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Файл:Физика (Physics). Английский язык. Тексты для чтения, перевода и обсуждения. Учебно-методическое пособие
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persist [pR'sɪst] 1) (persist in / with) упорствовать, настойчиво, упорно прод о лжать 2) удерживаться, сохраняться, продолжать существовать
The tendency still persists. — Эта тенденция всё ещё сохраняется.
sharp [ʃɑːp] 1) остр ы й, остроконечный; отточенный 2) определённый, отчёт-
ливый (о различии, очертании и т.п.)
sharp contrast — резкий контраст
revolve [rɪ'vɔlv] 1) вращаться; вертеться, поворачиваться 2) (revolve about /
around) вертеться вокруг (чего-л.) 3) обдумывать, размышлять
to revolve a situation in the mind — серьёзно обдумывать ситуацию
integer ['ɪntɪʤR] 1) целое, нечто целое 2) целое число
algebraic integer — целое алгебраическое число
positive integer — положительное целое число, натуральное число
disturbance [dɪ'stɜːb(R)n(t)s] 1) нарушение (тишины, покоя, порядка) 2) беспо-
койство, тревога; возбуждение 3) непорядок, беспорядок; нарушение порядка 4)
возмущение, возмущающее воздействие, мешающее действие, нарушение, помеха
to cause / create / make a disturbance — причинять беспокойство
disturbances of a long nature — систематические нарушения заданного режима
работы
random disturbance — случайное возмущение
accompany [R'kʌmpRnɪ] сопровождать, следовать вместе
The speaker accompanied his angry words with forceful movements of the hands.
— Докладчик сопровождал свои резкие слова энергичными взмахами рук.
accompanied сопровождаемый
be accompanied — сопровождаться
accuracy ['ækjRrRsɪ] 1) правильность, соответствие, точность, прецизионность
accuracy of measurement — точность измерения
assembling accuracy — точность сборки
Quantum Mechanics
Within a few years, roughly between 1924 and 1930, an entirely new theoretical approach to dynamics was developed to account for subatomic behavior. Named quantum mechanics or wave mechanics, it started with the suggestion in 1923 by the French physicist Louis Victor, Prince de Broglie, that not
only electromagnetic radiation but matter could also have wave as well as particle aspects. The wavelength of the so-called matter waves associated with a

52
particle is given by the equation λ = h/mv, where m is the particle mass and v
its velocity. Matter waves were conceived of as pilot waves guiding the particle motion, a property that should result in diffraction under suitable conditions. This was confirmed in 1927 by the experiments on electron-crystal interactions by the American physicists Clinton Joseph Davisson and Lester
Halbert Germer and the British physicist Sir George Paget Thomson. Subsequently, Werner Heisenberg, Max Born, and Ernst Pascual Jordan of Germany
and the Austrian physicist Erwin Schrödinger developed Broglie's idea into a
mathematical form capable of dealing with a number of physical phenomena
and with problems that could not be handled by classical physics. In addition
to confirming Bohr's postulate regarding the quantization of energy levels in
atoms, quantum mechanics now provides an understanding of the most complex atoms, and has also been a guiding spirit in nuclear physics. Although
quantum mechanics is usually needed only on the microscopic level (with
Newtonian mechanics still satisfactory for macroscopic systems), certain macroscopic effects, such as the properties of crystalline solids, also exist that can
only be satisfactorily explained by principles of quantum mechanics.
Going beyond Broglie's notion of the wave-particle duality of matter, additional important concepts have since been incorporated into the quantummechanical picture. These include the discovery that electrons must have some
permanent magnetism and, with it, an intrinsic angular momentum, or spin, as
a fundamental property. Spin was subsequently found in almost all other elementary particles. In 1925 the Austrian physicist Wolfgang Pauli expounded
the exclusion principle, which states that in an atom no two electrons can have
precisely the same set of quantum numbers. Four quantum numbers are needed
to specify completely the state of an electron in an atom. The exclusion principle is vital for an understanding of the structure of the elements and of the periodic table. Heisenberg in 1927 put forth the uncertainty principle, which asserted the existence of a natural limit to the precision with which certain pairs
of physical quantities can be known simultaneously.
Finally, a synthesis of quantum mechanics and relativity was made in 1928
by the British mathematical physicist Paul Adrien Maurice Dirac, leading to
the prediction of the existence of the positron and bringing the development of
quantum mechanics to a culmination.

