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1                                              Hf-, Sn-, and Zr-Beta zeolites catalyze the cross-aldol
2                                              Hf-NU-1000-ZrBn is found to be a promising single-compon
3 )N)(3)M(mu-H)(mu-NMe(2))(2)](2)M (M = Zr, 1; Hf, 2) were observed to be intermediates and characteriz
4  Reactions of d0 amides M(NMe2)4 (M = Zr, 1; Hf, 2) with O2 have been found to yield unusual trinucle
5 fined correlation between the Th/Hf and (176)Hf/(177)Hf ratios in chondrites that reflects remobiliza
6 08,207,206)Pb/(204)Pb, (143)Nd/(144)Nd, (176)Hf/(177)Hf, and (230)Th/(232)Th.
7                             Evidence of (176)Hf excess in select meteorites older than 4556Ma was sug
8 rrelation between the Th/Hf and (176)Hf/(177)Hf ratios in chondrites that reflects remobilization of
9 06)Pb/(204)Pb, (143)Nd/(144)Nd, (176)Hf/(177)Hf, and (230)Th/(232)Th.
10 actions define distinct initial (182)Hf/(180)Hf corresponding to a 13.8 +/- 5.3 million year apparent
11 scopy between Stark-Zeeman sublevels in (180)Hf(19)F(+) with a coherence time of 100 milliseconds.
12                                         (182)Hf-(182)W chronometry of terrestrial rocks points to acc
13                                Accurate (182)Hf-(182)W chronology of early planetary differentiation
14 lization of the lunar magma ocean after (182)Hf was no longer extant-that is, more than about 60 mill
15 adioisotopes (e.g., (26)Al, (41)Ca, and (182)Hf) synthesized in one or multiple stars and added to th
16 vertheless, some N-body simulations and (182)Hf-(182)W and (87)Rb-(87)Sr chronology of some lunar roc
17                  The decoupling between (182)Hf and (26)Al requires distinct stellar origins: steady-
18 resulting from the decay of now-extinct (182)Hf, among five magmatic iron meteorite groups.
19 particular, the abundances inferred for (182)Hf (half-life = 8.9 million years) and (129)I (half-life
20 te galactic stellar nucleosynthesis for (182)Hf and late-stage contamination of the protosolar molecu
21 metal fractions define distinct initial (182)Hf/(180)Hf corresponding to a 13.8 +/- 5.3 million year
22  asymptotic giant branch stars produces (182)Hf.
23        In contrast, our results support (182)Hf homogeneity and chronological significance of the (18
24 on of the hafnium-tungsten systematics ((182)Hf decaying to (182)W and emitting two electrons with a
25                               Using the (182)Hf-(182)W chronometer, we show that a FUN CAI recording
26 y and chronological significance of the (182)Hf-(182)W clock.
27 le, which can be investigated using the (182)Hf-(182)W decay system in shergottite-nakhlite-chassigni
28                                     The (182)Hf-(182)W system provides a powerful complement to the (
29 gen ligand, [(eta(5)-C(5)H(2)-1,2,4-Me(3))(2)Hf](2)(mu(2),eta(2),eta(2)-N(2)), by addition of CySiH(3
30 f (C(5)H(5))(2)Zr(CH(3))(2) or (C(5)Me(5))(2)Hf(CH(3))(2) with diphenyldiazomethane is limited to the
31 ted hafnocene product, (eta(5)-C(5)Me(4)H)(2)Hf(OTf)(N(2)(CH(3))) provides a platform for additional
32 yl diazenide compound, (eta(5)-C(5)Me(4)H)(2)Hf(OTf)(N(2)(CH(3))), arising from methylation of one of
33 the hafnocene complex [(eta(5)-C(5)Me(4)H)(2)Hf](2)(mu(2),eta(2),eta(2)-N(2)) underwent clean carbony
34 nd dinitrogen ligand, [(eta(5)-C(5)Me(4)H)(2)Hf](2)(mu(2),eta(2),eta(2)-N(2)), with two equivalents o
35  functionalization in [(eta(5)-C(5)Me(4)H)(2)Hf](2)(N(2)C(2)O(2)) was also accomplished with silanes
36 e oxamidide ligand in [(eta(5)-C(5)Me(4)H)(2)Hf](2)(N(2)C(2)O(2)) was explored due to the high symmet
37 (2)(N(2)C(2)O(2)) and [(eta(5)-C(5)Me(4)H)(2)Hf](2)(N(2)C(2)O(2)), prepared from CO-induced N(2) bond
38  for (C(5)Me(5))(2)MCl(2) (M = Ti, 1; Zr, 2; Hf, 3; Th, 4; U, 5), where we can directly compare a cla
39 e2)6(mu-NMe2)3(mu3-O)(mu3-ONMe2) (M = Zr, 3; Hf, 4) in high yields.
