Laser Physics by Milonni P.W., Eberly J.H. .pdf

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LASER PHYSICS

PETER W. MILONNI JOSEPH H. EBERLY

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LASER PHYSICS

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LASER PHYSICS

PETER W. MILONNI JOSEPH H. EBERLY

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Published by John Wiley & Sons, Inc., Hoboken, New Jersey Published simultaneously in Canada

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Library of Congress Cataloging-in-Publication Data:

Milonni, Peter W.

Laser physics/Peter W. Milonni, Joseph H. Eberly p. cm.

Includes bibliographical references and index.

ISBN 978-0-470-38771-9 (cloth)

1. Lasers. 2. Nonlinear optics. 3. Physical optics. I. Eberly, J. H., 1935- II. Title.

QC688.M55 2008 621.36⁰6—dc22

2008026771

Printed in the United States of America 10 9 8 7 6 5 4 3 2 1

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To our wives, Mei-Li and Shirley

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PREFACE

Judged by their economic impact and their role in everyday life, and also by the number of Nobel Prizes awarded, advances in laser science and engineering in the past quarter-century have been remarkable. Using lasers, scientists have produced what are believed to be the coldest temperatures in the universe, and energy densities greater than in the center of stars; have tested the foundations of quantum theory itself; and have controlled atomic, molecular, and photonic states with unprecedented precision.

Questions that previous generations of scientists could only contemplate in terms of thought experiments have been routinely addressed using lasers. Atomic clock frequencies can be measured to an accuracy exceeding that of any other physical quantity.

The generation of femtosecond pulses has made it possible to follow chemical processes in action, and the recent availability of attosecond pulses is allowing the study of phenomena on the time scale of electron motion in atoms. Frequency stabilization and the frequency-comb spectra of mode-locked lasers have now made practical the measurement of absolute optical frequencies and promise ever greater precision in spectroscopy and other areas. Lasers are being used in adaptive optical systems to obtain image resolution with ground-based telescopes that is comparable to that of telescopes in space, and they have become indispensable in lidar and environmental studies.

Together with optical ﬁbers, diode lasers have fueled the explosive growth of optical networks and the Internet. In medicine, lasers are ﬁnding more and more uses in surgery and clinical procedures. Simply put, laser physics is an integral part of contemporary science and technology, and there is no foreseeable end to its progress and application.

The guiding theme of this book is lasers, and our intent is for the reader to arrive at more than a command of tables and formulas. Thus all of the chapters incorporate explanations of the central elements of optical engineering and physics that are required for a basic and detailed understanding of laser operation. Applications are important and we discuss how laser radiation interacts with matter, and how coherent and often very intense laser radiation is used in research and in the ﬁeld. We presume that the reader xiii

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has been exposed to classical electromagnetic theory and quantum mechanics at an undergraduate or beginning graduate level, but we take opportunities throughout to review parts of these subjects that are particularly important for laser physics.

The perceptive reader will notice that there is substantial overlap with a book we wrote 20 years ago called simply Lasers, also published by Wiley and still in print without revision or addition. Many readers and users of that book have told us that they particularly appreciated the frequent concentration on background optical physics as well as explanations of the physical basis for all aspects of laser operation. Naturally a book about lasers that is two decades old needs many new topics to be added to be even approximately current. However, while recognizing that additions are necessary, we also wanted to resist what is close to a law of nature, that a second book must weigh signiﬁcantly more than its predecessor. We believe we have accomplished these goals by describing some of the most signiﬁcant recent developments in laser physics together with an illustrative set of applications based on them.

The basic principles of lasers have not changed in the past twenty years, but there has been a shift in the kinds of lasers of greatest general interest. Considerable attention is devoted to semiconductor lasers and fiber lasers and amplifiers, and to considerations of noise and dispersion in fiber-optic communications. We also treat various aspects of chirping and its role in the generation of extremely short and intense pulses of radiation.

Laser trapping and cooling are explained in some detail, as are most of the other applications mentioned above. We introduce the most important concepts needed to understand the propagation of laser radiation in the turbulent atmosphere; this is an important topic for free-space communication, for example, but it has usually been addressed only in more advanced and specialized books. We have attempted to present it in a way that might be helpful for students as well as laser scientists and engineers with no prior exposure to turbulence theory.

The book is designed as a textbook, but there is probably too much material here to be covered in a one-semester course. Chapters 1 – 7 could be used as a self-contained, elementary introduction to lasers and laser—matter interactions. In most respects the remaining chapters are self-contained, while using consistent notation and making reference to the same fundamentals. Chapters 9 and 10, for example, can serve as introductions to coherent propagation effects and nonlinear optics, respectively, and Chapters 12 and 13 can be read separately as introductions to photon detection, photon counting, and optical coherence. Chapters 14 and 15 describe some applications of lasers that will likely be of interest for many years to come.

We are grateful to A. Al-Qasimi, S. M. Barnett, P. R. Berman, R. W. Boyd, L. W.

Casperson, C. A. Denman, R. Q. Fugate, J. W. Goodman, D. F. V. James, C. F.

Maes, G. H. C. New, C. R. Stroud, Jr., J. M. Telle, I. A. Walmsley, and E. Wolf for comments on some of the chapters or for contributing in other ways to this effort.

