[Data Sufficiency]
试题详情
题目:
If n is an integer and
, what is the value of x ?
(1) x is an integer.
(2) 
选项:
答案:
E
| Line | Frazier and Mosteller assert that medical research |
| could be improved by a move toward larger, simpler | |
| clinical trials of medical treatments. Currently, | |
| researchers collect far more background information | |
| (5) | on patients than is strictly required for their trials— |
| substantially more than hospitals collect—thereby | |
| escalating costs of data collection, storage, and | |
| analysis. Although limiting information collection | |
| could increase the risk that researchers will overlook | |
| (10) | facts relevant to a study, Frazier and Mosteller |
| contend that such risk, never entirely eliminable from | |
| research, would still be small in most studies. Only | |
| in research on entirely new treatments are new and | |
| unexpected variables likely to arise. | |
| (15) | Frazier and Mosteller propose not only that |
| researchers limit data collection on individual | |
| patients but also that researchers enroll more | |
| patients in clinical trials, thereby obtaining a more | |
| representative sample of the total population with | |
| (20) | the disease under study. Often researchers restrict |
| study participation to patients who have no ailments | |
| besides those being studied. A treatment judged | |
| successful under these ideal conditions can then be | |
| evaluated under normal conditions. Broadening the | |
| (25) | range of trial participants, Frazier and Mosteller |
| suggest, would enable researchers to evaluate a | |
| treatments efficacy for diverse patients under various | |
| conditions and to evaluate its effectiveness for | |
| different patient subgroups. For example, the value | |
| (30) | of a treatment for a progressive disease may vary |
| according to a patients stage of disease. Patients | |
| ages may also affect a treatments efficacy. |
| Line | When asteroids collide, some collisions cause |
| an asteroid to spin faster; others slow it down. If | |
| asteroids are all monoliths—single rocks—undergoing | |
| random collisions, a graph of their rotation rates | |
| (5) | should show a bell-shaped distribution with statistical |
| tails of very fast and very slow rotators. If asteroids | |
| are rubble piles, however, the tail representing the | |
| very fast rotators would be missing, because any | |
| loose aggregate spinning faster than once every few | |
| (10) | hours (depending on the asteroids bulk density) |
| would fly apart. Researchers have discovered that | |
| all but five observed asteroids obey a strict limit on | |
| rate of rotation. The exceptions are all smaller than | |
| 200 meters in diameter, with an abrupt cutoff for | |
| (15) | asteroids larger than that. |
| The evident conclusion—that asteroids larger than | |
| 200 meters across are multicomponent structures | |
| or rubble piles—agrees with recent computer modeling | |
| of collisions, which also finds a transition at that | |
| (20) | diameter. A collision can blast a large asteroid to bits, |
| but after the collision those bits will usually move | |
| slower than their mutual escape velocity. Over several | |
| hours, gravity will reassemble all but the fastest | |
| pieces into a rubble pile. Because collisions among | |
| (25) | asteroids are relatively frequent, most large bodies |
| have already suffered this fate. Conversely, most | |
| small asteroids should be monolithic, because impact | |
| fragments easily escape their feeble gravity. |