「cosmological」の共起表現一覧(1語右で並び替え)
該当件数 : 199件
It has been quoted in cognitive, | cosmological, and philosophical scholarship. |
creator as first cause, invoking the Kalam | cosmological argument; |
entropy in the Universe, and so inducing a | cosmological arrow of time. |
Step 2: Set the | cosmological boundary conditions. |
um bridge between contracting and expanding | cosmological branches. |
"Detecting dark energy in orbit: The | cosmological chameleon". |
hor of a midrash on Parashat Terumah, whose | cosmological conceptions seem to have been influenced by |
Some | cosmological concepts are present in the Vedas, as are n |
with several articles on astrophysical and | cosmological consequences of long-range modified models |
ly incorporate a mechanism for relaxing the | cosmological constant to very small values, consistent w |
supernovae data supporting inclusion of the | cosmological constant in the standard model indicates th |
ry of the accelerating universe, a positive | cosmological constant has been revived as a simple expla |
n - dropped to very low concentrations, the | cosmological constant term started to dominate the energ |
ata, first indications of the action of the | cosmological constant were found, shortly before major s |
l Steinhardt et al (1999) partly solves the | cosmological constant problem. |
ng to the Lambda-CDM model (ΛCDM model) the | cosmological constant will dominate in the future. |
ply to a de Sitter universe with a positive | cosmological constant with the cosmological horizon in p |
de Sitter space describe the effects of the | cosmological constant in the real world four dimensional |
field equations with a positive (repulsive) | cosmological constant Λ (corresponding to a positive vac |
an appreciable net electric charge, and the | cosmological constant is now thought to be non-zero. |
nother problem arises with inclusion of the | cosmological constant in the standard model: i.e., the a |
ysics such as the hierarchy problem and the | cosmological constant problem. |
only term in the stress-energy tensor is a | cosmological constant term. |
radiation in the universe is reset, but the | cosmological constant is not. |
gravitational instantons to have a nonzero | cosmological constant or a Riemann tensor which is not s |
curred in the early universe, where first a | cosmological constant much larger than the present one c |
indicating the presence of a dark energy or | cosmological constant dominating the mass/energy of the |
In particular, Bertolami studied the | cosmological constant problem and its connection with th |
implying the existence of dark energy or a | cosmological constant in the Universe. |
It is assumed that the | cosmological constant equals zero. |
Sometimes, a | cosmological constant Λ is included in the Lagrangian so |
Instead, the | cosmological constant gradually diminishes over many cyc |
ation of gravity and its application to the | cosmological constant problem. |
The existence of a | cosmological constant is thus equivalent to the existenc |
change of the perspective occurred when the | cosmological constant or dark energy was first observed |
se may be accelerating, fueled perhaps by a | cosmological constant or some other field possessing lon |
A | cosmological constant can be introduced by changing the |
The identification of dark energy as a | cosmological constant does not appear to be consistent w |
icists of the twentieth century assumed the | cosmological constant is zero. |
For example, the | cosmological constant may be a fundamental constant, but |
Sitter or anti de Sitter depending upon the | cosmological constant). |
tein field equations (EFE), with or without | cosmological constant). |
e Einstein field equations, with or without | cosmological constant). |
e past sign of the pressure assigned to the | cosmological constant, changing from the current negativ |
odel and general relativity with a positive | cosmological constant, occur in at least one of them. |
, and only holds for a positive sign of the | cosmological constant, the sign that was observed to be |
rather than decelerating due to a positive | cosmological constant, meaning any two regions of the un |
with the gauge group SO(2,2) for a negative | cosmological constant, and SO(3,1) for a positive one, w |
developed a key test for the presence of a | cosmological constant, also recently confirmed. |
The value of the | cosmological constant, Λ, is ~2 x 10−35s−2. |
expansion include some form of dark energy: | Cosmological Constant, Quintessence, Dark Fluid or Phant |
s a version of general relativity without a | cosmological constant, it is called Minkowski space. |
solution has been generalized to include a | cosmological constant. |
contains the Einstein-Hilbert action with a | cosmological constant. |
onflict in the analysis used to support the | cosmological constant. |
hat the quantum vacuum is equivalent to the | cosmological constant. |
olutions were shown to exist for a negative | cosmological constant. |
ive force of unknown nature, which may be a | cosmological constant; other theories suggest this could |
For non-zero | cosmological constants, on curved spacetimes quantum fie |
er hand, such models typically predict huge | cosmological constants. |
as in asymptotically flat spacetimes (zero | cosmological curvature), can the notion of incoming and |
after the big bang, which brought to an end | cosmological dark ages,. |
creditable attempt to incorporate all known | cosmological data at the time, and indicates the sophist |
erse as given by the tracker solutions with | cosmological data, a main feature of tracker solutions i |
of this model are in agreement with current | cosmological data, but there are interesting differences |
Each successive | cosmological decade represents a ten-fold increase in th |