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USEFUL TABLES

TABLE 3 The Electromagnetic Spectrum Typical Wavelength

(cm)

Frequency (Hz)

Photon Energy (eV)

Longwave radio 310⁵ 10⁵ 410²¹⁰

AM radio 310⁴ 10⁶ 410²⁹

FM radio 300 10⁸ 410²⁷

Radar 3 10¹⁰ 410²⁵

Microwave 0.3 10¹¹ 410²⁴

Infrared 310²⁴ 10¹⁴ 0.4

Light (orange) 610²⁵ 510¹⁴ 2

Ultraviolet 310²⁶ 10¹⁶ 40

X-rays 310²⁸ 10¹⁸ 4000

Gamma rays 310²¹¹ 10²¹ 410⁶

Cosmic-ray photons 310²¹³ 10²³ 410⁸

Human eyes are sensitive to only a rather narrow band of wavelengths ranging from about 430 to 690 nm.

Figure 9.11 shows the wavelength sensitivity of the human eye for a “standard observer.”

TABLE 1 Physical Constants

Velocity of light in vacuum c¼2.99810⁸m/s

Electron charge e¼1.60210²¹⁹C

Coulomb force constant 1/4pe0¼8.98810⁹N-m²/C² e²/4pe₀¼1.440 eV-nm

Electron rest mass me¼9.10810²³¹kg

Proton rest mass m_p¼1.67210²²⁷kg

Bohr radius a0¼0.528 A˚ ¼0.0528 nm

Planck’s constant h¼6.62610²³⁴J-s

h ¼h/2p¼1.05410²³⁴J-s hc¼1240 eV-nm

Avogadro’s number NA¼6.02310²³

Boltzmann constant k¼1.38010²²³J/K

Universal gas constant R¼NAk¼8.314 J/K

Stefan – Boltzmann constant s¼5.67010²⁸Watt/m²-K⁴

TABLE 2 Conversion Factors

1 electron volt (eV)¼1:60210¹⁹joule (J)

¼1:1610⁴K

¼2:4210¹⁴Hz

¼8:0710³cm¹ 300 K¼2:5910²eV₄₀¹ eV 760 Torr¼1.01310⁵N/m²

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1 INTRODUCTION TO LASER OPERATION

1.1 INTRODUCTION

The word laser is an acronym for the most significant feature of laser action: light amplification by stimulated emission of radiation. There are many different kinds of laser, but they all share a crucial element: Each contains material capable of amplifying radiation. This material is called the gain medium because radiation gains energy pas- sing through it. The physical principle responsible for this amplification is called stimulated emission and was discovered by Albert Einstein in 1916. It was widely recognized that the laser would represent a scientific and technological step of the greatest magnitude, even before the first one was constructed in 1960 by T. H. Maiman. The award of the 1964 Nobel Prize in physics to C. H. Townes, N. G. Basov, and A. M. Prokhorov carried the citation “for fundamental work in the field of quantum electronics, which has led to the construction of oscillators and amplifiers based on the maser-laser principle.” These oscillators and amplifiers have since motivated and aided the work of thousands of scientists and engineers.

In this chapter we will undertake a superﬁcial introduction to lasers, cutting corners at every opportunity. We will present an overview of the properties of laser light, with the goal of understanding what a laser is, in the simplest terms. We will introduce the theory of light in cavities and of cavity modes, and we will describe an elementary theory of laser action.

We can begin our introduction with Fig. 1.1, which illustrates the four key elements of a laser. First, a collection of atoms or other material amplifies a light signal directed through it. This is shown in Fig. 1.1a. The amplifying material is usually enclosed by a highly reflecting cavity that will hold the amplified light, in effect redirecting it through the medium for repeated amplifications. This refinement is indicated in Fig. 1.1b. Some provision, as sketched in Fig. 1.1c, must be made for replenishing the energy of the amplifier that is being converted to light energy. And some means must be arranged for extracting in the form of a beam at least part of the light stored in the cavity, perhaps as shown in Fig. 1.1d. A schematic diagram of an operating laser embodying all these elements is shown in Fig. 1.2.

It is clear that a well-designed laser must carefully balance gains and losses. It can be anticipated with conﬁdence that every potential laser system will present its designer with more sources of loss than gain. Lasers are subject to the basic laws of physics, and every stage of laser operation from the injection of energy into the amplifying medium to the extraction of light from the cavity is an opportunity for energy loss

Laser Physics. By Peter W. Milonni and Joseph H. Eberly Copyright#2010 John Wiley & Sons, Inc.

1

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and entropy gain. One can say that the success of masers and lasers came only after physicists learned how atoms could be operated efﬁciently as thermodynamic engines.

One of the challenges in understanding the behavior of atoms in cavities arises from the strong feedback deliberately imposed by the cavity designer. This feedback means that a small input can be amplified in a straightforward way by the atoms, but not inde- finitely. Simple amplification occurs only until the light field in the cavity is strong enough to affect the behavior of the atoms. Then the strength of the light as it acts on the amplifying atoms must be taken into account in determining the strength of the light itself. This sounds like circular reasoning and in a sense it is. The responses of the light and the atoms to each other can become so strongly interconnected that they cannot be determined independently but only self-consistently. Strong feedback also means that small perturbations can be rapidly magnified. Thus, it is accurate to anticipate that lasers are potentially highly erratic and unstable devices. In fact, lasers can provide dramatic exhibitions of truly chaotic behavior and have been the objects of fundamental study for this reason.

