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Rhombohedral BN: Structure & Optical Response

Updated 12 July 2026
  • Rhombohedral BN is a layered sp²-bonded boron nitride polytype with ABC stacking that exhibits distinct electronic and optical properties.
  • Stacking order and interlayer spacing in rBN critically affect vibrational modes, second-harmonic generation, and defect photophysics.
  • Advanced growth techniques like MOVPE and iron-flux methods enable controlled synthesis of rBN for photonics and quantum applications.

Rhombohedral boron nitride (rBN) is a layered sp2sp^2-bonded boron nitride polytype built from two-dimensional hexagonal sheets of alternating B and N atoms with an ABCABC stacking sequence. In this form, strong in-plane σ\sigma-bonding coexists with weaker interlayer π\pi-type interactions, so stacking order, interlayer separation, and stacking disorder directly affect the unoccupied electronic states, vibrational response, nonlinear optics, and defect photophysics. Across recent work, rBN is treated both as a distinct layered BN polytype that must be discriminated from hhBN, Bernal BN, twinned rBN, and turbostratic BN, and as a host material whose broken inversion symmetry or reduced local symmetry modifies quantum-defect selection rules and radiative properties (Olovsson et al., 2022, Gale et al., 21 Feb 2025).

1. Structure, stacking, and nomenclature

Layered rBN consists of hexagonal B–N sheets stacked in an ABCABC\ldots sequence, in contrast to the ABAB\ldots or AAAA^\prime descriptions used for hhBN in different registry conventions. The in-plane bonding is strong and σ\sigma-type, whereas interlayer coupling is weaker and mediated by ABCABC0-type interactions. X-ray diffraction in one XANES study identified a dominant rBN phase with the ABCABC1 reflection corresponding to ABCABC2 Å, implying ABCABC3 Å; in the same work, a twin-rBN model used ABCABC4 Å and ABCABC5 Å, yielding ABCABC6 Å per layer. Independent work on UV photoluminescence in MOVPE-grown material likewise reported that the interlayer spacing in ABCABC7 BN is essentially identical across stackings at ABCABC8 nm, while a recent iron-flux study refined rBN lattice parameters in the hexagonal setting to ABCABC9 Å and σ\sigma0 Å (Olovsson et al., 2022, Iwański et al., 2024, Desrat et al., 21 Sep 2025).

Several closely related layered polytypes recur in the literature. Twinned rBN is obtained by doubling the rBN unit cell along the σ\sigma1-axis and rotating the repeated cell by σ\sigma2, producing an σ\sigma3 stacking with three inequivalent B sites. Turbostratic BN (tBN) is partially disordered layered BN with planes stacked roughly parallel to the normal but with random in-plane translations and, in reality, rotations; in the cited XANES work it was modeled with fixed random translations and an average interlayer spacing σ\sigma4 Å, spanning σ\sigma5–σ\sigma6 Å. Bernal BN (bBN) and σ\sigma7BN also appear as comparison phases in optical and growth studies (Olovsson et al., 2022, Shi et al., 2024, Iwański et al., 2024).

The symmetry assignment of layered rBN is not presented uniformly across papers. One DFPT study reported σ\sigma8-stacked r-BN in space group σ\sigma9 (No. 166) and point group π\pi0, whereas recent spectroscopy and iron-flux work described rBN as non-centrosymmetric with space group π\pi1 and point group π\pi2. Defect studies also emphasized that the local crystal field experienced by π\pi3 in rBN is reduced to π\pi4, in contrast to π\pi5 in π\pi6BN (Mishra et al., 22 May 2025, Desrat et al., 21 Sep 2025, Estaji et al., 22 Mar 2026).

A separate nomenclature issue concerns dense rhombohedral BN phases. Two crystal-chemistry papers used “rh-BN,” “rh-Bπ\pi7Nπ\pi8,” “hexagonal Bπ\pi9Nhh0,” or “hexagonal h-Bhh1Nhh2” for predicted three-dimensional hh3 tetrahedral networks derived from 3R graphite-like precursors. Those phases are structurally and physically distinct from the layered hh4 polytype usually denoted rBN in spectroscopy, growth, and quantum-defect studies (Matar et al., 2021, Matar et al., 2021).