53
Largely as a result of Bohr's ideas, a different and statistical approach developed in modern physics. The fully deterministic cause-effect relations produced by Newtonian mechanics were supplanted by predictions of future
events in terms of statistical probability only. Thus, the wave property of matter also implies that, in accordance with the uncertainty principle, the motion
of the particles can never be predicted with absolute certainty even if the forces
are known completely. Although this statistical aspect plays no detectable role
in macroscopic motions, it is dominant on the molecular, atomic, and subatomic scale.
behaviour [bɪ'heɪvjR] 1) образ действий, поступки; манеры; поведение 2) хорошие манеры, хорошее поведение 3) режим (работы), поведение (физической
системы)
to exhibit behaviour — демонстрировать (какое-л.) поведен и е
dynamic behavior — динамическое поведение
equation [ɪ'kweɪʒ(R)n] 1) уравнение; равенство 2) выравниван ие ; стаби ли зац ия
according to equation — по уравнению
to formulate / state an equation — сформ улиров ать уравнение
to solve / work an equation — решить уравнение
term of equation — член уравнения
conceive [kRn'siːv] 1) постигать, понимать 2) вбивать себе в голову 3) (conceive
as) задумывать 4) испытать, ощутить, почувствовать 5) (conceive of) представлять,
воображать 6) дать начало чему-л.
suitable ['suːtRbl ], ['sjuːtRbl] годный, подходящий, пригодный, применимый,
соответствующий
eminently suitable — в высшей степени подходящий
Would it be suitable to discuss this matter at lunch? — А удобно будет обсудить
этот вопрос за обедом?
The most suitable season for transplanting the roots. — Наиболее подходящий се-
зон для пересадки корней.
subsequently ['sʌbsɪkwRntlɪ] впоследствии, позд н ее , п оз ж е , по сл е , по т ом
handle ['hændl] 1. 1) рукоять, рукоятка, ручка (двери, инструмента ) 2) удоб-
ный случай, возможность; повод, предлог 2. обрабатывать
starting handle — выключатель; пусковая рукоятка
to give / leave a handle to / for smth. — дать повод к чему-л.
to take a thing by the best handle — использовать ситуацию наилучшим
образом

54
duality [dju'ælRtɪ] 1) двойственность; дуализм 2) дуальность (в теории
адронов)
permanent ['pɜːm(R)nRnt] 1) постоянный, неизменный; долговременный; пер-
манентный 2) долговечный; постоянный 3) устойчивый; стабильный
permanent job —постоянная работа
intrinsic [ɪn'trɪn(t)sɪk ], [ɪn'trɪnzɪk] 1) присущий, свойствен ны й 2) важный, значительный, существенный
intrinsic part of the plan — существенная часть плана
spin [spɪn] вращаться, собственное вращение, закручивать, закручиваться,
собственный магнитный момент, спин
expound [ɪk'spaund ], [ek'spaund] 1) (пространно) излагать (теорию, доктрину,
принципы, идею) 2) объяснять, пояснять, интерпретировать, разъясня ть, то лко вать
The speaker has an hour to expound his views to the public. — У докладчика есть
час на изложение слушателям своих взглядов.
specify ['spesɪfaɪ] 1) точно опред ел я ть , устанавливать, предписывать; детально
излагать 2) включать в качестве пункта спецификации, подробного описания 3)
наделять особыми свойствами, придавать особый характер 4) задавать (величину,
условие), конкретизировать; детализировать
He specified the reasons of their failure. — Он проанализировал причины их не-
удачи.
The instructions specify how the medicine is to be taken. — В инструкции по
применению рассказано, как нужно принимать препарат.
to graphically specify — задавать графически, задавать графическими сред-
ствами (напр. на дисплее)
completely [kRm'pliːtlɪ] вполне, всецело, полностью, совершенно, совсем, це-
ликом
vital ['vaɪt(R)l] 1) жизненный 2) (жизненно) важный, насущный, существенный; необходимый
vital force — жизненная сила
vital energy — жизненная энергия
question of vital importance — вопрос первостепенной важности
Their aid is vital to our success. — Их помощь очень важна для успеха нашего
дела.
It is vital to be prepared for any eventuality. — Важно быть готовым к любым
случайностям.
culmination [ˌkʌlmɪ'neɪʃ(R)n] 1) кульминация; зенит 2) наивысшая точк а; высшая степень; кульминационный пункт; кульминация, вершина; венец