For our purposes lasers are principally interesting, however, when they operate stably, with well-determined output intensity and frequency as well as spatial mode structure.

Atoms

(a) (b)

(d)

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Atoms

1 2

4 3 in out

Figure 1.1 Basic elements of a laser.

High power flash lamp Transparent medium or cell with atoms, and light being amplified

100%

Mirror

90%

Mirror

Output of laser

Figure 1.2 Complete laser system, showing elements responsible for energy input, ampliﬁcation, and output.

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The self-consistent interaction of light and atoms is important for these properties, and we will have to be concerned with concepts such as gain, loss, threshold, steady state, saturation, mode structure, frequency pulling, and linewidth.

In the next few sections we sketch properties of laser light, discuss modes in cavities, and give a theory of laser action. This theory is not really correct, but it is realistic within its own domain and has so many familiar features that it may be said to be “obvious.” It is also signiﬁcant to observe what is not explained by this theory and to observe the ways in which it is not fundamental but only empirical. These gaps and missing elements are an indication that the remaining chapters of the book may also be necessary.

1.2 LASERS AND LASER LIGHT

Many of the properties of laser light are special or extreme in one way or another. In this section we provide a brief overview of these properties, contrasting them with the properties of light from more ordinary sources when possible.

Wavelength

Laser light is available in all colors from red to violet and also far outside these conventional limits of the optical spectrum.¹Over a wide portion of the available range laser light is “tunable.” This means that some lasers (e.g., dye lasers) have the property of emitting light at any wavelength chosen within a range of wavelengths. The longest laser wavelength can be taken to be in the far infrared, in the neighborhood of 100 – 500mm. Devices producing coherent light at much longer wavelengths by the

“maser – laser principle” are usually thought of as masers. The search for lasers with ever shorter wavelengths is probably endless. Coherent stimulated emission in the XUV (extreme ultraviolet) or soft X-ray region (10 –15 nm) has been reported.

Appreciably shorter wavelengths, those characteristic of gamma rays, for example, may be quite difﬁcult to reach.

Photon Energy

The energy of a laser photon is not different from the energy of an “ordinary” light photon of the same wavelength. A green – yellow photon, roughly in the middle of the optical spectrum, has an energy of about 2.5 eV (electron volts). This is the same as about 410²¹⁹J ( joules)¼410²¹²erg. The large exponents in the last two numbers make it clear that electron volts are a much more convenient unit for laser photon energy than joules or ergs. From the infrared to the X-ray region photon energies vary from about 0.01 eV to about 100 eV. For contrast, at room temperature the thermal unit of energy iskT₄₀¹ eV¼0:025 eV. This is two orders of magnitude smaller than the typical optical photon energy just mentioned, and as a consequence thermal excitation plays only a very small role in the physics of nearly all lasers.

1A list of laser wavelengths may be found in M. J. Weber,Handbook of Laser Wavelengths, CRC, Boca Raton, FL, 1999.

1.2 LASERS AND LASER LIGHT 3

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Directionality

The output of a laser can consist of nearly ideal plane wavefronts. Only diffraction imposes a lower limit on the angular spread of a laser beam. The wavelength l and the areaA of the laser output aperture determine the order of magnitude of the beam’s solid angle (DV) and vertex angle (Du) of divergence (Fig. 1.3) through the relation

DVl²

A (Du)²: (1:2:1) This represents a very small angular spread indeed if l is in the optical range, say 500 nm, and A is macroscopic, say (5 mm)². In this example we compute DV (500)²10²¹⁸m²/(5²10²⁶m²)¼10²⁸sr, orDu_¼1/10 mrad.

Monochromaticity

It is well known that lasers produce very pure colors. If they could produce exactly one wavelength, laser light would be fully monochromatic. This is not possible, in principle as well as for practical reasons. We will designate by Dl the range of wavelengths included in a laser beam of main wavelength l. Similarly, the associated range of frequencies will be designated byDn, the bandwidth. In the optical region of the spectrum we can taken510¹⁴Hz (hertz, i.e., cycles per second). The bandwidth of sunlight is very broad, more than 10¹⁴Hz. Of course, filtered sunlight is a different matter, and with sufficiently good filtersDncould be reduced a great deal. However, the cost in lost intensity would usually be prohibitive. (See the discussion on spectral brightness below.) For lasers, a very low value ofDnis 1 Hz, while a bandwidth around 100 Hz is spectroscopically practical in some cases (Fig. 1.4). ForDn¼100 Hz the relative spectral purity of a laser beam is quite impressive: Dn/n 100/(510¹⁴)¼210²¹³.

A Dq

Figure 1.3 Sketch of a laser cavity showing angular beam divergence Du at the output mirror (areaA).

Sun Dn~10¹⁴Hz

Dn~100Hz

n Laser

Figure 1.4 Spectral emission bands of the sun and of a representative laser, to indicate the much closer approach to monochromatic light achieved by the laser.

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This exceeds the spectral purity (Qfactor) achievable in conventional mechanical and electrical resonators by many orders of magnitude.

Coherence Time

The existence of a ﬁnite bandwidthDnmeans that the different frequencies present in a laser beam can eventually get out of phase with each other. The time required for two oscillations differing in frequency by Dn to get out of phase by a full cycle is obviously 1/Dn. After this amount of time the different frequency components in the beam can begin to interfere destructively, and the beam loses “coherence.” Thus, Dt_¼1/Dn is called the beam’s coherence time. This is a general deﬁnition, not restricted to laser light, but the extremely small values possible forDn in laser light make the coherence times of laser light extraordinarily long.

