ATOMIC STRUCTURE

The discovery of the electron by Thomson gave proof that atoms must have a structure, that is, that atoms are not simple, indivisible particles of matter. But the electron could not account for the mass of atom, since the mass of the electron is very small in comparison to that of the atom, even the lightest atom known, hydrogen. And in addition the electron is negatively charged, but atoms are ordinarily neutral. J.J. Thomson and others at first thought that the mass of the atom was due to the presence of many electrons, 1840 of them in the case of hydrogen, many more for the atoms of heavier elements, and that they were embedded in some almost massless plasma of positive charge that would make the atom as a whole electrically neutral. As early as 1898 Thomson had proposed a model of the atom in which the electrons were embedded in successive rings within a masive matrix of positive charge, which was thought to occupy a volume of about one atomic diameter, which was long known to be between 1 and 10 angstrom units (= 1 × 10-10 m.), a fact inferred from the sizes of molar volumes and Avogadro's number. This model has been called the "plum pudding" model because the electrons were imagined to be arranged like raisins in a pudding. But this concept of the structure of the atom was refuted by Ernest Rutherford's (1871-1937) with his discovery of the nucleus of the atom in 1911.

  1. ALPHA SCATTERING EXPERIMENT.
    Since there is no direct way to find out the structure of the atom, an indirect method must be used. Rutherford devised an apparatus using alpha particles emitted by an radioactive source which are limited to a fine beam by a thick lead screen having in it a small hole. The beam of alpha particles with speeds of about 2 × 109 cm/sec fall on a thin foil of gold about 4 × 10-5 cm thick, and those that are deviated or scattered by the gold foil are detected by counting the scintillations on a fluorescent screen placed at different angular positions about the gold foil. The alpha particles produce little flashes of light, or scintillations, on the fluorescent screen. Rutherford found that most of the alpha particles went straight through the gold foil with little deviation, showing that atoms are not "solid"; but that a few were scattered at large angles, some even nearly reversed in direction. Wide angle scattering was completely contrary to what had been expected from electrons; the electrons of which atoms were thought to be composed of would have little mass and negative charge that they could not produce such deviations. Rutherford said years later in 1936;
    "It was quite the most incredible event that has ever happened to me in my life. It was as though you had fired a 15-inch shell at a piece of tissue paper and it came back and hit you."
    Rutherford found that he could account for this result, if he assumed that all the positive charge repelling the positive alpha particles, and nearly all the mass of the atom as well, were confined to a very small volume at the center of the atom, which he called the nucleus of the atom. Rutherford showed that a tremendous amount of force necessary to produce the backward scattering would be exerted only at a distance of about 10-12 cm, and by a positive charge which for case of gold he first estimated to about 100 times the charge on the electron. The correct value was later determined to be 79 and not 100. He concluded that the atomic diameter must be in the order of 10-8 cm. This experiment clearly indicated that the negatively charged electrons must be distributed throughout the volume of this diameter and that the positive charge and most of the mass of the atom are much more concentrated. The mass of the electrons being almost negligible compared with that of even the lighest atom as a whole, most of the mass is concentrated within a radius that compared to the total atomic radius is analogous to that between the sun's radius and the radius of the total solar system at Pluto's orbit. This view of the atom is that the atom is mostly empty space. Only this account for the relative ease that they are penetrated by the alpha particles through thousands of atoms. On the basis of the atomic dimensions deduced from kinetic theory, the gold foil consisted of about 103 layers of atoms.

    It occurred to Rutherford and others that each atom is like a miniature solar system, with the electrons orbiting about the nucleus like the planets orbiting about sun, and with electrical attraction between the positive nucleus and the negative electrons instead of the gravitational attraction between the sun and the planets in the solar system. But there were objections to this view. The electrons in their circular orbit about the nucleus would be accelerating, and according to the principles of electricity and magnetism any accelerated charge would emit electromagnetic radiation and thus loses energy. Calculations showed that electrons would lose their kinetic energy and would spiral into the attracting nucleus in a very short period of time, but the matter that we are experiencing have not collapsed nor radiated electromagnetic radiation as that would be given off by a spiraling electron. This raises the problem how the radiation is emitted by atoms. Any satisfactory model of the atom must account for the radiation that is actually observed.

