ライフサイエンスコーパス: cosmology

1 iscussed in particle physics, astronomy, and cosmology.

2 relevance in fields from particle physics to cosmology.

3 erent approach to the dark energy problem in cosmology.

4 d to illustrate the fine-tuning mechanism in cosmology.

5 wined with ancestors myths from contemporary cosmology.

6 e between idea and discovery, as SDSS did in cosmology.

7 arch fields, ranging from fluid mechanics to cosmology.

8 physics models from quantum field theory to cosmology.

9 se, with implications to network science and cosmology.

10 the galactic halo according to the standard cosmology.

11 outstanding puzzles in particle physics and cosmology.

12 ntral tenet of the cold dark matter model in cosmology.

13 ere is still a great deal left to explore in cosmology.

14 waves, the Lense-Thirring effect, and modern cosmology.

15 rse that engages today's burgeoning field of cosmology.

16 which remains one of the unsolved puzzles of cosmology.

17 hich is difficult in high-energy physics and cosmology.

18 lenge that drives the field of computational cosmology.

19 rom condensed matter to particle physics and cosmology.

20 rf galaxies naturally emerge in the Standard Cosmology.

21 k times of 1.3-2.8 billion years in standard cosmology.

22 physical contexts, from condensed matter to cosmology.

23 n be used to distinguish between alternative cosmologies.

24 at can constrain galaxy formation models and cosmology(10).

25 cations for multi-messenger astrophysics and cosmology(14,15).

26 (1,2)) led to scientific discoveries across cosmology(3), nuclear physics(4-6) and gravity(7).

27 hift as expected from the standard LambdaCDM cosmology(4).

28 The current Lambda cold dark matter cosmology--a simple (but strange) flat cold dark matter

29 how this scenario fits naturally with cyclic cosmologies and recent conjectures about quantum gravity

30 of physics ranging from high-energy physics, cosmology and astrophysics to biology, magneto- and hydr

31 tems and the exploration of their analogs in cosmology and astrophysics.

32 be applied to a variety of scenarios within cosmology and fluid dynamics.

33 f phenomena ranging from particle physics to cosmology and from astrophysics to quantum chemistry.

34 ve probes of stellar and galactic evolution, cosmology and fundamental physics.

35 umans, central to past and present Iroquoian cosmology and mythology.

36 are tightly related in a way that depends on cosmology and on the nature of the dark matter.

37 Universe remains one of the prime puzzles of cosmology and particle physics today-80 y after the firs

38 tter problem is now a pressing issue in both cosmology and particle physics, and the detection of par

39 ne of the most fundamental open questions in cosmology and particle physics.

40 in systems ranging from condensed matter to cosmology and string theory.

41 ssential foundation of the standard model of cosmology and underlies our description of the black hol

42 e of structure formation in cold dark matter cosmologies, and not exotic, finely tuned environments a

43 red for research in astronomy, astrophysics, cosmology, and astronomical instrumentation.

44 many-body systems spanning condensed matter, cosmology, and beyond are hypothesized to be universal w

45 cting textures drawn from materials science, cosmology, and granular media, among other examples.

46 enetics, biochemistry, statistics, biometry, cosmology, and philosophy, although he himself possessed

47 tructure; summarize its impact on astronomy, cosmology, and physics; and look ahead by outlining the

48 ions of the arrow of time in thermodynamics, cosmology, and quantum mechanics.

49 ing from materials science to early-universe cosmology, and to engineering of laser beams.

50 termination of the fundamental parameters of cosmology, and to our understanding of both the past and

51 tandard siren approach of gravitational wave cosmology appeals to the direct luminosity distance esti

52 Current efforts in observational cosmology are focused on characterizing the mass-energy

53 e to view the observational side of physical cosmology as a subdiscipline of astrophysics, still in a

54 tory of the Universe is a key goal of modern cosmology, as it is crucial to our understanding of how

55 ion enables tests of fundamental physics and cosmology, as well as practical applications such as sat

56 the IRAS galaxy samples by generic big bang cosmology (BBC) and chronometric cosmology (CC), respect

57 In the late 20th century, cosmology became a precision science.

58 r historical example shows how a subfield of cosmology, big bang nucleosynthesis, grew in complexity

59 so its abundance is of interest not only for cosmology, but also for understanding stellar evolution

60 ic big bang cosmology (BBC) and chronometric cosmology (CC), respectively.

