ライフサイエンスコーパス: hole

1 w hundred gravitational radii from the black hole.

2 seed for the formation of a monstrous black hole.

3 owards the galactic centre to feed the black hole.

4 ecise arrangement and size of the individual holes.

5 dio flux ratios required for accreting black holes.

6 nentially with increasing distance from tree holes.

7 ith a catastrophic collapse to leave a black hole-a promising seed for the formation of a monstrous b

8 ide (Sa) hole donor and stilbenediether (Sd) hole acceptor separated by DNA G-quadruplex structures p

9 Of the remainder, 12% developed a macular hole and 8% elected to proceed with surgery for symptoms

10 gnetic field that is advected from the black hole and distorted by dissipation processes within the j

11 d-effect transistor embodiment that exhibits hole and electron mobilities of 213 +/- 15 and 166 +/- 5

12 The surface state connects hole and electron pockets that would otherwise be separa

13 V) blend, which is evidenced by the enhanced hole and electron transport abilities of the active laye

14 mate the herniation of chromatin through the hole and its relation to the lamin expression levels in

15 hysical models of accretion physics in black hole and neutron star binary systems.

16 ing, carrier field effect mobilities (41 for holes and 80 cm(2) V(-1) s(-1) for electrons) and device

17 ing few- to sub-femtosecond dynamics of both holes and electrons in complex semiconductor materials a

18 ance spectroscopies show that photogenerated holes and electrons in the frameworks have long lifetime

19 Due to the different diffusion lengths of holes and electrons, electron transporting materials (ET

20 n metal oxide radical that localizes surface holes and is required to oxidize water.

21 rom dataloggers placed inside deadwood, tree holes and leaf litter.

22 orated sheets with a dense periodic array of holes and observe that the critical temperature is contr

23 hich can effectively scavenge photogenerated holes and thus enable the color switching of redox dyes

24 (within the sphere of influence of the black hole), and that it can be swept away even at low radiati

25 tage of the jet, closer to its central black hole, and show that the prompt phase is produced via fas

26 The sigma-holes are binding sites for Lewis bases, and binding ene

27 ation of the motors using ultraviolet light, holes are drilled in the cell membranes.

28 rientations (that is, the spins of the black holes are randomly oriented with respect to the orbit of

29 or of the absorbing area was reduced to 28% (hole area: 72%), and it was theoretically maintained eve

30 or of the absorbing area was reduced to 19% (hole area: 81%).

31 otoresist template with well-defined contact hole array was fabricated, to which radio frequency magn

32 pecific heterodimer, guided by the knob-into-hole assembly, proved to be a stable conformation with h

33 insulators can exhibit both strong electron-hole asymmetry and a strong deviation from a linear disp

34 which the activity of the supermassive black hole at the center of the Milky Way, known as Sagittariu

35 When a supermassive black hole at the centre of a galaxy accretes matter, it gives

36 Xs are usually modeled as stellar-mass black holes (BHs) accreting at very high rates or intermediate

37 opposite chiralities in a graphene electron-hole bilayer at moderate magnetic fields.

38 lizing helical states, the graphene electron-hole bilayer can be used to build new 1D systems incorpo

39 onventional monoclonal antibodies, knob-into-hole bispecific antibodies face unique challenges in pro

40 The SAPT analysis shows that the sigma-hole bond between the lambda(3)-iodane and the nucleophi

41 ctral broadening, as observed using spectral hole burning measurements.

42 is a form of steady-state phononic spectral hole burning that produces a wideband transparency windo

43 layer depending on the size of the patterned holes by using a dc approximation method.

44 by the gravitational potential of the black hole; by radiative feedback; or by the interplay between

45 e shape, location, and strength of the sigma-holes can be tuned by the choice of ligands and measures

46 The density of sigma-holes can explain the increasing catalytic activity with

47 monstrate that we can reversibly control the hole carrier density (varying from >10(22) cm(-3) to int

48 render assignments of separate electron and hole carrier dynamics ambiguous.

49 We propose that the hot electron and hole carriers excited via Landau damping (during the pla

50 nabled by visible light photoredox initiated hole catalysis and the in situ Bronsted acid activation

51 effect, leaving a three-dimensional particle-hole channel EEI the most likely physical source.

