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1 dients (of more than 700 degrees Celsius per gigapascal).
2 o relatively modest pressures (less than 100 gigapascals).
3 serpentinization) at 200 degrees C and 0.03 gigapascal.
4 inous phases indicates pressures of up to 27 gigapascal.
5 these xenoliths record pressures of up to 22 gigapascal.
6 n be quenched to ambient temperature above 1 gigapascal.
7 ore mafic than the starting peridotite at 10 gigapascals.
8 - 270 kelvin upon shock compression above 80 gigapascals.
9 ned to be just above 1000°C from 5 to 11 gigapascals.
10 semblage at 4300 +/- 270 kelvin is 130 +/- 3 gigapascals.
11 ansforms to Pbnm-perovskite structure at 223 gigapascals.
12 al mode coupling were observed at 150 to 160 gigapascals.
13 phase relations at pressures from 45 to 100 gigapascals.
14 f pure forsterite, were measured to about 13 gigapascals.
15 chable polymorph) at pressures from 58 to 85 gigapascals.
16 metric structures in the phase diagram by 30 gigapascals.
17 ngton transition to metallic hydrogen at 495 gigapascals.
18 of D2 must occur at a pressure of above 380 gigapascals.
19 acked structure upon compression to over 770 gigapascals.
20 and tungsten in static experiments up to 500 gigapascals.
21 en studied so far only at pressures below 75 gigapascals.
22 ies at approximately 150 gigapascals and 440 gigapascals.
23 -nanometer nickel when compressed above 18.5 gigapascals.
24 ver an extended pressure range from 40 to 60 gigapascals.
25 n the diamond anvil cell between 145 and 157 gigapascals.
26 e undergoes a transition at approximately 17 gigapascals.
27 ound ranging from 9 to 16 kelvin at 23 to 80 gigapascals.
28 f the outermost layer varied from 270 to 950 gigapascals.
29 liquid deuterium to pressures from 22 to 340 gigapascals.
30 at shock pressures in the range of 10 to 180 gigapascals (0.1 to 1.8 megabars) and temperatures to 40
31 ,Fe)SiO3 perovskite at conditions (50 to 106 gigapascals, 1600 to 2400 kelvin) close to a mantle geot
32 d plasticity at high pressure (more than 150 gigapascals), a regime that recovery experiments cannot
35 e, pyrite-structured iron oxide (FeO2) at 76 gigapascals and 1,800 kelvin that holds an excessive amo
36 n garnet and silicate liquid from 1.5 to 2.0 gigapascals and 1250 degrees to 1350 degreesC show that
40 e ferropericlase have been measured up to 95 gigapascals and 2000 kelvin with x-ray emission in a las
42 closed packed (hcp) iron to a magnet at 16.9 gigapascals and 261 degrees centigrade suggests that hcp
49 e crystals under laboratory conditions of 26 gigapascals and 973 to 1473 kelvin (conditions typical o
50 (hcp-Fe) were measured at pressures up to 73 gigapascals and at temperatures up to 1700 kelvin with n
52 sical properties of dense hydrogen above 325 gigapascals and constrain the pressure and temperature c
53 ) precipitates, with a strength of up to 2.2 gigapascals and good ductility (about 8.2 per cent).
54 amond anvil cells, at pressures of 95 to 101 gigapascals and temperatures of 2200 to 2400 kelvin, we
56 form diamond at pressures between 10 and 50 gigapascals and temperatures of about 2000 to 3000 kelvi
57 ibited very high Young's moduli (up to ~14.0 gigapascals and up to 20 gigapascals when reinforced wit
58 tic modulus of restacked MoS2 layers (2 to 4 gigapascals) and fast proton diffusion between the nanos
59 unobserved Rh2O3 (II) structure at about 78 gigapascals, and it further transforms to Pbnm-perovskit
60 n measurements yielded a bulk modulus of 360 gigapascals, and radial diffraction indicated that ReB2
61 ral changes, observed at pressures up to 130 gigapascals, appear exclusively after melting, thus offe
62 the suggested phase V in H2 and HD up to 388 gigapascals at 300 kelvin, and up to 465 kelvin at 350 g
63 evidence that at pressures greater than 325 gigapascals at 300 kelvin, H2 and hydrogen deuteride (HD
65 D2O) compressed to a maximum pressure of 210 gigapascals at 85 to 300 kelvin exhibit a phase transiti
66 an exist at outer-core pressures (136 to 330 gigapascals) at temperatures below 5200 kelvin and lead
67 We have used in situ high-pressure (up to 2 gigapascals) boron-11 solid-state nuclear magnetic reson
68 psilon-Fe) have been measured from 15 to 152 gigapascals by using diamond-anvil cells with ultrapure
69 of SiO2 rises to 8300 K at a pressure of 500 gigapascals, comparable to the core-mantle boundary cond
70 centered cubic (bcc) phase up to at least 84 gigapascals (compared to approximately 10 gigapascals fo
71 n the diamond anvil cell between 104 and 130 gigapascals confining pressure and ambient temperature.
