scieee Open visual document viewer

Anomalous bond softening mediated by strain-induced Friedel-like oscillations in a BC2N superlattice

Xu, Tengfei

Abstract

The crystal structure of BC2N and the origin of its superhardness remain under constant debate, hindering its development. Herein, by evaluating the x-ray diffraction pattern, the thermodynamic stability at normal and high pressures of a series of BC2N candidates, the (111) BC2N2x2 superlattice (labeled R2u-BC2N) is identified as the realistic crystal structure of the experimentally synthesized BC2N. We further reveal that the strain-induced Friedel-like oscillations dominates the preferable slip systems of R2u-BC2N by drastically weakening the heterogenous bonds across the slip plane and thus leads to its ultralow dislocation slip resistance, which originates from the metallization triggered by the reduction in energy separation between bonding and antibonding interactions of the softened bonds. Our results rule out R2u-BC2N as the intrinsic superhard material surpassing c-BN, whereas the experimentally determined extreme hardness can be attributed to the nanocrystalline grains glued by interfacial amorphous carbon which provides a strong barrier for plastic deformation. These findings provide a view of the longstanding issue of the possible structure of experimentally observed BC2N, and establish a mechanism underlying the strain-driven electronic instability of superlattice structures, providing guidance towards rational design of superhard materials.

Full text

PHYSICAL REVIEW B 106, L060101 (2022) Le e Anomalous bond so ening media ed by s ain-induced F iedel-like oscilla ions in a BC2N supe la ice Teng ei Xu,1,2Zhao ui Liu,1,2Dominik Legu ,3,4and Rui eng Zhang 1,2,* 1School o Ma e ials Science and Enginee ing, Beihang Uni e si y, Beijing 100191, People’s Republic o China 2Cen e o In eg a ed Compu a ional Enginee ing (In e na ional Resea ch Ins i u e o Mul idisciplina y Science) and Key Labo a o y o High-Tempe a u e S uc u al Ma e ials & Coa ings Technology (Minis y o Indus y and In o ma ion Technology), Beihang Uni e si y, Beijing 100191, People’s Republic o China 3IT4Inno a ions, VSB-Technical Uni e si y o Os a a, 17. lis opadu 2172/15, 708 00 Os a a, Czech Republic 4Nano echnology Cen e , CEET, VSB-Technical Uni e si y o Os a a, 17. lis opadu 2172/15, 708 00 Os a a, Czech Republic (Recei ed 19 Ap il 2022; accep ed 26 July 2022; published 15 Augus 2022) The c ys al s uc u e o BC2N and he o igin o i s supe ha dness emain unde cons an deba e, hinde ing i s de elopmen . He ein, by e alua ing he x- ay di ac ion pa e n, he he modynamic s abili y a no mal and high p essu es o a se ies o BC2N candida es, he (111) BC2N2×2supe la ice (labeled R2u−BC2N) is iden i ied as he ealis ic c ys al s uc u e o he expe imen ally syn hesized BC2N. We u he e eal ha he s ain-induced F iedel-like oscilla ions domina es he p e e able slip sys ems o R2u−BC2N by d as ically weakening he he e ogenous bonds ac oss he slip plane and hus leads o i s ul alow disloca ion slip esis ance, which o igi- na es om he me alliza ion igge ed by he educ ion in ene gy sepa a ion be ween bonding and an ibonding in e ac ions o he so ened bonds. Ou esul s ule ou R2u−BC2N as he in insic supe ha d ma e ial su passing c-BN, whe eas he expe imen ally de e mined ex eme ha dness can be a ibu ed o he nanoc ys alline g ains glued by in e acial amo phous ca bon which p o ides a s ong ba ie o plas ic de o ma ion. These indings p o ide a iew o he longs anding issue o he possible s uc u e o expe imen ally obse ed BC2N, and es ablish a mechanism unde lying he s ain-d i en elec onic ins abili y o supe la ice s uc u es, p o iding guidance owa ds a ional design o supe ha d ma e ials. DOI: 10.1103/PhysRe B.106.L060101 Supe ha d B-C-N e na y compounds ha e gained signi - ican in e es because o hei unique he modynamic and mechanical p ope ies as well as nume ous po en ial applica- ions [1–6]. Howe e , un esol ed challenges ega