ライフサイエンスコーパス: gravitational

1 while confinement in the third dimension is gravitational.

2 Cancelling gravitational acceleration (for example, in atomtronic c

3 lity to measure tiny variations in the local gravitational acceleration allows, besides other applica

4 hem to isolate the signature of the changing gravitational acceleration as the rover climbs through G

5 u is the fluid's dynamic viscosity, g is the gravitational acceleration, and [Formula: see text] is a

6 and otolith signals to segregate linear and gravitational acceleration, evidence for how the cerebel

7 ed mice continues to distinguish linear from gravitational acceleration, suggesting that the underlyi

8 e g approximately 9.8 m/s(2) is the standard gravitational acceleration.

9 ight is given by Newton's laws as mass times gravitational acceleration.

10 s in the Universe and are formed through the gravitational accretion of matter over cosmic time(1).

11 ts of the equivalence principle, measure the gravitational Aharonov-Bohm effect, and eventually detec

12 has been traditionally described using only gravitational and frictional forces within a granular ma

13 rrent direct bounds on the ratio between the gravitational and inertial masses of the antihydrogen do

14 bound of 0.13% on the difference between the gravitational and inertial masses of the positron (antie

15 hypothesis, based on the comparison between gravitational and lobar perfusion data, perfusion was no

16 account for the effects of a distinct, axial-gravitational anomaly expected to be present in Weyl sem

17 However, the presence of a mixed gauge-gravitational anomaly has recently been tied to thermoel

18 mbalance, an effect known as the mixed axial-gravitational anomaly, but this anomaly has yet to be co

19 imentally accessible signature of this axial-gravitational anomaly, even beyond the hydrodynamic limi

20 onsistent with the presence of a mixed axial-gravitational anomaly, providing clear evidence for a th

21 pant used a motorised mobile arm support for gravitational assistance and to provide humeral abductio

22 xes of high adaptive relevance: the body and gravitational axes.

23 nd to arise from a complex interplay between gravitational, bending, and twisting energies of the rod

24 These results show that mapping where gravitational body forces encourage seismicity is crucia

25 Gravitational, centrifugal, thermal gradient, magnetic,

26 loration of adaptation of mammalian cells to gravitational changes.

27 Gravitational collapse of a massive primordial gas cloud

28 The early star that is born from the gravitational collapse of a molecular cloud reaches at s

29 ears old) massive clump, forming through the gravitational collapse of more than one billion solar ma

30 assed, viscous magma and may be destroyed by gravitational collapse or explosion.

31 rbed a cloud of gas and dust, triggering the gravitational collapse that led to the formation of the

32 Unbound planets can also be formed through gravitational collapse, in a way similar to that in whic

33 hat was not maintained because of subsequent gravitational collapse.

34 eir near-equilibrium behavior in a tilted 2D gravitational column.

35 ase with increasing radius, likely caused by gravitational compression.

36 of creating such conditions under the normal gravitational condition does not exist.

37 lance enabled the first determination of the gravitational constant by Henri Cavendish(1) and the dis

38 ack hole (the gravitational radius being the gravitational constant multiplied by the object mass, di

39 Here we present data from gravitational cores collected along the NW Iberian Margi

40 viability time of large oocytes, suggesting gravitational creep ages oocytes, with fatal consequence

41 kinetically stabilizes them by slowing down gravitational creep to ~2 months.

42 This observation suggests the brain takes gravitational cues to automatically update threat value

43 hat this vertical asymmetry is determined by gravitational cues: the probability that a threat will h

44 Gravitational deflection of starlight around the Sun dur

45 ice sheets is strongly nonuniform, owing to gravitational, deformational and Earth rotational effect

46 s of CPT (charge-parity-time) invariance) or gravitational differences (tests of the weak equivalence

47 e or transmural pressure distribution in the gravitational direction are implicated in the redistribu

48 s imparted through the ice column, including gravitational driving stress.

49 tric binary orbits can be used to study both gravitational dynamics and binary evolution.

