides because the wafer is exposed to air before being loaded into the selective epitaxial growth chamber or metal deposition system. Thus, in situ gas-phase cleaning techniques, such as downstream plasma etching,1–18 sputter etching,19–22 or HF vapor etching,23,24 were introduced to complement the wet cleaning process.

Nishino et al. reported a damage-free selective removal of native oxide using an NF3/NH3 downstream plasma and subsequent vacuum annealing at 100 °C.25 A cleaning process based on NF3/NH3 remote plasma was commercialized under the trademark SiConi1 and adopted in several applications, such as precleaning of silicon surface before the nickel deposition for silicidation8–10 or before the selective epitaxial growth of silicon-germanium,7,17 the profile modification of interlayer dielectric12,16 or shallow trench oxide,5 and removal of dummy gate oxides.2,4,6,15 The process represented a lower contact resistivity and a smoother surface than wet cleanings by HF.9 

The removal of the native oxide by the SiConiTM process comprises two steps. The first step is the formation of a fluorinated salt layer by a remote plasma of NF3/NH3 at near-room temperatures.26–29 The second step is the sublimation of the salt layer by annealing with a temperature of 100 °C or higher.1,10,26 The general reaction scheme has been established by several reports.25,27,30,31 The NF3/NH3 plasma has been reported to generate active species such as HF and ammonium fluoride (NH4F).32 The gas-phase etching by a mixture of HF and NH3 without plasma also showed an etching mechanism similar to NF3/NH3 plasma.30,31 Analysis by Fourier transform infrared spectroscopy and reflection absorption spectroscopy confirmed that the composition of the salt layer was ammonium hexafluorosilicate, (NH4)2SiF6.27,32 It was proposed that NH3 and HF adsorbed on the surface react with the etching byproduct, silicon tetrafluoride (SiF4), to form (NH4)2SiF6. However, more detailed reaction mechanisms have not yet been elucidated. The etching mechanism of SiO2 by HF to form SiF4 has been studied by density functional theory (DFT) using the SiO2 cluster model33 or SiO2 slab model34 as a substrate surface. The etching of SiO2 by HF is energetically favorable, with low activation energies of about 0.72–0.79 eV,34 implying continuous etching even at near-room temperatures. However, the etching mechanism by NH4F has not yet been reported. Also, the mechanism of the (NH4)2SiF6 salt formation on silicon oxide surfaces was not elucidated. Understanding the detailed reaction mechanism underlying the cleaning process by a mixture of HF and NH4F would lay a foundation for developing next-generation cleaning processes.

In the present study, we modeled and simulated the surface reaction mechanism during silicon oxide removal using a mixture of HF and NH4F by DFT calculation. First, we simulated the successive fluorination of silicon oxide using slab models. Next, we simulated the mechanism of the (NH4)2SiF6 salt formation on fluorinated SiO2 surfaces. Finally, we compared silicon with SiO2 to demonstrate the inherently selective etching of silicon oxide. We calculated the adsorption, reaction, and activation energies for the reactions to expect the probable route of the etching process.

The DFT calculations were carried out using the Dmol3 package, material studio 7.0 (BIOVIA, USA).35,36 The calculations used the generalized gradient approximation functional and the Perdew–Burke–Ernzerhof scheme correlation.37 For dispersion correction, the DFT-D2 using Grimme's method was applied.38 The basis set of the double numerical polarization (DNP) 4.4 was selected due to the relatively high accuracy and low computation cost.39,40 The accuracy and cost of the simulation were compared in Fig. S1 in the supplementary material.41 The self consistent field tolerance was 10−6 Ha. The calculations employed the Monkhorst-pack grid of 2 × 2 × 1 k-point parameter and the global orbital cutoff of 4.6 Å. The spin-unrestricted calculation condition was used. All geometry optimization calculations used the tolerance convergence energy of 10−6 Ha (1 Hartree = 27.2114 eV), the atomic force of 2 × 10−4 Ha/Å, and the maximum displacement of 0.005 Å, as the same parameter setting in the previous works.34,42,43

The hydroxylated and fluorinated SiO2 slab models were used for the DFT simulation: –Si(OH)2, –Si(OH)F, –SiF2, and –SiF3 terminated cristobalite SiO2 (001) 2 × 2 surfaces. Also, the hydrogenated and fluorinated Si surface slab models were used: –SiH2, –SiHF, –SiF2, and –SiF3 terminated Si (100) 2 × 2 surfaces. The details of the surface slab models can be found in our previous work.34 

