ライフサイエンスコーパス: strong magnetic field

1 o transform into metals under a sufficiently strong magnetic field.

2 lute metals upon application of sufficiently strong magnetic field.

3 crystallization process in the presence of a strong magnetic field.

4 of exciton is calculated for an arbitrarily strong magnetic field.

5 of a two-dimensional electron layer under a strong magnetic field.

6 tar is a variable of beta Cep-type and has a strong magnetic field.

7 on emission from relativistic electrons in a strong magnetic field.

8 iously only be realized in the presence of a strong magnetic field.

9 namics (QED)-induced vacuum birefringence in strong magnetic fields.

10 pins can be manipulated only optically or by strong magnetic fields.

11 he fluctuations were found to be enhanced in strong magnetic fields.

12 een at deep cryogenic temperatures and under strong magnetic fields.

13 kable transport anomaly commonly observed at strong magnetic fields.

14 egligible stray fields and is insensitive to strong magnetic fields.

15 superconductor in terms of its behaviour in strong magnetic fields.

16 by extreme radiation environments and super-strong magnetic fields.

17 ures because they use magnetic materials and strong magnetic fields.

18 enerate star G99-47, due to the existence of strong magnetic fields.

19 Fermi liquid formed by composite fermions in strong magnetic fields(1-10).

20 Magnetars are neutron stars with extremely strong magnetic fields (10(13) to 10(15) gauss)(1,2), wh

21 nd their supernovae may be affected by their strong magnetic fields(12).

22 table neutron star that spins rapidly with a strong magnetic field(5-8) (that is, a magnetar).

23 s in the quantum regime has often required a strong magnetic field(9-11) or a moire superlattice pote

24 gle crystals of uranium dioxide subjected to strong magnetic fields along threefold axes in the magne

25 Strong magnetic fields also suppress the AFM order at a

26 first evidence that this giant planet has a strong magnetic field and a large magnetosphere.

27 magnet was designed to generate the required strong magnetic field and field profile.

28 lled AFM memory that is fully operational in strong magnetic fields and has the potential for low-ene

29 Oscillations of conductance observed in strong magnetic fields are a striking manifestation of t

30 Two-dimensional electron systems subject to strong magnetic fields are expected to exhibit quantized

31 Strong magnetic fields are produced in the simulations,

32 Strong magnetic fields are required in many fields, such

33 s, whose X-ray emission is powered by a very strong magnetic field (B approximately 10(15) G).

34 do not have convective interiors to generate strong magnetic fields by dynamo(11), merger remnants ar

35 Moreover, strong magnetic fields can alter the average atmospheric

36 thicker Mn(Bi(1-x)Sb(x))(2)Te(4) films under strong magnetic fields can be interpreted by a theory of

37 of the interaction revealed the presence of strong magnetic fields characteristic of Weibel Instabil

38 the tendency of f-electrons to polarize in a strong magnetic field, consequently weakening the intera

39 In a two-dimensional electron gas under a strong magnetic field, correlations generate emergent ex

40 e unusually small electric polarization, its strong magnetic field dependence, and the negative therm

41 ached, we find magnetism to strengthen under strong magnetic fields due to suppression of the Kondo e

42 orescence measurements and the presence of a strong magnetic field effect indicate that up to 90% of

43 me fold or sequence, the maquettes exhibit a strong magnetic field effect that rivals those observed

44 ing in two dimensions under the influence of strong magnetic fields effectively lose their kinetic en

45 Strong magnetic-field effects (MFE) were observed for tw

46 confined to two dimensions and exposed to a strong magnetic field, electrons screen the Coulomb inte

47 Sunspots are regions where strong magnetic fields emerge from the solar interior an

48 icate that the ground state of graphene in a strong magnetic field exhibits spontaneous breaking of S

49 es and of the fission-fragment ejecta within strong magnetic fields experimentally.

50 ed when a single Landau level is occupied in strong magnetic fields, gives rise to unconventional sta

51 gnetic flux density is changed locally and a strong magnetic field gradient is formed.

