ライフサイエンスコーパス: chemical evolution

1 ysis is essential for the origin of life and chemical evolution.

2 nt changes relate directly to the underlying chemical evolution.

3 ssary for selection to act), as required for chemical evolution.

4 ough the galaxy, galaxy density, and stellar chemical evolution.

5 gents for the participation of phosphorus in chemical evolution.

6 er mantle are key to the Earth's thermal and chemical evolution.

7 onal chemistries operating at the origins of chemical evolution.

8 prebiotic chemical networks and early-stage chemical evolution.

9 arth and were possible contributors to early chemical evolution.

10 on the origin of complex functions in early chemical evolution.

11 d porous mineral surfaces and their roles in chemical evolution.

12 ing the Moon's formation and its thermal and chemical evolution.

13 rd the building of a systems-level theory of chemical evolution.

14 and may be restricted to galaxies of limited chemical evolution.

15 this is, we state, the last possible step of chemical evolution.

16 nization of the material and consequently to chemical evolution.

17 omparative methods to understand the mode of chemical evolution.

18 llisional processing in shaping planetesimal chemical evolution.

19 ion of water and rocks-a key driver of ocean chemical evolution-across a broad range of compositional

20 e previous work that aimed to understand the chemical evolution (aging) of POA and SOA has focused on

21 o characterize, and robust prediction of the chemical evolution and associated functionality of the r

22 Our results suggest that chemical evolution and selection can be observed in orga

23 e of the processes thought to be involved in chemical evolution and the origin of life.

24 es because of their implications for organic chemical evolution and the origin of life.

25 othesized functionality of peptides in early chemical evolution and their central role in current bio

26 timescales is crucial for understanding the chemical evolution and thermal histories of terrestrial

27 and other optical properties to examine the chemical evolution and transformation of oil components

28 rstellar medium (after allowing for Galactic chemical evolution), and indicates that the absorption s

29 f some of the chemical processes involved in chemical evolution, and a partial answer to the fundamen

30 ew the successes, and consider the future of chemical evolution as a tool.

31 the establishment of prebiotic attributes in chemical evolution as well as the origin of terrestrial

32 cative of an asymmetric influence on organic chemical evolution before the origin of life.

33 tical evolutionary constraints for achieving chemical evolution by natural selection in the lab.

34 principle in chemical evolution, rather than chemical evolution by natural selection.

35 The constraints imposed on chemical evolution by the second law of thermodynamics a

36 We propose that chemical evolution can take place by natural selection i

37 Lacking a comprehensive theory of chemical evolution capable of explaining the time-depend

38 of extraordinary behaviour such as primitive chemical evolution, chemotaxis, temporally controllable

39 The rapidity with which chemical evolution could have occurred within clouds acc

40 etween planets with parallel chemistries and chemical evolution could in principle amplify the develo

41 time that would have been required for early chemical evolution, countering the view that not enough

42 ork was able to resolve the volcanic plume's chemical evolution downwind of the eruption.

43 ation environments in comet-forming regions, chemical evolution during their long storage in reservoi

44 nd associated structural, morphological, and chemical evolutions during conversion reactions with alk

45 erials is largely governed by structural and chemical evolutions during electrochemical reactions.

46 drophobic monomers were optimized by dynamic chemical evolution for VEGF(165) affinity.

47 a surface reduced layer, to transition) and chemical evolution (formation of a surface reaction laye

48 abiogenesis (the development of life through chemical evolution from inorganic materials) can be esti

49 Propagating those yields with basic galactic chemical evolution (GCE) and comparing with the (205)Pb/

50 plication, a central mechanism driving early chemical evolution, have focused largely on the activity

51 A chemical evolution hypothesis set forth by Woese in 1979

52 By reducing the time required for early chemical evolution in a warm environment, these findings

53 time that would have been required for early chemical evolution in a warm environment.

54 for the study of surface reconstruction and chemical evolution in battery materials using combined d

55 lobal kinetic treatment is used to model the chemical evolution in the PFR and to produce synthetic e

56 of these monomers, the ice world (i.e., the chemical evolution in the range between the freezing poi

57 The results highlight that mimicking chemical evolution is feasible with primitive building b

58 supports the notion that Earth's thermal and chemical evolution is likely to have been largely regula

59 ulty for the widely held view that prebiotic chemical evolution leading to the formation of the first

60 for ionizable lipids discovered via directed chemical evolution may accelerate the development of LNP

61 Thus, a setting favoring rapid chemical evolution may be required.

62 A rapid process of chemical evolution may have been required in order that

63 However, chemical evolution may not have occurred continuously be

64 osited on the surface of the oceans, further chemical evolution might have transformed these molecule

65 Chemical evolution models and observed stellar Li abunda

66 deuterium is destroyed in stellar interiors, chemical evolution models predict that its Galactic Cent

67 d to have a solar metallicity in traditional chemical evolution models(5).