We defined the states for the reaction coordinates: the unbound reactant (UR), reactant (R), transition (TS), product (P), and unbound byproduct (UP) states. In UR, since the reactant gas molecule is assumed to be separated infinitely from the surface, the energy of UR is the sum of the energies of the slab (Eslab) and reactant gas molecule (Ereactant). Then, in R, the gas molecule physisorbs on the surface. Next, the molecule reacts with the surface in P to form byproducts. Finally, in UP, byproduct molecules are separated from the surface at an infinite distance. Therefore, the energy of UP was determined by the sum of the energy of the reacted slab (Ereacted slab) and byproduct gas molecule (Ebyproduct). TS between R and P was obtained using the complete linear and quadratic synchronous transit (LST-QST) or QST method. Then, it requires a repeated QST process and repeated conjugate gradient minimizations until the gradient's energy is lower than 0.002 Ha/Å.44 The details of the transition state search method can be found in the previous work.45 We determined the adsorption energy (Eads), activation energy (EA), reaction energy (ΔE), and desorption energy (Edes) of reactions using the following equations:
(1)
(2)
(3)
(4)
where ERn, ETSn, and EPn are the total energy of R, TS, and P for the reaction of the nth step. When the intermediate state (I) is obtained between R and P, the reaction and activation energies were calculated for R to I and I to P, respectively, as follows:
(5)
(6)
(7)
(8)
where ETSn(1) and ETSn(2) are the total energy of the transition state between R and I state and between I and P, respectively, for the reaction of the nth step. EIn is the total energy of I for the reaction of the nth step.
We summarized all possible reaction routes for the fluorination of SiO2 by a mixture of HF and NH4F in Fig. 1 with activation energy values. Successive fluorination reactions of SiO2 by HF were favorable due to the relatively low activation energies of about 0.72–0.79 eV.34 As a result, the continuous etching of SiO2 by HF is predicted without NH4F, which agrees well with well-known knowledge or experimental observations.24,46,47 In this study, we studied the fluorinations of SiO2 by NH4F molecules in four consecutive steps to form the SiF4 byproduct, similar to studying the reaction by HF in the previous work.34 The first, second, third, and fourth fluorination steps by NH4F were assumed, as shown in Eqs. (9)(12),
(9)
(10)
(11)
(12)
where * denotes a surface species. In every step, an Si–O bond of SiO2, H–F, and N–H bonds of NH4F are dissociated, and Si–F and O–H bonds are generated. The –SiOH* surface groups are replaced by –SiF* by Eqs. (9) and (10), and then regenerated by Eqs. (11) and (12). In the absence of HF, NH4F would produce fluorinated surface anions [–SiF2(OH)*, –SiF3*, or –SiF4*] and NH4+ cations. In the presence of HF, the surface anions would be transformed into another surface anion with an additional fluorine atom.
FIG. 1.

Schematic of reaction routes for the fluorination of SiO2 by a mixture of HF and NH4F with activation energy values. The activation energy values for the fluorination of SiO2 by HF were taken from previous work (Ref. 34).

FIG. 1.

Schematic of reaction routes for the fluorination of SiO2 by a mixture of HF and NH4F with activation energy values. The activation energy values for the fluorination of SiO2 by HF were taken from previous work (Ref. 34).

Close modal

For the fluorinations of SiO2 by NH4F molecules, we used four types of surface slab models with different degrees of fluorination for four fluorination steps by NH4F. Therefore, a single energy diagram could not represent the four fluorination steps. Also, since we used the same method in our previous paper on the reaction of HF, a direct comparison of the HF and NH4F reactions would be straightforward.

Figure 2 shows the energy diagram and the changes in atomistic structures during the first step in Eq. (9). At first, NH4F physisorbed on the –OH terminated SiO2 surface in R1, with an energy of −1.03 eV. It was more favorable than the adsorption of HF (−0.53 eV)34 due to the more hydrogen bonding of NH4F than HF. The length of the H–F bond of the physisorbed NH4F was 1.09 Å, elongated from 0.98 Å of isolated NH4F. Then, an F atom of NH4F replaced an OH group on the surface, producing a –Si(OH)F surface group, an H2O, and an NH3 molecule in P1. The reaction energy was −0.44 eV, which is similar to that of the first fluorination step by HF (−0.37 eV).34 The exothermicity can be described by the formation of Si–F (7.15 eV34) and O–H (5.20 eV34) bonds in P1 despite the dissociation of Si–O (6.15 eV34), H–F (6.76 eV), and N–H (0.71 eV) bonds. We calculated the bond dissociation energies of H–F and N–H using the same methods in the literature,48–50 as shown in Fig. S2 in the supplementary material.41 The desorption of the byproducts, H2O and NH3, was endothermic with an energy of 2.00 eV in UP1. However, H2O would spontaneously desorb at near-room temperature because Gibb's free energy change was negative above 11 °C, as shown in Fig. S3 in the supplementary material.41 On the other hand, NH3 would remain on the surface at near-room temperature because Gibb's free energy change was negative only above 106 °C, as shown in Fig. S4 in the supplementary material.41 However, in the mixture of HF and NH4F, NH3 would react with HF to form NH4F.

FIG. 2.

(a) Energy diagram, with the values of Eads, EA, and ΔE, and (b) the change in the atomistic structure for the first fluorination step of SiO2 by NH4F. Energy values and interatomic distances are displayed in eV and Å, respectively. The dotted lines represent hydrogen bonding.

FIG. 2.

(a) Energy diagram, with the values of Eads, EA, and ΔE, and (b) the change in the atomistic structure for the first fluorination step of SiO2 by NH4F. Energy values and interatomic distances are displayed in eV and Å, respectively. The dotted lines represent hydrogen bonding.

Close modal

In the transition state, TS1, NH4F was attached to –SiOH* to form an elongated Si–F bond with a length of 2.18 Å, as shown in Fig. 2(b). The H–F bond in NH4F was elongated from 1.09 Å in R1 to 1.18 Å in TS1. The Si–O bond of –SiOH* was also slightly elongated from 1.64 to 1.69 Å. There was no four-membered ring structure of –Si–O–H–F–, observed in the previous work with HF.34 Instead, an N–H bond was formed inside the NH4F molecule. The activation energy was low at 0.67 eV, possibly due to the absence of bond dissociation in TS1, and was similar to 0.77 eV of the HF case.34 Therefore, the first step would be kinetically plausible.

Figure 3 shows the energy diagram and the changes in the atomistic structures of the second step in Eq. (10). First, in R2, NH4F physisorbed on the –Si(OH)F terminated SiO2 surface with an energy of −0.78 eV. It was less favorable than in R1 due to the fewer hydrogen bondings. We assumed that F of NH4F was exchanged with OH of –Si(OH)F*, forming –SiF2*, H2O, and NH3 in P2.

FIG. 3.

(a) Energy diagram, with the values of Eads, EA, and ΔE, and (b) the change in the atomistic structure for the second fluorination step of silicon oxide by NH4F. Energy values and interatomic distances are displayed in eV and Å, respectively. The dotted lines represent hydrogen bonding.

FIG. 3.