50 aporation remains almost unchanged, as if no gravitational effect is present.

51 Being ideal, gravitational effects due to these clocks are ignored an

52 ed as a new technique for characterizing the gravitational effects of mutual planetary perturbations

53 urbation forces (e.g., Earth's geopotential, gravitational effects of the sun and moon, and solar rad

54 Gravitational effects on invertebrate cardiovascular and

55 xplain astronomical observations through its gravitational effects on stars and galaxies, gravitation

56 e oil and then dried horizontally, such that gravitational effects were excluded.

57 rom Keplerian orbits (that is, unaffected by gravitational effects) implied by the observed transit t

58 the expanding gas was able to lose internal gravitational energy and collapse to form stellar object

59 oling is further slowed by the liberation of gravitational energy from element sedimentation in the c

60 he cellular capacity for adaptation to a new gravitational environment.

61 of gravity to cope with life in the Earth's gravitational environment.

62 imetres per second, which corresponds to the gravitational escape velocity of kilometre-sized asteroi

63 fine water vapour to lower altitudes through gravitational fall and subsequent sublimation of ice cry

64 Therefore, it is possible to detect gravitational Faraday rotation by monitoring the X-ray p

65 The effect of gravitational Faraday rotation was predicted in the 1950

66 adjust their swimming motion relative to the gravitational field and thus counteract sedimentation to

67 Gravitational field measurements suggest a regional sout

68 ratory (GRAIL) spacecraft to investigate the gravitational field of Orientale at 3- to 5-kilometer (k

69 The gravitational field of the outer white dwarf strongly ac

70 nk with Earth was monitored to determine the gravitational field of the planet and the mass of its ri

71 ng wave energy flux and the work done by the gravitational field on the sources.

72 luence of body orientation with respect to a gravitational field on total escape probability, but a s

73 e measure hand tremor at different levels of gravitational field strength using a human centrifuge, t

74 ty is inferred from the measured decrease in gravitational field strength with elevation.

75 a human centrifuge to increase head-to-foot gravitational field strength, we were able to control fo

76 vided an accurate determination of Jupiter's gravitational field(2), which has been used to obtain in

77 amo is to measure its effect on the external gravitational field, a task to be soon undertaken by the

78 e ("uniqueness of free fall") in the Earth's gravitational field, obtained with three laser-ranged sa

79 We present gravitational field-flow fractionation and hydrodynamic

80 ves but by the speed-of-light changes of the gravitational field.

81 for the necessity of the quantisation of the gravitational field.

82 errogation time of freely falling atoms in a gravitational field.

83 nd during exposure to experimentally altered gravitational fields, 0 g and +1.8 g during parabolic fl

84 Gravimetry, the precise measurement of gravitational fields, can be used to probe the internal

85 ically cold orbits that enhanced the Earth's gravitational focusing factor(2), and the 'sawtooth' imp

86 h variation plays the role of the artificial gravitational force acting on a massive particle: excito

87 nimals have longer urethras and thus, higher gravitational force and higher flow speed.

88 e., where the direction of magnetization and gravitational force are parallel) cannot resolve differe

89 e., where the direction of magnetization and gravitational force are perpendicular) relative to the s

90 ls and step-wise increase or decrease of the gravitational force in four independent experiments.

91 For micrometer-sized colloids, however, the gravitational force is too small to produce significant

92 The role of gravitational force on colloid transport in water-satura

93 surface wave is likely driven by lunar tidal gravitational force.

94 Gravitational forces also cause creep displacement of nu

95 Gravitational forces are expected to excite spiral densi

96 ement of the solid Earth's surface caused by gravitational forces from the Moon and the Sun-is sensit

97 Gravitational forces in multiple star systems can disrup

98 -element models subjected to extensional and gravitational forces to study time-varying deformation a

99 the rarity of antimatter and weakness of the gravitational forces, the WEP has never been confirmed f

100 s inherent to extreme aviation, such as high gravitational forces.