52 This tool uses a magnetic particle and a strong magnetic field gradient to apply defined forces t

53 The use of strong magnetic field gradients and high magnetic fields

54 NMR probe hardware capable of generating strong magnetic field gradients enables (23)Na NMR-based

55 The inherently strong magnetic-field gradients of single-sided sensors

56 y mitigate artifacts related to evolution in strong magnetic-field gradients, magnetic fields that va

57 imately 5-12 s) neutron stars with extremely strong magnetic fields (>10(14 )G)--at least an order of

58 imit (QL) of an electron liquid, realised at strong magnetic fields, has long been proposed to host a

59 iant-branch (AGB) star can indeed generate a strong magnetic field, having as its origin a dynamo at

60 implemented, avoiding the limitation of the strong magnetic field imposed by the Faraday effect.

61 atmosphere, and would also need to possess a strong magnetic field in order to prevent its atmosphere

62 We demonstrate that strong magnetic fields in the cores of red giant stars c

63 cent of our sample show mode suppression, by strong magnetic fields in the cores, but this fraction i

64 BMO-like spherical shell is able to sustain strong magnetic fields, including axial dipolar fields s

65 erved and the magnetopause was threaded by a strong magnetic field, indicating a reconnection rate ~1

66 g from rotating neutron stars with extremely strong magnetic fields, known as magnetars; the origin o

67 Strong magnetic fields lead to Zak-type cloning of the t

68 ing between states near the Fermi level in a strong magnetic field limit.

69 es to a variety of hazard stimulus such as a strong magnetic field, noise level, and falling or drown

70 nger than about one micrometre, transport in strong magnetic fields occurs through a zero-energy stat

71 equence of partial alignment of SMM 1 in the strong magnetic field of the NMR spectrometer.

72 ion that are believed to be powered by ultra-strong magnetic fields of >10(14) G, according to the 'm

73 ns include accretion onto neutron stars with strong magnetic fields, onto stellar-mass black holes (o

74 zation is difficult to control, and requires strong magnetic fields or nonlinear optical effects, and

75 can create quantum Hall phases by applying a strong magnetic field perpendicular to a two-dimensional

76 The robustness against strong magnetic field perturbations combined with the mu

77 Jupiter's rapidly rotating, strong magnetic field provides a natural laboratory that

78 ic particle agglutination via application of strong magnetic field pulses, we obtained identical limi

79 erefore the most decisive test of QED in the strong magnetic field regime, we find a 7-sigma discrepa

80 The strong magnetic field requires considerable changes in t

81 ies of two-dimensional electron systems in a strong magnetic field revealed the quantum Hall effect(1

82 The application of a strong magnetic field significantly and beneficially alt

83 Lying supine in a strong magnetic field, such as in magnetic resonance ima

84 Strong magnetic fields, synchrotron emission, and Compto

85 lated cool white dwarf stars more often have strong magnetic fields than young, hotter white dwarfs,

86 gy gain by electrons from a laser pulse in a strong magnetic field that naturally arises in dense las

87 tronic system is subjected to a sufficiently strong magnetic field that the cyclotron energy is much

88 tics but it relies on radioactive tracers or strong magnetic fields that are unsuitable for many pati

89 Without an externally applied strong magnetic field, the observed ExMCh effect with a

90 In the absence of strong magnetic fields, the convective flows of the core

91 re confined in two dimensions and subject to strong magnetic fields, the Coulomb interactions between

92 Under strong magnetic fields, the topological properties of Di

93 hereas the QL typically requires unreachably strong magnetic fields, the topological semimetal ZrTe(5

94 es are split into finer quantum states under strong magnetic field, thus transitions between some tri

95 ountered with standard techniques by using a strong magnetic field to destabilize an otherwise stable

96 e of Io's plasma is captured by the planet's strong magnetic field to form a co-rotating torus at Io'

97 ma of deuterium and tritium is confined by a strong magnetic field to produce helium ions and release

98 ITER is of the tokamak based design using strong magnetic fields to confine the very hot plasma ne

99 urrent models of magnetars require extremely strong magnetic fields to explain their observed quiesce

100 lid target as it expands into a homogeneous, strong magnetic field (up to 30 T) that is transverse to

101 ion for the archetype Weyl semimetal TaAs in strong magnetic field, we observed a quasi-linear field

102 The strong magnetic fields were associated with unusually lo

103 Spectra recorded in strong magnetic fields were typical of diamagnetic syste

104 ions enabled by a structured optical pump or strong magnetic field, which are inconvenient for device

105 an support one-way chiral zero modes under a strong magnetic field, which leads to nonconservation of

106 By electromagnetic duality, a sufficiently strong magnetic field would similarly produce magnetic m

107 0.01(2) mms; analysis of spectra obtained in strong magnetic fields yields parameters characteristic