40 oup 4 difluorides (Cp2MF2, M = Ti 4a, Zr 5a, Hf 6a; Cp*2MF2, M = Ti 4b, Zr 5b, Hf 6b) are reported.
41 4a, Zr 5a, Hf 6a; Cp*2MF2, M = Ti 4b, Zr 5b, Hf 6b) are reported.
42 2-MIL-125(Ti), NH2-UiO-66(Zr) and NH2-UiO-66(Hf) are among the most studied MOFs for photocatalytic a
43  report a hafnium-containing MOF, hcp UiO-67(Hf), which is a ligand-deficient layered analogue of the
44 alogue of the face-centered cubic fcu UiO-67(Hf).
45 8)V*, Ni(8)W, Pd(8)Al(dagger), Pd(8)Fe, Pd(8)Hf, Pd(8)Mn, Pd(8)Mo*, Pd(8)Nb, Pd(8)Sc, Pd(8)Ta, Pd(8)T
46 Zn, Pd(8)Zr, Pt(8)Al(dagger), Pt(8)Cr*, Pt(8)Hf, Pt(8)Mn, Pt(8)Mo, Pt(8)Nb, Pt(8)Rh(dagger), Pt(8)Sc,
47      Here we report the rational design of a Hf-porphyrin nanoscale metal-organic framework, DBP-UiO,
48 ikely mechanism is hydration of the adsorbed Hf complex up to a coordination number of 7, followed by
49 ntegral alkyne units in a pair of Zr(4+) and Hf(4+) MOFs, which proceeds stereoselectively in a singl
50 ch as (t)BuNCO and CO(2) to form new N-C and Hf-O bonds.
51  the 40 elements: Ta, U, Ir, Rh, Th, Ce, and Hf showed the lowest Dmin values, </=10 nm; Bi, W, In, P
52 tentative correlation between S isotopes and Hf-W core segregation ages suggests that the two systems
53 oselectivity is observed, whereby Zr(IV) and Hf(IV) principally direct P-OR hydrolysis, whereas Th(IV
54 dimeric structure in the cases of Zr(IV) and Hf(IV).
55 y accelerated by Ce(IV), Th(IV), Zr(IV), and Hf(IV) cations.
56 discrepancy between the U-Pb (60-80 Myr) and Hf-W clocks (30 Myr) in determining the timescale of Ear
57                          The Pb, Sr, Nd, and Hf isotopic mixing arrays show that the Archean EM I mat
58  requiring the separation of Sr, Pb, Nd, and Hf only.
59 by addition of CySiH(3) resulted in N-Si and Hf-H bond formation and a compound poised for subsequent
60 , B, Na, Ga, Rb, Sr, Zr, Nb, Cs, Ba, Sm, and Hf, allows more than 80% of correct predictions in leave
61 ically unsaturated diene complexes of Ti and Hf.