101 In this posture, the gravitational gradient along the body is different than

102 g contributions from large blood vessels and gravitational gradients (all P < 0.05).

103 Fontan palliation, remodelling, or increased gravitational gradients from low flow.

104 pulmonary arterial hypertension (PAH), where gravitational gradients may be reduced secondary to high

105 3.98 +/- 0.91, P = 0.26), and the slopes of gravitational gradients were not different (Fontan = -0.

106 Gravitational gradients were similar between all groups,

107 explained by differences in mean perfusion, gravitational gradients, or large vessel anatomy.

108 xplainable by differences in mean perfusion, gravitational gradients, or large vessel anatomy.

109 sed by the relative dispersion (SD/mean) and gravitational gradients.

110 g contributions from large blood vessels and gravitational gradients.

111 tly, the visual horizon can be replaced by a gravitational horizon to inform the observed horizontal

112 for the existence of dark matter through its gravitational impact is clear in astronomical observatio

113 d a mixed sensitivity to head rotational and gravitational information and were differentially modula

114 Here, we report the discovery of a family of gravitational instabilities in granular particle mixture

115 clumps, which are thought to form by violent gravitational instabilities in highly turbulent gas-rich

116 density that can cause Rayleigh-Taylor-type gravitational instabilities.

117 as channeling mechanism also generates other gravitational instabilities: the rise of a granular bubb

118 rotostellar disk that has recently undergone gravitational instability, spawning one or two companion

119 tation of a massive protostellar disk due to gravitational instability.

120 relativistic mass-energy equivalence implies gravitational interaction between the clocks, whereas th

121 We demonstrate that gravitational interaction between the planet and its obl

122 The gravitational interaction of dust in the zodiacal cloud

123 te-of-the-art constraints on deviations from gravitational interaction, whether provided by neutron s

124 Strong gravitational interactions are apparent and provide the

125 the transits are measurably affected by the gravitational interactions between neighbouring planets.

126 of the planet is most probably the result of gravitational interactions, indicating the presence of a

127 Accurate analysis of a single gravitational lens can take up to a few weeks and requir

128 ght traversed multiple paths around a strong gravitational lens could be used to measure the rate of

129 atter distribution of these structures (the 'gravitational lens') has primarily been performed using

130 use the angular diameter distance to strong gravitational lenses as a suitable calibrator, which is

131 ermine the angular diameter distances to two gravitational lenses, [Formula: see text] and [Formula:

132 Gravitational lensing and dynamical perturbations of tid

133 Observations of gravitational lensing are used to characterize the prope

134 The gravitational lensing magnification shows how ionizing p

135 gravitational effects on stars and galaxies, gravitational lensing of light around these, and through

136 Magnification from gravitational lensing offers an opportunity to resolve t

137 f the large-scale structure in the universe, gravitational lensing, and the cosmic microwave backgrou

138 antifying image distortions caused by strong gravitational lensing-the formation of multiple images o

139 is typical in other studies of extragalactic gravitational lensing.

140 s to changes in the prosthesis mechanics and gravitational load.

141 l motor controller mimicked in vivo inertial/gravitational loading experienced by muscles during terr

142 asis can be modulated by muscle activity and gravitational loading.

143 By modeling the pulse as gravitational magnification (microlensing) along with Ke

144 Gravitational microlensing is the only method capable of

145 Using gravitational microlensing, we detected a cold terrestri

146 e = -0.137(0.167)) and increased nDNP in the gravitational middle lung [+500 ml = 0.098(0.058), +1 li

147 ed for accurately differentiating linear and gravitational movements through a conditional genetic si

148 an be used to shed new light on inaccessible gravitational objects.

149 g waves of any nature (e.g. electromagnetic, gravitational or acoustic), BISER provides a novel frame

150 Near the top of the column where the 2D gravitational osmotic pressure Pi(2D) is low, we observe

151 traps, we found 2 to 3 times higher rates of gravitational particle export near a deep-water front (3

152 brightness asymmetries that may result from gravitational perturbation by planets.