52 Here we show by means of core-hole clock spectroscopy that SnS2 exhibits spin-dependen

53 ith Pt as an electron collector and WO3 as a hole collector.

54 entional SPECT camera equipped with parallel hole collimators, and hybrid SPECT/CT images were acquir

55 high mobility, two-dimensional electron and hole conducting channels.

56 ling for materials with these levels of pure hole conductivity; the power factor compares favorably w

57 ice performance and stability of the derived hole-conductor-free printable mesoscopic PVSCs.

58 ness, which modulates the effective electron-hole confinement.

59 lls (PSC) are manufactured with a metal-free hole contact based on press-transferred single-walled ca

60 i surface and a compensation of electron and hole contributions.

61 develop a method to measure the electron and hole deformation potentials using coherent acoustic phon

62 s a unique class of isoenergetic wires where hole delocalization mainly occurs via dynamic hopping an

63 system at low temperatures and low electron-hole densities.

64 One more binary black-hole detection and a significant candidate event demonst

65 ers for each of the four likely binary black hole detections GW150914, LVT151012, GW151226 and GW1701

66 ly low electrical conductivity and a limited hole diffusion length that significantly affect the perf

67 rs vdW-DF, Vydrov-Van Voorhis (VV), exchange-hole dipole moment (XDM), Tkatchenko-Scheffler (TS), man

68 pins possessing a stilbenedicarboxamide (Sa) hole donor and stilbenediether (Sd) hole acceptor separa

69 We hole-dope the system away from half-filling, towards a r

70 he magnetic moments mu bare in electron- and hole-doped BaFe2As2.

71 tip-assist, a hidden equilibrium phase in a hole-doped bilayer of Sn on Si(111).

72 ions near (pi, pi) are analogous to those of hole-doped cuprates in several aspects, thus implying th

73 ely resembles the Fermi surface of optimally hole-doped cuprates, including its [Formula: see text] o

74 alogous momentum structure and dispersion to hole-doped cuprates.

75 honon-mediated high-T c superconductivity in hole-doped diamond-like cubic crystalline hydrocarbon K

76 ula: see text] electron shell (Mn compounds, hole-doped FeSCs) and decrease for systems with both hig

77 rature substantially enhances mu bare in the hole-doped region, which is naturally explained by the t

78 w temperature, mu bare is nearly constant in hole-doped samples, whereas it decreases upon electron d

79 pose that the unusual spin-valley locking in hole-doped TMDs together with repulsive interactions sel

80 Meanwhile, hole-doped TMDs with momentum-space-split spinless fermi

81 Specifically, we identify monolayer hole-doped transition metal dichalcogenide (TMD)s as can

82 c correlations via quantum gas microscopy of hole-doped ultracold Fermi-Hubbard chains.

83 The dynamic control over the hole doping density and fluorescence of copper sulfide n

84 s above 80 K at an experimentally accessible hole doping level of only a few percent.

85 Here, ultrafast electron and hole dynamics in germanium nanocrystalline thin films ar

86 ult in novel particle-antiparticle (electron-hole, e-h) pair generation effects, which may be exploit

87 spersive electronic bands, with electron and hole effective masses of 0.53 and 0.85 me, respectively.

88 , which corresponds to the transportation of holes, exhibits a linear dependence on SAW intensity and

89 ith mercaptopropionic acid allows for facile hole extraction from the QD films, resulting in a power

90 HTL's suitable band alignment and excellent hole extraction/collection properties.

91 al studies have difficulty growing the black hole fast enough.

92 re (high-T c) superconductors, which have no hole Fermi pockets, but have a notably high T c, have ch

93 We find a large hole Fermi surface that closely resembles the Fermi surf

94 g its [Formula: see text] orbital character, hole filling level, and strength of electronic correlati

95 into the environments in which binary black holes form.

96 report numerical simulations of early black hole formation starting from realistic cosmological cond

97 ransition state is stabilized by an oxyanion hole formed by the backbone amides of Ala102 and Leu186.

98 We also detected a 100 fs migration of holes from higher- to lower-energy sites, consistent wit

99 current age-reinforces models of early black-hole growth that allow black holes with initial masses o

100 is properly rearranged leading to the heavy-hole (HH) miniband being the top valence subband, which

101 ational destabilization and refolding of the hole-hole homodimer Fc.