ding hei heo e ical and expe imen al aspec s hinde hei de elop- men . The success ul syn hesis o single BC2N phase a high p essu e [7,8] ini ia ed a longs anding disag eemen ega d- ing i s ac ual c ys al s uc u e, i.e., whe he ca bon can be andomly dis ibu ed in BN la ice o ice e sa because hey a e he modynamically immiscible wi h mino la ice misma ch [9,10]. Al hough expe imen ally syn hesized BC2N was epo ed o possess ex eme ha dness, he o igin o i s su- pe ha dness emains unde deba e [9–13]. This is because he plas ici y migh shi om c ys al’s inside o in e ace when he c ys alline size app oaches he nanome e scale, e en ually inducing he s onges size e ec [6,14,15], ye hese ac s a e gene ally igno ed in p e ious s udies. Gene ally, wo classes o candida e s uc u es ha e been p oposed o i he expe imen ally syn hesized BC2Nby e- p oducing expe imen ally de e mined x- ay di ac ion (XRD) pa e ns and ollowing calcula ed o ma ion en halpy un- de ambien condi ions. The i s class includes subs i u- ional solid solu ions wi h diamondlike pa en la ices, e.g., BC2N−n(n=1–7) [16], -BC2N, z-BC2N, and z*-BC2N *Co esponding au ho : z @buaa.edu.cn [17,18]. Al hough hese s uc u es p o ide somehow con- sis ence o he XRD pa e ns, mino de ia ion s ill exis s, challenging he a ionali y o hese s uc u es, ye his ag ee wi h he high o ma ion en halpy o hese compounds unde ambien condi ions. To accoun o his de iciency, Chen e al. [12], Li e al. [19] and Liu e al. [20] successi ely sugges ed he second-class candida es, i.e., (111) supe la ice s uc u es o med by sequen ially s acking c-BN and diamond laye s, which ha e be e he modynamic s abili y han he solu ion ypes because o he immiscible ea u e be ween c-BN and diamond unde ambien condi ions. Howe e , he o ma ion en halpy unde ambien condi ions does no gua an ee he s abili y a high p essu e (i.e., he eal expe imen al p essu e ∼20 GPa o BC2N) which migh s abilize some no el un- s able/me as able s uc u es ia la ice dis o ion in ol ing he local bond wis ing, o a ing, and e en econs uc ion. Rega ding he o igin o he ex eme ha dness o BC2N, i is belie ed ha he diso de ing o BC2N solid solu ion may induce s eng h enhancemen owing o he andom dis- ibu ion o C-C bonds ha a e s onge han B-N bonds, and consequen ly his was used o explain he in insic su- pe ha dness o BC2N[17,18]. Un o una ely, his explana ion is only plausible i he s uc u e o BC2N is de e mined o be a solid solu ion, whe eas he ac ha he o ma ion en- halpy o BC2N solid solu ion is highe han ha o BC2N supe la ice unde ambien condi ions does no seem o sup- po his ype o s uc u e. In BC2N supe la ice, he pe iodic he e ogenous in e aces o med by he o de ed alignmen o 2469-9950/2022/106(6)/L060101(8) L060101-1 ©2022 Ame ican Physical Socie y XU, LIU, LEGUT, AND ZHANG PHYSICAL REVIEW B 106, L060101 (2022) FIG. 1. (a) Rela i e en halpy s p essu e o BC2N. bc-BC2N is aken as e e ence. (b) Simula ed XRD pa e ns o R2u−BC2Nand expe imen al pa e n ep oduced om Re . [8]. (c) C ys al s uc u e o R2u−BC2N. (d) Enla ged di ac ion peaks o simula ed XRD pa e ns o Rnu−BC2N(n=1–4) and expe imen al pa e n ep oduced om Re . [8]. B-N and C-C bonds may cause peculia elec onic beha io , e.g., cha ge pe u ba ions obse ed in nano winned c-BN [21] and TmN/SiNxnanocomposi e sys ems [22], which would also signi ican ly a ec he mechanical s eng h. Conside ing BC2N supe la ice is he mos ealis ic expe imen ally syn he- sized BC2N, we need o cla i y whe he BC2N is an in insic supe ha d ma e ial exceeding c-BN o no , and he o igin o i s expe imen ally obse ed supe io ha dness. This equi es a mo e ealis ic jus i ica ion based on bo h he in insic plas ic esis ance o cons i u e c ys al and he nano-size e ec s uned by s ongly bonded in e ace, because hese wo aspec s may compe e o se e as he majo plas ic and ac u e mechanisms o he expe imen ally syn hesized nanos uc u ed BC2N. He e we show ha supe la ice s uc u es main ain he op- imal he modynamic s abili y om no mal o high p essu es