For example, even a “broadband” laser withDn 1 MHz has the coherence time Dt1ms. This is enormously longer than most “typical” atomic ﬂuorescence lifetimes, which are measured in nanoseconds (10²⁹s). Thus even lasers that are not close to the limit of spectral purity are nevertheless effectively 100% pure on the relevant spectroscopic time scale. By way of contrast, sunlight has a bandwidthDnalmost as great as its central frequency (yellow light,n¼510¹⁴ Hz). Thus, for sunlight the coherence time isDt210²¹⁵s, so short that unﬁltered sunlight cannot be considered temporally coherent at all.

Coherence Length

The speed of light is so great that a light beam can travel a very great distance within even a short coherence time. For example, within Dt 1ms light travels Dz (310⁸m/s)(1ms)¼300 m. The distanceDz¼cDtis called the beam’s coherence length. Only portions of the same beam that are separated by less thanDzare capable of interfering constructively with each other. No fringes will be recorded by the ﬁlm in Fig. 1.5, for example, unless 2L,cDt_¼Dz.

Spectral Brightness

A light beam from a ﬁnite source can be characterized by its beam divergenceDV, source size (usually surface area A), bandwidth Dn, and spectral power density Pn

(watts per hertz of bandwidth). From these parameters it is useful to determine thespec- tral brightnessb_nof the source, which is deﬁned (Fig. 1.6) to be the power ﬂow per unit

Film Beam splitter

L

Figure 1.5 Two-beam interferometer showing interference fringes obtained at the recording plane if the coherence length of the light is great enough.

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area, unit bandwidth, and steradian, namelyb_n_¼Pn/ADV Dn. Notice thatPn/ADnis the spectral intensity, sob_ncan also be thought of as the spectral intensity per steradian.

For an ordinarynonlaser optical source, brightness can be estimated directly from the blackbody formula forr(n), the spectral energy density (J/m³-Hz):

r(n)¼8pn² c³

hn

e^hn=k^B^T1: (1:2:2)

The spectral intensity (W/m²-Hz) is thuscr, andcr_/DVis the desired spectral intensity per steradian. TakingDV¼4pfor a blackbody, we have

b_n¼2n² c²

hn

e^hn=k^B^T1: (1:2:3)

The temperature of the sun is aboutT¼5800K 20(300K). Since the main solar emission is in the yellow portion of the spectrum, we can takehn2.5 eV. We recall thatkBT₄₀¹ eV forT¼300K, sohn/kBT5, givinge^hn=k^B^T150 and ﬁnally

b_n1:510⁸ W=m²-sr-Hz (sun): (1:2:4) Several different estimates can be made for laser radiation, depending on the type of laser considered. Consider ﬁrst alow-power He – Ne laser. A power level of 1 mW is normal, with a bandwidth of around 10⁴ Hz. From (1.2.1) we see that the product of beam cross-sectional area and solid angle is justl², which for He – Ne light isl²(6328 10²¹⁰m)²410²¹³m². Combining these, we ﬁnd

b_n2:510⁵W=m²-sr-Hz (He–Ne laser): (1:2:5) Another common laser is themode-locked neodymium – glass laser, which can easily reach power levels around 10⁴MW. The bandwidth of such a laser is limited by the pulse duration, sayt_p 30 ps (3010²¹²s), as follows. Since the laser’s coherence time Dt is equal to t_p at most, its bandwidth is certainly greater than 1/t_p 3.310¹⁰s²¹. We convert from radians per second to cycles per second by dividing by 2p and getDn 510⁹Hz. The wavelength of a Nd : glass laser is 1.06mm, so l² 10²¹²m². The result of combining these, again usingADV¼l², is

b_n210¹² W=m²-sr-Hz (Nd : glass laser): (1:2:6)

A

DW

Figure 1.6 Geometrical construction showing source area and emission solid angle appropriate to discussion of spectral brightness.

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Recent developments have led to lasers with powers of terawatts (10¹²W) and even petawatts (10¹⁵W), sob_ncan be even orders of magnitude larger.

It is clear that in terms of brightness there is practically no comparison possible between lasers and thermal light. Our sun is 20orders of magnitude less bright than a mode-locked laser. This raises an interesting question of principle. Let us imagine a thermal light source ﬁltered and collimated to the bandwidth and directionality of a He – Ne laser, and the He – Ne laser attenuated to the brightness level of the thermal light. The question is: Could the two light beams with equal brightness, beam divergence, polarization, and bandwidth be distinguished in any way? The answer is that they could be distinguished, but not by any ordinary measurement of optics.

Differences would show up only in the statistical fluctuations in the light beam. These fluctuations can reflect the quantum nature of the light source and are detected by photon counting, as discussed in Chapter 12.

Active Medium

The materials that can be used as the active medium of a laser are so varied that a listing is hardly possible. Gases, liquids, and solids of every sort have been made tolase(a verb contributed to science by the laser). The origin of laser photons, as shown in Fig. 1.7, is most often in a transition between discrete upper and lower energy states in the medium, regardless of its state of matter. He – Ne, ruby, CO2, and dye lasers are familiar examples, but exceptions are easily found: The excimer laser has an unbound lower state, the semiconductor diode laser depends on transitions between electron bands rather than discrete states, and understanding the free-electron laser does not require quantum states at all.