62 r and Pb, LREE then La-Ce-Nd-Sm, Lu(Yb), and Hf, Th, and U, respectively) along with an additional, i
63 crystallographic analysis reveals the Zr and Hf complexes to be closely isostructural; the bond lengt
64             The high atomic number of Zr and Hf in the SBUs serves as effective X-ray antenna by abso
65 sis of a series of 14 interpenetrated Zr and Hf MOFs linked by functionalized 4,4'-[1,4-phenylene-bis
66 e of UiO materials, the d-orbitals of Zr and Hf, are too low in binding energy and thus cannot overla
67 In addition, the WB4 alloys with Ti, Zr, and Hf showed a substantially increased oxidation resistance
68 s show that when group IV (i.e., Ti, Zr, and Hf) or V (i.e., Nb and Ta) transition metals are substit
69 number, in the order Ti > Zr approximately = Hf, and that uranium displays approximately half the cov
70 oys with 8 at. % Ti, 8 at. % Zr, and 6 at. % Hf gave hardness values, Hv, of 50.9 +/- 2.2, 55.9 +/- 2
71 s application to poorly characterized binary Hf systems, believed to be phase-separating, defines thr
72 old-plastic forming of the typically brittle Hf-based bulk amorphous alloy through controlling homoge
73 Si(eta(5)-C(5)Me(4))(eta(5)-C(5)H(3)-3-(t)Bu)Hf(I)(NCO), demonstrating that C-C bond formation is rev
74 2)Si(eta(5)-C(5)Me(4))(eta(5)-C(5)H(3)-(t)Bu)Hf](2)(mu(2), eta(2), eta(2)-N(2)), yields the correspon
75 Si(eta(5)-C(5)Me(4))(eta(5)-C(5)H(3)-3-(t)Bu)Hf](2)(N(2)C(2)O(2)) and [(eta(5)-C(5)Me(4)H)(2)Hf](2)(N
76 Si(eta(5)-C(5)Me(4))(eta(5)-C(5)H(3)-3-(t)Bu)Hf](2)(N(2)C(2)O(2)) with I(2) yielded the monomeric iod
77 Si(eta(5)-C(5)Me(4))(eta(5)-C(5)H(3)-3-(t)Bu)Hf](2)(N(2)C(2)O(2)), undergoes facile cycloaddition wit
78 ter 54 h in air at 530 degrees C achieved by Hf addition onto LSC.
79                                    Better by Hf: Anion coordination to a bridging hafnocene nitride c
80 llylic and homoallylic alcohols catalyzed by Hf(IV)-bishydroxamic acid (BHA) complexes is described.
81 d homoallylic amine derivatives catalyzed by Hf(IV)-bishydroxamic acid complexes is described.
82               As a multifunctional catalyst, Hf-NU-1000 is also efficient for other epoxide activatio
83            The hafnium analogue of 1, Cp*(Cl)Hf(2,3-dimethylbutadiene) (14), has been reported to giv
84  of the mixed-ring silyl methyl complex CpCp*Hf[Si(SiMe3)3]Me (4) with B(C6F5)3 in bromobenzene-d5 yi
85                            Reactions of CpCp*Hf(SiR3)Me (SiR3 = SitBuPh2, SiHMes2) with B(C6F5)3 rapi
86 ary ligand, with the stabilities of the CpCp*Hf(SnPh(3))X compounds following the order X = NMe(2) >
87 p orbital mixing is enhanced for the diffuse Hf (5d) and Zr (4d) atomic orbitals in relation to the m
88 e orogenic processes which may have distinct Hf-Nd isotopic signatures.
89 ies (<10(-6) A/cm(2) at +/-2 V) and enhances Hf-SAND multilayer capacitance densities to nearly 1 muF
90                                 For example, Hf(OTf)4 mediates rapid endothermic ether right harpoon
91 . % for Ti, 10 at. % for Zr, and 8 at. % for Hf.
92 ion and silicate differentiation fractionate Hf from W.
93 rein a new Hf-based metal-organic framework (Hf-NU-1000) incorporating Hf6 clusters is reported.
94 mesoporous Hf-based metal-organic framework (Hf-NU-1000) is employed as a well-defined scaffold for a
95 ystem is much slower than that obtained from Hf-W systematics, and implies substantial accretion afte
96  titanium (Ti), zirconium (Zr), and hafnium (Hf), of different concentrations (0-50 at.
97 locked the plutonic archive through hafnium (Hf) and oxygen (O) isotope analysis of zoned zircon crys
98                                        Heavy Hf atoms in the SBUs efficiently absorb X-rays and trans
99 ands, enhanced intersystem crossing by heavy Hf centers, and facile (1)O2 diffusion through porous DB
100 bpy)3 ](2+) -derived tricarboxylate ligands (Hf-BPY-Ir or Hf-BPY-Ru; bpy=2,2'-bipyridine, ppy=2-pheny
101                                          Low Hf concentration films feature an aged surface of larger
102                                  U-Pb and Lu-Hf isotope analyses of zircons were made using ion probe
103                         Here, we combined Lu-Hf isotopes and U-Pb geochronology to map the four-dimen
104                         Lutetium-hafnium (Lu-Hf) isotope data for ALH indicate an igneous age of 4.09
105 esent an integrated zircon isotope (U-Pb, Lu-Hf, O) and trace element dataset from the paired Cu-Au (
106                            The calculated Lu/Hf and Sm/Nd (samarium/neodymium) ratios of the ALH pare
107 from M6(mu3-O)4(mu3-OH)4(carboxylate)12 (M = Hf or Zr) secondary building units (SBUs) and anthracene
108  n-Bu, i-Bu, and 2-ethylbutyl (5a-f) and M = Hf; R = i-Bu and t-Bu (6 and 7, respectively)] is descri
109           This work suggests that MNiSn (M = Hf, Zr, Ti) and perhaps most other half-Heusler thermoel
110 (3)-N-N=CPh(2)](CH(3)) (M = Zr, R = H or M = Hf, R = CH(3)).