  2. ATOMIC SPECTRA.
    When a continuous electrical discharge between two electrodes in a glass tube through a gas at low prssure, there is produced a glow of light whose wavelengths are characteristic of the particular gas in the tube. When this light is analyzed by a prism, instead of continuous spectrum, it is seen to consist of very few wavelengths, most of the spectrum being empty. Most spectroscopes are made with slit apertures, and so the spectrum appears on the screen or photographic plate as a series of lines corresponding to the wavelengths present in the original beam of light. This spectrum is called a line emission spectrum. Different gases give different number and arrangement of lines. In 1823 the British astronomer J. Herschel suggested that each gas could be identified from its unique line spectrum. Since then the line emission spectrum has been used like a fingerprints are used to identify and trace a person. This was the beginning of the important branch of physical science known as spectrum analysis. By the 1860's the physicist Gustav R. Kirchhoff and the chemist Robert W. Bunsen at the University of Heidelberg, who are regarded as the inventor of the spectrascope, had jointly discovered two new elements, rubidium and cesium, by noting that previously unidentified emission lines in the spectrum of mineral water.

    The simplest line spectrum comes from hydrogen gas. There is certain regularity in the line arrangement, but the difference in the wavelengths of the various lines diminishes rapidly toward the shorter wavelengths. This suggests that they could be represented by an algebraic or geometric series. But there is no simple series corresponding to the measured lines. In 1883 after many attempts, a German high school teacher, Johann Balmer (1825-1898), worked out a purely empirical formula that seemed to fit the measured lines very well.
    λ = 3645.6[n2/(n2 - 4)], (1)
    where λ is the wavelength in Angstroms = 10-8 cm, and n is a whole number equal to 3, 4, 5, 6, ... infinity. When n is placed equal to 3 in the formula, a wavelength is obtained very close to that of the first line in the hydrogen series. The following table shows the observed wavelengths and the calculated wavelengths using the Balmer formula.
    Balmer Series
    n Observed Wavelength Calculated Wavelength
    3 6562.84 6562.79
    4 4861.46 4861.33
    5 4340.58 4340.47
    6 4101.76 4101.74
    etc.
    There is extraordinarly good agreement between the observed and calculated wavelengths. Note there are no wavelength calculated for n equal to 1 and 2, because these calculations result in an infinite and a negative wavelength and do not correspond to physical wavelengths.

    The first half-dozen or so of these wavelengths are visible to the human eye. And when the spectrum is examined with an instrument sensitive to the ultraviolet and infrared light from hydrogen, more lines are found, and many of these do not fit with values given by the Balmer formula. In 1890 Johannes Rydberg showed that if the Balmer formula is modified, then the Balmer formula can be extended to include lines observed in the spectra of other elements. The following is the Rydberg formula:
    1/λ = R(1/m2 - 1/n2), (2)
    where
    λ is the wavelength of a line measured in meters,
    R is Rydberg's constant = 1.09678 × 107 m-1 for hydrogen,
    m is an integral number,
    n is an integral number = (m + 1), (m + 2), ... infinity.
    If m is set equal to 2 in the above formula, then it becomes equivalent to the formula given by Balmer.
    In 1908 Louis C. Paschen observed another series of lines at shorter wavelengths to those in the Balmer series. He showed that they correspond to the wavelengths calculated by the Rydberg formula when m = 3. Later another series still further in the infrared was found by Brackett, and yet a further one by Pfund. The lines in these series are given precisely by the Rydberg formula, if m is given the value of 4 and 5. Is there a series for m = 1? Yes, there is a series in the ultraviolet, and it was found by Theodore Lyman during the period from 1906 to 1916.
    Name of Series Date of Discovery Region of Spectrum Values in Rydberg Formula
    Lyman 1906-1914 Ultraviolet m = 1, n = 2, 3, 4, ...
    Balmer 1885 Uv & visible m = 2, n = 3, 4, 5, ...
    Paschen 1908 Infrared m = 3, n = 4, 5, 6, ...
    Brckett 1922 Infrared m = 4, n = 5, 6, 7, ...
    Pfund 1924 Infrared m = 5, n = 6, 7, 8, ...
    If λ is the wavelength of a spectral line measured in meters, then 1/λ gives the number of wavelengths that there ae in one meter. This is called the wave number k of the lines. Thus the Rydberg formula can be rewritten and can be expressed as difference between terms.
    k = R/m2 - R/n2, (3)
    where R/m2 and R/n2 are called terms.

