「perturbation」の共起表現一覧(1語右で並び替え)
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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 |
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