compa ed o any solid solu ions, and he R2u−BC2Nis u - he e i ied as he syn hesized BC2N phase no only based on i s s abili y, bu also by i s pe ec ly ep oduced XRD pa e n. By compa ing he plas ic desc ip o s, such as ideal s eng h [23,24] and Peie ls s ess [25,26], o R2u−BC2N and c-BN unde a ious de o ma ion condi ions, i is su p isingly ound ha he F iedel-like oscilla ions o alence cha ge densi y ema kably limi he disloca ion slip esis ance o R2u−BC2N by so ening he he e ogenous bonds ac oss he slip plane. Th ough la ge scale a omis ic simula ions, we demons a e u he ha he in e acial amo phous ca bon, a he han he c ys al’s inside, domina es he plas ic low in nanos uc u ed BC2N, p o iding a ealis ic explana ion o he measu ed ex- eme ha dness, albei weak bonding na u e o R2u−BC2N. The modynamic s abili y a no mal p essu e does no gua an ee he s abili y a high p essu e because p essu e will undamen ally change he s abili y sequence o di e - en phases depending on hei o ma ion en halpy. Howe e , since i s disco e y h ough high p essu e expe imen s, he possible s uc u es o BC2N we e p oposed based on he ene - ge ic s abili y unde ambien condi ions, while neglec ing he p essu e con ibu ions. To demons a e he eal candida e o BC2N, we sys ema ically in es iga ed he p essu e-dependen he modynamic s abili ies o wo sho pe iod (111) BC2N supe la ices (i.e., R1u-BC2N and R2u−BC2N), and hose o se e al subs i u ional solu ions p oposed in p e ious s udies [12,16,18,27–29] [Fig. 1(a)]. I is clea ly seen ha wo BC2N supe la ices possess he lowes o ma ion en halpy among all he p oposed candida es unde ze o p essu e, which is consis- en wi h heo e ical calcula ions [12,19,20]. As he p essu e inc eases om 0 o 200 GPa, he supe la ice R2u−BC2N emains he mos ene ge ically s able phase, wi h o ma- ion en halpies much lowe han hose o he solu ions and ∼0.07 eV/a om lowe han ha o R1u-BC2Na anex- pe imen al p essu e o 20 GPa [8]. The XRD pa e n o R2u−BC2N was simula ed wi h x- ay wa eleng h λ= 0.424 Å and g ain size d=5 nm, which a e iden ical o L060101-2 ANOMALOUS BOND SOFTENING MEDIATED BY … PHYSICAL REVIEW B 106, L060101 (2022) FIG. 2. (a) Tensile and shea s ess-s ain cu es o R2u−BC2N, and hose o c-BN along i s weakes ensile di ec ion and shea pa h. Inse s shows he key bond leng hs (ma ked as “L1” o “L4”) a ia ions in R2u−BC2Nandc-BN unde ensile and shea s ains. Snapsho s o de o med s uc u es a equilib ium, peak and ins abili y s ains: (b)–(d) R2u−BC2N and (e)–(g) c-BN unde ensile s ains, (h)–(j) R2u−BC2N and (k)–(m) c-BN unde shea s ains. The s uc u e ans o ma ion o B-N laye s in R2u−BC2N unde shea loading a e highligh ed as pale b own a eas. he expe imen al condi ions [8]. Ob iously, all he simula ed di ac ion peaks o R2u−BC2N show excellen ag eemen wi h he expe imen al ones [Fig. 1(b)] ha can be seen as he s acking o wo laye s o c-BN and wo double laye s o diamond as illus a ed in Fig. 1(c). I is in e es ingly ound u he ha he o al ene gy dec eases as he numbe o s ack- ing laye s (i.e., supe la ice pe iod) inc eases, sugges ing ha he longe pe iod s uc u es a e mo e ene ge ically a o ed han R2u−BC2N[9,12]. Ne e heless, he simula ed XRD pa e ns o he o he supe la ice candida es do no ma ch he expe imen al XRD pa e n, which shows wo signi ican de ia ions be ween 5 ° and 10 ° [Fig. 1(d)], disquali ying hem as BC2N candida es. The la ice s abili y o R2u−BC2Nis u he e alua ed. In Fig. S2, he phonon dispe sions a p es- su es om 0 o 20 GPa a e posi i e o all wa e ec o s in he whole B illouin zone, i.e., no imagina y modes a e p esen , indica ing i s dynamical s abili y a ze o and high p essu es. Addi ionally, he mechanical s abili y o R2u−BC2N is co - obo a ed by calcula ing i s single-c ys al elas ic cons an s a ze o and high p essu es, all o which sa is y he elas ic s abili y c i e ion [30,31] (Table S1 in he Supplemen al Ma e- ial [32], Re s. [14,24,25,31,33–63]). Hence, he supe la ice R2u−BC2N ep esen s he mos ealis ic c ys al s uc u e o he expe imen ally