Type of Laser Cavity

All laser cavities share two characteristics that complement each other: (1) They are basically linear devices with one relatively long optical axis, and (2) the sides parallel to this axis can be open, not enclosed by reﬂecting material as in a microwave cavity.

There is no single best shape implied by these criteria, and in the case of ring lasers the long axis actually bends and closes on itself (Fig. 1.8). Despite what may seem

hn E2 – E₁ E₂

E₁

Figure 1.7 Photon emission accompanying a quantum jump from level 2 to level 1.

Figure 1.8 Two collections of mirrors making laser cavities, showing standing-wave and traveling- wave (ring) conﬁgurations on left and right, respectively.

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obvious, it is not always best to design a cavity with the lowest loss. In the case ofQ switching an extra loss is temporarily introduced into the cavity for the laser to over- come, and very high-power lasers sometimes use mirrors that are deliberately designed to deﬂect light out of the cavity rather than contain it.

Applications of Lasers

There is apparently no end of possible applications of lasers. Many of the uses of lasers are well known by now to most people, such as for various surgical procedures, for holography, in ultrasensitive gyroscopes, to provide straight lines for surveying, in supermarket checkout scanners and compact disc players, for welding, drilling, and scribing, in compact death-ray pistols, and so on. (The sophisticated student knows, even before reading this book, that one of these “well-known” applications has never been realized outside the movie theater.)

1.3 LIGHT IN CAVITIES

In laser technology the termscavityandresonatorare used interchangeably. The theory and design of the cavity are important enough for us to devote all of Chapter 7 to them.

In this section we will consider only a simpliﬁed theory of resonators, a theory that is certain to be at least partly familiar to most readers. This simpliﬁcation allows us to introduce the concept of cavity modes and to infer certain features of cavity modes that remain valid in more general circumstances. We also describe the great advantage of open, rather than closed, cavities for optical radiation.

We will consider only the case of a rectangular “empty cavity” containing radiation but no matter, as sketched in Fig. 1.9. The assumption that there is radiation but no matter inside the cavity is obviously an approximation if the cavity is part of a working laser. This approximation is used frequently in laser theory, and it is accurate enough for many purposes because laser media are usually only sparsely ﬁlled with active atoms or molecules.

L_z

L_y L_x

y

z x

0

Figure 1.9 Rectangular cavity with side lengthsLx,Ly,Lz.

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In Chapter 7 full solutions for the electric ﬁeld in cavities of greatest interest are given.

For example, thezdependence of thexcomponent of the ﬁeld takes the form

E_x(z)¼E₀sink_zz, (1:3:1) whereE0is a constant. However, here we are interested only in the simplest features of the cavity ﬁeld, and these can be obtained easily by physical reasoning.

The electric ﬁeld should vanish at both ends of the cavity. It will do so if we ﬁt exactly an integer number of half wavelengths into the cavity along each of its axes. This means, for example, thatlalong thezaxis is determined by the relationL¼n(l_/2), wheren¼ 1, 2,. . ., is a positive integer andLis the cavity length. If we use the relation between wave vector and wavelength,k¼2p_/l, this is the same as

k_z¼p

Ln, (1:3:2)

for thezcomponent of the wave vector. By substitution into the solution (1.3.1) we see that (1.3.2) is sufﬁcient to guarantee that the required boundary condition is met, i.e., thatEx(z)¼0 for bothz¼0 andz¼L.

If there were reﬂecting sides to a laser cavity, the same would apply to thexandy components of the wave vector. As we will show later, if the three dimensions are equiv- alent in this sense, the number of available modes grows extremely rapidly as a function of frequency. For example, a cubical three-dimensionally reﬂecting cavity 1 cm on a side has about 400 million resonant frequencies within the useful gain band of a He – Ne laser. Then lasing could occur across the whole band, eliminating any possibility of achieving the important narrow-band, nearly monochromatic character of laser light that we emphasized in the preceding sections.

The solution to this multimode dilemma was suggested independently in 1958 by Townes and A. L. Schawlow, R. H. Dicke, and Prokhorov. They recognized that a one-dimensional rather than a three-dimensional cavity was desirable, and that this could be achieved with an open resonator consisting of two parallel mirrors, as in Fig. 1.10. The difference in wave vector between two modes of a linear cavity, according to Eq. (1.3.2), is just p_/L, so the mode spacing is given byDk¼(2p_/c)Dn, orDn¼ c/2L. ForL¼10 cm we ﬁnd

Dn¼310⁸m=s

(2)(0:10 m) ¼1500 MHz, (1:3:3)

for the separation in frequency of adjacent resonator modes. As indicated in Fig. 1.11, the number of possible modes that can lase is therefore at most

1500 MHz

1500 MHz¼1: (1:3:4)

(a) (b)

Figure 1.10 Sketch illustrating the advantage of a one-dimensional cavity. Stable modes are associated only with beams that are retroreﬂected many times.

1.3 LIGHT IN CAVITIES 9

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The maximum number, including two choices of polarization, is therefore 2, consider- ably smaller than the estimate of 400 million obtained for three-dimensional cavities.