68 However, in Galactic chemical evolution models, neutron-star mergers alone ca

69 However, models of galactic chemical evolution must arbitrarily increase the superno

70 Here we describe the chemical evolution of a DNAzyme with strong catalytic ac

71 designing these interfaces, such as the (bio)chemical evolution of adaptive or buffer zones.

72 used a one-dimensional model to simulate the chemical evolution of air masses in the tropical Atlanti

73 resolved mass that describe the physical and chemical evolution of aircraft exhaust plumes on the tim

74 in the epoch of cosmic reionization and the chemical evolution of early galaxies.

75 ed rocks to reconstruct the lithological and chemical evolution of Earth's continental crust.

76 of such water on the physical properties and chemical evolution of Earth's interior, it is essential

77 zone environments, profoundly affecting the chemical evolution of Earth.

78 The chemical evolution of extraterrestrial environments lead

79 t affect arsenic concentrations, such as the chemical evolution of groundwater, redox differences, an

80 tal insights into molecular behavior and the chemical evolution of life on Earth.

81 and could therefore have contributed to the chemical evolution of life.

82 simulations using our new data reproduce the chemical evolution of melt inclusions from arc volcanoes

83 ionization could yield accurate data for the chemical evolution of mixed component particles undergoi

84 ify the role of ion-neutral reactions in the chemical evolution of molecular clouds.

85 provides insights into the morphological and chemical evolution of molten salt dealloying in bulk mat

86 ndamental understanding of the hydraulic and chemical evolution of natural dehydrating systems.

87 ducts as the human-made equivalent, i.e. the chemical evolution of natural product structure.

88 Prediction of the chemical evolution of OA depends on its reactivity with

89 id (162173) Ryugu provide information on the chemical evolution of organic molecules in the early sol

90 e explored the role of the inorganics in the chemical evolution of organic species in mixed aerosols.

91 Chemical evolution of planetary bodies, ranging from ast

92 rsity and mixing state for investigating the chemical evolution of rBC-containing particles and the p

93 inerals is critical for modeling the thermal-chemical evolution of rocky planets.

94 hree dimensions, a correlated structural and chemical evolution of Si and SEI.

95 o the possible roles of such interactions in chemical evolution of structure and function.

96 od that possesses the ability to monitor the chemical evolution of supercritical CO(2) in relevant co

97 ord important information on the thermal and chemical evolution of the Archean-Proterozoic Earth.

98 (HCCCCH) and triacetylene (HCCCCCCH) in the chemical evolution of the atmosphere of Saturn's moon Ti

99 The structural and chemical evolution of the catalysts studied by TEM, XAS,

100 Subduction zones modulate the chemical evolution of the Earth's mantle.

101 for understanding stellar evolution and the chemical evolution of the Galaxy.

102 (APXPS) was applied to evaluate the in situ chemical evolution of the lithium metal surface under ni

103 ization approach to study the structural and chemical evolution of the metal sulfide-utilizing powder

104 Models of the chemical evolution of the Milky Way suggest that the obs

105 anisotropic filament orientations, then the chemical evolution of the network follows the anisotropi

106 The chemical evolution of the organic aerosol inside the PAM

107 in total electron yield mode can resolve the chemical evolution of the SEI during electrochemical for

108 resulting elucidation of the structural and chemical evolution of the system leads to a new descript

109 re we track three-dimensional structural and chemical evolution of tin anodes in sodium-ion batteries

110 he role of these key reaction classes in the chemical evolution of Titan's orange-brownish haze layer

111 w questions regarding their influence on the chemical evolution of viscous SOA particles, where CIs m

112 The chemical evolution of wine was the most important phenom

113 Together, these results demonstrate that chemical evolution offers a powerful approach for discov

114 , the time that would have been required for chemical evolution on a warm earth.

115 Complementing our previous models of chemical evolution on mineral surfaces, in which selecti

116 e results provide valuable insights into the chemical evolution ongoing during wine ageing, accentuat

117 sotopic reservoir but they diverged in their chemical evolution owing to subsequent fractionation by

118 s, provides insight to the morphological and chemical evolution pathways leading to core-shell partic

119 een hypothesized as an ordering principle in chemical evolution, rather than chemical evolution by na

120 ovide insight into an outcome of early solar chemical evolution that differs from any seen so far in

121 Here we establish an experimental model of chemical evolution to investigate general processes by w

122 atter (PM) lifetimes, in order to link their chemical evolution to toxicological changes.

123 d on Ni(2+) -Nb(5+) pair; the structural and chemical evolution upon cycling of DRXs with an increasi

124 We propose that rapid prebiotic chemical evolution was facilitated on the primordial Ear

125 Using ligand-based virtual screening and chemical evolution, we developed pathway-selective agoni

126 Through five cycles of such directed chemical evolution, we identified dozens of biodegradabl

127 functions would have been a key step in the chemical evolution which led to life.

128 e to analyze structural characterization and chemical evolution with its powerful and unique applicat

129 eptides that could have contributed to early chemical evolution, with an emphasis on molecular intera