102 Compared with the hole-hole homodimer under different storage conditions,

103 hy (HIC) profile change was observed for the hole-hole homodimer, and the multiple HIC peaks were exp

104 croscopy to comprehensively characterize the hole-hole homodimer.

105 Protein-based "hole" hopping typically involves spatially arranged redo

106 spectroscopies show that CuZ degrees is a 1-hole (i.e., 3Cu(I)Cu(II)) state with spin density deloca

107 s is a consequence of the formation of sigma-holes, i.e., maxima in the surface electrostatic potenti

108 been placed on the mass of a putative black hole in 47 Tucanae (NGC 104) from radio and X-ray observ

109 e show there is evidence for a central black hole in 47 Tucanae with a mass of solar masses when the

110 itons, the bound states of an electron and a hole in a solid material, play a key role in the optical

111 ed electron in an NO pi* orbital or electron hole in an Fe dpi orbital.

112 The existence of an intermediate-mass black hole in the centre of one of the densest clusters with n

113 Our project has patched the hole in the genetic map of Eurasia: we demonstrated comp

114 ectra of states in CS2 and SF6 with a double hole in the K-shell and one electron exited to a normall

115 skills are useful in combination and fill a hole in the labor market.

116 show formation of a reinforced circular port-hole in the prey wall, L,D-transpeptidaseBd-mediated D-a

117 the first direct detection of merging black holes in 2015, the era of gravitational wave (GW) astrop

118 Specifically, whereas photogenerated holes in Cu(+):CdSe NCs localize primarily in Cu(3d) orb

119 lts further suggest that at low temperatures holes in deep ground states are localized on N atoms axi

120 directly through the endothelium by opening holes in endothelial cells, known as transcellular tunne

121 this hypothesis by analyzing predatory drill holes in fossil marine shells, which provide a 500-mill

122 lack holes that grow into supermassive black holes in galaxies.

123 between 80 and 100% of the deep valence-band holes in graphene are filled via an Auger transition.

124 y hemostasis by forming aggregates that plug holes in injured vessels.

125 Laser engraving and holes in PMMA along with spacing from surface provide fl

126 scopy to image the dynamics of electrons and holes in silicon after excitation with a short laser pul

127 at a prophage-encoded endolysin can generate holes in the cell wall through which cytoplasmic membran

128 p is the process by which supermassive black holes in the centres of galaxies may moderate the growth

129 The origin of super-massive black holes in the early universe remains poorly understood.

130 oulomb interaction between the electrons and holes in the molecular bridge, so-called exciton-binding

131 to recruit additional ESCRT-III proteins to holes in the nuclear membrane.

132 lysin in a sub-population of cells generates holes in the peptidoglycan cell wall.

133 majority of the accreting supermassive black holes in the Universe are obscured by large columns of g

134 Auger processes involving the filling of holes in the valence band are thought to make important

135 er graphene as a result of the decay of deep holes in the valence band.

136 The metallic NWs can act as an efficient hole injection layer on top of 2H-MoTe2 due to favorable

137 on process during the thermal annealing, the hole-injection-assisted reactions happen at selective mo

138 from quasi-freestanding polymers assisted by hole injections from a scanning tunnelling microscope (S

139 In halogen compounds, sigma-hole interaction was identified as a force in crystal pa

140 amical Mean Field Theory, including the core-hole interaction.

141 ysicochemical origins of this class of sigma-hole interaction.

142 More recently, sigma-hole interactions were also shown to affect the reactivi

143 y weakly covalent and can be viewed as sigma-hole interactions, similar to those encountered in halog

144 complexes can be described by means of sigma-hole interactions.

145 s capable of initiating etching by injecting holes into the semiconductor valence band.

146 ces between pre-edge states near single core holes investigated in X-ray absorption spectra and the c

147 ithin a few gravitational radii of the black hole ionizing the disk wind hundreds of gravitational ra

148 ty change is delocalized when an electron or hole is added.

149 magnetic counterpart suggests that the black hole is not accreting at a sufficient rate to make it el

150 er, the existence of intermediate-mass black holes is still uncertain, and their formation process is

151 ates and the more complex (and less studied) hole-like states in a high-mobility two-dimensional elec

152 Hole-like states, which have fractional Landau-level fil

153 S at which the large Fermi surface goes from hole-like to electron-like, so that p* </= p FS.

154 e of tools for quick assessment, sorting and hole masking of electron micrographs.