These results do not include the effects of diffraction of radiation at the mirror edges. Diffraction determines thex,ydependence of the field, which we have ignored completely. Accurate calculations of resonator modes, including diffraction, are often done with computers. Such calculations were first made in 1961 for the plane-parallel resonator of Fig. 1.10 with either rectangular or circular mirrors. Actually lasers are seldom designed with flat mirrors. Laser resonator mirrors are usually spherical surfaces, for reasons to be discussed in Chapter 7. A great deal about laser cavities can nevertheless be understood without worrying about diffraction or mirror shape. In particular,for most practical purposes, the mode-frequency spacing is given accurately enough byDn¼c/2L.

1.4 LIGHT EMISSION AND ABSORPTION IN QUANTUM THEORY

The modern interpretation of light emission and absorption was ﬁrst proposed by Einstein in 1905 in his theory of the photoelectric effect. Einstein assumed the difference in energy of the electron before and after its photoejection to be equal to the energyhnof the photon absorbed in the process.

This picture of light absorption was extended in two ways by Bohr: to apply to atomic electrons that are not ejected during photon absorption but instead take on a higher energy within their atom, and to apply to the reverse process of photon emission, in which case the energy of the electron should decrease. These extensions of Einstein’s idea ﬁtted perfectly into Bohr’s quantum mechanical model of an atom in 1913.

This model, described in detail in Chapter 2, was the first to suggest that electrons are restricted to a certain fixed set of orbits around the atomic nucleus. This set of orbits was shown to correspond to a fixed set of allowed electron energies. The idea of a “quantum jump” was introduced to describe an electron’s transition between two allowed orbits.

The amount of energy involved in a quantum jump depends on the quantum system.

Atoms have quantum jumps whose energies are typically in the range 1 – 6 eV, as long as an outer-shell electron is doing the jumping. This is the ordinary case, so atoms usually absorb and emit photons in or near the optical region of the spectrum. Jumps by inner-shell atomic electrons usually require much more energy and are associated with X-ray photons. On the other hand, quantum jumps among the so-called Rydberg energy levels, those outer-electron levels lying far from the ground level and near to

1500 MHz

Gain curve

Cavity mode frequencies

n

Figure 1.11 Mode frequencies separated by 1500 MHz, corresponding to a 10-cm one-dimensional cavity. A 1500-MHz gain curve overlaps only 1 mode.

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the ionization limit, involve only a small amount of energy, corresponding to far-infrared or even microwave photons.

Molecules have vibrational and rotational degrees of freedom whose quantum jumps are smaller (perhaps much smaller) than the quantum jumps in free atoms, and the same is often true of jumps between conduction and valence bands in semiconductors. Many crystals are transparent in the optical region, which is a sign that they do not absorb or emit optical photons, because they do not have quantum energy levels that permit jumps in the optical range. However, colored crystals such as ruby have impurities that do absorb and emit optical photons. These impurities are frequently atomic ions, and they have both discrete energy levels and broad bands of levels that allow optical quantum jumps (ruby is a good absorber of green photons and so appears red).

1.5 EINSTEIN THEORY OF LIGHT – MATTER INTERACTIONS

The atoms of a laser undergo repeated quantum jumps and so act as microscopic transducers. That is, each atom accepts energy and jumps to a higher orbit as a result of some input or “pumping” process and converts it into other forms of energy—for example, into light energy (photons)—when it jumps to a lower orbit. At the same time, each atom must deal with the photons that have been emitted earlier and reﬂected back by the mirrors. These prior photons, already channeled along the cavity axis, are the origin of the stimulated component to the atom’s emission of subsequent photons.

In Fig. 1.12 we indicate some ways in which energy conversion can occur. For sim- plicity we focus our attention on quantum jumps between two energy levels, 1 and 2, of an atom. The ﬁve distinct energy conversion diagrams of Fig. 1.12 are interpreted as follows:

(a) Absorption of an incrementDE¼E₂2E₁of energy from the pump: The atom is raised from level 1 to level 2. In other words, an electron in the atom jumps from an inner orbit to an outer orbit.

(b) Spontaneous emission of a photon of energy hn¼E22E1: The atom jumps down from level 2 to the lower level 1. The process occurs “spontaneously” without any external inﬂuence.

(c) Stimulated emission: The atom jumps down from energy level 2 to the lower level 1, and the emitted photon of energy hn¼E₂2E₁ is an exact replica of a photon already present. The process is induced, or stimulated, by the incident photon.

(d) Absorption of a photon of energyhn¼E22E1: The atom jumps up from level 1 to the higher level 2. As in (c), the process is induced by an incident photon.

(e) Nonradiative deexcitation: The atom jumps down from level 2 to the lower level 1, but no photon is emitted so the energyE₂2E₁must appear in some other form [e.g., increased vibrational or rotational energy in the case of a molecule, or rearrangement (“shakeup”) of other electrons in the atom].

All these processes occur in the gain medium of a laser. Lasers are often classiﬁed according to the nature of the pumping process (a) which is the source of energy for the output laser beam. In electric-discharge lasers, for instance, the pumping occurs

1.5 EINSTEIN THEORY OF LIGHT – MATTER INTERACTIONS 11

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as a result of collisions of electrons in a gaseous discharge with the atoms (or molecules) of the gain medium. In an optically pumped laser the pumping process is the same as the absorption process (d), except that the pumping photons are supplied by a lamp or perhaps another laser. In a diode laser an electric current at the junction of two different semiconductors produces electrons in excited energy states from which they can jump into lower energy states and emit photons.

This quantum picture is consistent with a highly simpliﬁed description of laser action.