153 ed Lidov-Kozai migration mechanism, in which gravitational perturbations from a distant tertiary comp

154 is ring around the star without the expected gravitational perturbations.

155 re from the cosmic expansion and arises from gravitational perturbations; a map of peculiar velocitie

156 Many gravitational phenomena that lie at the core of our unde

157 The gravitational point mass is GM = 666.2 +/- 0.2 cubic met

158 itored airborne pollen, year- round, using a gravitational pollen sampler (Durham's sampler), at more

159 ne pollen all year around since July 1986 by gravitational pollen sampler, Durham's sampler, at more

160 During VVS, gravitational pooling excessively reduces central blood

161 The cluster's gravitational potential also creates multiple images of

162 Published geodynamic models, incorporating gravitational potential energy and tractions from plate

163 After seconds of hold time, gravitational potential energy differences from as littl

164 A model minimizing the combined strain and gravitational potential energy explains the propagation

165 to seismogenic intraplate deformation, while gravitational potential energy variations have a minor r

166 , producing bursts powered by the release of gravitational potential energy.

167 mulations and analytical models suggest that gravitational potential fluctuations tied to efficient s

168 ark matter through a coupling based on rapid gravitational potential fluctuations, explaining the obs

169 ate passing through different regions of the gravitational potential of Earth.

170 arises from the sublimation of dust; by the gravitational potential of the black hole; by radiative

171 Our approach allows gravitational potentials to be measured by holding, rath

172 ophysical sources and the nature of absolute gravitational potentials.

173 e origin time, implying that shaking induced gravitational processes were not the primary driving mec

174 serves as a confirmation of the conventional gravitational properties of antimatter without common as

175 This gas has been heated up by the cluster's gravitational pull and is now feeding its core.

176 ps' probably sequester as much carbon as the gravitational pump, helping to close the carbon budget a

177 TF J153932.16+502738.8 is a strong source of gravitational radiation close to the peak of LISA's sens

178 period binaries emit considerable amounts of gravitational radiation.

179 lack holes is truncated at a few hundreds of gravitational radii from the black hole(17,18).

180 he emission originates within three or fewer gravitational radii from the black hole, implying a spin

181 the speed of light) disk winds a few hundred gravitational radii from the black hole.

182 lack hole ionizing the disk wind hundreds of gravitational radii further away as the X-ray flux rises

183 g the fastest infalling gas to within 10,000 gravitational radii of the black hole (the gravitational

184 scales: the X-ray emission from within a few gravitational radii of the black hole ionizing the disk

185 istance of the inflow of approximately 1,000 gravitational radii, possibly overlapping with the outer

186 ecting the jets within the inner few hundred gravitational radii.

187 0 gravitational radii of the black hole (the gravitational radius being the gravitational constant mu

188 mission region to be smaller than 20% of the gravitational radius of its central black hole.

189 pinning top shape, can form directly through gravitational reaccumulation.

190 ed a combination of special relativistic and gravitational redshift, quantified using the redshift pa

191 represents scene structure aligned with the gravitational reference frame in which objects move and

192 Data were evaluated across gravitational regions (dependent, middle, non-dependent)

193 gas and blood volume fractions within three gravitational regions calculated and normalized to lung

194 rved space-through local electromagnetic and gravitational responses of the bulk material.

195 Gravitational scattering of planetesimals towards the wh

196 of PAA-nano-ZVI aggregates doubled, inducing gravitational sedimentation and possibly straining as me

197 A 5-10min period of quiescence allows for gravitational sedimentation of the red blood cells, leav

198 melt mobility, which is high and can lead to gravitational segregation.

199 ication of the Schrodinger equation due to a gravitational self-interaction.

200 ich reveal depth-proportional signals set by gravitational settling in soil air at the time of rechar

201 he deep ocean and is thought to function via gravitational settling of organic particles from surface

202 rt owing to a variety of processes including gravitational settling, attachment to in-stream structur

203 acteria-Fe aggregates that can be removed by gravitational settling.