There were an infinite number of | cosmological decades between the Big Bang and the Planck |
The emblem might took form of a | cosmological diagram haloed by typical "Surya Majapahit" |
in our Milky Way, and other galaxies out to | cosmological distances in order to determine their compo |
foundation for the modern understanding of | cosmological distances. |
nt of the idea that gamma-ray bursts are at | cosmological distances. |
slamic Iranian history, uses native Iranian | cosmological division system of the world. |
tion is a series of six volumes, and also a | cosmological doctrine, authored by Max and Alma Theon ar |
of topological defects in field theory; and | cosmological dynamics of extra spacetime dimensions. |
t neutral atomic Hydrogen emission from the | cosmological Epoch of Reionization, to study the sun/hel |
Experimental data casting light on this | cosmological epoch has been scant or non-existent until |
The Ambarkanta - | cosmological essays, maps, and diagrams |
The current | cosmological estimates of the age of the universe, in co |
e Jain Path, epistemological, metaphysical, | cosmological, ethical and practical, otherwise unorganiz |
mics is more general than black holes, that | cosmological event horizons also have an entropy and tem |
So the Hubble limit need not define the | cosmological event horizon (that is, the boundary separa |
ini, R; Pullin, J Discrete quantum gravity: | cosmological examples CLASSICAL AND QUANTUM GRAVITY, 20 |
India when the established mythologies and | cosmological explanations of the vedas came under ration |
wrence Durrell's Cefalu, Henry Miller's The | Cosmological Eye and Sunday After the War, Vladimir Nabo |
of general relativity (e.g., black holes or | cosmological geometries) are modeled by other physical s |
nishing of the Weyl curvature tensor of the | cosmological gravitational field near the Big Bang. |
ntropy of a black hole and the entropy of a | cosmological horizon in an inflationary model of the uni |
Cosmological horizon, a limit of observability | |
mponent on a fixed radius sphere called the | cosmological horizon. |
eans we may neglect what happens beyond the | cosmological horizon. |
se (that is, they lie outside one another's | cosmological horizons). |
The "monopole problem" refers to the | cosmological implications of Grand unification theories |
They weren't aware of the | cosmological implications, nor that the supposed nebulae |
n mode grows larger than the horizon during | cosmological inflation before coming back inside the hor |
If | cosmological inflation had never happened, and radiation |
Cosmological Inflation and Large Scale Structure, ISBN 0 | |
Cosmological Inflation and Large Scale Structure (2000), | |
working on an alternative to the theory of | cosmological inflation with David Wands of Portsmouth Un |
During | cosmological inflation, the Hubble radius is constant. |
s two books on early universe cosmology and | cosmological inflation. |
us experiments have not been carried out on | cosmological length scales, general relativity could con |
The | cosmological model of concentric or homocentric spheres, |
This may indicate that the prevailing | cosmological model is insufficient to describe the mass |
A Gold universe is a | cosmological model of the universe. |
lem de Sitter (Early relativist; gave first | cosmological model predicting a redshift.) |
The Einstein-de Sitter universe is the | cosmological model for flat matter-only FLRW universe. |
He has offered a young Earth creationist | cosmological model to deal with the distant starlight pr |
rotic universe, or ekpyrotic scenario, is a | cosmological model of the origin and shape of the univer |
r lambdavacuum, often referred to as the dS | cosmological model, |
ghly improbable under the currently favored | cosmological model. |
er apparent contradiction with the standard | cosmological model. |
“the same degree of tuning required in any | cosmological model.” |
ng the world lines of the dust particles in | cosmological models which are exact dust solutions of th |
In general relativity, some | cosmological models have a preferred frame that allows m |
the Gowdy vacua (Robert H. Gowdy) ( | cosmological models constructed using gravitational wave |
Kantowski-Sachs dusts ( | cosmological models which exhibit perturbations from FLR |
A cyclic model is any of several | cosmological models in which the universe follows infini |
Currently all recurring | cosmological models are very controversial within the sc |
According to standard | cosmological models, the motion of galaxy clusters with |
ed to a serious problem in the then current | cosmological models, a problem which was later addressed |
s, but contain enough matter to be possible | cosmological models, or models of cosmological structure |
introduce effects not seen in more standard | cosmological models. |
r of the size of the universe when studying | cosmological models. |
ence for the foundation of current standard | cosmological models. |
It also fails in | cosmological models. |
e are a widely used family of inhomogeneous | cosmological models. |
at Austin, where he wrote a dissertation on | cosmological models. |
verse, and suggesting correspondences among | cosmological, numerological, and physiological aspects o |
However, subsequent | cosmological observations have shown that this model is |
ect for nature will necessarily result from | cosmological or transpersonal identification with nature |
Galaxy; and possibly from other sources of | cosmological origin, such as the very early phase of the |
ce of the Big Bang as the dominant physical | cosmological paradigm, there have been a variety of reac |
Bentley's paradox is a | cosmological paradox pointing to a problem occurring whe |
violation, they argue that it explains two | cosmological paradoxes. |
