Deprecated: The each() function is deprecated. This message will be suppressed on further calls in /home/zhenxiangba/zhenxiangba.com/public_html/phproxy-improved-master/index.php on line 456
「perturbation」の共起表現(1語右で並び替え) - Weblio英語共起表現検索
[go: Go Back, main page]


小窓モード

プレミアム

ログイン
設定

設定

Weblio 辞書 > 英和辞典・和英辞典 > perturbationの意味・解説 > perturbationに関連した共起表現

「perturbation」の共起表現一覧(1語右で並び替え)

該当件数 : 85



The effects of the perturbation accumulate at each passage pushing the sate
ations (24) and (28) of the article Orbital perturbation analysis (spacecraft)
s from equation (28) of the article Orbital perturbation analysis (spacecraft) as the factor
Equation (20) of the article Orbital perturbation analysis (spacecraft) gives that the preces
an 0 and less than 1, where 0 represents no perturbation and 1 represents total loss of aromaticity
l of the gas giants, and the possibility of perturbation as a result of cometary outgassing/fragment
hly elliptical and subject to intense Solar perturbation at apojove which eventually pulls the comet
bright limb (day-time) because of a smaller perturbation by background light.
Such perturbation can involve more faculties in the presence
y potential that results from a third-order perturbation correction to the attractive London dispers
is used to modulate a beam of light with a perturbation device.
This explains the origin of cosmological perturbation fluctuations in inflationary models.
This is usually done through the use of perturbation functions which are simple functions which
ransition probability, based on first-order perturbation Hamiltonians, can be found in Thompson and
ν of the flat Minkowski metric plus a small perturbation hμν, and then dropping all terms which are
isentropic, which means that the fractional perturbation in the entropy of each species of particle
itical motives, seek to aggravate religious perturbation in Mexico...The names Protestant, Methodist
The tensor perturbation is truly gauge independent, since it is the
We let H be the exact matrix and P be a perturbation matrix that represents the uncertainty.
on gas model which includes a weak periodic perturbation meant to model the interaction between the
And he initiated a novel singular perturbation method, the method of composite expansions.
wrote a seminal book on this body of work: Perturbation Methods in Applied Mathematics.
, mechanics of armour penetration, singular perturbation methods, variational principles and general
The physical wavelength of a perturbation mode (dashed line) is also shown.
The plot illustrates how the perturbation mode grows larger than the horizon during c
niverse was homogeneous on the scale of the perturbation mode.
hydrodynamic efficiency to minimise the perturbation of water.
based on a perturbation of Elara on July 15, 1949.
se encounters, Vesta causes a gravitational perturbation of Arete, allowing the mass of Vesta to be
the oxygen results in the strongest single perturbation of one heteroatom in a six-membered ring.
ms by electromagnetic radiation or possible perturbation of the functioning of medical equipment by
Manev's gravitational law, given by a small perturbation of Newton's law, in the general context of
This perturbation of Daisyworld's receipt of solar radiation
tance will cause the greatest gravitational perturbation of our solar system.
, relativistic flows, quantum field theory, perturbation of the continuous spectrum, scattering theo
a book describing planetary motion and the perturbation of one planet on another in 1761, along wit
his is because the strength of the planet's perturbation on the satellite's orbit is much stronger f
the neutral-atmosphere density is the major perturbation on satellites in low earth orbit.
erstellar cloud, resulting in gravitational perturbation on a time scale that is much less than the
ld South Junction to Tapton Junction during perturbation or engineering work on the fast lines in th
a clump in the CND, which fell due to some perturbation, perhaps the supernova explosion responsibl
To correct for this orbital perturbation, regular orbital stationkeeping maneuvers a
The largest geomagnetic perturbation, resulting presumably from a "prehistoric"
Ignoring higher order perturbation terms, the following value is conserved
Depending on the symmetry of the perturbation that is used to write the LPFG, modes of di
ation interaction (MRCI) or multi-reference perturbation theories like complete active space perturb
Cavity Perturbation Theory describes methods for derivation of
s possess one asymptotic freedom within the perturbation theory described limits.
Perturbation theory is the only known approach to manage
ovides a power-counting formalism for doing perturbation theory in the small parameter ΛQCD/Q in a s
rgy limit of QCD, a description by means of perturbation theory is not possible.
caused some difficulties doing cosmological perturbation theory in this system, however the problems
mal black holes are usually performed using perturbation theory around the extremal black hole; the
Phil 1975; thesis entitled "Applications of perturbation theory to the high energy scattering of ele
In some cases, chiral perturbation theory has been successful in describing th
eloped (with N. Papanicolaou) a new type of perturbation theory for eigenvalue problems in quantum m
sing many-body techniques such as many-body perturbation theory (MBPT) and, in particular coupled cl
a region where the coupling is weak (and so perturbation theory is valid) and another region where t
The underlying assumption of cavity perturbation theory is that electromagnetic fields insid
complicated free volume techniques such as Perturbation theory and the statistical associating flui
Chiral perturbation theory (ChPT) is an effective field theory
LS force field, and his work on free-energy perturbation theory for modeling reactions in solution;
ng DFT and Hartree-Fock exchange, many-body perturbation theory (the GW method) and dynamical electr
short distance interactions, thus allowing Perturbation theory techniques to be applied.
See also: k·p perturbation theory#Effective mass
approach to renormalization theory (causal perturbation theory), where ultraviolet divergences are
f the theory (meaning they do not appear in perturbation theory).
g the spin-orbit Hamiltonian to first order perturbation theory, the energy level is given by
Compared to the perturbation theory, functional renormalization does not
methods, non-normal operators and spectral perturbation theory, Toeplitz matrices, random matrices,
ty functional theory and density functional perturbation theory, using plane wave basis sets and pse
Absence of intruder states: in perturbation theory, divergencies can occur if the energ
In contrast, perturbation theory, which deals with small perturbation
corrections can be obtained by conventional perturbation theory.
onformal invariance is kept at any order of perturbation theory.
roblem of so-called "small denominators" in perturbation theory.
f structure in the universe in cosmological perturbation theory.
an be analyzed by the methods of degenerate perturbation theory.
elativity, which adds a small inverse-cubic perturbation to the normal Newtonian gravitational poten
ber effect) to that system, where a lack of perturbation to dimensions of the network, prohibits a s
ift varies depending on moment of intertia, perturbation torques, tidal gradients, etc.
vides an efficient way to predict the field perturbation when the susceptibility distribution is kno
But the slightest perturbation will make the pencil fall into a more stabl
his Ph.D. in 1966 entitled On Partly Gentle Perturbation with Application to Perturbation by Annihil
                                                                                                    


こんにちは ゲスト さん

ログイン

Weblio会員(無料)になると

会員登録のメリット検索履歴を保存できる!

会員登録のメリット語彙力診断の実施回数増加!

無料会員に登録する
英→日 日→英
こんにちは ゲスト さん

ログイン

Weblio会員(無料)になると

会員登録のメリット検索履歴を保存できる!

会員登録のメリット語彙力診断の実施回数増加!

無料会員に登録する

©2025 GRAS Group, Inc.RSS