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But he postulated a change of human nature fostered by communism. It took many generations to prove him wrong. With the exception of a few diehards, none of today’s communist leaders hold to that orthodoxy. In the West, the moral validity of property rights is accepted, or at least acquiesced in, by virtually the whole of the population. This is true even in societies which are disdainful of competition. Attitudes toward property ownership are passed from one generation to the next through family values and education. These attitudes derive from the deepest values governing social interaction that people hold.
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しかし彼は、共産主義によりはぐくまれた人間性の変化を前提としました。彼の間違いを証明するのに何世代もかかりました。数名の頑固な抵抗者以外、今日の共産主義指導者は誰もその正当性に固執していません。 西洋では、事実上人口全体として、財産権の道徳的正当性を受け入れているか少なくとも同意しています。これは競争をさげすむ社会においてでも成り立ちます。資産の所有権に対する姿勢は1つの世代から次の世代へ、家族観や教育を通じて受け継がれていきます。こうした姿勢は人々が持つ、社会的相互作用（※1）を左右するもっとも深い価値観から生じるのです。 ※1：下記をご参照ください。 http://ja.wikipedia.org/wiki/%E7%A4%BE%E4%BC%9A%E7%9A%84%E7%9B%B8%E4%BA%92%E4%BD%9C%E7%94%A8
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しかし、彼は共産主義で育て人間性の変化を仮定した。それは彼が間違っていることを証明するために多くの世代を取った。少数のdiehardsを除いて、今日の共産主義指導者のいずれも、その正統性を保持しない。 西洋では、財産権の道徳的正当性が受け入れられているか、少なくとも人口のほぼ全体で、で黙認。これも競争の軽蔑アール社会において真である。財産の所有権に対する態度は、1つの世代から家族の価値観や教育を通して次に渡されます。これらの態度は、人々が保有している社会的な相互作用を支配する最も深い価値観に由来しています。 途中の文で書いていませんか？ これくらいなら翻訳できます。
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The numbers of collision orbits found in the present calculations are shown in Table 4 for the representative sets of (e,i). From these numbers we can expect the magnitude of statistical error in the evaluation of <P(e,i)> to be a few percent for small e, i and within 10% for large e, i for r_p=0.005 are shown in Table 5, together with those of the two-dimensional case. Interpolating these values, we have obtained the contour of <P(e,i)> and R(e,i) on the e-I plane. They are shown in Figs. 14 and 15. From Fig. 15 we can read out the general properties of the collisional rate in the three-dimensional case: (i) <P(e,i)> is enhanced over <P(e,i)>_2B except for small e and i, (ii) <P(e,i)> reduces to <P(e,i)>_2B for (e^2+i^2)^(1/2)≧4, and (iii) there are two peaks in R(e,i) near regions where e≒1 (i<1) and where i≒3 (e<0.1): the peak value is at most as large as 5. In the vicinity of small v(=(e^2+i^2)^(1/2)) and i, R(e,i) rapidly reduces to zero. This is due to a singularity of <P(e,i)>_2B at v=0 and i=0 in the ordinary expression given by Eq. (29) and hence unphysical; the behavior of collisional rate in the vicinity of small v and i will be discussed in detail later. Thus, we are able to assert, more strongly, the property (i) mentioned in the last paragraph: that is, solar gravity always enhances the collisional rate over that of the two-body approximation. One of the remarkable features of R(e,i) found in Fig. 15 is the property (ii). That is, the collisional rate between Keplerian particles is well described by the two-body approximation, for (e^2+i^2)^(1/2)≧4. This is corresponding to the two-dimensional result that R(e,0)≒1 for e≧4. よろしくお願いします。
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Regrettably, the notion of rights of ownership of capital and other income-earning assets remains conflicted, especially in societies that still believe that profit seeking is not quite moral. A key purpose of property rights, after all, is to protect assets in order to use them to profit or personally benefit. Such rights are not supportable in a society that holds any significant remnant of the view of property as “theft.” That notion embraced by Karl Marx rests on the presumption that gained wide acceptance in the first half of the twentieth century that wealth created under a division of labor is produced jointly, and hence should be owned collectively.
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We evaluated <P(e, 0)> for 12 cases of e between 0 and 6: e=0.0, 0.01, 0.1, 0.5, 0.75, 0.9, 1.0, 1.2, 1.5, 2.0, 4.0, and 6.0. As for r_p, we considered three cases: r_p=0.005, 0.001, and 0.0002. These are representative values of radii of protoplanets at the Earth, Jupiter, and Neptune orbits regions, respectively. The numbers of collision orbits found by our orbital calculation are shown in Table 3 for representative values of e. From Table 3 we can expect the statistical errors in the evaluated collisional rate to be within 5% for the cases of e≦1.5 and within 8% for e=4 and 6; they are smaller than that of the previous studies by Nishida (1983) and by Wetherill and Cox (1985). The calculated collisional rate is summarized in terms of the enhancement factor defined by Eq. (27) and shown in Fig.11, as a function of e and r_p. From Fig.11 one can see that the collisional rate is always enhanced by the effect of solar gravity, compared with that of the two-body approximation <P(e,0)>_2B. In particular, in regions where e≦1, R(e,0) is almost independent of e, having a value as large as 3. At e≦1, R(e,0) has a notable peak beyond which the enhancement factor decreases gradually with increasing e. For large values of e, i.e., e≧4, <P(e,0)> tends rapidly to <P(e,0)>_2B. As seen in the next section, we will find a similar dependence on e even in the three-dimensional case (i≠0) as long as we are concerned with cases where i≦2. お手数ですが、よろしくお願いします。
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Furthermore, ρ is the density of the planet and is taken to be 4.45g/cm^3 according to Lewis. The values of r_p/h are tabulated in Table I for various regions from the Sun. It is to be noticed that the planetary radius decreases as the increase in the distance from the Sun in the system of units adopted here. Orbital calculations are performed by means of the 4th order Runge-Kutter-Gill method with an accuracy of double precision. よろしくお願いします。
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To clarify the dynamics depending on k, we have reported a bifurcation diagram in Fig. 4. It shows different values of quantity for different values of k, particularly between 0.15 and 0.29. It is easily illustrated that we move from stability through a sequence of a period doubling bifurcations to chaos.