2. Stability, phase competition, and synthesis

High-level total-energy work places layered rBN among the low-energy BN polymorphs that are very close in energy. In the RPA-based treatment of bulk BN polymorphism, r-BN was identified explicitly as hh5-BN(hh6); at hh7 K, hh8-BN is the ground state and lies about hh9–ABCABC\ldots0 kJ/mol lower in energy than each of the layered polymorphs ABCABC\ldots1-BN(ABCABC\ldots2), ABCABC\ldots3-BN, ABCABC\ldots4-BN(ABCABC\ldots5), and ABCABC\ldots6-BN(ABCABC\ldots7) (r-BN). At finite temperature, ABCABC\ldots8-BN(ABCABC\ldots9) becomes thermodynamically most stable over ABAB\ldots0-BN at ABAB\ldots1 K, while ABAB\ldots2-BN, ABAB\ldots3-BN(ABAB\ldots4), and ABAB\ldots5-BN(ABAB\ldots6) “follow closely” and all fall within about ABAB\ldots7 kJ/mol of ABAB\ldots8-BN(ABAB\ldots9) for AAAA^\prime0 K. This indicates that rBN is thermodynamically competitive near ambient temperature, but not uniquely isolated by a wide stability window (Cazorla et al., 2018).

Recent growth studies show that rBN can be realized by several routes. MOVPE on 70 nm AlN templates on 2-inch sapphire produced samples with tunable AAAA^\prime1BN:rBN ratios; longer ramp times to the AAAA^\prime2C FME stage correlated with higher rBN fractions, and TEM classified one sample as rBN-dominant, one as mixed, and one as AAAA^\prime3BN-rich. Chemical vapor deposition on single-crystal Fe–Ni(111) thin films yielded large-area multilayer BN single crystals with unidirectional AB and AAAA^\prime4 stackings; AAAA^\prime5 stacking was effectively excluded by the “first-meet-first-connect” mosaic stitching mechanism of pyramid-shaped domains. At AAAA^\prime6 Fe, unidirectional alignment reached AAAA^\prime7, continuous single-crystal multilayers were AAAA^\prime8 nm thick, residue non-connecting islands were AAAA^\prime9 nm thick, and intact transfer was demonstrated on hh0-inch SiOhh1/Si (Iwański et al., 2024, Shi et al., 2024).

An iron-flux method at atmospheric pressure produced predominantly rhombohedral bulk crystallites. In that study, boron powder and iron powder were mixed at a ratio of hh2 wt% boron in iron, melted, saturated with nitrogen for 24 hours, and slowly cooled from hh3C or hh4C. The resulting BN shell comprised many triangular bulk crystallites, with the largest up to hh5m laterally and hh6 mm along the growth axis, and powder XRD indicated hh7 rBN by weight, with no evidence of turbostratic BN (Desrat et al., 21 Sep 2025).

3. Electronic structure and core-level spectroscopy

All hh8 BN polytypes discussed in the cited work are wide band gap semiconductors or insulators, but the numerical gap depends strongly on methodology. In the XANES-plus-core-hole DFT study, PBE-GGA underestimated absolute gaps relative to experiment, but relative trends across polytypes were retained: tBN models gave hh9–σ\sigma0 eV with an average near σ\sigma1 eV, the twin-rBN model yielded σ\sigma2 eV, and rBN lay in the same wide-gap region, typically slightly larger than tBN and comparable to σ\sigma3BN within that methodology. A separate PBE+vdW study reported an indirect σ\sigma4–σ\sigma5 gap of σ\sigma6 eV for r-BN, while many-body calculations for defect-hosted rBN used a host gap of σ\sigma7 eV at the σ\sigma8-point. Another experimental/comparative study summarized rBN as possessing a wide bandgap of approximately σ\sigma9 eV (Olovsson et al., 2022, Mishra et al., 22 May 2025, Estaji et al., 22 Mar 2026, Gale et al., 21 Feb 2025).

The core-level spectroscopy of rBN is especially sensitive to stacking. At the ABCABC00-edge, XANES probes ABCABC01-like conduction states under the dipole selection rule ABCABC02, with absorption coefficient

ABCABC03

Experimentally, the B ABCABC04-edge exhibited a sharp ABCABC05 resonance split by ABCABC06 eV into peaks at ABCABC07 eV and ABCABC08 eV, and a broader ABCABC09 “camel-back” doublet at ABCABC10–ABCABC11 eV with ABCABC12 eV splitting. At the N ABCABC13-edge, the ABCABC14 edge peak occurred at ABCABC15 eV and the ABCABC16 peak near ABCABC17 eV, with a shoulder at ABCABC18 eV (Olovsson et al., 2022).