155 times the luminosity of the Sun and a black-hole mass of 8 x 10(8) solar masses.

156 Pd17 Al69 provides an example of an electron-hole matching approach to inducing frustration in interm

157 The electron-hole matching approach's ability to combine structural c

158 proving the connection between binary black hole mergers and active galactic nuclei as hosts, even i

159 iscovered with the detection of binary black-hole mergers and they should also be detectable from low

160 ational waves from stellar-mass binary black hole mergers by the Laser Interferometer Gravitational-w

161 binary black hole observations.Binary black hole mergers have recently been observed through the det

162 Probing the origin of binary black hole mergers will be difficult due to the expected lack

163 Idiopathic macular holes (MHs) are a cause of decreased vision among older

164 This intermediate-mass black hole might be a member of an electromagnetically invisib

165 separation ) with minimized influence on the hole-migration property of TiO2 photoelectrodes, leading

166 Our results reveal high electron and hole mobilities of 2,800 and 9,400 cm(2) V(-1) s(-1), re

167 an enable good semiconducting materials with hole mobilities ranging from approximately 0.03 to 1.7 c

168 F2,3 counterpart, consistent with the higher hole mobilities.

169 ,6 achieved the highest average field-effect hole mobility (5.1 cm(2) V(-1) s(-1)).

170 sponse, well-matched energy levels, and high hole mobility from optimized BHJ morphology afford a ver

171 The hole mobility is enhanced by 25 times to 227 cm(2)V(-1)s

172 Alloying also increases the hole mobility to 560 cm(2) V(-1) s(-1), yielding a high

173 with the CPDS and IDSe copolymers exhibiting hole mobility up to 0.15 and 6.4 cm(2) V(-1) s(-1), resp

174 atic contribution is reflected in the 'sigma hole' model in which a positive patch on E attracts the

175 We acquired repeated down hole MS logging data in boreholes at a HC-contaminated f

176 hemorrhage (n = 40), full-thickness macular hole (n = 33), recurrent proliferative vitreoretinopathy

177 The same infusion rates given through 1 end hole (n=6) or in the contralateral artery (n=6) did not

178 t a viscoelastic model of the evolution of a hole nucleated by deformations of the nuclear lamina and

179 trophysical questions probed by binary black hole observations.Binary black hole mergers have recentl

180 well-suited for directly observing transient hole occupation during charge transport between a stilbe

181 dy of the temporal-evolution of the electron-hole occupation number of the excited states of the QDs

182 olaron states, in which two electrons or two holes occupy a single molecule or conjugated polymer seg

183 Newly formed black holes of stellar mass launch collimated outflows (jets)

184 The halogen bond formed between the sigma-hole on bromobenzene (BrPh) and the lone pair(s) of Pz s

185 Holes on Co3O4 recombined with electrons of the reduced

186 med by trapping photogenerated, valence band holes on different reactive sites of the oxide surface.

187 rough hundreds of millions of nanoscale vent holes on each chip by gas-phase Xenon difluoride etching

188 on is second order in the density of surface holes on hematite and independent of the applied potenti

189 rrelation contributions and the localized pi holes on their surface promise unique selectivities.

190 atomic resolution, which reveals an unusual "hole" on the surface, surrounded by five encephalitic-sp

191 lts in rapid injection of the photogenerated hole onto the molecular wire and concurrent formation of

192 ravitational waves from merging binary black holes opens up a window into the environments in which b

193 all energy isosurfaces, electron velocities, hole or electron conductivity, effective mass and inner

194 Whether the sigma hole or n-->sigma* model applies, any octet expansion is

195 f binary stars containing an accreting black hole or neutron star often show x-ray emission extending

196 patients developed a full-thickness macular hole or required surgical intervention for symptoms.

197 ing in Fe-rich conditions, can generate free holes (p-type doping), while the replacement of Fe(2+) b

198 Electron-hole pairing can occur in a dilute semimetal, transformi

199 on of excited electronic states and electron-hole pairs (excitons) at molecular interfaces and addres

200 When electron-hole pairs are excited in a semiconductor, it is a prior

201 applications, where photogenerated electron-hole pairs are exploited to induce catalysis.