(a) Energy diagram, with the values of Eads, EA, and ΔE, and (b) the change in the atomistic structure for the second fluorination step of silicon oxide by NH4F. Energy values and interatomic distances are displayed in eV and Å, respectively. The dotted lines represent hydrogen bonding.

Close modal
A stable intermediate state (I2) was obtained between R2 and P2 with a –Si(OH)F2* surface anion and an NH4+ cation. Therefore, we considered a two-step reaction from R2 to I2 and then I2 to P2 as described in Eqs. (10a) and (10b),
(10a)
(10b)

The reaction energy from R2 to I2 in Eq. (10a) was −0.14 eV. In TS2(1) between R2 and I2, NH4F was attached to –Si(OH)F* with an elongated Si–F bond (2.17 Å), as shown in Fig. 3(b), which is similar to TS1. The activation energy was low at 0.29 eV, also due to the absence of bond dissociation. Therefore, the formation of I2 in Eq. (10a) would be energetically and kinetically favorable. The reaction from I2 to P2 in Eq. (10b) was endothermic, with an energy of 0.35 eV, mainly due to the strong ionic interaction between the NH4+ cation and the –Si(OH)F2* surface anion. A transition state, TS2(2), was discovered between I2 and P2 with the formation of Si–OH2*, as shown in Fig. 3(b). The activation energy was 0.53 eV due to the N–H bond dissociation, O–H bond formation, and Si–O bond elongation. As a result, the energy diagram of Fig. 3(a) suggested that the reaction with NH4F would stop in I2.

Since the second fluorination step by NH4F would not be plausible, the –SiF2* terminated surface would not be generated by NH4F. However, we considered the further fluorination of the –SiF2* terminated surface by NH4F because the –SiF2* terminated surface is generated by HF. Figure 4 shows the energy diagram and the changes in the atomistic structures for the third-step reaction in Eq. (11). Initially, NH4F is physisorbed on the –SiF2 terminated surface, with an energy of −0.58 eV. It was less favorable than R1 or R2 due to the weaker interaction between NH4F and the –SiF2 terminated surface. We assumed that the Si–O bonds of the surface were cleavaged by NH4F, forming –SiF3*, –SiOH*, and NH3 in P3.

FIG. 4.

(a) Energy diagram, with the values of Eads, EA, and ΔE, and (b) the change in the atomistic structure for the third fluorination step of silicon oxide by NH4F. Energy values and interatomic distances are displayed in eV and Å, respectively. The dotted lines represent hydrogen bonding.

FIG. 4.

(a) Energy diagram, with the values of Eads, EA, and ΔE, and (b) the change in the atomistic structure for the third fluorination step of silicon oxide by NH4F. Energy values and interatomic distances are displayed in eV and Å, respectively. The dotted lines represent hydrogen bonding.

Close modal
Similar to the second fluorination by NH4F in Eq. (10), the reaction of NH4F with the –SiF2 terminated surface in Eq. (11) formed a stable intermediate state (I3) of a –SiF3* anion and an NH4+ cation. Therefore, we considered a two-step reaction from R3 to I3 and then I3 to P3, as described in Eqs. (11a) and (11b),
(11a)
(11b)

The reaction energy from R3 to I3 in Eq. (11a) was −0.21 eV. The transition state between R3 and I3, TS3(1), shows the attachment of NH4F to –SiF2* to form an elongated Si–F bond (2.10 Å), as shown in Fig. 4(b), similar to TS1 and TS2(1). The activation energy was low at 0.10 eV due to the absence of bond dissociation. Therefore, the formation of I3 in Eq. (11a) would be energetically and kinetically favorable. The reaction from I3 to P3 in Eq. (11b) was endothermic, with a reaction energy of 0.57 eV. The transition state, TS3(2), was discovered between I3 and P3 with the formation of Si2O–H*, as shown in Fig. 4(b). The activation energy was 0.80 eV due to N–H dissociation, O–H formation, and Si–O elongation. As a result, the energy diagram of Fig. 4(a) suggested that the reaction would stop in I3.

The reaction in Eq. (11) would not be plausible, similar to the reaction in Eq. (10). However, we considered the fourth fluorination step by NH4F in Eq. (12) because HF generates –SiF3* terminated surface, just like we did for the third step. We assumed that the Si–O bonds of the surface were cleavaged by NH4F, forming SiF4, –SiOH*, and NH3 in P4. Figure 5 shows the energy diagram and the changes in the atomistic structures. The physisorption of NH4F on the –SiF3 terminated SiO2 surface could not be obtained because an intermediate state with a –SiF4* surface anion and an NH4+ cation was formed immediately by geometry optimization. Therefore, we considered a two-step reaction from UR4 to I4 and then I4 to P4, as described in Eqs. (12a) and (12b),
(12a)
(12b)
FIG. 5.

(a) Energy diagram, with the values of Eads, EA, and ΔE, and (b) the change in the atomistic structure for the fourth fluorination step of silicon oxide by NH4F. Energy values and interatomic distances are displayed in eV and Å, respectively. The dotted lines represent hydrogen bonding.

FIG. 5.

(a) Energy diagram, with the values of Eads, EA, and ΔE, and (b) the change in the atomistic structure for the fourth fluorination step of silicon oxide by NH4F. Energy values and interatomic distances are displayed in eV and Å, respectively. The dotted lines represent hydrogen bonding.

Close modal

The formation of the intermediate state in Eq. (12a) was exothermic, with a reaction energy of −1.35 eV. However, the formation of P4 from I4 in Eq. (12b) was endothermic, with a reaction energy of 0.69 eV. The transition state, TS4, was discovered between I4 and P4 with the formation of Si2O–H*, as shown in Fig. 5(b). The activation energy was 0.85 eV due to the N–H bond dissociation, O–H bond formation, and Si–O bond elongation, similar to the TS2(2) and TS3(2) cases. Therefore, the energy diagram of Fig. 5(a) suggested that the reaction in Eq. (12) would also stop in I4.