111                            This new material Hf-NU-1000-ZrBn is fully characterized by a variety of s
112       A structurally well-defined mesoporous Hf-based metal-organic framework (Hf-NU-1000) is employe
113 ed compounds (M = Sc, Ti, V, Cr, Zr, Nb, Mo, Hf, Ta) with F-, H-, O-, and OH-functionalized surfaces
114       Here we report the clay-sized (<2 mum) Hf-Nd isotope data from Asian dust sources to better con
115 ](2-MeO[bond]C(6)H(4))(2,4,6-Me(3)C(6)H(2))N]Hf(CH(2)Ph) (3) (1), which is capable of polymerizing 1-
116 oxide-organic self-assembled nanodielectric (Hf-SAND) material consisting of regular, alternating pi-
117 y discovered body-centered cubic (BCC) Ta-Nb-Hf-Zr-Ti high-entropy alloy superconductor appears to di
118 d zircons, together with the unradiogenic Nd-Hf isotope of the host quartz diorite, appears to sugges
119                                 Herein a new Hf-based metal-organic framework (Hf-NU-1000) incorporat
120  reconstructions and ground-truthed with new Hf-Nd isotope data, suggest that uppermost mantle at one
121 ore a comprehensive data set of isotopic (O, Hf) and chemical proxies in precisely U-Pb dated zircon
122 s-tert-butyl phenyl substituted complexes of Hf and Zr, when activated by MAO at 50-80 degrees C, gen
123 f the molecular weight distribution (MWD) of Hf-bound polymers via UV-GPC analysis.
124 rm is produced by solution phase reaction of Hf(NEtMe)4 with ammonia followed by low-temperature pyro
125 sed for deprotonation of YHf and transfer of Hf+ against the thermodynamic potential.
126              We propose that the transfer of Hf+ from formate to the active site base Y- is thermodyn
127 tion at the Hf center, and chain transfer of Hf-bound polymers to ZnEt2 is fast and quasi-irreversibl
128           Large-area devices (>0.2 mm(2)) on Hf-SAND (6.5 nm thick) achieve mA on currents at ultralo
129                                     Based on Hf-W chronometry on Allende chondrules and matrix, this
130 mbient (400 degrees C) has limited impact on Hf-SAND leakage densities (<10(-6) A/cm(2) at +/-2 V) an
131 derived tricarboxylate ligands (Hf-BPY-Ir or Hf-BPY-Ru; bpy=2,2'-bipyridine, ppy=2-phenylpyridine) an
132 plexes [Cp*2MCH3](+)[B(C6F5)4](-) (M = Zr or Hf) with trimethylsilyl(diarylphosphino)acetylenes Ar2P-
133 organic frameworks (MOFs), M-MTBC (M = Zr or Hf), constructed from the tetrahedral linker methane-tet
134 oxide complexes [(PNP)M(CH3)2(OAr)] (M=Zr or Hf; PNP(-)=N[2-P(CHMe2)2-4-methylphenyl]2); Ar=2,6-iPr2C
135                 Here we present new Sr-Nd-Pb-Hf isotope data from the older parts of this hotspot tra
136 ns and their host oxide gabbro have positive Hf isotope compositions (epsilonHf = +15.7-+12.4), sugge
137 educed Mo(IV) state with the formate proton, Hf+, transferring to a nearby base Y-.
138 how that there is a more positive radiogenic Hf isotopic composition with clay-sized fractions than t
139                In the halichondrin C series, Hf(OTf)4 was used to convert the double oxy-Michael prod
140                                  The sizable Hf-SAND capacitances are attributed to relatively large
141                               The clay-sized Hf-Nd isotopic compositions of the desert samples from t
142 lso exists in MC-ICPMS, e.g., Nd, Ce, W, Sr, Hf, Ge, Hg, and Pb isotopes, the nature of mass bias for
143 H interaction and formation of a stabilizing Hf-arene interaction.
144 anoscale metal-organic framework (nMOF), TBC-Hf, and a small-molecule immunotherapy agent that inhibi
145 arbon nanotube transistors were used to test Hf-SAND utility in electronics and afforded record on-st
146 nd a well-defined correlation between the Th/Hf and (176)Hf/(177)Hf ratios in chondrites that reflect
147                                          The Hf-Nd isotopic compositions of dust in the North Pacific
148  the C-C bond of a cyclopropane ring and the Hf.