  3. PLANCK'S QUANTUM HYPOTHESIS.
    In addition to the line emission spectra there are continuous emission spectra. Newton had shown, in the "celebrated experiment," that the light from the sun could be resolved into a spectrum (Newton coined the word) of various colors; this "rainbow" spectrum could also obtained by examining the light from all glowing solids (wire filament, carbon arc) and glowing liquids (molten metals). These emission spectra have three common features.
    1. They are continuous spectra, that is, there are no gaps, no color bands missing from the spectrum, even if the observations are carried into the infrared or ultraviolet region. An exception is the spectrum of sunlight. When sunlight is passed through a narrow slit and its visible spectrum very carefully examined with a good prism system, the continuity of colors appeared to be distrupted by a series of fine, steady, irregularly spaced dark lines. In 1814 the German optician Joseph Fraunhofer studied this peculiarity and he counted more than 700 such lines and assigned the letters A, B, C, ... to the most prominent ones. They are still referred to as the Fraunhofer lines. In 1859 the German physicist Gustav B. Kirchhoff found that two prominent yellow emission lines from heated varpor of sodium metal had the same wavelength as the two prominent dark lines in the solar spectrum to which Fraunhofer had assigned the letter D. When Kirchhoff demonstrated that if the light from a glowing solid, which a continuous spectrum, is allowed to pass through sodium vapor, having a temperature lower than that of the solid emitter, and then dispersed by a prism, then the spectrum exhibits two prominent dark lines at exactly the same place in the spectrum as D-lines of the sun's spectrum. Evidently sodium vapor in some way absorbed light of certain wavelength from the passing "white" light; hence such a pattern of dark lines is called a line absorption spectrum to distinguish it from the bright-line emission spectrum that the sodium vapor would emit at a high temperature. Kirchhoff showed that the wavelength corresponding to each absorption line is equal to a wavelengthof the bright line in the emission spectrum of the same gas.
    2. All glowing solids and liquids, no matter what their chemical composition, send out light with about the same color balance if they are at the same temperature. More precisely, the energy distribution at various wavelength is continuous reaching a peak energy at a wavelength that depends on the temperature; at very short wavelengths the energy distribution approaches zero. The distribution of energy for all emitters are the same at the same temperature.
    3. All hot solid or liquid emitters have in common their energy distribution shifts with changing temperature. And with increasing temperature more energy is radiated in each wavelength region, and the peak energy moves toward shorter wavelengths. This feature was summarized by the German physicist Wilhelm Wien in 1893 in his Displacement Law, which in part states that for a perfect emitter of continuous spectra, the product of the peak wavelength λm (in cm) and its temperature T (in degrees Kelvin) is a constant with the empirical value of 0.2897 cm-°K:
      λmT = 0.2897 cm-°K.
      For example, the peak wavelength λm for the sun is, by experiment, about 5.5 × 10-5 cm. It follows from Wein's law that T is about 5300 °K. This number is a little low, partly because some of the energy radiated by the sun, particularly at short wavelengths, is absorbed in the atmosphere before reaching the measuring instrument, so that the true peak wavelength is lower; and also because the sun is not the ideal radiator (the so-called "blackbody radiator") for which Wein's Displacement Law describes.
    Wein's Displacement Law can be derived theoretically from classical (Maxwellian) theory of light emission, and that is another impressive victory for that theory. But there is a problem. The classical theory did not yield adequately a prediction of the shape of the distribution curve for any temperature. The general way for deriving the shape of curve on theoretical grounds is as follows: postulate some basic model of emission and then compute from it the fraction of individual oscillators responsible for each range of emitted frequencies, and then add their individual contributions to obtain the overall curve. Various theorists tackled the problem, but none with complete success. There were two most successful attemps.
    Theory I (Wein's equation) yielded a curve valid only for short wavelengths (high frequencies), while
    Theory II (Rayleigh-Jean's equation) led to a curve useful only for very long wavelengths (very low frequencies).
    The Rayleigh-Jean's equation, although it fits well for long wavelengths, it heads toward infinity in what has been dramatically called the "ultraviolet catastrophe." Theoretically, the Rayleigh model must be taken more seriously than Wein's model. It was derived rigourously on the basis of classical physics. And it involves no arbitary constants, and where it does fit the experimental curve, it fits exactly. Whereas the failure of the Wein's model was "too bad," the failure of Rayleigh model presented a crisis. It indicated that classical theory was unable to account for an important experimental observations.