syn hesized BC2N, which suppo s he indings o Li e al. [19] albei he p essu e dependence being neglec ed o he la e . The in insic la ice and ex insic mic oscopic con i- bu ions [14] we e conside ed simul aneously o ob ain a ealis ic quan i ica ion o he mechanis ic o igin o he BC2N supe ha dness. We i s demons a e he o me by compa ing he calcula ed ideal s eng h, ideal clea age/slide s ess, and Peie ls s ess. Figu e 2(a) shows he aniso opic s ess-s ain ela ionships o R2u−BC2N unde a ious a ine ension and shea loadings. The ensile s ess o R2u−BC2N along he [001] di ec ion exhibi s he lowes peak alue (74.8 GPa), which is highe han ha o c-BN (65.4 GPa) along he [111] di ec ion. The bond leng h a ia ions unde he [001] s ain clea ly show ha , while he ou non-equi alen bonds [“L1” o “L4” in Fig. 2(b)] weaken wi h inc easing s ain and b eak a he same s ain o 0.13, “L3” (1.51 Å) and “L4” (1.50 Å) a e much sho e han he B-N bond (1.55 Å) in c-BN [“L1” in Fig. 2(e)] unde equilib ium condi ion. This cha ac e is ic is main ained o a wide s ain ange o 0.00–0.12, indica ing hese wo s onge bonds a e he main load-bea ing uni s e- sis ing he applied s ain, he eby p oducing a la ge ensile s ess han ha o c-BN. A simila s acking sequence be ween (001) o R2u−BC2N and (111) o c-BN allows simila b eak- age modes unde ensile de o ma ion [Figs. 2(d) and 2(g)], i.e., s ain-induced g aphi iza ion [64,65]. In e es ingly, along he weakes (001) [¯ 2¯ 10] shea pa h, he ideal shea s eng h o R2u−BC2N (62.7 GPa) is sligh ly lowe han ha o c-BN (65.3 GPa). This o igina es om he mo e p o ound so ening o B-N bond in i s B-N laye s han B-N bond in c-BN when s ain inc eases, i.e., he bond leng h o “L1” in R2u−BC2N [Fig. 2(h)] inc eased by 0.23 Å when he s ain inc eases om 0.00 o 0.24, whe eas ha o “L2” in c-BN inc eased by 0.10 Å [Fig. 2(k)]. In s a k con as o he la ice ins abil- i y mode o c-BN, “L1” in R2u−BC2N immedia ely b eaks L060101-3 XU, LIU, LEGUT, AND ZHANG PHYSICAL REVIEW B 106, L060101 (2022) FIG. 3. (a) Topological s uc u e o R2u−BC2N wi h he possible weakes clea age/slip planes ma ked as do ed lines. (b) GSFEs o di e en slip planes, (c) de i ed slide s ess o shu le-se planes, and (d) Peie ls s ess o di e en slip planes in R2u−BC2N, oge he wi h hose in c-BN shown o compa ison. R2u−n(n=1–4) in (d) ep esen s he co esponding Peie ls s ess o S/G1-4. when he s ess d ops, and he ini ial la ice con igu a ion is ans o med in o a new one ha exhibi s mi o like symme y wi h he o iginal B-N laye [highligh ed a eas in Figs. 2(i) and 2(j). This unexpec ed in e io shea s eng h ela i e o c-BN cas s a doub on he p e ious conclusion o he in insic supe ha dness o BC2N. The weakes links o he R2u−BC2N c ys al we e de e - mined h ough compa ing aniso opic ideal s eng hs along di e en c ys allog aphic di ec ions o slip sys ems o co - ela e he clea age ac u e o slip disloca ion mobili y, espec i ely [14,42,66]. As shown in Fig. 3(a), he e a e eigh nonequi alen (001) clea age/slip planes including ou shu le-se (“S1” o “S4”) and ou glide-se (“G1” o “G4”) planes. The clea age ene gies o shu le-se planes a e much lowe han ha o he glide-se planes (Fig. S3) because he e ical bonds wi hin he shu le-se plane a e much weake han he connec ed iple-bonds ela ed o he glide-se planes when he alias ensile de o ma ion is applied. The shu le-se planes we e u he examined and a minimum ideal clea age s ess o 96.47 GPa o R2u−BC2N is obse ed along he no - mal di ec ion o “S4”, which is lowe han ha o c-BN (99.2 GPa), sugges ing i s in e io decohesion esis ance o c-BN. The key desc ip o ep esen ing he h eshold s ess ha makes he disloca ion mo e i e e sibly, i.e., Peie ls s ess, which is ul ima ely linked o he ha dness o a eal ma e ial [14], was analyzed ho oughly o de e mine he plas ici y e- sis ance. As seen in Fig. 3(b), he p o iles o he gene alized s acking aul ene gy (GSFE) o R2u−BC2N ag ee wi h hose o c-BN. The e o e, simila o c-BN, he uns able s acking aul ene gies (SFEs) o shu le-se planes along