Suppose that lasing occurs on the transition deﬁned by levels 1 and 2 of Fig. 1.12. In the most favorable situation the lower level (level 1) of the laser transition is empty. To maintain this situation a mechanism must exist to remove downward jumping electrons from level 1 to another level, say level 0. In this situation there can be no detrimental absorption of laser photons due to transitions upward from level 1 to level 2. In practice the number of electrons in level 1 cannot be exactly zero, but we will assume for sim- plicity that the rate of deexcitation of the lower level 1 is so large that the number of atoms remaining in that level is negligible compared to the number in level 2; this is a reasonably good approximation for many lasers. Under this approximation laser action can be described in terms of two “populations”: the numbernof atoms in the upper level 2 and the numberqof photons in the laser cavity.

The number of laser photons in the cavity changes for two main reasons:

(i) Laser photons are continually being added because of stimulated emission.

(ii) Laser photons are continually being lost because of mirror transmission, scattering or absorption at the mirrors, etc.

E₂

E₁

E₂

E₁

hn

E₂ hn

hn hn

(a) (b)

(c)

(d) (e)

E₁ hn

E₂

E₁

E₂

E₁

Figure 1.12 Energy conversion processes in a lasing atom or molecule: (a) absorption of energy DE¼E₂2E₁from the pump; (b) spontaneous emission of a photon of energyDE; (c) stimulated emission of a photon of energyDE; (d) absorption of a photon of energyDE; (e) nonradiative deexcitation.

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Thus, we can write a (provisional) equation for the rate of change of the number of photons, incorporating the gain and loss described in (i) and (ii) as follows:

dq

dt ¼anqbq: (1:5:1)

That is, the rate at which the number of laser photons changes is the sum of two separate rates: the rate of increase (ampliﬁcation or gain) due to stimulated emission, and the rate of decrease (loss) due to imperfect mirror reﬂectivity.

As Eq. (1.5.1) indicates, the gain of laser photons due to stimulated emission is not only proportional to the numbernof atoms in level 2, but also to the numberqof photons already in the cavity. The efficiency of the stimulated emission process depends on the type of atom used and other factors. These factors are reflected in the size of the amplification orgain coefficient a. The rate of loss of laser photons is simply proportional to the number of laser photons present.

We can also write a provisional equation forn. Both stimulated and spontaneous emission causento decrease (in the former case in proportion toq, in the latter case not), and the pump causesnto increase at some rate we denote byp. Thus, we write

dn

dt ¼ anqfnþp: (1:5:2) Note that the ﬁrst term appears in both equations, but with opposite signs. This reﬂects the central role of stimulated emission and shows that the decrease ofn(excited atoms) due to stimulated emission corresponds precisely to the increase ofq(photons).

Equations (1.5.1) and (1.5.2) describe laser action. They show how the numbers of lasing atoms and laser photons in the cavity are related to each other. They do not indicate what happens to the photons that leave the cavity, or what happens to the atoms when their electrons jump to some other level. Above all, they do not tell how to evaluate the coefﬁcientsa,b,f,p. They must be taken only as provisional equations, not well justiﬁed although intuitively reasonable.

It is important to note that neither Eq. (1.5.1) nor (1.5.2) can be solved independently of the other. That is, (1.5.1) and (1.5.2) arecoupledequations. The coupling is due phys- ically to stimulated emission: The lasing atoms of the gain medium can increase the number of photons via stimulated emission, but by the same process the presence of photons will also decrease the number of atoms in the upper laser level. This coupling between the atoms and the cavity photons is indicated schematically in Fig. 1.13.

We also note that Eqs. (1.5.1) and (1.5.2) are nonlinear. The nonlinearity (the product of the two variables nq) occurs in both equations and is another manifestation of

Atoms

Cavity photons Equation

(1.5.1)

Equation (1.5.2)

Figure 1.13 Self-consistent pair of laser equations.

1.5 EINSTEIN THEORY OF LIGHT – MATTER INTERACTIONS 13

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stimulated emission. No established systematic methods exist for solving nonlinear differential equations, and there is no known general solution to these laser equations.

However, they have a number of well-deﬁned limiting cases of some practical importance, and some of these do have known solutions. The most important case is steady state.

In steady state we can put bothdq/dtanddn/dtequal to zero. Then (1.5.1) reduces to n¼b

a;n_t, (1:5:3)

which can be recognized as athresholdrequirement on the number of upper-level atoms.

That is, ifn,b/a, thendq/dt,0, and the number of photons in the cavity decreases, terminating laser action. The steady state of (1.5.2) also has a direct interpretation.

Fromdn/dt¼0 andn¼nt¼b/awe ﬁnd q¼ p

b f

a: (1:5:4)

This equation establishes a threshold for the pumping rate, since the number of photons q cannot be negative. Thus, the minimum or threshold value of p compatible with steady-state operation is found by puttingq¼0:

pt ¼ f b

a ¼f nt: (1:5:5)

In words, the threshold pumping rate just equals the loss rate per atom times the number of atoms present at threshold.

In Chapters 4 – 6 we will return to a discussion of laser equations. We will deal there with steady state as well as many other aspects of laser oscillation in two-level, three- level, and four-level quantum systems.