55
deterministic [dɪˌtɜːmɪ'nɪstɪk] детерминистический; детерминистский, обусловленный
supplant [sR'plɑːnt] выжить, вытеснить; занять (чьё-л.) место (особ. хитро-
стью)
probability [ˌprɔbR'bɪlRtɪ] 1) возмо ж но е, осуществимое, правдоподобное 2) вероятность, возможность, шанс
What are our probabilities? — Каковы наши шансы?
There is little probability that he will succeed — Маловероятно, что он
преуспеет.
There is a strong probability that the problem will recur if we do not solve it now —
Есть большая вероятность, что эта проблема вновь встанет, если не решить её
сейчас
in all probability — по всей вероятности, по всей видимости
probability of achievement of goal — вероятность выполнения задания
imply [ɪm'plaɪ] 1) предполагать, подразумевать, заключать в себе, значить 2)
выражать неявно, иметь в виду, намекать
rights imply obligations — наличие прав предполагает и наличие обязанностей
His silence implied consent. — Его молчание означало согласие.
It is not directly asserted, but it seems to be implied. — Это не утверждается
открыто, но, видимо, подразумевается.
logically imply — логически влечь
directly imply — непосредственно влечь
uncertainty [ʌn'sɜːt(R)ntɪ] 1) неуверенность, н ереш ительн ость 2) неизвес тность, неясность, неопределённость 3) недостоверность, сомнительность
statistical uncertainty — статистическая недостоверность
to be in a state of uncertainty — сомневаться, колебаться
uncertainty of measurement — недостоверность измерений (характеризующая
область нахождения истинного значения измеряемой величины)
detectable [dɪ'tektRbl] могущий быть обнаруженным
Nuclear Physics
The understanding of atomic structure was also facilitated by Becquerel's
discovery in 1896 of radioactivity in uranium ore. Within a few years radioactive radiation was found to consist of three types of emissions: alpha rays, later
found by Rutherford to be the nuclei of helium atoms; beta rays, shown by
Becquerel to be very fast electrons; and gamma rays, identified later as very

56
short wavelength electromagnetic radiation. In 1898 the French physicists Marie and Pierre Curie separated two highly radioactive elements, radium and
polonium, from uranium ore, thus showing that radiations could be identified
with particular elements. By 1903 Rutherford and the British physical chemist
Frederick Soddy had shown that the emission of alpha or beta rays resulted in
the transmutation of the emitting element into a different one. Radioactive processes were shortly thereafter found to be completely statistical; no method
exists that could indicate which atom in a radioactive material will decay at
any one time. These developments, in addition to leading to Rutherford's and
Bohr's model of the atom, also suggested that alpha, beta, and gamma rays
could only come from the nuclei of very heavy atoms. In 1919 Rutherford
bombarded nitrogen with alpha particles and converted it to hydrogen and oxygen, thus producing the first artificial transmutation of elements.
Meanwhile, a knowledge of the nature and abundance of isotopes was
growing, largely through the development of the mass spectrograph. A model
emerged in which the nucleus contained all the positive charge and almost all
the mass of the atom. The nuclear-charge carriers were identified as protons,
but except for hydrogen, the nuclear mass could be accounted for only if some
additional uncharged particles were present. In 1932 the British physicist Sir
James Chadwick discovered the neutron, an electrically neutral particle of
mass 1.675 × 10
-27
kg, slightly more than that of the proton. Now nuclei could
be understood as consisting of protons and neutrons, collectively called nucleons, and the atomic number of the element was simply the number of protons
in the nucleus. On the other hand, the isotope number, also called the atomic
mass number, was the sum of the neutrons and protons present. Thus, all atoms
of oxygen (atomic no. 8) have eight protons, but the three isotopes of oxygen,
17
O16, O
, and O18, also contain within their respective nuclei eight, nine, or ten
neutrons.
Positive electric charges repel each other, and because atomic nuclei (except for hydrogen) have more than one proton, they would fly apart except for
a strong attractive force, called the nuclear force, or strong interaction that
binds the nucleons to each other. The energy associated with this strong force
is very great, millions of times greater than the energies characteristic of electrons in their orbits or chemical binding energies. An escaping alpha particle