204 This is a universally predictable gravitational signal that requires both high sensitivity

205 We calculate the gravitational signature of non-axisymmetric convective m

206 Enhanced vertical carbon transport (gravitational sinking and subduction) at mesoscale ocean

207 is at 3 kiloparsecs), which is far from the gravitational sphere of influence (about 100 parsecs for

208 galaxies extends over the same radius as the gravitational sphere of influence of the central black h

209 t organs in different species in response to gravitational stimuli.

210 at we are possibly witnessing the effects of gravitational stirring due to the orbital evolution of h

211 d after prolonged space-flight where lack of gravitational stress prevents daily lowering of ICP asso

212 ompressive tectonic stresses to near-surface gravitational stresses is relatively large, and it paral

213 Such a gravitational-sweep sedimentation approach has previousl

214 , which reveals analogies with, for example, gravitational systems, and establishes a new scenario th

215 foundation of General Relativity and of most gravitational theories.

216 e from the asteroid belt and drifted via non-gravitational thermal forces into resonant escape routes

217 m the interplay of different forms of energy-gravitational, thermal, magnetic and radiative.

218 a variety of altered AF patterns, including gravitational tracts, extended beyond the posterior 50 d

219 Here, we study an alternative magneto-gravitational trap for diamagnetic particles, such as di

220 ertia, which requires the measurement of its gravitational variation together with either precession

221 Tilting the MagLev device relative to the gravitational vector enables the magnetic force to be de

222 ne of four head/body positions orienting the gravitational vector parallel or orthogonal to the EVS r

223 ocentric coordinates defined relative to the gravitational vector.

224 n of merging black holes in 2015, the era of gravitational wave (GW) astrophysics began.

225 The standard siren approach of gravitational wave cosmology appeals to the direct lumin

226 Although the gravitational wave data indicate that GW170817 is consis

227 d sensing capabilities in areas ranging from gravitational wave detection to biomedical applications.

228 the moment of inertia, break degeneracies in gravitational wave detection to measure spin in binary i

229 ents ranging from atomic force microscopy to gravitational wave detection.

230 telescope is expected to produce 10(4)-10(5) gravitational wave detections per year, 50-100 of which

231 ortant components of devices that range from gravitational wave detectors to cellular telephones.

232 nology, from the antennas of interferometric gravitational wave detectors to chip-scale quantum micro

233 detect the decay of the binary orbit due to gravitational wave emission by observing two tidal disru

234 tical counterpart of the binary neutron star gravitational wave event GW170817.

235 t observational constraint for low-frequency gravitational wave experiments.

236 binary neutron star merger, reinforcing the gravitational wave result.

237 ly measured time delays from strongly lensed gravitational wave signals with the images and redshifts

238 ently been observed through the detection of gravitational wave signatures.

239 Eleven hours after the detection of gravitational wave source GW170817 by the Laser Interfer

240 Through their detection via follow-up of gravitational-wave (GW), short gamma-ray bursts (sGRBs)

241 we review the history and accomplishments of gravitational-wave astronomy and look towards the future

242 Since then, gravitational-wave astronomy has enabled tests of the na

243 As this nascent field of gravitational-wave astrophysics is emerging we are looki

244 GW170817 was the first gravitational-wave detection of a binary neutron-star me

245 l laws of physics(21-23), geodesy(24-26) and gravitational-wave detection(27).

246 Once at design sensitivity, the gravitational-wave detectors Advanced LIGO(2), VIRGO(3)

247 eral proposals to improve the sensitivity of gravitational-wave detectors by mitigating QRPN(5-10), b

248 overy of the neutron-star merger GW170817 by gravitational-wave detectors(10)-was the first kilonova

249 In interferometric gravitational-wave detectors, higher laser powers reduce

250 ve the sensitivity of the next generation of gravitational-wave detectors.

251 room temperature at frequencies relevant to gravitational-wave detectors.