73 kelvin, and G (at room conditions) = 113(1) gigapascals, dG/dP = 1.5(1), and dG/dT = -0.017(1) gigap
74 moduli yield K (at room conditions) = 172(2) gigapascals, dK/dP = 4.2(1), and dK/dT = -0.012(1) gigap
77 texturing is observed at pressures above 3.0 gigapascals for 500-nanometer nickel and at greater than
82 strength of this layer ranged from 11 to 63 gigapascals for the set of 19 MWCNTs that were loaded.
83 London dispersion)] to predict that above 60 gigapascal (GPa) the most stable form of N2O (the laughi
84 erved on a GeO(2) glass at a pressure of 5.5 gigapascal (GPa), based on in situ density and x-ray dif
85 ssion at peak normal elastic stresses of ~73 gigapascals (GPa) and strain rates of 10(9) per second.
86 tra have been measured at pressures up to 80 gigapascals (GPa) for the lower-mantle oxide magnesiowus
91 demonstrated that deuterium shocked above 55 gigapascals has an electrical conductivity characteristi
93 transition at 60 gigapascals in H2O ice (70 gigapascals in D2O ice) on the basis of their infrared r
94 300 kelvin exhibit a phase transition at 60 gigapascals in H2O ice (70 gigapascals in D2O ice) on th
95 y that Jupiter should become metallic at 140 gigapascals in the fluid, and the electrical conductivit
99 of nanoparticle assembly in the presence of gigapascal level stress rebalances interparticle forces
101 ale multilayers have hardnesses exceeding 50 gigapascals, making these films highly resistant to abra
104 etic field to tune the density of bosons and gigapascals of hydrostatic pressure to regulate the unde
105 hase persisted to the maximum pressures (210 gigapascals) of the measurements, although changes in vi
106 d quasi-hydrostatic pressures of about three gigapascals on previously deformed olivine aggregates an
107 scals, dK/dP = 4.2(1), and dK/dT = -0.012(1) gigapascals per kelvin, and G (at room conditions) = 113
110 ous experimental data in the several hundred gigapascal pressure range, particularly near the melt bo
111 ll-on-disk tests at contact pressures of 1.3 gigapascals reveal that these tribofilms nearly eliminat
112 etworks comprising this macromer possessed a gigapascal-storage modulus at body temperature and a T(t
113 e complexity of the phase behavior above 100 gigapascals suggests extraordinary liquid and solid stat
115 ansition temperature Tc of 203 kelvin at 155 gigapascals--the highest Tc reported for any superconduc
116 s, then for pressures greater than about 175 gigapascals they are predicted to sit exactly halfway be
117 ing pressure from andesitic composition at 1 gigapascal to more mafic than the starting peridotite at
118 f up to one-third million atmospheres, or 33 gigapascals) to germanium, we report here a complex grad
119 on ReB2 indicated an average hardness of 48 gigapascals under an applied load of 0.49 newton, and sc
121 The eutectic temperature in the system at 14 gigapascals was about 400°C lower than that extrapol
122 ments on natural amphibole-rich veins at 1.5 gigapascals, we found that partial melts of metasomatic
123 s at 300 kelvin, and up to 465 kelvin at 350 gigapascals; we do not observe phase V in deuterium (D2)
124 moduli (up to ~14.0 gigapascals and up to 20 gigapascals when reinforced with surface-treated carbon
125 arable melting temperatures above 500 to 700 gigapascals, which could favor long-lived magma oceans f
128 carbon films with a Young's modulus of 14.5 gigapascals, with the possibility of further transfer on
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