he [¯ 12¯ 10] di ec ion wi h he associa ed Peie ls s ess, and hose o he glide-se ones along he [¯ 1010] di ec ion wi h he associa ed Peie ls s ess o a pa ial disloca ion a e c ucial o com- p ehending he ha dness o R2u−BC2N[40]. As shown in Fig. 3(d), he lowes Peie ls s ess (1.17 GPa) o glide-se plane in R2u−BC2N is obse ed in “G4” and lowe han ha o c-BN (3.28 GPa) because o i s lowe SFE compa ed o c-BN [Fig. 3(b)]. Su p isingly, he lowes Peie ls s ess o shu le-se plane obse ed in “S2” is much lowe han c-BN (10.13 GPa), a 3.87 GPa, which is highly unusual because he R2u−BC2N has much highe SFE and slide s ess in “S2” han c-BN [Figs. 3(b) and 3(c)]. By compa ing he shape o hei GSFE cu es, a “ la peak” can be obse ed o R2u−BC2N [g een a ea in Fig. 3(b)], ha co esponds o a “smoo h u n” in i s slide s ess cu e s a ing om u=0.35 [g een a ows in Fig. 3(c)]. This beha io sugges s he appea ance o bond so ening, which may be esponsible o i s anomalously ul alow Peie ls s ess. To gain in-dep h insigh in o he unp eceden ed bond so - ening in R2u−BC2N, we aced he bond leng h a ia ions o L060101-4 ANOMALOUS BOND SOFTENING MEDIATED BY … PHYSICAL REVIEW B 106, L060101 (2022) FIG. 4. (a) Bond leng h a ia ions in se e al laye s a ound slip plane “S2” as a unc ion o he displacemen u in R2u−BC2N, compa ed wi h hose in c-BN. VCDD o (b)–(d) R2u−BC2N and (e)–(g) c-BN. DOS cu es o (h) R2u−BC2Nand(i)c-BN unde a ious displacemen s u. The same isosu ace le el o ±0.017 elec ons/Boh 3is used. Yellow and blue egions signi y he s a es o cha ge accumula ion (posi ion) and deple ion (nega i e), espec i ely. The Fe mi le el is se o ze o. The elec onic pe u ba ions a e highligh ed as ligh pu ple a eas in VCDDs. se e al laye s a ound he slip plane “S2” wi h he associa ed alence cha ge densi y di e ence (VCDD) e olu ions, and compa ed hese wi h hose o c-BN. As shown in Fig. 4(a), when he s ain inc eases om 0.00 o 0.30, he C1-N1 bond wi hin “S2” in R2u−BC2N emain sho e han he B1-N1 bond in c-BN, indica ing he s onge bonding cha ac e o C1-N1 bond han B1-N1 bond. A e he s ain o 0.30, unex- pec edly, he C1-N1 bond leng h inc eases s eeply o 2.40 Å a he s ain o 0.50, being much longe , i.e., weake han he B1-N1 bond (2.16 Å) in c-BN. This sugges s ha signi ican bond so ening occu ed in C1-N1 bond because o he la ge shea s ain, explaining he appea ance o he “ la peak” in i s L060101-5 XU, LIU, LEGUT, AND ZHANG PHYSICAL REVIEW B 106, L060101 (2022) FIG. 5. COHP cu es o se e al bonds a ound slip plane “S2” in R2u−BC2N unde di e en slip displacemen s u: (a) u=0.00, and (b) u=0.50. The co esponding esul s o (c) c-BN a e shown o compa ison. The Fe mi le el is se o ze o. GSFE cu e. E en mo e s ikingly, simila beha io can also be ound in he i s and second adjacen laye s o “S2”, in which he su ges in he bond leng h a ia ions appea when he s ain su passes 0.30, whe eas hese bond leng h changes a e negligible in c-BN. The no able di e ence in he bond leng h a ia ions be ween R2u−BC2N and c-BN is a ibu ed o hei dis inc localized cha ge ans e p ocess du ing slip- ping whe e a wide elec onic pe u ba ion pe pendicula o he “S2” is obse ed in R2u−BC2N, in ol ing he sequen- ial s eng hening/weakening o he bonds adjacen o C1-N1 bond [ ed and blue a ows in [Figs. 4(b)–4(d)]. These oscil- la ions o bond leng hs and s eng h ep esen he F iedel-like oscilla ions o alence cha ge densi y, shown in Figs. S4(a) and S4(b), analogous o he phenomenon ound adjacen o he su aces and in e aces o elec onically pe u bed solids [22,67]. As a consequence, he bond s eng h o C1-N1 de- c eases d as ically, leading o i s ul alow Peie ls s ess. While in c-BN, he cha ge pe u ba ions occu p edominan ly wi hin he slip plane, and a ely a ec he nea -neighbo ing a oms [Figs. 4(e)–4(g) and Figs. S4(c) and S4(d)]. Densi y o s a e (DOS) analysis e eals ha he s ain-induced F iedel-like oscilla ions accompanied by he me alliza ion o R2u−BC2N, which co esponds o he eme gence o elec onic s a es a he Fe mi le el a e he c i