GRE-练习二十及答案解析.doc
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1、GRE-练习二十及答案解析(总分:100.00,做题时间:90 分钟)一、BIndefinite item(总题数:27,分数:100.00)1.If a supernova (the explosion of a massive star) triggered star formation from dense clouds of gas and dust, and if the most massive star to be formed from the cloud evolved into a supernova and triggered a new round of star fo
2、rmation, and so on, then a chain of star-forming regions would result. If many such chains were created in a differentially rotating galaxy, the distribution of stars would resemble the observed distribution in a spiral galaxy.This line of reasoning underlies an Uexciting/U new theory of spiral-gala
3、xy structure. A computer simulation based on this theory has reproduced the appearance of many spiral galaxies without assuming an underlying density wave, the hallmark of the most widely accepted theory of the large-scale structure of spiral galaxies. That theory maintains that a density wave of sp
4、iral form sweeps through the central plane of a galaxy, compressing clouds of gas and dust, which collapse into stars that form a spiral pattern. The authors attitude toward the new theory of spiral-galaxy structure can best be described as A. euphoric. B. enthusiastic. C. concerned. D. critical. E.
5、 disputatious.(分数:4.00)A.B.C.D.E.2.A mysterious phenomenon is the ability of over-water migrants to travel on course. Birds, bees, and other species can keep track of time without any sensory cues from the outside world, and such “biological clocks“ clearly contribute to their “compass sense“. For e
6、xample, they can use the position of the Sun or stars, along with the time of day, to find north. But compass sense alone cannot explain how birds navigate the ocean: after a flock traveling east is blown far south by a storm, it will assume the proper northeasterly course to compensate. Perhaps, so
7、me scientists thought, migrants determine their Ugeographic position on Earth by celestial navigation/U, almost as human navigators use stars and planets, Ubut this would demand of the animals a fantastic map sense./U Researchers now know that some species have a magnetic sense, which might allow mi
8、grants to determine their geographic location by detecting variations in the strength of the Earths magnetic field.In maintaining that migrating animals would need “a fantastic map sense“ to determine their geographic position by celestial navigation, the author intends to express A. admiration for
9、the ability of the migrants. B. skepticism about celestial navigation as an explanation. C. certainty that the phenomenon of migration will remain mysterious. D. interest in a new method of accounting for over-water migration. E. surprise that animals apparently navigate in much the same way that hu
10、man beings do.(分数:4.00)A.B.C.D.E.3.Tocqueville, apparently, was wrong. Jacksonian America was not a fluid, egalitarian society where individual wealth and poverty were ephemeral conditions. At least so argues E. Pessen in his iconoclastic study of the very rich in the United States between 1825 and
11、1850.Pessen does present a quantity of examples, together with some Urefreshingly intelligible statistics,/U to establish the existence of an inordinately wealthy class. Though active in commerce or the professions, most of the wealthy were not self-made, but had inherited family fortunes. In no sen
12、se mercurial, these great fortunes survived the financial panics that destroyed lesser ones. Indeed, in several cities the wealthiest one percent constantly increased its share until by 1850 it owned half of the communitys wealth. Although these observations are true, Pessen overestimates their impo
13、rtance by concluding from them that the undoubted progress toward inequality in the late eighteenth century continued in the Jacksonian period and that the United States was a class-ridden, plutocratic society even before industrialization.The authors attitude toward Pessens presentation of statisti
14、cs can be best described as A. disapproving B. shocked C. suspicious D. amused E. laudatory(分数:4.00)A.B.C.D.E.4.The intensive work of materials scientists and solid-state physicists has given rise to a class of solids known as amorphous metallic alloys, or glassy metals. There is a growing interest
15、among theoretical and applied researchers alike in the structural properties of these materials.When a molten metal or metallic alloy is cooled to a solid, a crystalline structure is formed that depends on the particular alloy composition. In contrast, molten nonmetallic glass-forming materials, whe
16、n cooled, do not assume a crystalline structure, but instead retain a structure somewhat like that of the liquidan amorphous structure. At room temperature, the natural long-term tendency for both types of materials is to assume the crystalline structure. The difference between the two is in the kin
17、etics or rate of formation of the crystalline structure, which is controlled by factors such as the nature of the chemical bonding and the ease with which atoms move relative to each other. Thus, in metals, the kinetics favors rapid formation of a crystalline structure, whereas in nonmetallic glasse
18、s the rate of formation is so slow that almost any cooling rate is sufficient to result in an amorphous structure. For glassy metals to be formed, the molten metal must be cooled extremely rapidly so that crystallization is suppressed.The structure of glassy metals is thought to be similar to that o
19、f liquid metals. One of the first attempts to model the structure of a liquid was that by the late J.D. Bernal of the University of London, who packed hard spheres into a rubber vessel in such a way as to obtain the maximum possible density. The resulting dense, random-packed structure was the basis
20、 for many attempts to model the structure of glassy metals. Calculations of the density of alloys based on Bernal-type models of the alloys metal component agreed fairly well with the experimentally determined values from measurements on alloys consisting of a noble metal together with a metalloid,
21、such as alloys of palladium and silicon, or alloys consisting of iron, phosphorus, and carbon, although small discrepancies remained. One difference between real alloys and the hard spheres used in Bernal models is that the components of an alloy have different sizes, so that models based on two siz
22、es of spheres are more appropriate for a binary alloy, for example, the smaller metalloid atoms of the alloy might fit into holes in the dense, random-packed structure of the larger metal atoms.One of the most promising properties of glassy metals is their high strength combined with high malleabili
23、ty. In usual crystalline materials, one finds an inverse relation between the two properties, whereas for many practical applications simultaneous presence of both properties is desirable. UOne residual obstacle to practical applications that is likely to be overcome is the fact that glassy metals w
24、ill crystallize at relatively low temperatures when heated slightly./UThe authors attitude toward the prospects for the economic utilization of glassy metals is one of _. A. disinterest B. impatience C. optimism D. apprehension E. skepticism(分数:4.00)A.B.C.D.E.5.When the same parameters and quantitat
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