he foremost problems in astronomy since the | cosmological parameters of the Universe may be constrain |
sands of example Universes and packages the | cosmological parameters describing these Universes as wo |
rnova Cosmology Project, which measured the | cosmological parameters Omega and Lambda using the light |
celeration of the universe) by constraining | cosmological parameters. |
ackground radiation for an arbitrary set of | cosmological parameters. |
isotropy of the CMB for an arbitrary set of | cosmological parameters. |
the growth of structure in the universe in | cosmological perturbation theory. |
This explains the origin of | cosmological perturbation fluctuations in inflationary m |
roblems have caused some difficulties doing | cosmological perturbation theory in this system, however |
founded its NSF Physics Frontier Center for | Cosmological Physics. |
Nevertheless, its | cosmological predictions appear to be consistent with ob |
ly isotropic and homogenous, supporting the | Cosmological Principle that the Universe looks the same |
smology is based on the assumption that the | Cosmological principle is almost, but not exactly, true |
If the universe is finite in extent and the | cosmological principle (not to be confused with the cosm |
own by direct observational evidence of the | Cosmological Principle and the Copernican Principle, whi |
on on Earth: as Andrew Liddle puts it, "the | cosmological principle [means that] the universe looks t |
The Perfect | Cosmological Principle is an extension of the Cosmologic |
The Perfect | Cosmological Principle states that the Universe is homog |
The | cosmological principle contains three implicit qualifica |
The | cosmological principle represents both the principle on |
Arthur Milne (named the | Cosmological Principle and advocated a major rival to Ge |
ote from Barrow and Tipler's "The Anthropic | Cosmological Principle": "At the instant the Omega Point |
mathematician, he rejected some of Kepler's | cosmological principles, including Copernican theory. |
Among his major research interests are | Cosmological probes of Dark Matter and Dark Energy. |
own for his research in using supernovae as | Cosmological Probes. |
Pierre Teilhard de Chardin to describe the | cosmological process of the creation of the Universe. |
me for himself by publishing a paper on the | cosmological production of superheavy magnetic monopoles |
to the mounds they built for ceremonial and | cosmological purposes, they constructed a defensive 12-f |
curred from the universe's creation until a | cosmological redshift of approximately 3400, at which po |
mained optically thick to radiation until a | cosmological redshift of approximately 1100, when the un |
gravitational attraction of matter, on the | cosmological scale, is more than counteracted by negativ |
The | cosmological scales that we nowadays observe correspond |
ation of matter and gravitational energy on | cosmological scales which is a feature of a zero-energy |
n, based on the torsion of spacetime, for a | cosmological scenario of fecund universes proposed earli |
Enoch receives a revelation of | cosmological secrets of creation (3 Enoch 13:1-2) |
face the rising sun", perhaps to suggest a | cosmological significance to its placement. |
irtual Observatory), it starts dealing with | cosmological simulation computed with Gadget2, Enzo and |
y problem is one that arises from numerical | cosmological simulations that predict the evolution of t |
The cuspy halo problem arises from | cosmological simulations that seem to indicate cold dark |
t and strongest results derived from N-body | cosmological simulations." |
n given in the context of isotropic initial | cosmological singularities e.g. in the articles.. Penros |
Near the initial | cosmological singularity (the Big Bang), he proposes, th |
A complete | cosmological solution may or may not be needed. |
Case, or that of the comoving fluid of the | cosmological solution. |
t is seen and the expected time dilation of | cosmological sources has also been observed - and effect |
sed on strong parallels between Upanishadic | cosmological statements and the meditative goals of the |
possibilities, the view put forward is that | cosmological statements in the Upanishads reflect a cont |
Given gravitation's predominance in shaping | cosmological structures, accurate predictions of the uni |
on, the Urarina have an elaborate animistic | cosmological system predicated on ayahuasca shamanism, w |
brightness test is one out of a half-dozen | cosmological tests that was conceived in the 1930s to ch |
ogy, fractal cosmology is a set of minority | cosmological theories which state that the distribution |
phase transitions in the early universe in | cosmological theories and is widely recognized as a semi |
He was responsible for positing numerous | cosmological theories that have a profound impact on und |
y and cosmology, and the formulation of new | cosmological theories, have occurred through the resolut |
superspaces like the configuration space of | cosmological theories. |
on galactic structure, he also developed a | cosmological theory based on the work of Johann Heinrich |
Big Bang model or theory is the prevailing | cosmological theory of the early development of the univ |
recent theoretical investigation found the | cosmological time, dt, diverges for any finite interval, |
ch means this happened very recently on the | cosmological timescale. |
shes his "Italian Dialogues", including the | cosmological tracts La Cena de le Ceneri ("The Ash Wedne |
ortant works are astrological allegories or | cosmological tracts. |
Essential Relativity: Special, General, and | Cosmological was published in 1969 by Van Nostrand Reinh |
こんにちは ゲスト さん
ログイン |
Weblio会員(無料)になると 検索履歴を保存できる! 語彙力診断の実施回数増加! |
こんにちは ゲスト さん
ログイン |
Weblio会員(無料)になると 検索履歴を保存できる! 語彙力診断の実施回数増加! |