As we have seen so far, the second, third, and fourth fluorination reactions by NH4F would stop in intermediate states consisting of the fluorinated surface anion [–Si(OH)F2*, –SiF3*, or –SiF4*] and NH4+ cation. The presence of stable intermediate states in the NH4F reaction steps is the most significant difference from the HF reaction. NH4F would be ionized into NH4+ and F on the surface to form surface salt species consisting of a surface anion and an ammonium cation. The surface salt species is expected to inhibit further fluorination of the surface by NH4F. So we considered the fluorination of the fluorinated surface anions by HF. We assumed that HF fluorinates I2 and I3 to form I3 and I4, respectively, as shown in Eqs. (13) and (14),
(13)
(14)
In these reactions, the NH4+ cation is a spectator.

Figure 6 shows the energy diagrams and the changes in the atomistic structures during the reaction in Eq. (13). UR3' is I2 with the addition of an HF molecule at an infinite distance, and P3' is I3 with the addition of an H2O molecule as the byproduct. The apostrophe symbol indicates the fluorination of a surface anion by HF. The adsorption of HF was favorable, with an energy of −0.64 eV. The OH of –SiF2(OH)* in R3' was exchanged with F of HF to form a –SiF3* surface anion and H2O in P3', with a reaction energy of −0.59 eV. The transition state, TS3', was found between R3' and P3', as shown in Fig. 6(b). The H–F bond was dissociated, the O–H bond was formed, and the Si–O bond was elongated in TS3'. Since the activation energy was low at 0.37 eV, we concluded that HF would further fluorinate I2 to form I3, as shown in Eq. (13).

FIG. 6.

(a) Energy diagram, with the values of Eads, EA, and ΔE, and (b) the change in the atomistic structure of the reaction of I2 with an HF molecule, as shown in Eq. (13). Energy values and interatomic distances are displayed in eV and Å, respectively. The dotted lines represent hydrogen bonding.

FIG. 6.

(a) Energy diagram, with the values of Eads, EA, and ΔE, and (b) the change in the atomistic structure of the reaction of I2 with an HF molecule, as shown in Eq. (13). Energy values and interatomic distances are displayed in eV and Å, respectively. The dotted lines represent hydrogen bonding.

Close modal

Figure 7 shows the energy diagrams and the changes in the atomistic structures during the reaction in Eq. (14). UR4' is I3 with the addition of an HF molecule at an infinite distance, and P4' is I4 with the addition of –SiOH*. The adsorption of HF was favorable, with an energy of −0.62 eV. The Si–O bond beneath the –SiF3* in R4' reacted with HF to form –SiF4* and –SiOH* in P4'. The reaction was exothermic, with an energy of −0.25 eV. The transition state, TS4', was obtained between R4' and P4', as shown in Fig. 7(b). One Si–O bond was dissociated, the O–H bond was formed, the H–F bond was elongated, and the other Si–O bond was shortened in TS4'. A low activation energy of 0.61 eV indicates that the reaction in Eq. (14) would be energetically and kinetically favorable at near-room temperatures.

FIG. 7.

(a) Energy diagram, with the values of Eads, EA, and ΔE, and (b) the change in the atomistic structure for the reaction of I3 with an HF molecule, as shown in Eq. (14). Energy values and interatomic distances are displayed in eV and Å, respectively. The dotted lines represent hydrogen bonding.

FIG. 7.

(a) Energy diagram, with the values of Eads, EA, and ΔE, and (b) the change in the atomistic structure for the reaction of I3 with an HF molecule, as shown in Eq. (14). Energy values and interatomic distances are displayed in eV and Å, respectively. The dotted lines represent hydrogen bonding.

Close modal

As explained so far, the intermediate states, I2 and I3, can be further fluorinated by HF to form I4 eventually. As a result, two product states are formed by a mixture of HF and NH4F: (1) a surface with SiF4 molecules and new –OH* groups produced by HF only and (2) a surface with –SiF4* surface anions and NH4+ cations formed by a mixture of HF and NH4F. In Subsection III B, we will examine the (NH4)2SiF6 formation from these two products.

In Subsection III A, the final products of the fluorination reaction of SiO2 by a mixture of HF and NH4F were a SiF4 molecule and –OSiF4* surface anion with an NH4+ cation, as illustrated in Fig. 7. We modeled the salt formation reactions, as shown in Eqs. (15) and (16),
(15)
(16)
We assumed that the reaction in Eq. (15) occurs on the –SiF3 terminated surface in two steps, each with an NH4F molecule, as described in Eqs. (15a) and (15b),
(15a)
(15b)

Figure 8(a) shows the energy diagram for the first step in Eq. (15a). P5 was spontaneously formed from UR5 by geometry optimization, with an energy difference of −1.49 eV, and the physisorption of the first NH4F molecule could not be obtained. The F atom of NH4F was attached to the Si atom of SiF4, as shown in Fig. 8(b).

FIG. 8.

(a) Energy diagram and (b) the change in the atomistic structure for the reaction in Eq. (15a). Energy values and interatomic distances are displayed in eV and Å, respectively. The dotted line represents hydrogen bonding. The dashed line represents the interatomic distance between F atoms.

FIG. 8.

(a) Energy diagram and (b) the change in the atomistic structure for the reaction in Eq. (15a). Energy values and interatomic distances are displayed in eV and Å, respectively. The dotted line represents hydrogen bonding. The dashed line represents the interatomic distance between F atoms.