202 f the emergence of local patches of particle-hole pairs generated by SU(2) symmetry fluctuations.

203 We demonstrate that photogenerated electron-hole pairs give rise to a stable anodic photocurrent who

204 her on photocurrent generation from electron-hole pairs in semiconductor structures or on bolometry f

205 rge motion may be key to separating electron-hole pairs into free charges against the Coulomb interac

206 ped region, and the photo-generated electron-hole pairs need to diffuse into the junction region, res

207 based on the Stark effect caused by electron-hole pairs photo-generated across the interface.

208 n such a way that the generation of electron-hole pairs under illumination relative to the total Cr c

209 Instead, the creation of electron/hole pairs was considered to be the mechanism that drove

210 Excitons, Coulomb-bound electron-hole pairs, are elementary photo-excitations in semicond

211 tions evolve into Coulomb-bound electron and hole pairs, called excitons, and unbound charge carriers

212 ng on the spin configuration of the electron-hole pairs, intra-valley excitons of TMD monolayers can

213 ns that can be used to generate two electron-hole pairs, leading to a predicted approximately 50% enh

214 harge-separated states comprised of electron-hole pairs.

215 able SAW phononic crystals, based on annular holes patterned in a SAW substrate.

216 Longer than 1 ns lifetimes for holes photoexcited to the lower valence subband offer a

217 two-photon absorption induced Drude electron-hole plasma.

218 antibacterial activity was evaluated by the hole plate and MIC techniques and the antimutagenic acti

219 iron pnictides containing both electron and hole pockets.

220 emerge at the boundary between electron and hole pockets.

221 f CH3 domain dimerization (due to the three "hole" point mutations), resulting in a unique storage- a

222 otostimulated excitations, e.g., electron or hole polaronic trap states, can be studied using IR-spec

223 ly lifted in the valence band, spreading the hole population among several states at room temperature

224 ets (both pristine and oxidized) can produce holes (pores) in the membranes of A549 and Raw264.7 cell

225 The Electron Microscopy Hole Punch (EMHP) is a streamlined suite of tools for qu

226 e orbital symmetry conservation rules favour hole rather than electron injections for the GNR formati

227 rks, and the presence or absence of electron/hole recombination centers.

228 thermore, we find that second-order electron-hole recombination of photo-excited charges is retarded

229 Stokes photon emission generated by electron-hole recombination within quartz or feldspar; it relies,

230 poxic conditions via N3-facilitated electron-hole reduction of adsorbed water molecules.

231 the tuning transforms the nonclassical sigma-hole regions into coordination sites, which allows us to

232 Separate electron and hole relaxation times are observed as a function of hot

233 Clogging of 150 mum diameter leak holes represented by glass capillary tubes, in recircula

234 ), retinal vein occlusion (RR 12.9), macular hole (RR 7.7), and epiretinal membrane (RR 5.7).

235 citation, together with spontaneous electron-hole separation and charge trapping induced by the atomi

236 co-doped graphitic sheets with stereoscopic holes (SHG) act as effective tri-functional catalysts fo

237 ong modern drilling predators and that drill-hole size (and thus inferred predator size and power) ro

238 We show that drill-hole size is a robust predictor of body size among moder

239 y symbiosis-related trait, domatium entrance hole size, which filters symbionts by size.

240 ition metal oxide nanosheets with adjustable hole sizes that enable greatly enhanced alkali-ion stora

241 report that, if the magnitudes of the black hole spins are allowed to extend to high values, the eff

242 nts is the angular distribution of the black hole spins.

243 dicals with varying dihedral angles that the hole stabilization shows two different regimes where the

244 different regimes where the mechanism of the hole stabilization switches over from (static) delocaliz

245 and NC calculations shows that the confined hole state is exclusive to NCs.

246 nd the corresponding states near double core holes studied here are brought out.

247 non drag contributions are essential for the hole surface carriers.

