誓约流，建议没考的筒子们去看看那个暗物质原文

crystalli15

今天下午考的，730，不是啥高分就不多说了。四篇月度都是狗，期中那个暗物质的记忆犹新，所以建议大家去看看考古里的暗物质原文，是那个从GOOGLE图书下来的哦~~别看错了。 做题的时候发现基本不用看文章，按照背景知识直接勾了~（其实有很多句子几乎和考古里的原文一样）。
还有输血精一定要看，特别是200+以后的，我遇到很多200+以后的题~~在想是不是裤子末期考的题是不是也侧重特定的一些~~因为考前看到几个北美的筒子的精，发现很高相似度~~或者大家都在北美的缘故？~算了，巧合吧，别理我了。
不再多说，没有精我输血就没有满分了~
坐稳AA是organic food， AI是，leader 是不是要是最experienced那个~
祝大家好运呀~~

killerinJP

感谢~

waner821

感谢Lz，Lz觉得语法遇到的题常规不？还是很难之类的？~看这几天的貌似语法都比较棘手...

阿狸猪

好像很多都反映月度狗狗很全的样子了。。
哎 是不是这是换裤裤的标志了啊？
真担心。。。

angelazhao222

暗物质 dark matter可以回忆一下题目吗？谢谢！恭喜搂住！！！

vivianxiong

暗物质 dark matter可以回忆一下题目吗？谢谢！恭喜搂住！！！

-- by 会员 angelazhao222 (2010/10/7 16:14:14)

我的阅读狗狗里头有收入那个dark matter的片段哈~
可以下来看看~

berniceyunle

谢谢，并祈祷后天不要换裤子~~

qushangxue

哪里有暗物质原文？  这个月的狗狗里？

qushangxue

暗物质 dark matter可以回忆一下题目吗？谢谢！恭喜搂住！！！

-- by 会员 angelazhao222 (2010/10/7 16:14:14)

我的阅读狗狗里头有收入那个dark matter的片段哈~
可以下来看看~

-- by 会员 vivianxiong (2010/10/7 17:08:15)

是google的？

chelseadu

Passage 8
Virtually everything astronomers known about objects
outside the solar system is based on the detection of
photons-quanta of electromagnetic radiation. Yetthere
isanotherformofradiationthatpermeatestheuniverse:
(5)neutrinos. With (as its name implies) no electric charge,
and negligible mass, the neutrino interacts with other
particles so rarely that a neutrino can cross the entire
universe, even traversing substantial aggregations of
matter, without being absorbed or even deflected. Neu-
(10) trinos can thus escape from regions of space where light
and other kinds of electromagnetic radiation are blocked
by matter. Furthermore, neutrinos carry with them
information about the site and circumstances of their
production: therefore, the detection of cosmic neutrinos
(15) could provide new information about a wide variety of
cosmic phenomena and about the history ofthe uni-
verse.
But how can scientists detect a particle that interacts
so infrequently with other matter? Twenty-five years
(20) passed between Pauli's hypothesis thatthe neutrino
existed and its actual detection: since then virtually all
research with neutrinos has been with neutrinos created
artificially in large particle accelerators and studied
under neutrino microscopes. But a neutrino telescope,
(25) capable of detecting cosmic neutrinos, is difficult to co-
nstruct. No apparatus can detect neutrinos unless it is
extremely massive, because great mass is synonymous
with huge numbers of nucleons (neutrons and protons),
and the more massive the detector, the greater the pro-
(30) bability of one of its nucleon's reacting with a neutrino.
In addition, the apparatus must be sufficiently shielded
from the interfering effects of other particles.
Fortunately, a group of astrophysicists has proposed
a means of detecting cosmic neutrinos by harnessing the
(35) mass ofthe ocean. Named DUMAND, for Deep Under-
water Muon and Neutrino Detector, the project calls for
placing an array of light sensors at a depth of five kilo-
meters under the ocean surface. The detecting medium is
the seawater itself: when a neutrino interacts with a
(40)particle in an atom of seawater. the result is a cascade of
electrically charged particles and a flash of light that can
be detected by the sensors. The five kilometers of sea-
water above the sensors will shield them from the interf-
ering effects of other high-energy particles raining down
(45) through the atmosphere.
The strongest motivation for the DUMAND project
isthat it will exploit an important source of information
about the universe. The extension of astronomy from
visible light to radio waves to x-rays and gamma rays
(50) never failed to lead to the discovery of unusual objects
such as radio galaxies, quasars, and pulsars. Each of
these discoveries came as a surprise. Neutrino astronomy
will doubtless bring its own share of surprises.

1. Which ofthe following titles best summarizes the passage as a whole?
(A) At the Threshold of Neutrino Astronomy
(B) Neutrinos and the History ofthe Universe
(C) The Creation and Study of Neutrinos
(D) The DUMAND System and How It Works
(E) The Properties ofthe Neutrino
2. With which ofthe following statements regarding neutrino astronomy would the author be most likely to agree?
(A) Neutrino astronomy will supersede all present forms of astronomy.
(B) Neutrino astronomy will be abandoned if the DUMAND project fails.
(C) Neutrino astronomy can be expected to lead to major breakthroughs in astronomy.
(D) Neutrino astronomy will disclose phenomena that will be more surprising than past discoveries.
(E) Neutrino astronomy will always be characterized by a large time lag between hypothesis and experimental confirmation.
3. In the last paragraph, the author describes the development of astronomy in order to
(A) suggest thatthe potential findings of neutrino astronomy can be seen as part of a series of astronomical successes
(B) illustrate the role of surprise in scientific discovery
(C) demonstrate the effectiveness ofthe DUMAND apparatus in detecting neutrinos
(D) name some cosmic phenomena that neutrino astronomy will illuminate
(E) contrast the motivation of earlier astronomers with thatofthe astrophysicists working on the DUMAND project
4. According to the passage, one advantage that neutrinos have for studies in astronomy isthat they
(A) have been detected for the last twenty-five years
(B) possess a variable electric charge
(C) are usually extremely massive
(D) carry information about their history with them
(E) are very similar to other electromagnetic particles
5. According to the passage, the primary use ofthe apparatus mentioned in lines 24-32 would be to
(A) increase the mass of a neutrino
(B) interpret the information neutrinos carry with them
(C) study the internal structure of a neutrino
(D) see neutrinos in distant regions of space
(E) detect the presence of cosmic neutrinos
6. The passage states that interactions between neutrinos and other matter are
(A) rare
(B) artificial
(C) undetectable
(D) unpredictable
(E) hazardous
7. The passage mentions which ofthe following as a reason that neutrinos are hard to detect?
(A) Their pervasiveness in the universe
(B) Their ability to escape from different regions of space
(C) Their inability to penetrate dense matter
(D) The similarity of their structure to thatof nucleons
(E) The infrequency of their interaction with other matter
8. According to the passage, the interaction of a neutrino with other matter can produce
(A) particles that are neutral and massive
(B) a formofradiationthatpermeatesthe universe
(C) inaccurate information about the site and circumstances ofthe neutrino’s production
(D) charged particles and light
(E) a situation in which light and other forms of electromagnetic radiation are blocked
9. According to the passage, one ofthe methods used to establish the properties of neutrinos was
(A) detection of photons
(B) observation ofthe interaction of neutrinos with gamma rays
(C) observation of neutrinos that were artificially created
(D) measurement of neutrinos that interacted with particles of seawater
(E) experiments with electromagnetic radiation