Close modal

Next, we simulated the second step of the salt formation of Eq. (15b), and the energy diagram is shown in Fig. 9(a). The second NH4F molecule in UR6 reacted with SiF5 and NH4+ to form (NH4)2SiF6 in P6. The adsorption of the second NH4F molecule was favorable in R6, with an energy of −1.24 eV. The reaction from R6 to P6 was also exothermic, with a reaction energy of −0.08 eV, due to the ionic interaction between NH4+ cations and SiF6 anion. The activation energy was low at 0.27 eV, which attributes to the interaction between H and F atoms, despite the dissociation of the weak NH4–F bond, which was already elongated in R6. Therefore, the salt formation of Eq. (15) would be expected to be favorable and fast because both steps were exothermic with low activation energies.

FIG. 9.

(a) Energy diagram, with the values of Eads, EA, and ΔE, and (b) the changes in the atomistic structures for the reaction in Eq. (15b). Energy values and interatomic distances are displayed in eV and Å, respectively. The dotted lines represent hydrogen bonding.

FIG. 9.

(a) Energy diagram, with the values of Eads, EA, and ΔE, and (b) the changes in the atomistic structures for the reaction in Eq. (15b). Energy values and interatomic distances are displayed in eV and Å, respectively. The dotted lines represent hydrogen bonding.

Close modal
Similar to the reaction in Eq. (15), we assumed that the reaction in Eq. (16) occurs in two steps, with HF and NH4F molecules. The first step of the reaction creating a SiF5* anion and an –OH* surface group can be described by Eq. (16a) or (16b), depending on the first molecule approaching the surface,
(16a)
(16b)

Figure 10 shows the energy diagrams and the changes in the atomistic structures during the reactions in Eqs. (16a) and (16b). The adsorption of HF was favorable, with an energy of −0.71 eV. However, the reaction was endothermic, with an energy of 0.12 eV, indicating that the chemisorption was unfavorable. The adsorption of NH4F was more exothermic than HF, with an energy of −1.12 eV. The reaction was endothermic, with an energy of 0.90 eV. As a result, both HF and NH4F only physisorb on the surface.

FIG. 10.

(a) Energy diagrams for the reactions in Eqs. (16a) and (16b), (b) the changes in the atomistic structures during the reaction in Eq. (16a), and (c) the changes in the atomistic structures during the reaction in Eq. (16b). Energy values and interatomic distances are displayed in eV and Å, respectively. The dotted lines represent hydrogen bonding.

FIG. 10.

(a) Energy diagrams for the reactions in Eqs. (16a) and (16b), (b) the changes in the atomistic structures during the reaction in Eq. (16a), and (c) the changes in the atomistic structures during the reaction in Eq. (16b). Energy values and interatomic distances are displayed in eV and Å, respectively. The dotted lines represent hydrogen bonding.

Close modal

Since both Eqs. (16a) and (16b) were endothermic, we modeled the (NH4)2SiF6 formation reaction from the physisorption states in Fig. 10. Resulting reaction equation is the same as Eq. (16). Figure 11 shows the energy diagram and the change in the atomistic structure. The adsorption energy of HF on the surface where NH4F was already physisorbed was −0.67 eV. The reaction of HF with the surface to form (NH4)2SiF6 was exothermic, with a reaction energy of −0.16 eV. The activation energy was low at 0.30 eV, which is similar to that of 0.27 eV for Eq. (15b). Therefore, the salt formation reactions of both Eqs. (15) and (16) would be favorable even for near-room temperature processing.

FIG. 11.

(a) Energy diagram, with the values of Eads, EA, and ΔE, and (b) the change in the atomistic structure for the reaction in Eq. (16). Energy values and interatomic distances are displayed in eV and Å, respectively. The dotted lines represent hydrogen bonding.

FIG. 11.

(a) Energy diagram, with the values of Eads, EA, and ΔE, and (b) the change in the atomistic structure for the reaction in Eq. (16). Energy values and interatomic distances are displayed in eV and Å, respectively. The dotted lines represent hydrogen bonding.

Close modal

We summarized all possible reaction routes for the (NH4)2SiF6 formation by a mixture of HF and NH4F in Fig. 12 with activation energy values. Our previous work shows that HF without NH4F forms volatile SiF4 with low activation energies, resulting in the continuous etching of SiO2. This work shows that the etching of SiO2 by NH4F is energetically unfavorable at near-room temperatures without HF. Instead, we found that NH4F contributes to surface modification by forming a salt layer, (NH4)2SiF6.

FIG. 12.

Schematic of reaction routes for the (NH4)2SiF6 formation by a mixture of HF and NH4F with activation energy values.

FIG. 12.

Schematic of reaction routes for the (NH4)2SiF6 formation by a mixture of HF and NH4F with activation energy values.

Close modal

Next, we investigated the mechanism by which the silicon oxide film is selectively removed over silicon by a mixture of HF and NH4F. We summarized the reaction routes for the fluorination of Si by HF or NH4F in Fig. 13 with activation energy values. In the previous work, we studied the fluorinations of silicon by HF molecules in four consecutive steps to form the SiF4 byproduct.34 The etching of silicon by HF is kinetically unfavorable, with relatively high activation energies of about 1.22–1.56 eV, indicating that continuous etching of silicon is impossible at near-room temperatures. However, since NH4F is also present in the mixture, we investigated whether NH4F could etch silicon at near-room temperature in the present work.

FIG. 13.

Schematic of reaction routes for the fluorination of Si by a mixture of HF and NH4F with activation energy values. The activation energy values for the fluorination by HF were taken from previous work (Ref. 34).

FIG. 13.

Schematic of reaction routes for the fluorination of Si by a mixture of HF and NH4F with activation energy values. The activation energy values for the fluorination by HF were taken from previous work (Ref. 34).