252 e aim of improving the sensitivity of future gravitational-wave detectors.

253 n [Formula: see text] million years owing to gravitational-wave emission.

254 We performed a joint analysis of the gravitational-wave event GW170817 with its electromagnet

255 robustly inferred from the detection of the gravitational-wave event GW170817.

256 orted by multimessenger observations(1-3) of gravitational-wave event GW170817: this production route

257 unterparts AT2017gfo and GRB170817A, and the gravitational-wave event GW190425, both originating from

258 y confirmed electromagnetic counterpart to a gravitational-wave event(1,2).

259 e properties of subsequent binary-black-hole gravitational-wave events.

260 Gravitational-wave experiments have detected black holes

261 r masses once second-generation ground-based gravitational-wave observatories reach full sensitivity.

262 On 17 August 2017, the Laser Interferometer Gravitational-Wave Observatory (LIGO) and the Virgo inte

263 l waves by the Advanced Laser Interferometer Gravitational-Wave Observatory (LIGO) detectors.

264 turally produced in the Laser Interferometer Gravitational-wave Observatory (LIGO).

265 source GW170817 by the Laser Interferometer Gravitational-Wave Observatory and Virgo Interferometers

266 ack hole mergers by the Laser Interferometer Gravitational-wave Observatory opened the door to altern

267 le phenomena: a short burst of gamma-rays, a gravitational-wave signal, and a transient optical-near-

268 ies of a bright kilonova associated with the gravitational-wave source GW170817 and gamma-ray burst G

269 The gravitational-wave source GW170817 arose from a binary n

270 ery of an electromagnetic counterpart to the gravitational-wave source GW170817 represents the first

271 ramework within which to interpret the first gravitational-wave source, GW150914, and to predict the

272 electromagnetic counterpart (EM170817) with gravitational waves (GW170817) detected from merging neu

273 (LIGO) and the Virgo interferometer detected gravitational waves (GWs) emanating from a binary neutro

274 Gravitational waves (GWs) from binary neutron stars enco

275 On 17 August 2017, gravitational waves (GWs) were detected from a binary ne

276 mergers with distinct messengers, including gravitational waves and electromagnetic signals, can be

277 Aharonov-Bohm effect, and eventually detect gravitational waves and phase shifts associated with gen

278 indicates that neutron-star mergers produce gravitational waves and radioactively powered kilonovae,

279 Gravitational waves are expected to be radiated by super

280 September 14, 2015, with direct detection of gravitational waves by the Advanced Laser Interferometer

281 rates and properties(14,15) of the resulting gravitational waves depend on the distribution of post-d

282 A stochastic superposition of gravitational waves from all such binary systems would m

283 The direct detection of gravitational waves from merging binary black holes open

284 omized by the exciting prospect of detecting gravitational waves from merging black holes.

285 The recent discovery of gravitational waves from stellar-mass binary black hole

286 s of taking data, Advanced LIGO has detected gravitational waves from two binary black hole mergers,

287 Gravitational waves have been detected from a binary neu

288 ified by direct detection: the production of gravitational waves in spacetime by accelerating objects

289 ns of a double neutron star merger producing gravitational waves led to a focus on multi-messenger as

290 supermassive black hole binaries, which emit gravitational waves prior to their coalescence.

291 onserved stress energy tensor for weak field gravitational waves propagating in vacuum is derived dir

292 Gravitational waves were discovered with the detection o

293 the software stack used in the discovery of gravitational waves(1) and in the first imaging of a bla

294 ons will improve not only the observation of gravitational waves, but also more broadly future quantu

295 monstration that the limited localization of gravitational waves, previously written off as not usefu

296 lar masses) black holes has been detected in gravitational waves.

297 ngth observations would be more sensitive to gravitational waves.

298 d through both electromagnetic radiation and gravitational waves.

299 Global and intermediate gravitational zones [(18)F]fluoro-2-deoxy-D-glucose upta

300 rated regions--corresponding to intermediate gravitational zones--are the primary targets of the infl