    Among those theorist who had been working, without success, to develop an adequate theory of emission of continuous spectra was the German physicist Max Planck (1858-1947). Since Theory I and II each led to the correct curve for part of the spectrum, one for short wavelengths, the other for very long wavelengths. He thought that an equation could be set up empirically that would combine the best features of each. This Planck succeeded in doing. Finally, there was a single equation which fitted the observed data for the complete energy distribution curve at any temperature. This equation was announced by Planck on October, 1900, to the Deutsche Physikalische Gesellschaft.

    Planck's method of obtaining this equation was not just a blind search for an equation that would fit the data; he was guided in part by the results of Theories I and II, which were based on two different classical models. Two month later, as Planck tells us, "after a few weeks of the most strenuous labor in my life, the darkness lifted and a new unimagined prospect began to dawn." His solution was announced by him on December 14, 1900. This was the birth of the Quantum theory and the beginning of a new physics.

    In developing his solution he consider the energy distribution of what is called (somewhat misleadingly) a "blackbody radiator." By a blackbody is meant a body from which no light, or practically no light, from the outside is reflected by the body under consideration. That is, a blackbody absorbs all the radiation falling on it. According to Kirchhoff's law of thermal radiation, a good absorber is a good radiator, while a body that radiates poorly will also absorb very little radiant energy. A perfect radiator is defined as a body that absorbs all radiation falling upon it. Since it reflects nothing, such a body would appear black when illuminated with visible light. The perfect radiator is called the blackbody. A hollow box or cavity with a small hole in it approximates this condition. Very little light from the outside can be reflected through this hole. If, therefore, the whole box is heated to a very high temperature, then the resulting light coming from the interior and given off through the hole can be studied, the condition of blackbody radiation is approximated.

    To explain the empirical data of blackbody radiation, Planck proposed a radical postulate. Considering Hertz's discovery of the electromagnetic waves emitted by oscillating charges, Planck became convinced that the radiation of light originates in submicroscopic electric oscillators in the cavity walls. He assumed that each oscillator has its own fixed frequency f and emits radiation at that frequency. All frequencies are represented in the enormous number of different oscillators, and hence all frequencies are present in the emitted radiation; the spectrum is continuous. While the oscillators are radiating, they must be losing energy, and thus the emitter will cool unless energy of some form, say heat, is continuously suppied to it. This is the function of the oven around the cavity. The resulting kinetic energy imparted to the particles of the emitter, including oscillators, is further distributed among them because of their incessant collisions. Now when any osciallator absorbs or radiates energy, only the amplitude of vibration changes, for its frequency is fixed. The higher its natural frequency and the greater its amplitude at the moment, the larger is the energy possessed by an oscillator. Now this is consistent with classical principles. But the classical model also implies two other postulates.

    (1) the energy E of an individual oscillator can be any amount, from zero upward, and the oscillator can radiate or absorb any amount of energy, with its amplitude continuously changing while it does so.
    (2) Since any electric charge emits radiation whenever it is accelerated, an electric oscillator must radiate all the time that it is vibrating.
    It was from these two classical postulates that Planck now broke away in order to get a theoretical basis. Planck replaced them with two new postulates.
    (1) Each oscillator can have only certain definite energies. These allowed energies are integral multiples of a quantity hf, where h is a new universal constant now known as Planck's constant, and f is the frequency of the oscillator. Thus the oscillator's energy E at any moment may be 0, 1hf, 2hf, 3hf, or in general nhf, where n is any integer, but will never be a fraction of hf. That is,
    E = hf, (4)
    where hf is called the quantum of energy corresponding to the frequency f. In other words, the total energy of oscillator is "quantized" in lumps of energy of magnitude hf each. This means that the change ΔE in the energy of an oscillator must occur, not gradually and continuously, but suddenly and discontinuously.

