ライフサイエンスコーパス: chemical evolution

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

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

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

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

5 nization of the material and consequently to chemical evolution.

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

27 A chemical evolution hypothesis set forth by Woese in 1979

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

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

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

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

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

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

34 However, chemical evolution may not have occurred continuously be

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

36 Chemical evolution models and observed stellar Li abunda

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

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

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

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

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

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

43 The chemical evolution of extraterrestrial environments lead

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

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

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

47 Chemical evolution of planetary bodies, ranging from ast

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

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

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

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

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

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

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

55 The chemical evolution of the organic aerosol inside the PAM

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

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

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

59 The chemical evolution of wine was the most important phenom

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

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

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

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

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

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

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

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

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

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