ical shea displacemen [ ed a ows in Fig. 4(h)]. In con as , he band gap o c-BN dec eases wi h inc easing s ain and no me alliza ion is obse ed [Fig. 4(i)]. By u he analyzing he c ys al o bi al Hamil on pop- ula ion (COHP) o he bonds a ound he slip plane in R2u−BC2N, and compa ed wi h ha o c-BN, a deep un- de s anding is ob ained on he a o emen ioned me alliza ion. Unde equilib ium condi ion, he C1-N1 bond o R2u−BC2N displays an an ibonding inge p in below he Fe mi le el [blue a ow in Fig. 5(a)], which may explain i s me as able ea u e wi h espec o diamond and c-BN. A e slipping along “S2”, he ema kably weakened B1-N2 and C2-C3 bonds caused by he F iedel-like oscilla ions, exhibi la ge bonding s a es a ound he Fe mi le el [ ed a ow in Fig. 5(b)]. These ascina ing bonding ea u es indica e ha , as he B1-N2 and C2-C3 bonds weaken, he ene gy o he bonding s a es inc eases and ha o he an ibonding ones dec eases, esul ing in he closu e o he ene gy gap. This d i es he localized bonding elec ons a ound “S2” in o a delocalized an ibonding s a e, he eby elici ing he me alliza ion. In compa ison, no bonding s a es a e ound in c-BN ha c oss he Fe mi le el [Fig. 5(c)]. I is no ed ha hese oscilla ions do no occu when slipping in he weakes glide-se plane “G4” in R2u−BC2N. As shown in Figs. S5(a)–S5(g), he bond leng h a ia ions and cha ge dis ibu ions a ound “G4” in R2u−BC2N a e essen- ially equi alen o hose in c-BN. The e o e, no me alliza ion is ound in ei he R2u−BC2No c-BN [Figs. S5(h) and S5(i)], while a lowe Peie ls s ess han c-BN is mainly a - ibu ed o he lowe in insic bonding s eng h o N1-B1 bond wi hin “G4” han ha o he N1-B1 bond in c-BN, because as he s ain inc eases, he la e becomes mo e sho e and s onge han he o me . Besides, di e en om he F iedel oscilla ions obse ed o occu in Ti-Si-N nanocomposi es sys ems [68,69] a equilib ium and leads o poo s eng h unde uni o m s ain, he me alliza ion in R2u−BC2N does no occu unde hese condi ions (Fig. S6), which explains i s ideal shea s eng h is only sligh ly lowe han ha o c-BN. Based on he a o emen ioned in es iga ions on he in insic mechanical p ope ies o R2u−BC2N, i can be concluded ha R2u−BC2N canno be anked as he in insic supe - ha d ma e ial supe io o c-BN, due o i s lowe ideal shea s eng h, weake in e plana clea age, and disloca ion slip esis ance. This conclusion s ongly challenges he p e i- ous conclusion on he supe ha dness o BC2N based on he in insic mechanical s eng h [11,12,20]. The mic oscopic o igin o nanos uc u ed BC2N ma e ials was u he in es- iga ed using la ge-scale molecula dynamics simula ions. Acco ding o expe imen al in o ma ion, he BC2N ma e ials wi h a nanoc ys alline s uc u e adhe ed oge he by ca bon amo phous in e acial laye (AIL) wi h a ying hicknesses (illus a ed in Fig. S7) we e cons uc ed and hen loaded by uniaxial s ess. Compa ed wi h he BC2N nanos uc u e wi h- ou AIL, he disloca ion nuclea ion and pene a ion a g ain bounda ies educed conside ably in he BC2N nanos uc u e con aining a 1-nm- hick AIL [Figs. S7(b) and S7(c)]. As he hickness o AIL inc eases o 2 nm [Fig. S7(d)], such as ha in he expe imen ally syn hesized sample [8], almos no la ice disloca ions a e obse ed, indica ing ha he de o ma- ion mechanism swi ched om la ice disloca ion o in e ace sliding. This phenomenon is consis en wi h ha obse ed in he nanos uc u ed diamond and me allic ma e ials [15,70,71]. Hence, he amo phous bounda y is e i ied as being p ima ily esponsible o he expe imen ally obse ed ex eme ha dness o BC2N. L060101-6 ANOMALOUS BOND SOFTENING MEDIATED BY … PHYSICAL REVIEW B 106, L060101 (2022) In summa y, h ough e alua ing he XRD pa e ns, and p essu e-dependen he modynamic, mechanical, and phonon s abili ies, we iden i ied he expe imen ally syn hesized BC2N phase as R2u−BC2N. We u he unco e ed a non adi ional bond de o ma ion mechanism media ed by a peculia s ain- d i en elec onic beha io . A e he c i ical shea s ain, owing o he appea ance o me alliza ion, F iedel-like os- cilla ions