    (2) An oscillator radiates only when it changes from one allowable energy value to the next smaller one, and the energy change ΔE that it loses with this sudden decrease in amplitude is emitted as a pulse of electromagnetic radiation of energy hf. Similarly, an oscillator can absorb a quantium of energy hf of incident radiation and consequently it changes immediately to its next higher allowable energy value. According to this postulate, an oscillator does not radiate as long as it remains in any quantum state nhf, even though it is all the time accelerating.

    The quantization of energy can be graphically pictured by the concept of energy levels. If any individual oscillator has constant frequency f, with only its amplitude changing, then the allowable energy levels which it can reach at one time or another may be pictured as equally spaced rungs on a ladder. At any moment the oscillator, with regard to its energy content, is located on one another of these energy levels, if it is not changing levels. Each step or changes of levels happens by the absorption or emission of energy corresponding to a single quantum of energy of the magnitude hf.
    From these new postulates, Planck deduced an equation for the rate at which radiation Eλ of wavelength λ is emitted from a unit area of an ideal blackbody surface of temperature T.
    Eλ = 2πchf / λ4(ehf/kT - 1). (5)
    where h is Planck's constant, c is the speed of electromagnetic radiation in vacuum, and k is Boltzmann's constant. In this equation, Planck's constant h is the only unknown quantity, since c and k are known, and the value of the rate of radiation for any particularly wavelength λ and cavity temperature T can be found expeimentally. Inserting these values in the equation and solving for h we get
    h = 6.625 × 10-34 joule-sec. (6)
    Although initially evaluated in this way, Planck's constant has since then been determined in several independent ways.

    Planck's son later tells that during a walk in the Grunewald in Berlin in 1900 his father announced to him, "Today I have made a discovery as important as that of Newton." Try as he would, Planck could not find a way to explain the experimental data other than by the revolutionary concept of a basic discontinuity in nature. At first, other scientist remained skeptical, unwilling to accept such a departure from the well established principle of continuity of energy. It was not until Einstein applied Planck's hypothesis to photoelectric effects and Bohr applied it to atomic structure that the resistance to the conception disappeared. It was the younger scientists who accepted, applied, and extended Planck's hypothesis.

  4. THE PHOTOELECTRIC EFFECT.
    In 1905, the young Albert Einstein, working in the patent office at Berne, Switzerland, wrote three short scientific papers, any one of which would have assured him with lasting fame. One of these announced his special theory of relativity, another was on the Brownian motion, and the third was on the photoelectric effect, which applied Planck's quantum theory more broadly than Planck had thought necessary.

    The photoelectric effect was discovered incidently by Heinrich Hertz in 1887 during the course of his experimental research that at the time furnished the most convincing proof of Maxwell's classical electromagnetic theory. Hertz noticed that electric sparks would jump more readily across the air gap between the metal spheres of the spark gap in the receiving circuit, if they were polished. He soon found that the sparks were influence by the light coming from the sparks in the spark gap of the transmitting circuit. Upon further investigation, he concluded that ultraviolet radiation was responsible for the phenomena and that the effect was greatest when the light fell on the negative terminal (cathode) of the spark gap. Being concerned with other problems, Hertz abandoned further study of the effect. Many others carried on a more detailed investigation of the phenomena. Wilhelm Hallwach showed that this emmission consisted of negative electricity and in 1899 J.J. Thomson published a paper in the Philosophical Magazine in which he showed that the negative electricity ejected by the ultraviolet light have the same e/m ratio as cathode rays. P. Lennard also obtained the same result. These electrons were called photoelectrons.

    The photoelectric effect consists in the fact that light upon striking certain metals cause electrons to be given off, transforming the radiant energy absorbed by the metal into kinetic energy of emitted electrons. According classical physics, it would be expected that as the intensity (thus energy) of light increases, the kinetic energy of the electrons emitted will increase. This would imply that, as the intensity of the beam increases, the velocity of the electrons emitted would increase. The classical view requires that the kinetic energy equal
    Ek = ½mev2,
    where me is the mass of the electron, and v its velocity. But experimentally this is not what happens. Instead, the maximum velocity given to the electron is constant, regardless of the intensity of the light, but varies in direct proportion to the frequency.