57
(consisting of two protons and two neutrons), therefore, will have to overcome
this strong interaction force to escape from a radioactive nucleus such as uranium. This apparent paradox was explained by the American physicists Edward U. Condon, George Gamow, and Ronald Wilfred Gurney, who applied
quantum mechanics to the problem of alpha emission in 1928 and showed that
the statistical nature of nuclear processes allowed alpha particles to “leak” out
of radioactive nuclei, even though their average energy was insufficient to
overcome the nuclear force. Beta decay was explained as a result of a neutron
disruption within the nucleus, the neutron changing into an electron (the beta
particle), which is promptly ejected, and a residual proton. The proton left behind leaves the “daughter” nucleus with one more proton than its “parent” and
thus increases the atomic number and the position in the periodic table. Alpha
or beta emission usually leaves the nucleus with excess energy, which it unloads by emitting a gamma-ray photon.
In all these nuclear processes a large amount of energy, given by Einstein's
E = mc2 equation, is released. After the process is over, the total mass of the
product is less than that of the parent, with the mass difference appearing as
energy.
facilitate [fR'sɪlɪteɪt] облегчать; содействовать; способствовать; помогать, про-
двигать
separate 1. ['sep(R)rRt] 1. отдельный; обособленный; разрозненный, разъединённый 2. выделять, отделять
to separate out — отделяться; разделяться; выпадать в осадок
transmutation [ˌtrænzmjuː'teɪʃ(R)n ],[ ˌtræn(t)smjuː'teɪʃ(R)n] 1) изменение, превращение, преобразование 2) превращение, трансмутация (в радиобиологии)
nuclear transmutation — ядерное превращение
decay [dɪ'keɪ] 1. 1) гнить, разлагаться (об органических веществах) 2) разрушаться, ветшать (о физических предметах) 3) а) угасать, расстраиваться, иссякать (о здоровье, силах) 4) приходить в упадок, разлагаться 5) затухать (спадат ь) ,
распад, распадаться, спад
decay of oscillations — затухание колебаний
initial rapid decay — начальный быстрый спад (нейтронов)
artificial [ˌɑːtɪ'fɪʃ(R)l] 1) искусственный, ненатуральный, неестественный
artificial atmosphere — кондиционированный воздух
artificial intelligence искусственный интеллект

58
meanwhile [ˌmiːn'waɪl] 1) = in the meanwhile тем временем, между тем, пока 2)
тем временем, в это время, одновременно 3) в то же время, при этом
I knew I wouldn't get my exam results for several weeks, and I wasn't sure what to
do in the meanwhile. — Я знал, что результаты экзаменов будут только через не-
сколько недель, и не знал, что мне делать всё это время.
abundance [R'bʌndRn(t)s] 1) изобилие; избыток 2) относительное содержание
3) распространённость
abundance ratio — относительная распространённость
repel [rɪ'pel] 1) отбрасывать, отражать 2) подавлять, сдерживать
average ['æv(R)rɪʤ] 1. 1) средний 2) нормальный, обыкновенный, обычный,
средний 2. среднее число; средняя величина; среднее (по сумме нескольких вели-
чин) 3. выводить среднее число, усреднять
above the average — выше среднего
below the average — ниже среднего
on average — в среднем
average output — средний выпуск (продукции)
average rate of profit — средняя норма прибыли
roughness average — среднее арифметическое отклонение профиля
disruption [dɪs'rʌpʃ(R)n] 1) разрушение, поломка (напр. инструмента)2) разрыв; подрыв 3) распад, дезинтеграция (пород) 4) пробой 5) неустой чи во сть срыва,
разрушение, срыв (разряда)
complete, total disruption — полное разрушение
DEVELOPMENTS IN PHYSICS SINCE 1930
The rapid expansion of physics in the last few decades was made possible
by the fundamental developments during the first third of the century, coupled
with recent technological advances, particularly in computer technology, electronics, nuclear-energy applications, and high-energy particle accelerators.
Accelerators
Rutherford and other early investigators of nuclear properties were limited
to the use of high-energy emissions from naturally radioactive substances to
probe the atom. The first artificial high-energy emissions were produced in
1932 by the British physicist Sir John Douglas Cockcroft and the Irish physi-