Calculated chemical shifts provide polytype fingerprints. Using rBN as the reference at the higher-energy ABCABC19 position, the B ABCABC20-edge chemical shifts were ABCABC21 eV for ABCABC22BN, ABCABC23 eV for twin-rBN, and ABCABC24 eV for tBN; monolayer BN lay ABCABC25 eV above rBN. Increasing interlayer spacing shifted the B ABCABC26 peak to higher energy, decreasing spacing shifted it lower, and ten tBN model structures showed an absolute B ABCABC27 dispersion of ABCABC28–ABCABC29 eV. The unusually large ABCABC30 eV experimental splitting at the B ABCABC31-edge was therefore interpreted as a superposition of ordered rBN and turbostratic contributions, consistent with XRD evidence for a dominant rBN phase plus a tBN shoulder. This directly links stacking disorder and interlayer ABCABC32-coupling to band-edge shifts (Olovsson et al., 2022).

The computational framework behind those spectra used all-electron DFT within the full-potential APW+lo scheme in WIEN2k with PBE-GGA and a core-hole final-state approximation. Supercells were ABCABC33 in plane; rBN used 3 layers (54 atoms), ABCABC34BN 4 layers (72 atoms), twin-rBN 6 layers (108 atoms), and tBN 7 layers (126 atoms). Lorentzian broadening employed FWHM ABCABC35 eV at the B ABCABC36-edge and ABCABC37 eV at the N ABCABC38-edge, and enlarging the supercell from ABCABC39 to ABCABC40 changed relative ABCABC41 shifts by only ABCABC42 eV (Olovsson et al., 2022).

4. Vibrational, nonlinear, and ultraviolet optical response

A central theme in recent work is that rBN exhibits stacking-dependent optical activity not present in bulk ABCABC43BN. Because ABCABC44 stacking breaks inversion symmetry in several of the cited studies, bulk rBN supports a nonzero ABCABC45, strong second-harmonic generation, and parametric down-conversion, whereas bulk ABCABC46BN with ABCABC47 stacking suppresses second-order processes. In nonlinear-optical notation, the intensity scaling is written ABCABC48, and phase mismatch in bulk phase-matching contexts is ABCABC49. Experimentally, reflected SHG was recorded from exfoliated rBN under ABCABC50 eV (ABCABC51 nm) excitation, and the cited work noted recent reports of stacking-controlled rBN films with SHG conversion efficiencies up to ABCABC52 (Gale et al., 21 Feb 2025).

First-principles vibrational studies likewise identify stacking-specific fingerprints. In one DFPT study, ABCABC53-stacked r-BN with vdW corrections had ABCABC54 Å and ABCABC55 Å, a cohesive energy of ABCABC56 eV per atom, and an indirect ABCABC57–ABCABC58 gap of ABCABC59 eV. The ABCABC60-point optical modes included low-frequency shear modes at ABCABC61 and ABCABC62 cmABCABC63, breathing modes at ABCABC64 cmABCABC65, an ABCABC66 mode at ABCABC67 cmABCABC68, and a very strong co-active ABCABC69 mode at ABCABC70 cmABCABC71 with IR intensity ABCABC72 and Raman intensity ABCABC73. The same study emphasized that many r-BN modes are labeled both IR- and Raman-active, unlike the largely mutually exclusive selection rules of ABCABC74BN (Mishra et al., 22 May 2025).

An experimental iron-flux study proposed a more restrictive primitive-cell picture for rBN: a rhombohedral primitive cell with two atoms, point group ABCABC75, and only six phonon modes in total. In that description, rBN is characterized spectroscopically by the absence of any low-energy Raman mode near ABCABC76 cmABCABC77, the presence of an extended Raman band from ABCABC78 cmABCABC79 to ABCABC80 cmABCABC81, and an in-plane ABCABC82 mode near ABCABC83 cmABCABC84 with FWHM ABCABC85 cmABCABC86. The same work argued that treating ABCABC87 stacking in a non-primitive hexagonal cell can obscure the absence of the shear mode at ABCABC88 by band folding (Desrat et al., 21 Sep 2025).

