ライフサイエンスコーパス: cosmology

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

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

3 arch fields, ranging from fluid mechanics to cosmology.

4 physics models from quantum field theory to cosmology.

5 se, with implications to network science and cosmology.

6 the galactic halo according to the standard cosmology.

7 outstanding puzzles in particle physics and cosmology.

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

9 erent approach to the dark energy problem in cosmology.

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

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

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

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

14 which remains one of the unsolved puzzles of cosmology.

15 lenge that drives the field of computational cosmology.

16 wined with ancestors myths from contemporary cosmology.

17 n be used to distinguish between alternative cosmologies.

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

48 Inflationary cosmology is a highly successful framework for exploring

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

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

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

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

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

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

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

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

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

58 Cosmology is undergoing a revolution.

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

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

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

62 0, Lambda = 0 denoted as C1 and chronometric cosmology (no relevant adjustable parameters) denoted as

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

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

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

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

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

68 It is not a cosmology that was predicted.

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

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

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

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

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

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

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

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

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

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

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

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