61 adjustable parameters) denoted as C2 are the cosmologies considered.

62 Cosmology finds itself in a paradoxical situation.

63 A complete understanding of cosmology, from the earliest moments to the ultimate fat

64 on serves as a fundamental tool for studying cosmology, galaxy formation and the nature of dark matte

65 City plans symbolizing cosmologies have long been recognized as a defining elem

66 The theoretical side of cosmology, in contrast, has its deep base in general rel

67 m provides support for the standard model of cosmology, in which dark matter and dark energy are the

68 titatively just as predicted by chronometric cosmology, in which there is no such evolution.

69 ranging implications from medical physics to cosmology including an intimate but subtle connection in

70 The C1 predictions of these cosmology-independent quantities are deviant by as much

71 Inflationary cosmology is a highly successful framework for exploring

72 for the dark matter (DM) of the hot big bang cosmology is about as good as it gets in natural science

73 volution hypothesis in the frame of big-bang cosmology is confirmed at a high level of statistical si

74 ure radiation phase of the Standard Model of Cosmology is embedded as a single point in this family.

75 The 'standard' model of cosmology is founded on the basis that the expansion rat

76 Cosmology is in the midst of a period of revolutionary d

77 th the universe and the laws that govern it, cosmology is on the verge of a golden age.

78 A major result of observational cosmology is that an expansion of the Universe arose fro

79 A principal discovery in modern cosmology is that standard model particles comprise only

80 One of the key questions in observational cosmology is the identification of the sources responsib

81 Cosmology is undergoing a revolution.

82 Within conventional big bang cosmology, it has proven to be very difficult to underst

83 In the era of precision cosmology, it is essential to determine the Hubble const

84 Although general relativity underlies modern cosmology, its applicability on cosmological length scal

85 la: see text] pairs resemble domain walls in cosmology models with biased vacuums and ferromagnets in

86 past 20 years have seen dramatic advances in cosmology, mostly driven by observations from new telesc

87 0, Lambda = 0 denoted as C1 and chronometric cosmology (no relevant adjustable parameters) denoted as

88 r of our expanding Universe, thereby putting cosmology on a firm empirical footing.

89 n simulations(3) with the standard LambdaCDM cosmology only if more diffuse dwarfs formed in low-mass

90 concept in many areas of physics, including cosmology, particle physics and condensed matter.

91 ark matter is one of the central problems of cosmology, particle physics, and gravity.

92 nature, appearing in contexts as diverse as cosmology, particle physics, superfluidity, liquid cryst

93 as previously been employed to study quantum cosmology, quantum paradoxes, and the quantum-to-classic

94 ions for tests of unification models and for cosmology (source counts, measurements of the Hubble con

95 that Y(conc) is robust against variations in cosmology, subgrid physics, and cosmic variance.

96 tion as exotic textures in particle physics, cosmology, superfluids, and many other systems.

97 ment simulations are better suited for axion cosmology than the previously-used static lattice simula

98 It is not a cosmology that was predicted.

99 rameters (in contrast to the two in big-bang cosmology), the hypothesized evolution appears from the

100 In the cold dark matter cosmology, the baryonic components of galaxies-stars and

101 nt as dark matter is in our understanding of cosmology, the detection of these particles has thus far

102 e computational systems originally built for cosmology, the Sloan Digital Sky Survey (SDSS), are now

103 ns that the three fundamental observables in cosmology-the age of the Universe, the distance-redshift

104 er effect is out of the mainstream of modern cosmology, this article opened the way to investigation

105 structure formation in condensed matter and cosmology to biomedical imaging.

106 of phase transitions in systems ranging from cosmology to condensed matter and quantum materials.

107 ive arguments that led to the connections of cosmology to nuclear and particle physics.

108 e variety of physical contexts, ranging from cosmology to superconductors.

109 oblem in many areas of physics, ranging from cosmology, to particle physics, to thermodynamics and st

110 one of the main challenges in observational Cosmology today.

111 d as challenging the Lambda cold dark-matter cosmology (where Lambda is the cosmological constant)(7-

112 oincides with the prediction of chronometric cosmology, which estimates R as 160 +/- 40 Mpc (1 parsec

113 odel as represented by the Friedman-Lemaitre cosmology with parameters qo = 0, Lambda = 0 denoted as

114 ena ranging from condensed-matter physics to cosmology, yet they are generally difficult to simulate.