    Einstein explained this in the following way. Electrons are embedded in the atoms of the metal and are held there by attractive forces. When light is shined on the surface of the metal of sufficient energy, the energy is used in two ways:
    (1) to overcome the attractive forces holding the electron to the metal atoms, and,
    (2) if there is any energy left over, it imparts that energy to the electron as kinetic energy.
    Therefore, for those electrons near the surface of the metal, less energy is required to overcome the "binding force," and there is more kinetic energy available. The "surface" electrons therefore acquire the maximum kinetic energy. Einstein expressed this relation by the following formula:
    hf = W + ½mev2, (7)
    where W is the work required to free the electrons from the metal and is equal hf0 where f0 is the threshhold frequency below which light will not free the electron. Thus there is a linear relation between the frequency and the maximum kinetic energy of the electrons emitted. Note that there is nothing in the equation relating to the intensity of the light causing electron emission. But although the velocity of the elctrons does not depend in any way on the intensity of light, the number of electrons emitted does so depend. From this, Einstein, following Planck, concluded that the light is made up of quanta or, as Einstein called them, photons. The energy of a single photon is given by hf. However, the more intense of the light, the greater the number of electrons emitted. The photoelectric emission of a single electron depends upon the absorption of a single photon. If the number of photons is increased, the number of emitted electrons is increased, but no change occurs in the maximum kinetic energy and hence the velocity of electrons. The Planck's constant h is the same for all metals. The threshold energy W required to release electrons, does vary from metal to metal, being so large in the case of some metals, for example, platinum, that no photoelectric effect occurs.

    Now on the basis of the classical wave theory of light, all these phenomena are impossible to be explained. According that theory the energy of a wave of given frequency is dependent on its amplitude. If light consists of waves, the kinetic energy given to the electrons depends upon the amphlitude of the light waves. This explanation fails to hold true for the photoelectric effect.

    Einstein introduced modification of this classical theory of electromagnetic waves to account for photoelectric effect. Planck had modified the classical theory by quantizing the atomic oscillators. But Einstein further modified the theory by quantizing the waves or radiation. Light consists of quanta of energy, called photons. This theory of Einstein that light consists of photons, seemed to be a return to Newton's corpuscular theory. But light is not material particles but is now regarded as composed of bundles of energy, called photons, each photon having a certain amount of energy depending on its frequency or color. In addition, it can be shown that each photon has certain momentum, equal to hf/c, and that as the photons strike a substance and are reflected, the change of momentum causes a small but measurable pressure. But according to the older wave theory light also had momentum and causes pressure. Is light, waves or particles? Since the wave theory cannot explain the photoelectric effect and similar quantum phenomena, and since the particle theory cannot explain many phenomena of interference and diffraction, both theories are needed to explain all these phenomena; they complement each other. Just as light waves have properties like particles, so light particles have properties like waves.

  5. THE BOHR MODEL OF THE ATOM.
    In the empirical formula of Rydberg, there is no explanation of the terms of the equation and in particular the constant R. In 1913 the twenty-eight year old Danish physicist, Niels Bohr, who was born 1855, the year of Balmer's publication concerning the hydrogen spectrum, formulated an explanation. He had just received his Ph.D. degree from the University of Copenhagen in 1911 and then he came to England. He joined J.J. Thomson in Cambridge as a visiting researcher; but after a few months he left to join Rutherford's group at Manchester. The work at that laboratory was just getting evidence for the theory of the nuclear atom. But there were problems with the theory of the movement of the electrons about the nucleus. As Rutherford said later, "I was perfectly aware when I put forward the theory of the nuclear atom that according to classical theory the electron ought to fall into the nucleus..." Any revolving charges should continually spiral closer and closer to the nucleus with ever increasing speed while emitting light of steadily increasing frequency. This obviously is not what is happening. It is at this point that Bohr entered the picture. Bohr was aware of the radical theory of Planck that energy of radiation comes in bundles or quanta. According to this quantum theory, radiation is emitted in the form of photons of definite energy, one photon at a time, during the occasional changes in the energy level of the atom. Bohr postulated that the classical electromagnetic theory, although verified by Hertz for radiation from large electric circuits, does not apply to the atomic phenomena. Instead he postulated that the orbiting electron normally does not radiate energy. This was necessary to explain why the electron does not continuously radiate energy and destroy itself. The radiation from the atom takes place only in certain circumstances. Consider for example the electric discharge through a glass tube filled with hydrogen. The moving electrons and ions of the electric discharge bombard the gas atoms and transfer energy to them. Now in this bombardment the orbital electrons will receive sufficient energy to jump to a larger-sized orbit at a higher energy level, but not enough to remove the electron from the atom and ionize it. The atom is now in an "excited state." Bohr proposed that at some time later the electron would "fall" or jump back from the outer orbit into its original orbit, with a decrease in its energy. If E2 is the energy in the larger outer orbit and E1 is the energy of the smaller inner orbit, then the energy change is
    ΔE = E1 - E2.
    Here Bohr ask himself, "Might it not be possible that the explanation of discrete frequencies emitted by the atom could be found on the basis of the quantum theory?" According to Planck's quantum theory the energy of radiation is discrete, and is always equal to some multiple of the frequency f times a constant h, called Planck's constant. Bohr assumed that the energy change ΔE was emitted as a photon of energy hf, and
    hf = E1 - E2. (8)
    And the frequency f of the photon and the light is ΔE/h. Thus this model now has a mechanism which might account for the observation that hydrogen gas emits light of only certain frequencies, that is, as a line spectrum. The different lines of the spectrum are the result of electrons falling or jumping from any one of many larger orbits. Bohr postulated that there are only certain orbits that the electron may occupy and that energy is radiated when the electron fell or jumped from one of the higher allowed orbits to lower allowed orbits.