o alence cha ge densi y in ensely weaken he he e ogenous bonds ac oss he slip plane, hus ema kably limi ing he disloca ion slip esis ance o R2u−BC2N. The in e acial amo phous ca bon, a he han he c ys al’s inside, p edominan ly con ibu es o i s measu ed ex eme ha dness. Ou ongoing wo k sugges ha such oscilla ions a e likely o be a ubiqui ous phenomenon ha occu s also in o he (111) supe la ice bo on ca bon ni ides, e.g., BC4N[72,73] and BC10N[74], which emind us ha a oiding hese os- cilla ions h ough combining nanos uc u e enginee ing and g ain bounda y enginee ing is necessa y o achie e supe io ha dness o B-C-N ma e ials. The au ho s acknowledge he Na ional Na u al Science Founda ion o China (NFSC) wi h No. 51672015, Na ional Key Resea ch and De elopmen P og am o China (G an No. 2017YFB0702100), “111 P ojec ” (No. B17002), Na ional Thousand Young Talen s P og am o China, and Fundamen al Resea ch Funds o he Cen al Uni e si ies. D.L. acknowl- edges suppo by he Eu opean Regional De elopmen Fund in he IT4Inno a ions na ional supe compu ing cen e - Pa h o Exascale p ojec , No. CZ.02.1.01/0.0/0.0/16_013/0001791 wi hin he Ope a ional P og amme Resea ch, De elopmen and Educa ion and he p ojec e-INFRA CZ (ID:90140) by he Minis y o Educa ion, You h, and Spo o he Czech Republic. We would also hank D . S. Zhang o his help ul discussions. [1] S. Nakano, M. Akaishi, T. Sasaki, and S. Yamaoka, Chem. Ma e . 6, 2246 (1994). [2] E. Kni le, R. B. Kane , R. Jeanloz, and M. L. Cohen, Phys. Re . B51, 12149 (1995). [3] T. Koma su, M. Nomu a, Y. Kakuda e, and S. Fujiwa a, J. Ma e . Chem. 6, 1799 (1996). [4]R.B.Kane ,J.J.Gilman,andS.H.Tolbe ,Science 308, 1268 (2005). [5] Z. S. Zhao, B. Xu, and Y. J. Tian, Annu. Re . Ma e . Res. 46, 383 (2016). [6]X.T.Ren,X.Z.Yan,L.P.Wang,Y.S.Zhao,andS.M.Wang, J. Supe ha d Ma e . 43, 307 (2021). [7] V. L. Solozhenko, D. And aul , G. Fique , M. Mezoua , and D. C. Rubie, Appl. Phys. Le . 78, 1385 (2001). [8] Y. Zhao, D. W. He, L. L. Daemen, T. D. Shen, R. B. Schwa z, Y. Zhu, D. L. Bish, J. Huang, J. Zhang, G. Shen e al.,J. Ma e . Res. 17, 3139 (2002). [9] C. Chen and H. Sun, Phys.Re .Le .99, 159601 (2007). [10] S. Chen, X. G. Gong, and S. H. Wei, Phys. Re . Le . 99, 159602 (2007). [11] Z. Pan, H. Sun, and C. Chen, Phys.Re .Le .98, 135505 (2007). [12] S. Chen, X. G. Gong, and S. H. Wei, Phys. Re . Le . 98, 015502 (2007). [13] Y. Zhang, H. Sun, and C. Chen, Phys. Re . Le . 93, 195504 (2004). [14] R. F. Zhang, S. H. Zhang, Y. Q. Guo, Z. H. Fu, D. Legu , T. C. Ge mann, and S. Vep ek, Phys. Rep. 826, 1 (2019). [15] Q. Zhang, C. Wang, H. Zhang, S. Zhang, Z. Liu, D. Legu , S. Vep ek, and R. Zhang, Ca bon 170, 394 (2020). [16] H. Sun, S. H. Jhi, D. Roundy, M. L. Cohen, and S. G. Louie, Phys.Re .B64, 094108 (2001). [17] X. F. Zhou, J. Sun, Y. X. Fan, J. Chen, H. T. Wang, X. Guo, J. He, and Y. Tian, Phys. Re . B 76, 100101(R) (2007). [18] X. F. Zhou, J. Sun, Q. R. Qian, X. Guo, Z. Liu, Y. Tian, and H. T. Wang, J. Appl. Phys. 105, 093521 (2009). [19] Q. Li, M. Wang, A. R. Ogano , T. Cui, Y. Ma, and G. Zou, J. Appl. Phys. 105, 053514 (2009). [20] L. Liu, Z. Zhao, T. Yu, S. Zhang, J. Lin, and G. Yang, J. Phys. Chem. C 122, 6801 (2018). [21] S. Zheng, R. Zhang, R. Huang, T. Taniguchi, X. Ma, Y. Ikuha a, andI.J.Beye lein,Appl. Phys. Le . 109, 081901 (2016). [22] R. F. Zhang, A. S. A gon, and S. Vep ek, Phys. Re . Le . 102, 015503 (2009). [23] D. Roundy and M. L. Cohen, Phys.Re .B64, 212103 (2001). [24] S. H. Zhang, Z. H. Fu, and R. F. Zhang, Compu . Phys. Commun. 238, 244 (2019). [25] B. Joos, Q. Ren, and M. S. Duesbe y, Phys.Re .B50, 5890 (1994). [26] Y. Q. Guo, S. H. Zhang, I. J. Beye lein, D. Legu , S. L. Shang, Z. K. Liu, and R. F. Zhang, Ac a Ma e . 181, 423 (2019). [27] M. Ma esini and S. F. Ma a , In l. J. Ino gan. Ma e . 3, 943 (2001). [28] X. Luo, X. Guo, B. Xu, Q. Wu, Q. Hu, Z. Liu, J. He, D. Yu, Y. Tian, and H. T. Wang, Phys. Re . B 76, 094103 (2007). [29] X. G. Luo, X. J. Guo, Z. Y. Liu, J. L. He, D. L. Yu, B. Xu, Y. J. Tian, and H. T. Wang, Phys. Re . B 76, 092107 (2007). [30] Z. J. Wu, E. J. Zhao, H. P. Xiang, X. F. Hao, X. J. Liu, and J. Meng, Phys.Re .B76, 054115 (2007). [31] S. H. Zhang and R. F. Zhang, Compu . Phys. Commun. 