Close modal
We modeled the fluorinations of Si by NH4F in four consecutive steps to form the SiF4 byproduct, similar to studying the reaction by HF in the previous work.34 We assumed the first, second, third, and fourth fluorination reactions by NH4F, as shown in Eqs. (17)–(20),
(17)
(18)
(19)
(20)

In the first two steps, Si–H, H–F, and N–H bonds are dissociated while Si–F and H–H bonds are formed. Then, in the last two steps, Si–Si, H–F, and N–H bonds are cleavaged, whereas Si–F and Si–H bonds are generated. The –SiH* surface groups are replaced by –SiF* by Eqs. (17) and (18), and then regenerated by Eqs. (19) and (20). The reactions were simulated using the –SiH2, –SiHF, –SiF2, and –SiF3 terminated Si surfaces.

Figure 14 shows the energy diagram and the change in the atomistic structure for the first step in Eq. (17). In the beginning, NH4F is physisorbed on the –SiH2 terminated Si surface in R1, with an energy of −0.42 eV. It was less favorable than the physisorption of NH4F on SiO2 in Eq. (9) due to the absence of a hydrogen bond. Then, an F atom of NH4F was replaced with an H atom on the surface, forming a –SiHF* surface group, an H2 molecule, and an NH3 molecule in P1. Unlike the first fluorination by NH4F on the SiO2 surface or by HF on the Si surface, the reaction was endothermic, with an energy of +0.15 eV. The endothermicity of the reaction can be described by the dissociation of Si–H (3.23 eV34), H–F (6.76 eV), and N–H (0.71 eV) bonds in R1 despite the formation of Si–F (5.97 eV34) and H–H (4.25 eV34) bonds in P1. Unlike HF showing an exothermic reaction with the Si surface, NH4F requires the dissociation of the N–H bond. The desorption of the byproducts, H2 and NH3, was endothermic with an energy of 0.18 eV in UP1.

FIG. 14.

(a) Energy diagram, with the values of Eads, EA, and ΔE, and (b) the change of atomistic structure for the first fluorination step of Si by NH4F. Energy values and interatomic distances are displayed in eV and Å, respectively. The dotted lines represent hydrogen bonding.

FIG. 14.

(a) Energy diagram, with the values of Eads, EA, and ΔE, and (b) the change of atomistic structure for the first fluorination step of Si by NH4F. Energy values and interatomic distances are displayed in eV and Å, respectively. The dotted lines represent hydrogen bonding.

Close modal

In TS1, HF, dissociated from NH4F, attached to –SiH* to form a four-membered ring of –Si–H–H–F–, as shown in Fig. 14(b), which is similar to the previous work with HF.34 The elongated Si–F and H–H bonds were formed with a length of 2.02 and 0.96 Å. The Si–H bond of –SiH* and the H–F bond in HF were elongated from 1.49 and 1.00 Å in R1 to 1.69 and 1.25 Å in TS1, respectively. The activation energy was very high at 1.94 eV, which is even higher than the HF case, due to the dissociation of N–H and the elongation of two bonds despite the formation of elongated Si–F and H–H bonds. Therefore, the first step with NH4F would be energetically and kinetically unfavorable.

Figures S5–S7 in the supplementary material41 show the energy diagrams and the changes in the atomistic structures of the second, third, and fourth steps in Eqs. (18)–(20). Unlike the first step, the second to the fourth steps were exothermic, with a reaction energy of −0.51, −0.76, and −2.01 eV. The transition state geometries for the second to the fourth steps, TS2, TS3, and TS4, were very similar to those by HF in previous work.34 The only difference from the HF cases was the dissociation of NH4F into HF and NH3 at the surface. As a result, the activation energies of the four steps by NH4F (1.94–2.46 eV) were higher than HF cases (1.22–1.56 eV) due to the dissociation of N–H (0.71 eV) of NH4F. Therefore, the fluorination of Si by NH4F would be kinetically unfavorable at near-room temperatures.

In the mixture HF and NH4F, the etch selectivity of SiO2 against Si originated from the low activation energy values for the fluorinations of silicon oxide and high values for silicon. For the reaction with SiO2, HF plays a dominant role in fluorination. The fluorination of silicon oxide by HF showed lower activation energy values of 0.72–0.79 eV.34 It is because all transition states showed the formation of stable four-membered ring structures of –Si–O–H–F– without bond dissociations. On the other hand, the fluorination of silicon showed relatively higher activation energy values than the silicon oxide case, 1.22–1.56 eV by HF (Ref. 34) and 1.94–2.46 eV by NH4F. The relatively high activation energy for Si can be explained by less stable transition state structures. In addition, the stronger Si–F bond on SiO2 than on Si in the transition states also contributed to the lower activation energies for the SiO2 substrate. We discussed the origin of selectivity in the previous work.34 

The next-generation cleaning process requires self-limited surface modification and the removal of the modified layer. In this work, we modeled and simulated the selective cleaning process of SiO2 over Si by DFT. The same strategy can be applied to designing the selective self-limited cleaning process of different materials. Generally, the fluorinations of dielectric materials, such as silicon oxide, silicon nitride, and metal oxides, are exothermic due to the formation of strong bonds between F and Si or metal atoms. Hence, reaction energy alone cannot expect if the material can be etched by fluorine-containing molecules. However, the activation energy can expect if the etching is possible at a specific process temperature. Therefore, the DFT study can provide the information to design the next-generation etching or cleaning process of different materials.

We studied the selective etching mechanism of silicon oxide using a mixture of HF and NH4F gases by DFT calculation using surface slab models. The fluorination reactions of silicon oxide by the mixture produced a volatile SiF4 molecule or a surface anion of –OSiF4* with an NH4+ cation with low activation energies. Unlike HF, NH4F produced surface salt species consisting of a surface anion and an ammonium cation. From the two reaction products, (NH4)2SiF6 can be formed exothermally with low activation energies (0.27 or 0.30 eV). The fluorination reactions of silicon by the mixture were also exothermic, except for the first fluorination step by NH4F. However, the activation energies were significantly higher than the silicon oxide cases, 1.22–1.56 eV by HF and 1.94–2.46 eV by NH4F due to the less stable transition state geometries. Therefore, the selective salt formation on silicon oxide, not on silicon, is expected in near-room temperature processing, which enables selective etching of silicon oxide.