    Bohr's original paper was published in the Philosophical Magazine in July 1913 under the title "On the Constitution of Atoms and Molecules"; other papers followed from time to time. We will not follow Bohr's own line of thought exactly because of its advanced mathematical level, and partly because, as Max Planck himself once exclaimed, Bohr's work is written "in a style that is by no means simple." We will here faithfully develope his theory with algebra only.
    Bohr begins reviewing Rutherford's atomic model and the difficulties it raised concerning electronic orbits and light radiation. Then he sets forth the postulates of his theory that he proposed as a solution of those difficulties. Bohr at first confined his attention to the element hydrogen, whose atom is the simplest of all the atoms.
    The following are the postulates of Bohr's theory.

    Postulate 1. The orbit of electrons are circular with the nucleus at their center. The force keeping them in orbit is the Coulomb force of attraction between the electron and the positively charged nucleus. The charge on the nucleus is equal to the product of Z, the atomic number, times e1, the unit of charge. Let e2 is the charge on the electron. Thus the force of attraction is
    F = KQ1Q2 / r2 = K(Ze1)e2 / r2,
    where K is the constant of proportionality and is equal 9 × 109 newton-meter2 per coulomb2 in MKS units.
    This force is equal to the force accelerating the electron in a circular orbit, that is,
    F = ma = m(v2 / r) = mv2 / r.
    Equating the right side of these equations we get
    mv2 / r = KZe2 / r2, or
    mv2 = KZe2 / r, (9)
    since e1 = e2 = e, the charge on an electron.
    Thus far, Bohr has introduced nothing new in his model. These equations are based on known laws of classical mechanics.

    Postulate 2. Only certain orbits are permissible and that these orbits are determined by the law that the angular momentum times 2π must be equal to a whole number times Planck's constant h. The angular momentum of an object traveling in circle of radius r is the linear momentum times r. Thus
    mvr = nh, (10)
    where n is a whole number 1, 2, 3, ... etc.
    Bohr here in this postulate has introduced a radical innovation. This is a quantum condition. Bohr gave no justification for this postulate; he merely stated it, and showed that it led to verifiable results.

    One immediate consequence of these postulates is that equations (9) and (10) contain two unknowns: v and r. The whole number n is assigned for the different orbits being discussed. Every other constant is known. We shall solve equation (9) for r,
    r = KZe2/(mv2),
    and equation (10) for v,
    v = nh/(2πmr).
    We will substitute for v in the first equation from the second equation, eliminating v from the first equation. We get
    r = (n2h2) / (4π2KZe2m). (11)
    For hydrogen of atomic number 1, Z = 1. The other constants are
    h = 6.62 × 10-24 joules-sec.
    K = 9 × 109 newton-m2/coul2.
    e = 1.6 × 10-19 coul.
    m = 9.1 × 10-31 kg.
    Substituting these values, we get
    r = (n2)(5.3 × 10-10 m).
    This tells us that for n = 1, when the radius is the smallest and the atom is in its lowest energy or ground state, the radius of the hydrogen atom is 0.53 × 10-10 m or 10-8 cm, which agrees with the values previously obtained for other estimates of the size. And in addition, it means that the radius can be 1, 4, 9, 16, etc. times as great as its ground state, when in an excited state.