248 The particle-hole symmetry characteristic to the BDI symmetry class s

249 to the cyclotron gap in a Ge two-dimensional hole system increases with decreasing density owing to i

250 and radio observations of the Galactic black hole system V404 Cygni, showing a rapid synchrotron cool

251 within the molecule, which refills the core holes that are created in the heavy atom, providing furt

252 -third of trees through the creation of tree holes that are now used, presumably as predation or ther

253 ed of application of rodenticide, sealing of holes that could serve as entry points for mice, trap pl

254 romagnetically invisible population of black holes that grow into supermassive black holes in galaxie

255 velength survey of hard-X-ray-selected black holes that reveals that radiative feedback on dusty gas

256 ctron following transfer of the photoexcited hole to Ag(+).

257 uced, self-healing mechanisms that allow the hole to be closed after the deformation-induced strains

258 Forward transfer of the hole to Co3O4 catalyst proceeds in 255 +/- 23 ps.

259 preventing AA from scavenging photogenerated holes to the photoactive modified electrode.

260 bstituents can be utilized to accelerate the hole transfer (HT) between redox sites attached in para-

261 The unusually efficient hole transfer coupling of a molecular light absorber wit

262 The mechanism of visible light-induced hole transfer from a molecular light absorber, in the fo

263 1.03+/-0.09 ns(-1) respectively), ultrafast hole transfer occurs only from PbS QDs to 5-CT.

264 A(*+) pKa results in DNA damage arising from hole transfer.

265 60.3+/-6.1 % to 71.8+/-6.2 % by suppressing hole transfer.

266 was investigated for an evaluation of direct hole-transfer between the enzyme and electrode at a bio-

267 ology and kinetics of ITIC --> donor polymer hole-transfer in boosting the performance of polymer:ITI

268 Hole-transfer is observed from ITIC to PBTI3T and PBTSA3

269 s in proteins and on functional and aberrant hole-transfer reactions in metallo-enzymes.

270 tion by a factor of 1.6, by facilitating the hole-transfer step.

271 The hole transport dynamics of DNA hairpins possessing a sti

272 Deuteration of the PEDOT:PSS hole transport layer results in a behavior that is inter

273 s a shallow hole trap, or as an intermediate hole transport site when a deeper trap state is present.

274 of tens of micrometers are directly grown on hole-transport-layer covered substrates by a hydrophobic

275 Developing dopant-free hole transporting layers (HTLs) is critical in achieving

276 assivates voids or pinholes generated in the hole-transporting layer.

277 has been further converted to blue-emissive hole-transporting material via a simple chemical transfo

278 up the entire class of organics as scalable hole-transporting materials for perovskite solar cells.

279 This series includes (i) semicrystalline hole-transporting P3HT, (ii) semicrystalline electron-tr

280 -transporting N2200, (iii) low-crystallinity hole-transporting PBDTT-FTTE, and (iv) low-crystallinity

281 conduit for positive charge rather than as a hole trap when inserted into a duplex, as previously pos

282 ploying EG, we observe its role as a shallow hole trap, or as an intermediate hole transport site whe

283 nt absorption measurements, we conclude that hole-trap filling in the arms and partial state-filling

284 The more probable involves hole tunneling by superexchange, which rationalizes the

285 itons that are split into free electrons and holes using heterojunctions of electron donor and accept

286 tor motif to spatially separate electron and hole wave functions.

287 investigation also reveals that the electron-hole wavefunction overlaps are remarkably large in the I

288 hermore, our study reveals that the electron-hole wavefunction overlaps in the AlN/GaN DA structure c

289 FT was found increased, and diameters of the hole were found reduced since the first month after oper

290 y control the buckling direction, masks with holes were used to guide site-specific swelling of the h

291 The existence of this supermassive black hole when the Universe was only 690 million years old-ju

292 y chalcogen atoms contain Lewis acidic sigma-holes which are able to form attractive supramolecular i

293 swelling of the high-swelling gel under the holes, which built a transient through-thickness gradien

294 Dodecagonal holes with a diameter of approximate 5.8 A are regularly

295 By laser-perforating holes with different sizes and spacings in the electrosp

296 he simultaneous observation of electrons and holes with extreme ultraviolet transient absorption spec

297 of early black-hole growth that allow black holes with initial masses of more than about 10(4) solar

298 It has long been suspected that black holes with masses 100 to 10,000 times that of the Sun sh

299 iased and complete sample of accreting black holes, with reliable information on gas column density,

300 parsecs of the accreting supermassive black hole (within the sphere of influence of the black hole),