Ultraviolet defect spectroscopy provides another sensitive discriminator. For the ABCABC89 eV carbon-dimer defect ABCABC90 (CBCN), cryogenic PL and CL established a ZPL at ABCABC91 eV (ABCABC92 nm) for rBN and ABCABC93 eV (ABCABC94 nm) for ABCABC95BN, a shift of ABCABC96 meV. The rBN ZPL was asymmetric and broadened on its low-energy side by coupling to acoustic and low-energy out-of-plane phonons; the hBN ZPL was symmetric with FWHM ABCABC97 meV, whereas the high-energy side of the rBN ZPL fit a Gaussian with FWHM ABCABC98 meV. The Huang–Rhys factor increased from ABCABC99 in σ\sigma00BN to σ\sigma01 in rBN, and low-energy out-of-plane modes near σ\sigma02 meV contributed to the rBN lineshape. Time-resolved PL yielded σ\sigma03 ns for σ\sigma04BN and σ\sigma05–σ\sigma06 ns for rBN-dominated samples (Iwański et al., 2024).

Near the band edge, low-temperature PL of high-quality iron-flux crystals showed that rBN retained the four principal phonon-assisted transitions known from σ\sigma07BN, but all were red-shifted. A linear fit of rBN peak energies against σ\sigma08BN peak energies gave an offset of σ\sigma09 meV, and fitting to the rhombohedral dispersion was consistent with an indirect gap of σ\sigma10 eV for rBN compared with σ\sigma11 eV for σ\sigma12BN. A weak ZA-assisted transition at σ\sigma13 eV was observed in rBN and interpreted as symmetry-allowed in non-centrosymmetric rBN (Desrat et al., 21 Sep 2025).

5. Quantum defects, single-photon emission, and spin physics

rBN has become a distinct quantum-defect host because stacking modifies both optical selection rules and spin relaxation pathways. For the negatively charged boron vacancy σ\sigma14, σ\sigma15BN was described as providing σ\sigma16 symmetry with mirror-parity labels, so the lowest triplet transitions are parity-forbidden and emission is vibronically activated. In rBN, the local crystal field is reduced to σ\sigma17; the mirror parity is removed, and a direct zero-phonon optical transition from the σ\sigma18 ground state to the first σ\sigma19 triplet excited state becomes allowed. Many-body GW+BSE calculations placed the first excitonic peak at σ\sigma20 eV and the room-temperature PL center at σ\sigma21 eV (σ\sigma22 nm). Jahn–Teller σ\sigma23 coupling lowered the excited-state energy by σ\sigma24 eV with JT barriers of σ\sigma25 meV, and the total Huang–Rhys factor was σ\sigma26, implying σ\sigma27 (Estaji et al., 22 Mar 2026).

The radiative-rate estimate for the rBN σ\sigma28 ZPL used

σ\sigma29

with σ\sigma30 and σ\sigma31 D, yielding σ\sigma32s for the σ\sigma33 emission in rBN. In σ\sigma34BN, the corresponding parity-forbidden transition has σ\sigma35s and quantum efficiency σ\sigma36. The predicted brightness enhancement in rBN was at least one order of magnitude, and the many-body analysis indicated up to two orders of magnitude increase in σ\sigma37 (Estaji et al., 22 Mar 2026).

The spin Hamiltonian for σ\sigma38 was written as

σ\sigma39

For rBN, theory gave σ\sigma40 GHz, consistent with experiment near σ\sigma41 GHz in irradiated rBN; the σ\sigma42-tensor was approximately isotropic with σ\sigma43, and three equivalent nearest-neighbor σ\sigma44N nuclei produced a resolved seven-line hyperfine pattern with σ\sigma45 MHz per σ\sigma46N. A separate spin-phonon study found that σ\sigma47 in rBN has a longer room-temperature σ\sigma48 than in σ\sigma49-stacked σ\sigma50BN despite the opening of single-quantum relaxation channels by symmetry reduction. The key out-of-plane mode in rBN appeared at σ\sigma51 meV, slightly above the σ\sigma52 meV mode in σ\sigma53BN, and the spin-phonon coupling amplitude in rBN was about four times weaker than in σ\sigma54BN. Across monolayer BN, σ\sigma55BN, and rBN, the high-temperature regime showed the universal σ\sigma56 scaling characteristic of two-phonon Raman relaxation (Estaji et al., 31 Mar 2025, Estaji et al., 22 Mar 2026).