    Postulate 3. An electron may "jump" from one orbit to another and in doing so emits or absorbs energy in quanta. The energy emitted or absorbed must be whole quanta or hf to agree with Planck's theory. This was necessary to explain the discrete spectral emissions. The electron would have to "jump" instantaneously from one orbit to the next, never occupying any intermediate position. At the same instant the electron disappeared from one orbit it would appear in the next. Bohr in this postulate was carrying out Planck's hint of discontinuity in nature one step further.

    This postulate was used by Bohr to explain the Balmer seies of spectral lines. This explanation can be developed in following way. In each orbit the electron has a total energy which is the sum of its kinetic energy and its potential energy. That is,
    E = Ek + Ep.
    These energies are completely determined by the first and second postulates. Solving equation (9) for v2,
    v2 = KZe2 / mr,
    hence, the kinetic energy
    Ek = ½mv2 = (m/2)[(KZe2) / mr] = KZe2 / 2r.
    Analysis shows that the proper expression of the potential energy Ep of the electron at a distance r from the nucleus is
    Ep = -KZe2 / r.
    Thus the total energy E is
    E = Ek + Ep = KZe2/2r + (-KZe2/r) = [KZe2/2r - KZe2/r] = -KZe2/r[(1/2)-1] = KZe2/r.
    Subsituting into this equation the value of r in equation (11) and simplifying, we get
    En = -(2π2K2Z2 e4m) / (n2h2), (12)
    where En are the energy levels or states that is possible for an electron to have and they are determined by the integers n = 1, 2, 3, ..., called the total or principle quantum number. The values of n determines the energies of the state. Where n is large, the energy of the state is large, that is, less negative than those for small integer n.
    Now using postulate 3, the energy difference between any two orbits should equal to a quantum of energy hf. That is,
    hf = En2 - En1 = [(2π2K2Z2 e4m) / (nn22h2)] - [(2π2K2Z2 e4m) / (nn12h2)].
    Thus between an outer orbit where n = n2 = n2 and an inner orbit where n = n1 = n1.
    hf = [2π2K2Z2 e4m / h2] [(1/n22) - (1/n12)],
    which is the energy difference between an outer orbit where n = n2 and an inner orbit where n = n1. Solving for the frequency of the radiation, we get
    f = [2π2K2Z2 e4m / h3] [(1/n22) - (1/n12)]
    and since c = fλ, or λ = c/f, then the wave number k = 1/λ = f/c.
    k = f/c = [2π2K2Z2 e4m / ch3] [(1/n22) - (1/n12)] = RZ2[(1/n22) - (1/n12)]. (13)
    Evaluating the coefficient R = 2π2K2e4m / ch3 (letting Z = 1, for hydrogen), the value is exactly the same as the Rydberg constant R, that is, 3.26 × 1015 sec-1, within a fraction of one percent. This equation (13) is the Rydberg formula, equation (3),
    k = R/m2 - R/n2, or
    k = R(1/m2 - 1/n2).
    where m = n2 and n = n1.
    Here is a tremendous triumph for the Bohr model. It gives a numerical confirmation and systematic explanation of the spectral lines of hydrogen. But more than this, it also could be used for predicting other spectral lines. We get the Balmer series when m = 2. And if m = 1, we get a series that was discovered a year after Bohr announced his model, and was called the Lyman series. The other series for m = 3 (Paschen series in 1908) and m = 4 (Brackett series in 1922) were already known. Later the series for m = 5 (Pfund series in 1924) was discovered.

    Bohr's model was applied to the spectra of other elements. The spectral lines of a singly ionized helium atom were calculated by Bohr and found to agree with experimental measurement of them. The helium atom, which is normally has two electrons, is singly ionized, if one of the two electrons is stripped from it. But in the case of the heavier elements the exact calculations of frequencies become extremely difficult. There are so many electrons involved that interact with each other, causing such large perturbations in each other's orbit, that ordinary mathematical analysis breaks down. Other methods had to be devised.

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