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As living requires physical property-food, clothing, homes- people need the legal protection to own and dispose of such property without the threat of arbitrary confiscation by the state or mobs in the street. To be sure, people have to, and do survive, in totalitarian, centrally planned societies where individual property rights are de minimis. But theirs is a lesser existence. 4行目のde minimis はラテン語で「最小限に」という意味です
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Lattice type and systematic absences In indexing the powder patterns it has been assumed that all the possible reflections are observed, that is, scattering from each of the different lattice planes is sufficiently intense to contribute to the diffraction profile. This is normally so for a primitive lattice, but for body centred and face centred lattices restrictions occur on the values that h, k and I may take if the reflections are to have any intensity. This results in certain reflections not being observed in the powder diffraction pattern and these are known as systematic absences. The origin of these absences can be illustrated with regard to Fig.2.3. という文章です。できれば翻訳サイト丸々ってのは控えてほしいです。
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Before a detailed description of our numerical procedures, we comment on above simplifications. As seen in an example of e=1.0 and i=0.5, n-recurrent (n≧3) collision orbits contribute by only 1% or less to the collision rate. On the one hand, from calculations with other e and i, the degree of contribution by n-recurrent (n≧3) collision orbits is found to be largest in the case e≒1. Hence, the error in <P(e, i)> introduced by simplification (i) is of the order of 1% or less. As for the applicability of the two-body approximation, we have confirmed in PaperII that the orbit are well described by the two-body formula inside the two-body sphere, whose radius is given by Eq. (13). No appreciable error in <P(e, i)> comes from simplification (ii). Simplification (iii) follows the discussion in the last section. Using above simplifications, we have developed numerical procedures for obtaining <P(e, i)> efficiently; their flow chart is illustrated in Fig. 10. Choosing initial values of orbital elements (e, i, b, τ_s, ω_s), we start to compute numerically Hill’s equations (6) by an ordinary fourth-order Runge-Kutta method from a starting point given by Eqs. (21) and (22). The distance r is checked at every time step of the numerical integration. If the particle flies off to a sufficient distance from the protoplanet after approaching it, i.e., if |y|>y_0+2e, (26) then, the orbital computation is stopped. If a particle approaches the protoplanet and crosses the two-body sphere surface, i.e., if r≦r_cr, the two-body formula is employed to predict whether or not a collision occurs. When no collision occurs at the first encounter, the numerical integration of Hill’s equations is continued. Since a particle which enters the two-body sphere inevitably escapes from the sphere (see Paper II), the particle follows alternatives: one is that it departs to such a distance that Eq. (26) is satisfied, and the other is that it crosses the two-body sphere surface again. In the former case, we stop the computation, considering that the orbit is non-collisional. In the latter case, the occurrence of collision is checked in the same way as earlier by means of the two-body formula, and the orbital calculation is terminated. Using the numerical procedures developed in this way, we obtain <P(e, i)> in many sets of (e, i); the results are presented in the preceeding sections. Fig. 10. Flow chart of orbital calculation for finding collision orbits. Fig. 10. 拡大画像↓ http://www.fastpic.jp/images.php?file=2113240192.jpg 長文になりますが、よろしくお願いします。
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Since the early 18th century, however, the force of the rule of law has fostered standards of living that rose by 20 times in that part of the world that embraced competitive markets. Life expectancy more than doubled. And in the developing countries that have abandoned central planning for markets since the end of the Cold War, hundreds of millions of people have been elevated from subsistence poverty. Other hundreds of millions are now experiencing a level of affluence that people born in developed nations have experienced all their lives.
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There is some evidence that these improvements in the characteristics of elders have resulted in more positive views of aging. Tibbitts claimed that during the past 30 to 40 years, U.S. society has moved from holding negative stereotypes of old people to holding positive views in which elders are seen as being able to contribute to the quality of life for themselves, their communities, and society as a whole. Schonfield even argued that the assumption of negative attitudes toward old people is a "social myth" perpetuated by the gerontological literature. We will be examining these attitudes in derail in Chapter 2, but there does appear to be a substantial shift from negative to positive attitudes. The improvements in the physical, mental,social, and economic characteristics of elders have been so marked, and there have been so many programs and services developed for elders only, that many have begun to criticize these programs as discrimination in favor of the aged, or positive ageism. We will be discussing examples of positive ageism throughout this book; but the ones that have drawn most criticism so far are the Medicare program and some features of the Social Security System, such as the automatic cost of living increases in benefits and the tax-exemption of Social Security benefits for most elders. Perhaps these programs have been criticized the most because they involve the most money. Critics are beginning to argue that since elders are no longer deprived economically and since they are now much better off mentally, physically, and socially than they were in the past, it is no longer necessary or fair to continue the enormous expense of these special supports and programs available only to elders. Some argue that the way to reduce positive ageism is to make these supports and programs available to all ages on the basis of need. For example, they recommend that the national health insurance, which only elders now enjoy, be extended to all ages. It is clear that positive ageism is becoming an important issue and promises to become even more important as we are faced with more older people and more expensive programs for "seniors only."
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