This work was supported by the Ministry of Trade, Industry & Energy (MOTIE) of the Republic of Korea (Project No. 20012588) and the Korea Semiconductor Research Consortium (KSRC) support program for the development of the future semiconductor device. This research was partly supported by the Korea Basic Science Institute (National Research Facilities and Equipment Center) grant funded by the Ministry of Education (No. 2022R1A6C101A774).

The authors have no conflicts to disclose.

Romel Hidayat: Conceptualization (lead); Data curation (lead); Formal analysis (lead); Investigation (lead); Methodology (lead); Validation (lead); Visualization (lead); Writing – original draft (lead); Writing – review & editing (supporting). Khabib Khumaini: Formal analysis (equal); Investigation (equal); Methodology (equal); Validation (equal); Writing – review & editing (equal). Hye-Lee Kim: Conceptualization (equal); Formal analysis (equal); Investigation (equal); Methodology (equal); Validation (equal); Visualization (equal); Writing – review & editing (equal). Tanzia Chowdhury: Formal analysis (equal); Investigation (equal); Methodology (equal); Validation (equal); Writing – review & editing (equal). Tirta Rona Mayangsari: Investigation (equal); Methodology (equal); Validation (equal); Writing – review & editing (equal). Byungchul Cho: Conceptualization (equal); Methodology (equal); Validation (equal). Sangjoon Park: Conceptualization (equal); Methodology (equal); Validation (equal). Jongwan Jung: Conceptualization (equal); Methodology (equal); Validation (equal). Won-Jun Lee: Conceptualization (equal); Formal analysis (equal); Funding acquisition (lead); Methodology (equal); Project administration (lead); Resources (lead); Supervision (lead); Writing – review & editing (lead).

The data that support the findings of this study are available within the article and its supplementary material (Ref. 41).