1.6 SUMMARY

The theory of laser action and the description of cavity modes presented in this chapter can be regarded only as caricatures. In common with all caricatures, they display outstanding features of their subject boldly and simply. All theories of laser action must address the questions of gain,loss, steady state, and threshold. The virtues of our caricatures in addressing these questions are limited. They do not even suggest mat- ters such aslinewidth,saturation,output power,mode locking,tunability, andstability.

Obviously, one must not accept a caricature as the truth. Concerning the many aspects of the truth that are distorted or omitted by these ﬁrst discussions, it will take much of this book to get the facts straight. This is not only a matter of dealing with details within the caricatures, but also with concepts that are larger than the caricatures altogether.

One should ask whether lasers are better described by photons or electric ﬁelds. Also, is Einstein’s theory always satisfactory, or does Schro¨dinger’s wave equation play a role?

Are Maxwell’s equations for electromagnetic waves signiﬁcant? The answer to these

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questions is no, yes, yes. Laser theory is usually based on Schro¨dinger’s and Maxwell’s equations, neither of which was needed in this chapter.

From a different point of view another kind of question is equally important in trying to understand what a laser is. For example, why were lasers not built before 1960? Are there any rules of thumb that can predict, approximately and without detailed calculation, how much one can increase the output power or change the operating frequency? What are the most sensitive design features of a gas laser? a chemical laser? a semiconductor laser? Is a laser essentially quantum mechanical, or can classical physics explain all the important features of laser operation?

It will not be possible to give detailed answers to all of these questions. However, these questions guide the organization of the book, and many of them are addressed individually. In the following chapters the reader should encounter the concepts of physics and engineering that are most important for understanding laser action in general and that provide the background for pursuing further questions of particular theoretical or practical interest.

1.6 SUMMARY 15

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2 ATOMS, MOLECULES, AND SOLIDS

2.1 INTRODUCTION

It is frequently said that quantum physics began with Max Planck’s discovery of the correct blackbody radiation formula in 1900. But it was more than a quarter of a century before Planck’s formula could be fully derived from a satisfactory theory of quantum mechanics. Nevertheless, once formulated, quantum mechanics answered so many questions that it was adopted and reﬁned with remarkable speed between 1925 and 1930. By 1930 there were new and successful quantum theories of atomic and molecular structure, electromagnetic radiation, electron scattering, and thermal, optical, and magnetic properties of solids.

Lasers can be understood without a detailed knowledge of the quantum theory of matter. However, several consequences of the quantum theory are essential. This chapter provides a review of some results of quantum theory applied to simple models of atoms, molecules, and semiconductors.

2.2 ELECTRON ENERGY LEVELS IN ATOMS

In 1913 Niels Bohr discovered a way to use Planck’s radiation constanthin a radically new, but still mostly classical, theory of the hydrogen atom. Bohr’s theory was the ﬁrst quantum theory of atoms. Its importance was recognized immediately, even though it raised as many questions as it answered.

One of the most important questions it answered had to do with the Balmer formula:

l_¼ ^bn

2

n²4, (2:2:1)

wheren denotes an integer. This relation had been found in 1885 by Johann Jacob Balmer, a Swiss school teacher. Balmer pointed out that if b were given the value 3645.6, thenlequaled the wavelength (measured in A˚ ngstrom units, 1 A˚¼10²¹⁰m) of a line in the hydrogen spectrum¹ for n¼3, 4, 5, and 6 (and possibly for higher integers as well, but no measurements existed to conﬁrm or deny the possibility).

Laser Physics. By Peter W. Milonni and Joseph H. Eberly Copyright#2010 John Wiley & Sons, Inc.

1Historically, the term spectral “line” arose because lines appeared as images of slits in spectrometers.

17

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For almost 30 years the Balmer formula was a small oasis of regularity in the field of spectroscopy—the science of measuring and cataloging the wavelengths of radiation emitted and absorbed by different elements and compounds. Unfortunately, the Balmer formula could not be explained, or applied to any other element, or even applied to other known wavelengths emitted by hydrogen atoms. It might well have been a mere coincidence, without any significance. Bohr’s model of the hydrogen atom not only explained the Balmer formula, but also gave scientists their first glimpse of atomic structure. It still serves as the basis for most scientists’ working picture of an atom.

Bohr adopted Rutherford’s nuclear model that had been successful in explaining scattering experiments with alpha particles between 1910 and 1912. In other words, Bohr assumed that almost all the mass of a hydrogen atom is concentrated in a positively charged nucleus, allowing most of the atomic volume free for the motion of the much lighter electron. The electron was assumed attracted to the nucleus by the Coulomb force law governing opposite charges (Fig. 2.1). In magnitude this force is

F¼ 1 4pe₀

e²

r²: (2:2:2)

Bohr also assumed that the electron travels in a circular orbit about the massive nucleus. Moreover, he assumed the validity of Newton’s laws of motion for the orbit.

Thus, in common with every planetary body in a circular orbit, the electron was assumed to experience an inward (centripetal) acceleration of magnitude

a¼v²

r : (2:2:3)

Newton’s second law of motion,F¼ma, then gives mv²

r ¼ 1 4pe₀

e²

r², (2:2:4)

which is the same as saying that the electron’s kinetic energy,T¼¹₂mv², is half as great as the magnitude of its potential energy,V¼2e²/4pe0r. In the Coulomb ﬁeld of the

e

p r

Figure 2.1 The electron in the Bohr model is attracted to the nucleus with a force of magnitude F¼e²/4pe₀r².