220, 403 (2017). [32] See Supplemen al Ma e ial a h p://link.aps.o g/supplemen al/ 10.1103/PhysRe B.106.L060101 o u he de ails on he me hods used in his s udy, addi ional igu es and able. he Sup- plemen al Ma e ial also includes Re s. [14,24,25,31,33–63]. [33] G. K esse and J. Fu hmülle , Phys. Re . B 54, 11169 (1996). [34] G. K esse and D. Joube , Phys.Re .B59, 1758 (1999). [35] D. M. Cepe ley and B. J. Alde , Phys. Re . Le . 45, 566 (1980). [36] J. P. Pe dew and A. Zunge , Phys.Re .B23, 5048 (1981). [37] M. P. A. T. Me h essel and A. T. Pax on, Phys. Re . B 40, 3616 (1989). [38] H. J. Monkho s and J. D. Pack, Phys.Re .B13, 5188 (1976). [39] A. Togo and I. Tanaka, Sc . Ma e . 108, 1 (2015). [40] S. H. Zhang, D. Legu , T. C. Ge mann, S. Vep ek, H. J. Zhang, and R. F. Zhang, Phys.Re .B101, 014104 (2020). [41] S. H. Zhang, I. J. Beye lein, D. Legu , Z. H. Fu, Z. Zhang, S. L. L060101-7 XU, LIU, LEGUT, AND ZHANG PHYSICAL REVIEW B 106, L060101 (2022) Shang, Z. K. Liu, T. C. Ge mann, and R. F. Zhang, Phys. Re . B95, 224106 (2017). [42] S. H. Zhang, X. Zheng, Q. Q. Jin, S. J. Zheng, D. Legu , X. H. Yu,H.Y.Gou,Z.H.Fu,Y.Q.Guo,B.M.Yane al.,Phys. Re . Ma e . 2, 123602 (2018). [43] S. H. Zhang, D. Legu , and R. F. Zhang, Compu . Phys. Commun. 240, 60 (2019). [44] A. T. Blumenau, R. Jones, T. F auenheim, B. Willems, O. I. Lebede , G. Van Tendeloo, D. Fishe , and P. M. Ma ineau, Phys.Re .B68, 014115 (2003). [45] Y. Kamimu a, K. Edagawa, A. M. Iskanda o , M. Osawa, Y. Umeno, and S. Takeuchi, Ac a Ma e . 148, 355 (2018). [46] Z. R. Liu, B. N. Yao, and R. F. Zhang, Compu . Ma e . Sci. 210, 111027 (2022). [47] G. Vo onoi, J. Reine Angew. Ma h. 134, 198 (1908). [48] C. de Tomas, I. Sua ez. Ma inez, and N. A. Ma ks, Ca bon 109, 681 (2016). [49] J. Te so , Phys.Re .B49, 16349 (1994). [50] C. Huang, X. Peng, B. Yang, H. Xiang, S. Sun, X. Chen, Q. Li, D. Yin, and T. Fu, Ca bon 132, 606 (2018). [51] C. Huang, X. Peng, and B. Yang, Ce am. In . 47, 28659 (2021). [52] C. Huang, X. Peng, B. Yang, S. Weng, Y. Zhao, and T. Fu, Compu . Ma e . Sci. 157, 67 (2019). [53] Y. Liu, B. Li, and L. Kong, Compu . Ma e . Sci. 148,76 (2018). [54] S. Plimp on, J. Compu . Phys. 117, 1 (1995). [55] W. G. Hoo e , Phys.Re .A31, 1695 (1985). [56] W. G. Hoo e , Phys.Re .A34, 2499 (1986). [57] A. S ukowski, Model. Simul. Ma e . Sci. Eng. 18, 015012 (2010). [58] B. N. Yao and R. F. Zhang, Compu . Phys. Commun. 247, 106857 (2020). [59] S. Main z, V. L. De inge , A. L. Tchoug ée , and R. D onskowski, J. Compu . Chem. 37, 1030 (2016). [60] R. Nelson, C. E u al, J. Geo ge, V. L. De inge , G. Hau ie , and R. D onskowski, J. Compu . Chem. 41, 1931 (2020). [61] R. D onskowski and P. E. Blöchl, J. Phys. Chem. C 97, 8617 (1993). [62] V. L. De inge , A. L. Tchoug ée , and R. D onskowski, J. Phys. Chem. A 115, 5461 (2011). [63] J. A. Zimme man, C. L. Kelchne , P. A. Klein, J. C. Hamil on, andS.M.Foiles,Phys.Re .Le .87, 165507 (2001). [64] Y. Zhang, H. Sun, and C. Chen, Phys. Re . B 73, 144115 (2006). [65] S. Zhang, D. Legu , Z. Fu, T. C. Ge mann, and R. Zhang, Ca bon 137, 156 (2018). [66]C.Lu,Q.Li,Y.Ma,andC.Chen,Phys.Re .Le .119, 115503 (2017). [67] J. F iedel, Philos. Mag. 43, 153 (1952). [68] S. Hao, B. Delley, and C. S amp l, Phys. Re . B 74, 035424 (2006). [69] R. F. Zhang, A. S. A gon, and S. Vep ek, Phys. Re . B 79, 245426 (2009). [70] V. Tu lo and T. J. Rupe , Ac a Ma e . 151, 100 (2018). [71] G. Wu, K. Chan, L. Zhu, L. Sun, and J. Lu, Na u e (London) 545, 80 (2017). [72] S. Y. Chen, X. G. Gong, and S. H. Wei, Phys.Re .B77, 014113 (2008). [73] X. G. Luo, X. F. Zhou, Z. Y. Liu, J. L. He, B. Xu, D. L. Yu, H. T. Wang, and Y. J. Tian, J. Phys. Chem. C 112, 9516 (2008). [74] W. C. Chen, J. N. Schmid , D. Yan, Y. K. Voh a, and C. C. Chen, npj Compu . Ma e . 7, 114 (2021). L060101-8