1.
J.
Tang
,
N.
Ingle
, and
D.
Yang
, US8501629B2 (6 August 2013).
2.
S.
Ji
,
Q.-H.
Han
, and
H.-Y.
Zhang
,
ECS Trans.
75
,
15
(
2017
).
3.
D. A.
Ferrer
,
A.
Levesque
,
A.
Sirman
,
J.
Lee
,
A.
Subramaniyan
,
L.
Lanzerotti
,
D. F.
Hilscher
, and
E.
Alptekin
, in
2016 27th Annual SEMI Advanced Semiconductor Manufacturing Conference
, Saratoga Springs, NY, 16–19 May 2016 (
IEEE
,
New York
,
2016
), pp.
361
363
.
4.
M.
Labrot
,
F.
Cheynis
,
D.
Barge
,
P.
Maury
,
M.
Juhel
,
S.
Lagrasta
, and
P.
Müller
,
Microelectron. Eng.
180
,
56
(
2017
).
5.
A.
Redolfi
et al,
Solid-State Electron.
71
,
106
(
2012
).
7.
P. E.
Raynal
,
V.
Loup
,
L.
Vallier
,
M.
Martin
,
J.
Moeyaert
,
B.
Pelissier
,
P.
Rodriguez
,
J. M.
Hartmann
, and
P.
Besson
,
Microelectron. Eng.
187–188
,
84
(
2018
).
8.
M.
Grégoire
,
B.
Horvat
,
B. N.
Bozon
,
D.
Combe
,
K.
Dabertrand
, and
D.
Roy
,
Micro Nano Eng.
2
,
104
(
2019
).
9.
J.
Lei
et al, in
2006 IEEE International Symposium on Semiconductor Manufacturing
, Tokyo, Japan, 25–27 September 2006 (
IEEE
,
New York
,
2006
), pp.
393
396
.
10.
R.
Yang
,
N.
Su
,
P.
Bonfanti
,
J.
Nie
,
J.
Ning
, and
T. T.
Li
,
J. Vac. Sci. Technol. B
28
,
56
(
2010
).
11.
Y.
Bao
et al, in
2015 China Semiconductor Technology International Conference
, Shanghai, China, 15–16 March 2015 (
IEEE
,
New York
,
2015
), pp.
1
3
.
12.
F.-H.
Hsu
et al, in
25th Annual SEMI Advanced Semiconductor Manufacturing Conference (ASMC 2014)
, Saratoga Springs, NY, 19–21 May 2014 (
IEEE
,
New York
,
2014
), pp.
242
244
.
13.
J.
Kikuchi
,
M.
Iga
,
H.
Ogawa
,
S.
Fujimura
, and
H. Y.
Hiroshi Yano
,
Jpn. J. Appl. Phys.
33
,
2207
(
1994
).
14.
A.
Tavernier
,
L.
Favennec
,
T.
Chevolleau
, and
V.
Jousseaume
,
ECS Trans.
45
,
225
(
2012
).
15.
J.
Zhao
,
H. J.
Gao
,
Y. Z.
Zeng
,
K.
Awut
,
W. J.
Song
,
S. F.
Yu
,
G.
Cai
, and
B.
Zhang
,
ECS Trans.
60
,
721
(
2014
).
16.
K.-F.
Lo
,
F.-H.
Hsu
,
X.-G.
Lin
,
H.-J.
Lee
,
N.-T.
Lian
,
T.
Yang
, and
K.-C.
Chen
, in
2015 26th Annual SEMI Advanced Semiconductor Manufacturing Conference
, Saratoga Springs, NY, 3–6 May 2015 (
IEEE
,
New York
,
2015
), pp.
309
312
.
17.
M.
Mastari
et al,
Nanotechnology
29
,
275702
(
2018
).
18.
M.
Labrot
,
F.
Cheynis
,
D.
Barge
,
P.
Müller
, and
M.
Juhel
,
Appl. Surf. Sci.
371
,
436
(
2016
).
19.
S.
Matsuo
,
J. Vac. Sci. Technol.
17
,
587
(
1980
).
20.
U.
Niggerbrügge
and
P.
Balk
,
Solid-State Electron.
25
,
859
(
1982
).
21.
22.
C.
Han
,
Y.
Yang
,
W.
Liu
,
Y.
Lu
, and
J.
Cheng
,
SPIN
08
,
1850002
(
2018
).
23.
H.
Habuka
,
T.
Otsuka
, and
M.
Katayama
,
J. Cryst. Growth
186
,
104
(
1998
).
24.
N.
Miki
,
H.
Kikuyama
,
I.
Kawanabe
,
M.
Miyashita
, and
T.
Ohmi
,
IEEE Trans. Electron Devices
37
,
107
(
1990
).
25.
H.
Nishino
,
N.
Hayasaka
, and
H.
Okano
,
J. Appl. Phys.
74
,
1345
(
1993
).
26.
H. J.
Oh
,
J. H.
Lee
,
M. S.
Lee
,
W. G.
Shin
,
S. Y.
Kang
,
G. D.
Kim
, and
D. H.
Ko
,
ECS Trans.
61
,
1
(
2014
).
27.
H.-T.
Kim
,
J.-S.
Lim
,
M.-S.
Kim
,
H.-J.
Oh
,
D.-H.
Ko
,
G.-D.
Kim
,
W.-G.
Shin
, and
J.-G.
Park
,
Microelectron. Eng.
135
,
17
(
2015
).
28.
N.
Posseme
,
V.
Ah-Leung
,
O.
Pollet
,
C.
Arvet
, and
M.
Garcia-Barros
,
J. Vac. Sci. Technol. A
34
,
061301
(
2016
).
29.
J. W.
Park
,
M. G.
Chae
,
D. S.
Kim
,
W. O.
Lee
,
H. D.
Song
,
C.
Choi
, and
G. Y.
Yeom
,
J. Phys. D: Appl. Phys.
51
,
445201
(
2018
).
30.
Y.
Hagimoto
,
H.
Ugajin
,
D.
Miyakoshi
,
H.
Iwamoto
,
Y.
Muraki
, and
T.
Orii
,
Solid State Phenom.
134
,
7
(
2007
).
31.
S.
Saito
,
Y.
Hagimoto
,
H.
Iwamoto
, and
Y.
Muraki
,
Solid State Phenom.
145–146
,
227
(
2009
).
32.
H.
Ogawa
,
T.
Arai
,
M.
Yanagisawa
,
T.
Ichiki
, and
Y.
Horiike
,
Jpn. J. Appl. Phys.
41
,
5349
(
2002
).
33.
T.
Hoshino
and
Y.
Nishioka
,
J. Chem. Phys.
111
,
2109
(
1999
).
34.
R.
Hidayat
,
H.-L.
Kim
,
K.
Khumaini
,
T.
Chowdhury
,
T. R.
Mayangsari
,
B.
Cho
,
S.
Park
, and
W.-J.
Lee
,
Phys. Chem. Chem. Phys.
25
,
3890
(
2023
).
35.
B.
Delley
,
J. Chem. Phys.
113
,
7756
(
2000
).
36.
37.
J. P.
Perdew
,
K.
Burke
, and
M.
Ernzerhof
,
Phys. Rev. Lett.
77
,
3865
(
1996
).
38.
39.
B.
Delley
,
J. Chem. Phys.
92
,
508
(
1990
).
40.
M.
Khosravi
,
V.
Murthy
, and
I. D. R.
Mackinnon
,
Comput. Mater. Sci.
171
,
109225
(
2020
).
41.
See supplementary material at https://www.scitation.org/doi/suppl/10.1116/6.0002433 for basis set selection, bond dissociation energy (BDE) in NH4F molecule, free Gibbs energy of desorption of H2O or NH3, and the second to the fourth fluorination step of Si by NH4F.
42.
T.
Chowdhury
,
R.
Hidayat
,
T. R.
Mayangsari
,
J.
Gu
,
H.-L.
Kim
,
J.
Jung
, and
W.-J.
Lee
,
J. Vac. Sci. Technol. A
37
,
021001
(
2019
).
43.
T.
Chowdhury
,
R.
Hidayat
,
T. R.
Mayangsari
,
J.
Gu
,
H.-L.
Kim
,
J.
Jung
, and
W.-J.
Lee
,
J. Vac. Sci. Technol. A
40
,
047001
(
2022
).
44.
N.
Govind
,
M.
Petersen
,
G.
Fitzgerald
,
D.
King-Smith
, and
J.
Andzelm
,
Comput. Mater. Sci.
28
,
250
(
2003
).
45.
K.
Khumaini
,
R.
Hidayat
,
T. R.
Mayangsari
,
T.
Chowdhury
,
H.-L.
Kim
,
S.-I.
Lee
, and
W.-J.
Lee
,
Appl. Surf. Sci.
585
,
152750
(
2022
).
46.
R.
McIntosh
,
T.-S.
Kuan
, and
E.
Defresart
,
J. Electron. Mater.
21
,
57
(
1992
).
47.
M.
Wong
,
M. M.
Moslehi
, and
D. W.
Reed
,
J. Electrochem. Soc.
138
,
1799
(
1991
).
48.
A. K.
Chandra
and
T.
Uchimaru
,
J. Phys. Chem. A
104
,
9244
(
2000
).
49.
S. J.
Blanksby
and
G. B.
Ellison
,
Acc. Chem. Res.
36
,
255
(
2003
).
50.
S.
Kim
et al,
J. Mater. Chem. C
10
,
6696
(
2022
).

Supplementary Material