59
cist Ernest Thomas Sinton Walton, who used high-voltage generators to accelerate protons to about 700,000 eV and to bombard lithium with them, transmuting it into helium. One electron volt is the energy gained by an electron
when the accelerating voltage is 1 V; it is equivalent to about 1.6 × 10
-19
joule
(J). Modern accelerators produce energies measured in million electron volts
(usually written mega-electron volts, or MeV), billion electron volts (gigaelectron volts, or GeV), or trillion electron volts (tera-electron volts, or TeV).
Higher-voltage sources were first made possible by the invention, also in 1932,
of the Van de Graaff generator by the American physicist Robert van de
Graaff.
This was followed almost immediately by the invention of the cyclotron by
the American physicists Ernest Orlando Lawrence and Milton Stanley Livingston. The cyclotron uses a magnetic field to bend the trajectories of charged
particles into circles, and during each half-revolution the particles are given a
small electric “kick” until they accumulate the high energy level desired. Protons could be accelerated to about 10 MeV by a cyclotron, but higher energies
had to await the development of the synchrotron after the end of World War II
(1939-1945), based on the ideas of the American physicist Edwin Mattison
McMillan and the Soviet physicist Vladimir I. Veksler. After World War II,
accelerator design made rapid progress, and accelerators of many types were
built, producing high-energy beams of electrons, protons, deuterons, heavier
ions, and X rays. For example, the accelerator at the Stanford Linear Accelerator Center (SLAC) in Stanford, California, accelerates electrons down a
straight “runway,” 3.2 km (2 mi) long, at the end of which they attain an energy of more than 20 GeV.
While lower-energy accelerators are used in various applications in industry and laboratories, the most powerful ones are used in studying the structure
of elementary particles, the fundamental building blocks of nature. In such
studies elementary particles are broken up by hitting them with beams of projectiles that are usually protons or electrons. The distribution of the fragments
yields information on the structure of the elementary particles.
To obtain more detailed information in this manner, the use of more energetic projectiles is necessary. Since the acceleration of a projectile is achieved
by “pushing” it from behind, to obtain more energetic projectiles it is neces-

60
sary to keep pushing for a longer time. Thus, high-energy accelerators are generally larger in size. The highest beam energy reached at the end of World War
II was less than 100 MeV. A bigger accelerator, reaching 3 GeV, was built in
the early 1950s at the Brookhaven National Laboratory at Upton, New York. A
breakthrough in accelerator design occurred with the introduction of the strong
focusing principle in 1952 by the American physicists Ernest D. Courant, Livingston, and Hartland S. Snyder. Today the world's largest accelerators have
been or are being built to produce beams of protons beyond 1 TeV. Two are
located at the Fermi National Accelerator Laboratory, near Batavia, Illinois,
and at the European Organization for Nuclear Research, known as CERN, in
Geneva, Switzerland.
rapid ['ræpɪd] 1) быстрый, скорый, стремительный 2) быстро перемещаться;
перемещать на ускоренном ходу, перемещаться на ускоренном ходу
rapid growth — быстрый рост
application [ˌæplɪ'keɪʃ(R)n] 1) просьба; заявление; форма заявления 2) приме-
нение, использование, употребление; приложение; примени м ос ть
application of new techniques — применение новых технологий
the place of application of a force — место приложения силы
to file / make / put in / send in / submit an application — подавать заявление, по-
давать прошение
to reject application / turn down application — отказать в прошении
to withdraw an application — забирать прошение
substance ['sʌbst(R)n(t)s] 1) вещество 2) содержание, суть, сущность; существо
in substance — по существу; по сути
chemical substance — химическое вещество
hard substance — твёрдое вещество
harmful substance — вредное вещество
probe [prRub] 1. 1) зондировать 2) прощупы вать; опробовать; проводить испытание 2. 1) а) зонд б) зонд, щуп; датчик, пробник, щуп (измерительного прибора)
direct contact probe — 1) щуп; контактный датчик 2) контактная измерительная головка
optical triangulation probe — оптический триангуляционный датчик (напр. для
измерения сложных и объёмных контуров)
transmute [trænz'mjuːt ],[ træn(t)s'mjuːt] а) изменяться, превращаться, преобразовываться б) изменять, превращать, преобразовывать
to transmute water power into electrical power — преобразовывать силу воды в
электрическую энергию
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