Deterministic single-photon emitters have also been demonstrated in rBN. Electron irradiation activated blue B-center emitters whose room-temperature ZPL occurred at σ\sigma57 eV in rBN versus σ\sigma58 eV in σ\sigma59BN; at σ\sigma60 K, the rBN B-center ZPL was blue-shifted by σ\sigma61 meV relative to σ\sigma62BN. Autocorrelation measurements gave σ\sigma63 for rBN and σ\sigma64 for σ\sigma65BN. Vibronic replicas at σ\sigma66 meV and σ\sigma67 meV were attributed to TO and LO phonons, a replica near σ\sigma68 meV appeared in both polytypes, and rBN exhibited an additional broad shoulder around σ\sigma69 meV attributed to out-of-plane vibrational modes. Comparative DFT-based vibronic simulations favored an in-plane trans-Cσ\sigma70 defect as the most likely microscopic origin of the B-center in both σ\sigma71BN and rBN (Gale et al., 21 Feb 2025).

The combination of bulk nonlinear optics, quantum emitters, and spin defects gives rBN a distinct position among van der Waals materials. One recent study explicitly placed rBN alongside SiC as a platform that simultaneously offers intrinsic second-order nonlinearity and quantum defects for integrated photonics, and another argued that the direct σ\sigma72 ZPL transition in rBN, together with σ\sigma73s, σ\sigma74 GHz, and σ\sigma75s, makes room-temperature single-defect ODMR feasible without relying on ensembles or cavities. Suggested application directions include magnetometry, thermometry, strain sensing, frequency conversion, and entangled-photon generation in hybrid van der Waals photonic structures (Gale et al., 21 Feb 2025, Estaji et al., 22 Mar 2026).

Several identification problems remain active. Conventional σ\sigma76 XRD reflections are poor polytype discriminants because interlayer spacings are nearly identical across layered BN stackings, and high-frequency Raman modes are only weakly sensitive to stacking in many geometries. This has motivated the use of B σ\sigma77-edge XANES, SHG, and defect-related UV photoluminescence as stacking-sensitive probes. Even then, overlap with turbostratic disorder or stacking-fault-related bands can complicate interpretation: the XANES study explained a large σ\sigma78 splitting through rBN+tBN superposition, and the UV PL study noted that σ\sigma79 emission in the σ\sigma80–σ\sigma81 eV range overlaps with stacking-fault-related bands, so rBN was established structurally rather than by a uniquely isolated PL line in that energy window (Olovsson et al., 2022, Iwański et al., 2024, Shi et al., 2024).

Methodological limitations are also explicit in the cited work. PBE-GGA underestimates absolute band gaps; GW/BSE corrections are needed for quantitative agreement, especially for excitonic features. Vibrational effects are required to reproduce the σ\sigma82 camel-back splitting in XANES, tBN models with random translations omitted random rotations, and defect studies did not yet provide full charge stability, formation energies, or quantitative intersystem-crossing rates for σ\sigma83 in rBN. In spin-relaxation theory, low-temperature rates remain more uncertain because finite supercells can miss very low-energy phonons and non-phononic channels may dominate (Olovsson et al., 2022, Estaji et al., 31 Mar 2025, Estaji et al., 22 Mar 2026).

Finally, the term “rhombohedral boron nitride” itself requires care. In most recent spectroscopy, growth, and defect papers it denotes the layered σ\sigma84 σ\sigma85-stacked polytype discussed above. By contrast, crystal-chemistry papers have used rh-Bσ\sigma86Nσ\sigma87, hexagonal Bσ\sigma88Nσ\sigma89, or rh-BN/h-Bσ\sigma90Nσ\sigma91 for predicted dense three-dimensional σ\sigma92 rhombohedral networks with lattice parameters such as σ\sigma93 Å and σ\sigma94 Å in one formulation, or σ\sigma95 Å and σ\sigma96 Å in another, bulk moduli of σ\sigma97–σ\sigma98 GPa, and indirect gaps near σ\sigma99 eV. Those predicted ultra-hard phases are chemically stoichiometric BN, but they are not the same material as layered rBN and should not be conflated with the π\pi00 π\pi01-stacked host used in XANES, nonlinear-optical, and quantum-defect studies (Matar et al., 2021, Matar et al., 2021).

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