149 not influence the rate of propagation at the Hf center, and chain transfer of Hf-bound polymers to Zn
150 l similarity of the Hf and Zr complexes, the Hf complexes generate more highly stereoselective cataly
151     Using this relationship, we estimate the Hf/W ratio in Mars' mantle to be 3.51 +/- 0.45.
152 ggests optimal activation conditions for the Hf pre-catalyst in the presence of the activator [Ph3C][
153 riers than corresponding insertions into the Hf-alkyl bond.
154 culations show that such insertions into the Hf-aryl bond have lower barriers than corresponding inse
155 e driving forces for this insertion into the Hf-aryl bond include elimination of an eclipsing H-H int
156 thyl, consistent with 1,2-insertion into the Hf-aryl bond.
157 itially undergoes monomer insertion into the Hf-naphthyl bond, which permanently modifies the ligand
158     Despite the structural similarity of the Hf and Zr complexes, the Hf complexes generate more high
159 n of Cl upon increase in coordination of the Hf atom of the precursor.
160 osely isostructural; the bond lengths of the Hf complex are slightly shorter, but the maximum deviati
161 ed, demonstrating the flexible nature of the Hf(IV)-BHA system.
162 sponding bulk sample and a decoupling of the Hf-Nd couplets in the clay formation during the weatheri
163                          We suggest that the Hf-W timescale reflects the principal phase of core-form
164 g to a large uncertainty associated with the Hf/W ratio of the Martian mantle and as a result, contra
165                                        These Hf-SAND multilayers are grown from solution in ambient w
166                                        Thus, Hf-bound polymeryls are selectively labeled in the prese
167  is observed that the Ni interstitial and Ti,Hf/Sn antisite defects are collectively formed, leading
168        Moving down the periodic table (Ti to Hf) has a marked effect on the experimental transition i
169                         Variations in zircon Hf and U/Yb reaffirm that tin belt magmas contain greate
170 ctive metal complexes M(CH(2)Ph)(4) (M = Zr, Hf) and multiple activation conditions represent a new h
171 orks (MOFs), NU-1000 and UiO-66, for M = Zr, Hf.
172 3-ONa)4H6](6-) nodes in M(III)H-BTC (M = Zr, Hf; BTC is 1,3,5-benzenetricarboxylate) via bimetallic r
173 afnium polyazides [PPh4 ]2 [M(N3 )6 ] (M=Zr, Hf) were obtained in near quantitative yields from the c
174 carbon covalence in (C5H5)2MCl2 (M = Ti, Zr, Hf) has been evaluated using carbon K-edge X-ray absorpt
175  of oxygen-functionalized M2CO2 (M = Ti, Zr, Hf) MXenes are investigated using first-principles calcu
176                    M(NMe(2))(4) (M = Ti, Zr, Hf) were found to react with H(2)SiR'Ph (R' = H, Me, Ph)
177  [M(N3 )5 ](-) and [M(N3 )6 ](2-) (M=Ti, Zr, Hf) were studied by quantum chemical calculations at the
178 r)]}(2)(mu-N(2)) compounds where M = Ti, Zr, Hf, Ta, Mo, and W.
179 c structures of O(h)-MCl(6)(2-) (M = Ti, Zr, Hf, U) and C(4v)-UOCl(5)(-), and to determine the relati
180  actinide hexahalides, MCl6(2-) (M = Ti, Zr, Hf, U).
181 xes {PhB(C5H4)(Ox(R))2}M(NMe2)2 (M = Ti, Zr, Hf; Ox(R) = 4,4-dimethyl-2-oxazoline, 4S-isopropyl-5,5-d
182  large family of materials (WHM with W = Zr, Hf; H = Si, Ge, Sn; M = O, S, Se, Te) with identical ban
183                           Similar to the (Zr,Hf)NiSn based solid solutions, the unsubstituted ZrNiSn
184            They are the first examples of Zr/Hf MOFs with tetrahedral linkers.
185 stitution of the 8-connected nodes by the Zr/Hf clusters yielded MOFs with large octahedral interstit

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